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fagges
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faiged
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faiges
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felched
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felchered
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felchingly
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fellateing
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fellatioing
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feltched
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feltches
feltching
feltchly
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feomed
feomer
feomes
feoming
feomly
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fisteder
fistedes
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fisting
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fistyer
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fistying
fistyly
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floozyed
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floozyes
floozying
floozyly
floozys
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foaded
foader
foades
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foadly
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fondleer
fondlees
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foobarly
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freexed
freexer
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freexly
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frigga
friggaed
friggaer
friggaes
friggaing
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frigger
frigges
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friggly
friggs
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fubared
fubarer
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fubarly
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fuckedly
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fuckered
fuckerer
fuckeres
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The battle of the clot

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Preventing and treating thromboembolic disease remain vexing challenges for both physicians and patients. Warfarin has withstood the test of time as an inexpensive and effective anticoagulant, but it provokes angst in many prescribers because of its very narrow therapeutic window and many significant drug interactions. Low-molecular-weight heparins are easy to administer and have greatly simplified the acute and chronic treatment of thromboembolic disease, but they are quite expensive. Thus, it has been important to define the situations in which these drugs have the most to offer.

In this issue of the Journal we review two special situations in which low-molecular-weight heparins have special advantages. Babu and Carman discuss patients with cancer and thromboembolic disease. These patients are particularly difficult to manage since they tend to have recurrent thrombosis, sometimes even while on anticoagulant therapy, and they tend to have more bleeding complications from warfarin therapy. Inanition, drug interactions, and organ dysfunction make warfarin titration problematic, and the possibility of vascular metastases is always a concern. Low-molecular-weight heparins —which, unlike warfarin, work primarily by antagonizing factor Xa activity—have proven to be as effective as warfarin in reversing the many hypercoagulable effects of malignancy, although it wasn’t obvious at first that they would be.

Gibson and Powrie review the issues we face when pregnant patients need anticoagulation. While drug interactions and organ dysfunction are rarely problems in this setting, warfarin is teratogenic and is therefore strongly contraindicated early in pregnancy, and its peripartum use has been associated with bleeding complications. Furthermore, unfractionated heparin is associated with the development of osteoporosis, and it requires frequent injections. The low-molecular-weight heparins thus have a definite niche in the management of pregnant women, but with a caveat: dosing of these agents by weight alone in this setting is fraught with the potential for underdosing. Catastrophic outcomes have been reported in pregnant patients with older mechanical cardiac valves who were switched from warfarin to low-molecular-weight heparin therapy. Plus, if the patient is to receive neuraxial regional anesthesia, low-molecular-weight heparins should be discontinued at least 12 hours before catheter placement if prophylactic doses have been given, or 24 hours if therapeutic doses have been given.

Low-molecular-weight heparins have greatly enhanced our ability to treat thromboembolic disease. But, as the authors of these two papers discuss, many management nuances still must be noted.

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Preventing and treating thromboembolic disease remain vexing challenges for both physicians and patients. Warfarin has withstood the test of time as an inexpensive and effective anticoagulant, but it provokes angst in many prescribers because of its very narrow therapeutic window and many significant drug interactions. Low-molecular-weight heparins are easy to administer and have greatly simplified the acute and chronic treatment of thromboembolic disease, but they are quite expensive. Thus, it has been important to define the situations in which these drugs have the most to offer.

In this issue of the Journal we review two special situations in which low-molecular-weight heparins have special advantages. Babu and Carman discuss patients with cancer and thromboembolic disease. These patients are particularly difficult to manage since they tend to have recurrent thrombosis, sometimes even while on anticoagulant therapy, and they tend to have more bleeding complications from warfarin therapy. Inanition, drug interactions, and organ dysfunction make warfarin titration problematic, and the possibility of vascular metastases is always a concern. Low-molecular-weight heparins —which, unlike warfarin, work primarily by antagonizing factor Xa activity—have proven to be as effective as warfarin in reversing the many hypercoagulable effects of malignancy, although it wasn’t obvious at first that they would be.

Gibson and Powrie review the issues we face when pregnant patients need anticoagulation. While drug interactions and organ dysfunction are rarely problems in this setting, warfarin is teratogenic and is therefore strongly contraindicated early in pregnancy, and its peripartum use has been associated with bleeding complications. Furthermore, unfractionated heparin is associated with the development of osteoporosis, and it requires frequent injections. The low-molecular-weight heparins thus have a definite niche in the management of pregnant women, but with a caveat: dosing of these agents by weight alone in this setting is fraught with the potential for underdosing. Catastrophic outcomes have been reported in pregnant patients with older mechanical cardiac valves who were switched from warfarin to low-molecular-weight heparin therapy. Plus, if the patient is to receive neuraxial regional anesthesia, low-molecular-weight heparins should be discontinued at least 12 hours before catheter placement if prophylactic doses have been given, or 24 hours if therapeutic doses have been given.

Low-molecular-weight heparins have greatly enhanced our ability to treat thromboembolic disease. But, as the authors of these two papers discuss, many management nuances still must be noted.

Preventing and treating thromboembolic disease remain vexing challenges for both physicians and patients. Warfarin has withstood the test of time as an inexpensive and effective anticoagulant, but it provokes angst in many prescribers because of its very narrow therapeutic window and many significant drug interactions. Low-molecular-weight heparins are easy to administer and have greatly simplified the acute and chronic treatment of thromboembolic disease, but they are quite expensive. Thus, it has been important to define the situations in which these drugs have the most to offer.

In this issue of the Journal we review two special situations in which low-molecular-weight heparins have special advantages. Babu and Carman discuss patients with cancer and thromboembolic disease. These patients are particularly difficult to manage since they tend to have recurrent thrombosis, sometimes even while on anticoagulant therapy, and they tend to have more bleeding complications from warfarin therapy. Inanition, drug interactions, and organ dysfunction make warfarin titration problematic, and the possibility of vascular metastases is always a concern. Low-molecular-weight heparins —which, unlike warfarin, work primarily by antagonizing factor Xa activity—have proven to be as effective as warfarin in reversing the many hypercoagulable effects of malignancy, although it wasn’t obvious at first that they would be.

Gibson and Powrie review the issues we face when pregnant patients need anticoagulation. While drug interactions and organ dysfunction are rarely problems in this setting, warfarin is teratogenic and is therefore strongly contraindicated early in pregnancy, and its peripartum use has been associated with bleeding complications. Furthermore, unfractionated heparin is associated with the development of osteoporosis, and it requires frequent injections. The low-molecular-weight heparins thus have a definite niche in the management of pregnant women, but with a caveat: dosing of these agents by weight alone in this setting is fraught with the potential for underdosing. Catastrophic outcomes have been reported in pregnant patients with older mechanical cardiac valves who were switched from warfarin to low-molecular-weight heparin therapy. Plus, if the patient is to receive neuraxial regional anesthesia, low-molecular-weight heparins should be discontinued at least 12 hours before catheter placement if prophylactic doses have been given, or 24 hours if therapeutic doses have been given.

Low-molecular-weight heparins have greatly enhanced our ability to treat thromboembolic disease. But, as the authors of these two papers discuss, many management nuances still must be noted.

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Cancer and clots: All cases of venous thromboembolism are not treated the same

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Cancer and clots: All cases of venous thromboembolism are not treated the same

Venous thromboembolism (VTE) has various differing causes, so its treatment is not necessarily the same in all cases. Most cases of VTE are related to an easily identified risk factor. In patients with an apparently idiopathic event, identifying an underlying cause may alter therapy. In particular, identification of a malignancy may affect the choice of therapy and the duration of treatment.

In this review, we explore the role of cancer screening in patients with idiopathic VTE, then highlight the treatment for VTE in patients with cancer.

‘IDIOPATHIC’ VTE CAN BE DUE TO CANCER

Most patients with venous thrombosis have one of the components of Virchow’s triad: a hypercoagulable state, venous injury, or venous stasis. Those without identifiable risk factors for VTE are considered to have idiopathic VTE. In these patients, a search for a contributing factor may be indicated.

In 1861, the astute clinician Dr. Armand Trousseau noted a link between deep venous thrombosis and pancreatic cancer, stating that if cancer of an internal organ is suspected but the diagnosis cannot be verified, the diagnosis may be confirmed by the sudden, spontaneous appearance of thrombophlebitis in a large vein.1

Today, from 2% to 25% of patients with idiopathic VTE are found to have cancer within 24 months of the diagnosis of VTE.2–11 The goals of cancer screening in idiopathic VTE are to detect cancer at an early, treatable stage and to optimize the VTE therapy to decrease the risks of recurrence and anticoagulation-associated complications in patients who are found to have cancer. However, several questions must be considered first:

  • What are the risks and costs of the screening?
  • Will discovering the cancer sooner benefit the patient in terms of survival?
  • If cancer is found, what are the possible complications or risks of the additional procedures, interventions, or treatments required?
  • What is the psychological impact of the screening?

EVIDENCE SUPPORTING CANCER SCREENING AFTER IDIOPATHIC VTE

Piccioli et al12 recently performed a randomized, controlled trial comparing cancer-related death rates in 99 patients with idiopathic VTE screened for malignancy vs 102 patients with idiopathic VTE who were not screened.

The screened group underwent:

  • Abdominal and pelvic ultrasonography and computed tomography (CT)
  • Gastroscopy or double-contrast barium-swallow evaluation
  • Colonoscopy or sigmoidoscopy followed by barium enema
  • Testing for fecal occult blood
  • Sputum cytology
  • Measurement of carcinoembryonic antigen, alpha-fetoprotein, and cancer antigen 125.
  • Mammography and Papanicolaou smears (women)
  • Ultrasonography of the prostate and prostate-specific antigen testing (men).

Patients were followed for 2 years. The screening uncovered cancer in 13 patients. Cancer developed in one other patient in the screening group during follow-up; in the control group, 10 patients developed symptomatic cancer during follow-up. Overall, the time to cancer diagnosis was 11.6 months in the unscreened group vs 1 month in the screened group (P < .001). Nine of the 14 patients with cancer in the screened group had T1 or T2 disease without local or distant metastasis vs 2 of the 10 control patients with cancer (P = .047). Unfortunately, this study did not have adequate power to detect the effect of screening on survival.

Di Nisio et al13 used data from this trial to perform a decision analysis for cancer screening. They calculated that abdominal and pelvic CT, with or without mammography and with or without sputum cytologic testing, would cost the least per life-year gained and would harm the fewest number of patients. They also suggested that substituting CT of the chest for sputum cytology may provide additional diagnostic benefit.

However, this strategy has not been clinically tested. Given the limited number of patients and the short follow-up in this initial trial, larger trials are needed to look at the cost-effectiveness of this screening model and whether it increases survival.

Our recommendations

Because the data are limited, our approach to looking for an early, treatable malignancy in patients with idiopathic VTE follows the current consensus:

  • A thorough history and physical, including an extensive review of systems
  • Basic laboratory testing with a complete blood cell count, comprehensive metabolic profile, and urinalysis
  • Chest radiography
  • Other age- and sex-specific cancer screening tests.

Adding CT of the abdomen, pelvis, or chest to this evaluation may be considered. However, tumor marker testing, which typically has high false-positive rates, is not routinely warranted.13 Additional investigation should be considered if abnormalities are detected during the initial evaluation or in patients with recurrent VTE during therapy.

While this strategy may be most cost-effective, Monreal et al14 suggest that it may miss up to half of cancers ultimately discovered.

 

 

MANAGING VTE IN PATIENTS WITH KNOWN CANCER

Managing VTE is far more complex in cancer patients than in patients without cancer. Also, cancer patients with VTE have lower rates of survival than cancer patients without VTE and are at greater risk of adverse outcomes such as anticoagulant-associated bleeding and recurrent venous thrombotic events.15–17

Up to 21.5% of patients with VTE have another event within 5 years,18 but the risk is two to three times higher if they also have cancer.16,18 The risk of recurrence may be linked to the location of the thrombus and to the extent of the malignancy.

In one study, the 3-month rate of recurrence was up to 5.1% if the clot was in the popliteal vein, 5.3% if in the femoral vein, and 11.8% if in the iliac vein.19

Prandoni et al16 found that the risks of VTE recurrence and bleeding were higher in patients with extensive cancer than in those with less-extensive cancer. In this study, major bleeding was documented in 12.4% of patients with cancer vs 4.9% of patients without cancer. Compared with patients without cancer, the hazard ratio for a major bleeding event was 4.8 in patients with extensive cancer and 0.5 in patients with less-extensive cancer.

In addition, not all patients with bleeding had excessive levels of anticoagulation, and not all patients with recurrent events had subtherapeutic levels.16,17 Therefore, treatment of venous thrombosis in cancer patients requires a careful, individualized risk-to-benefit decision analysis.

ACUTE THERAPY FOR VTE: PARENTERAL AGENTS

Treatment in the first several hours or days after a thromboembolic event is with short-acting parenteral agents: unfractionated heparin; one of the low-molecular-weight heparins (LMWHs), ie, dalteparin (Fragmin), enoxaparin (Lovenox), or tinzaparin (Innohep); or fondaparinux (Arixtra).

Before starting anticoagulation, consider:

  • Does the patient have severe chronic kidney disease (ie, a creatinine clearance < 30 mL/min)? If so, unfractionated heparin may be better than an LMWH or fondaparinux, which are cleared by the kidney.
  • Does he or she need inpatient care? If not, LMWH therapy at home may be appropriate.
  • Are there concerns about the ease of anticoagulation administration (ie, whether the patient can give the injections or have a family member do it), the cost of the drugs, or the ability to reverse the anticoagulant effect, if necessary? If so, unfractionated heparin may be more appropriate.

For acute treatment, the 2008 guidelines of the American College of Chest Physicians20 (ACCP) recommend using an LMWH in a weight-based dose; unfractionated heparin given intravenously; unfractionated heparin given subcutaneously with monitoring and dosing adjustments; unfractionated heparin given subcutaneously at a fixed dose; or fondaparinux (grade 1A recommendation). The 2007 National Comprehensive Cancer Network (NCCN) guidelines21 recommend an LMWH, fondaparinux, or unfractionated heparin. Treatment should start promptly after the diagnosis of VTE is confirmed. However, if VTE is strongly suspected and a delay in diagnostic testing is anticipated, therapy should be started while awaiting the test results.

LONG-TERM THERAPY: LMWH OR WARFARIN

The ACCP and the NCCN guidelines recommend LMWH monotherapy for extended treatment of VTE in patients with active malignancy, when appropriate.20,21 However, if long-term LMWH is not appropriate, then oral anticoagulation with a vitamin K antagonist, such as the coumarin derivative warfarin (Coumadin), is an alternative and should be started on the same day as the heparin. The heparin and the warfarin therapy must overlap for a minimum of 4 or 5 days and until a stable, therapeutic level of anticoagulation is achieved, ie, an international normalized ratio (INR) of 2 to 3 for 2 consecutive days.20

The duration of anticoagulant therapy depends on comorbidities and the patient’s underlying predisposition for VTE. In patients with limited disease, the guidelines recommend continuing anticoagulation for a minimum of 3 to 6 months for deep venous thrombosis and pulmonary embolism.20–21 Patients with active malignancy, ongoing treatment for the cancer, or continued risk factors may need indefinite treatment. In some circumstances, such as catheter-associated deep venous thrombosis, anticoagulation should continue for as long as the catheter is in place and for 1 to 3 months after its removal.21

WARFARIN CAN BE DIFFICULT TO USE

In 1954, the US Food and Drug Administration (FDA) approved the vitamin K antagonist warfarin for medical use in humans. Experience has shown it to be effective in preventing and treating VTE. However, it can be somewhat difficult to use, for several reasons:

  • A narrow therapeutic window
  • Genetic polymorphisms and variability in dose response
  • Drug interactions and dietary considerations
  • The need for laboratory monitoring and dose adjustment
  • Patient noncompliance or miscommunication between the patient and physician.22

In cancer patients, the response to warfarin may be unpredictable because of poor nutrition, interactions with chemotherapy and antibiotics, and comorbid conditions.22 Furthermore, its onset of action can be delayed and its clearance may be prolonged, further increasing the risk of complications, especially in patients prone to developing chemotherapy-related anemia or thrombocytopenia.22 Bleeding risk is the highest in the first 3 months of therapy. In addition, the risk of bleeding is higher in older patients, women, and patients with a history of gastrointestinal bleeding, stroke, recent myocardial infarction, diabetes, renal insufficiency, malignancy, or anemia.23,24

 

 

ADVANTAGES AND DISADVANTAGES OF LMWH

The advantages of the LMWHs over unfractionated heparin include a lower risk of heparin-induced thrombocytopenia, greater bioavailability when given subcutaneously (which also permits once-daily or twice-daily dosing), and no need for laboratory monitoring in most patients. LMWHs have a short half-life, so omitting one or two doses will adequately interrupt therapy. Also, LMWHs have been shown to be as safe and effective as unfractionated heparin in treating VTE. They can be given safely at home, thus enhancing quality of life.25–31

On the other hand, these drugs cost more than unfractionated heparin or warfarin, their dosage must be adjusted in patients with renal insufficiency, their anticoagulant effect can be reversed only to a limited extent, and their dose must be adjusted according to weight in morbidly obese or in very thin patients.32,33

LMWHs are expensive, but may be worth it

As initial therapy, the LMWHs are cost-effective compared with unfractionated heparin in patients with VTE.34,35 However, they cost more with extended use. A cost-effectiveness analysis comparing 6 months of LMWH therapy to standard warfarin concluded that LMWH therapy was more costly.35 However, the impact of fewer hospitalizations, probably fewer bleeding complications, and better quality of life are difficult to analyze in this decision model and should also be considered when deciding about therapy for an individual patient.35

LMWHs are cleared by the kidney

All LMWHs are renally cleared, so patients with significant renal insufficiency (creatinine clearance < 30 mL/min) are at greater risk of bleeding complications. The rate below which clearance is impaired varies among the different LMWHs. Only enoxaparin has approved dosing regimens for use in patients with renal impairment.

If the patient has renal insufficiency, the ACCP guidelines suggest using unfractionated heparin, or if using LMWH, monitoring anti-factor Xa levels to avoid drug accumulation and increased bleeding risk.25 If bleeding occurs, LMWHs have limited reversibility with protamine sulfate, which is estimated to neutralize about 60% of the anti-factor Xa activity of LMWHs.25

Adjusting LMWHs for body weight

In the Registro Informatizado de la Enfermedad Tromboembólica (RIETE),33 patients weighing less than 50 kg had a higher risk of bleeding than patients weighing 50 to 100 kg, so in thinner patients the risk of bleeding from LMWH vs oral anticoagulation must be considered carefully and monitored prudently.

Although there is little evidence to suggest a higher bleeding risk in morbidly obese patients (> 150 kg), they may be at risk of subtherapeutic treatment, and monitoring with anti-factor Xa assays is recommended.25,32,33

LMWH VS WARFARIN FOR VTE IN CANCER PATIENTS

LMWHs are the first-line treatment for VTE in cancer patients.20,21 Several randomized controlled trials compared the efficacy of LMWH vs warfarin in patients with cancer.

Meyer et al36 randomized patients to receive either warfarin for 3 months at an INR between 2 and 3, or enoxaparin 1.5 mg/kg subcutaneously daily. Seventy-one patients received warfarin and 67 received enoxaparin. Fifteen (21%, 95% confidence interval [CI] 12%–32%) of the 71 patients assigned to warfarin experienced one major outcome event, defined as major bleeding or recurrent VTE, compared with 7 (10.5%) of the 67 patients assigned to receive enoxaparin (95% CI 4%–20%, P = .09). Six patients in the warfarin group died of bleeding vs none of the patients in the enoxaparin group. Overall, the warfarin group had a higher rate of bleeding, although this did not reach statistical significance. Despite weekly INR measurements, only 41% of the measured values were within the therapeutic range during the 3 months of treatment.36

Lee et al37 randomized cancer patients with deep venous thrombosis, pulmonary embolism, or both to receive 6 months of dalteparin alone, dosed at 200 IU/kg daily for 1 month, then decreased to 75% to 80% of the original dose (150 IU/kg) daily for the duration of therapy, or dalteparin followed by warfarin. During the 6-month follow-up, 17.4% of patients in the warfarin group had a recurrent thromboembolic event vs 8.8% in the dalteparin group (P = .0017). No statistically significant difference was noted in rates of major bleeding, minor bleeding, or death.37

Hull et al38 reported statistically significantly fewer episodes of recurrent VTE at 12 months in cancer patients treated with once-daily tinzaparin vs warfarin. In the tinzaparin group the recurrence rate was 7%, vs 16% in the warfarin group (P = .044). No difference in rates of bleeding or death were found.

Deitcher et al39 compared enoxaparin with long-term warfarin in 102 patients. While this trial did not have the power to detect clinical differences in recurrent thromboembolic events or bleeding complications, at 180 days they noted 97% compliance with once-daily or twice-daily enoxaparin therapy.

Noble and Finlay,40 in another small study, found LMWH therapy to be qualitatively more acceptable for palliative-care cancer patients than oral therapy.

In general, long-term therapy with once-daily or twice-daily LMWH is well tolerated. Currently, dalteparin is the only LMWH approved by the FDA for extended monotherapy in cancer-related VTE.

 

 

DO LMWHS AFFECT CANCER?

In vitro and animal studies indicate that LMWH may have antimetastatic and antiangiogenic properties.41–44

Altinbas et al45 reported significantly better chemotherapy-induced tumor response rates and survival rates in patients with small cell lung cancer randomized to receive combination chemotherapy plus prophylactic dalteparin 5,000 IU daily compared with combination chemotherapy alone. However, as provocative as these results may be, we need to test the effects of LWMHs on different cancer types in a prospective clinical trial. For now, this area remains controversial.

It has been suggested that anticoagulants may improve survival in patients with nonmetastatic cancer. Supporting this observation, a post hoc analysis of the trial by Lee et al37 found a statistically significantly lower cancer-specific mortality rate in nonmetastatic cancer patients treated with dalteparin vs oral therapy with a coumarin derivative. In patients without metastatic disease, the death rate at 12 months was 36% in patients treated with oral therapy vs 20% in patients treated with dalteparin (P = .03).46

These findings are consistent with those of the Fragmin Advanced Malignancy Outcome Study (FAMOUS),47 the first randomized, placebo-controlled trial of dalteparin 5,000 IU daily in patients with advanced solid tumors and without evidence of underlying thrombosis. Overall, dalteparin prophylaxis did not increase survival. However, in a subgroup of patients with a better prognosis and who were alive 17 months after diagnosis, survival was statistically significantly longer in patients treated with dalteparin.

Another small trial showed similar survival benefits in cancer patients without VTE.48 The results may suggest a long-term favorable effect of LMWH on tumor cell biology, which could translate into a favorable outcome in some patients. It is important to note, however, that not all trials have shown this same clinical benefit.49

In general, the growing body of laboratory and clinical data indicates that LMWHs may suppress tumor growth and metastasis. However, definitive conclusions about these effects are not yet possible because of variations in study design, tumor type, and patient populations. Further investigations into the role of LMWHs in the treatment of VTE and in cancer progression are ongoing.

THE EVIDENCE IN PERSPECTIVE

Illness and the recurrence of VTE in patients with cancer depend on the location and extent of the underlying cancer. Rates of death are higher in VTE patients with cancer than in VTE patients without cancer. Patients with limited or localized disease may not die of the cancer itself but of complications of acute pulmonary embolism. Therefore, it is important to recognize the different options for and the potential side effects of treating VTE.

If patients are hospitalized for an acute thromboembolic event and unfractionated heparin is chosen as the initial anticoagulant, using a weight-based nomogram has been shown to achieve therapeutic levels within 24 hours and reduce the rates of recurrence of thromboembolic events.50

Warfarin treatment may pose a particular challenge for both cancer patients and physicians, since multiple drug interactions, anorexia, and comorbid conditions contribute to an unpredictable response.

The risk of bleeding is higher in cancer patients than in the general population, and the decision to start anticoagulants should be based on an individualized risk-benefit profile. Several trials have shown LMWH to be more effective and safer than warfarin in cancer patients.

These considerations, along with the other advantages of LMWHs (ease of use, less need for laboratory monitoring, and better patient tolerance), make LMWHs a good choice for initial therapy. Extended LMWH therapy is currently favored for initial management in patients with cancer. Trials are under way to further assess the antitumor properties and potential survival benefit in patients with selected solid tumors.

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  21. National Comprehensive Cancer Network. Venous Thromboembolic Disease Clinical Practice Guidelines in Oncology (V.1.2007). Available at www.nccn.org/professionals/physician_gls/PDF/vte.pdf. Accessed 01/02/2008.
  22. Ansell J, Hirsh J, Poller L, Bussey H, Jacobson A, Hylek E. The pharmacology and management of the vitamin K antagonists: the Seventh ACCP Conference on Antithrombotic and Thrombolytic Therapy. Chest 2004; 126 suppl 3:204S233S.
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  31. van Dongen CJ, van den Belt AG, Prins MH, Lensing AW. Fixed dose subcutaneous low molecular weight heparins versus adjusted dose unfractionated heparin for venous thromboembolism. Cochrane Database Syst Rev 2004; 4:CD001100.
  32. Cook LM, Kahn SR, Goodwin J, Kovacs MJ. Frequency of renal impairment, advanced age, obesity, and cancer in venous thromboembolism patients in clinical practice. J Thromb Haemost 2007; 5:937941.
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  34. Segal JB, Strieff MB, Hofmann LV, Thornton K, Bass EB. Management of venous thromboembolism: a systematic review for a practice guideline. Ann Intern Med 2007; 146:211222.
  35. Aujesky D, Smith KJ, Cornuz J, Roberts MS. Cost-effectiveness of low-molecular-weight heparin for secondary prophylaxis of cancer-related venous thromboembolism. Thromb Haemost 2005; 93:592599.
  36. Meyer G, Marjanovic Z, Valcke J, et al. Comparison of low-molecular-weight heparin and warfarin for the secondary prevention of venous thromboembolism in patients with cancer: a randomized controlled study. Arch Intern Med 2002; 162:17291735.
  37. Lee AY, Levine MN, Baker RI, et al. Low-molecular-weight heparin versus a coumarin for the prevention of recurrent venous thromboembolism in patients with cancer. N Engl J Med 2003; 349:146153.
  38. Hull RD, Pineo GF, Brant RF, et al. Long-term low-molecular-weight heparin versus usual care in proximal-vein thrombosis patients with cancer. Am J Med 2006; 119:10621072.
  39. Deitcher SR, Kessler CM, Merli G, Rigas JR, Lyons RM, Fareed J ON-CENOX investigators. Secondary prevention of venous thromboembolic events in patients with active cancer: enoxaparin alone versus initial enoxaparin followed by warfarin for a 180-day period. Clin Appl Thromb Hemost 2006; 12:389396.
  40. Noble SI, Finlay IG. Is long-term low-molecular-weight heparin acceptable to palliative care patients in the treatment of cancer related venous thromboembolism? A qualitative study. Palliat Med 2005; 19:197201.
  41. Amirkhosravi A, Mousa SA, Amaya M, Francis JL. Antimetastatic effect of tinzaparin, a low-molecular-weight heparin. J Thromb Haemost 2003; 1:19721976.
  42. Kragh M, Binderup L, Vig Hjarnaa PJ, Bramm E, Johansen KB, Frimundt Petersen C. Non-anti-coagulant heparin inhibits metastasis but not primary tumor growth. Oncol Rep 2005; 14:99104.
  43. Mousa SA, Mohamed S. Anti-angiogenic mechanisms and efficacy of the low molecular weight heparin, tinzaparin: anti-cancer efficacy. Oncol Rep 2004; 12:683688.
  44. Bobek V, Kovarik J. Antitumor and antimetastatic effect of warfarin and heparins. Biomed Pharmacother 2004; 58:213219.
  45. Altinbas M, Coskun HS, Er O, et al. A randomized clinical trial of combination chemotherapy with and without low-molecular-weight heparin in small cell lung cancer. J Thromb Haemost 2004; 2:12661271.
  46. Lee AY, Rickles FR, Julian JA, et al. Randomized comparison of low molecular weight heparin and coumarin derivatives on the survival of patients with cancer and venous thromboembolism. J Clin Oncol 2005; 23:21232129.
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  49. Sideras K, Schaefer PL, Okuno SH, et al. Low-molecular-weight heparin in patients with advanced cancer: a phase 3 clinical trial. Mayo Clin Proc 2006; 81:758767.
  50. Bernardi E, Piccioli A, Oliboni G, Zuin R, Girolami A, Prandoni P. Nomograms for the administration of unfractionated heparin in the initial treatment of acute thromboembolism—an overview. Thromb Haemost 2000; 84:2226.
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Related Articles

Venous thromboembolism (VTE) has various differing causes, so its treatment is not necessarily the same in all cases. Most cases of VTE are related to an easily identified risk factor. In patients with an apparently idiopathic event, identifying an underlying cause may alter therapy. In particular, identification of a malignancy may affect the choice of therapy and the duration of treatment.

In this review, we explore the role of cancer screening in patients with idiopathic VTE, then highlight the treatment for VTE in patients with cancer.

‘IDIOPATHIC’ VTE CAN BE DUE TO CANCER

Most patients with venous thrombosis have one of the components of Virchow’s triad: a hypercoagulable state, venous injury, or venous stasis. Those without identifiable risk factors for VTE are considered to have idiopathic VTE. In these patients, a search for a contributing factor may be indicated.

In 1861, the astute clinician Dr. Armand Trousseau noted a link between deep venous thrombosis and pancreatic cancer, stating that if cancer of an internal organ is suspected but the diagnosis cannot be verified, the diagnosis may be confirmed by the sudden, spontaneous appearance of thrombophlebitis in a large vein.1

Today, from 2% to 25% of patients with idiopathic VTE are found to have cancer within 24 months of the diagnosis of VTE.2–11 The goals of cancer screening in idiopathic VTE are to detect cancer at an early, treatable stage and to optimize the VTE therapy to decrease the risks of recurrence and anticoagulation-associated complications in patients who are found to have cancer. However, several questions must be considered first:

  • What are the risks and costs of the screening?
  • Will discovering the cancer sooner benefit the patient in terms of survival?
  • If cancer is found, what are the possible complications or risks of the additional procedures, interventions, or treatments required?
  • What is the psychological impact of the screening?

EVIDENCE SUPPORTING CANCER SCREENING AFTER IDIOPATHIC VTE

Piccioli et al12 recently performed a randomized, controlled trial comparing cancer-related death rates in 99 patients with idiopathic VTE screened for malignancy vs 102 patients with idiopathic VTE who were not screened.

The screened group underwent:

  • Abdominal and pelvic ultrasonography and computed tomography (CT)
  • Gastroscopy or double-contrast barium-swallow evaluation
  • Colonoscopy or sigmoidoscopy followed by barium enema
  • Testing for fecal occult blood
  • Sputum cytology
  • Measurement of carcinoembryonic antigen, alpha-fetoprotein, and cancer antigen 125.
  • Mammography and Papanicolaou smears (women)
  • Ultrasonography of the prostate and prostate-specific antigen testing (men).

Patients were followed for 2 years. The screening uncovered cancer in 13 patients. Cancer developed in one other patient in the screening group during follow-up; in the control group, 10 patients developed symptomatic cancer during follow-up. Overall, the time to cancer diagnosis was 11.6 months in the unscreened group vs 1 month in the screened group (P < .001). Nine of the 14 patients with cancer in the screened group had T1 or T2 disease without local or distant metastasis vs 2 of the 10 control patients with cancer (P = .047). Unfortunately, this study did not have adequate power to detect the effect of screening on survival.

Di Nisio et al13 used data from this trial to perform a decision analysis for cancer screening. They calculated that abdominal and pelvic CT, with or without mammography and with or without sputum cytologic testing, would cost the least per life-year gained and would harm the fewest number of patients. They also suggested that substituting CT of the chest for sputum cytology may provide additional diagnostic benefit.

However, this strategy has not been clinically tested. Given the limited number of patients and the short follow-up in this initial trial, larger trials are needed to look at the cost-effectiveness of this screening model and whether it increases survival.

Our recommendations

Because the data are limited, our approach to looking for an early, treatable malignancy in patients with idiopathic VTE follows the current consensus:

  • A thorough history and physical, including an extensive review of systems
  • Basic laboratory testing with a complete blood cell count, comprehensive metabolic profile, and urinalysis
  • Chest radiography
  • Other age- and sex-specific cancer screening tests.

Adding CT of the abdomen, pelvis, or chest to this evaluation may be considered. However, tumor marker testing, which typically has high false-positive rates, is not routinely warranted.13 Additional investigation should be considered if abnormalities are detected during the initial evaluation or in patients with recurrent VTE during therapy.

While this strategy may be most cost-effective, Monreal et al14 suggest that it may miss up to half of cancers ultimately discovered.

 

 

MANAGING VTE IN PATIENTS WITH KNOWN CANCER

Managing VTE is far more complex in cancer patients than in patients without cancer. Also, cancer patients with VTE have lower rates of survival than cancer patients without VTE and are at greater risk of adverse outcomes such as anticoagulant-associated bleeding and recurrent venous thrombotic events.15–17

Up to 21.5% of patients with VTE have another event within 5 years,18 but the risk is two to three times higher if they also have cancer.16,18 The risk of recurrence may be linked to the location of the thrombus and to the extent of the malignancy.

In one study, the 3-month rate of recurrence was up to 5.1% if the clot was in the popliteal vein, 5.3% if in the femoral vein, and 11.8% if in the iliac vein.19

Prandoni et al16 found that the risks of VTE recurrence and bleeding were higher in patients with extensive cancer than in those with less-extensive cancer. In this study, major bleeding was documented in 12.4% of patients with cancer vs 4.9% of patients without cancer. Compared with patients without cancer, the hazard ratio for a major bleeding event was 4.8 in patients with extensive cancer and 0.5 in patients with less-extensive cancer.

In addition, not all patients with bleeding had excessive levels of anticoagulation, and not all patients with recurrent events had subtherapeutic levels.16,17 Therefore, treatment of venous thrombosis in cancer patients requires a careful, individualized risk-to-benefit decision analysis.

ACUTE THERAPY FOR VTE: PARENTERAL AGENTS

Treatment in the first several hours or days after a thromboembolic event is with short-acting parenteral agents: unfractionated heparin; one of the low-molecular-weight heparins (LMWHs), ie, dalteparin (Fragmin), enoxaparin (Lovenox), or tinzaparin (Innohep); or fondaparinux (Arixtra).

Before starting anticoagulation, consider:

  • Does the patient have severe chronic kidney disease (ie, a creatinine clearance < 30 mL/min)? If so, unfractionated heparin may be better than an LMWH or fondaparinux, which are cleared by the kidney.
  • Does he or she need inpatient care? If not, LMWH therapy at home may be appropriate.
  • Are there concerns about the ease of anticoagulation administration (ie, whether the patient can give the injections or have a family member do it), the cost of the drugs, or the ability to reverse the anticoagulant effect, if necessary? If so, unfractionated heparin may be more appropriate.

For acute treatment, the 2008 guidelines of the American College of Chest Physicians20 (ACCP) recommend using an LMWH in a weight-based dose; unfractionated heparin given intravenously; unfractionated heparin given subcutaneously with monitoring and dosing adjustments; unfractionated heparin given subcutaneously at a fixed dose; or fondaparinux (grade 1A recommendation). The 2007 National Comprehensive Cancer Network (NCCN) guidelines21 recommend an LMWH, fondaparinux, or unfractionated heparin. Treatment should start promptly after the diagnosis of VTE is confirmed. However, if VTE is strongly suspected and a delay in diagnostic testing is anticipated, therapy should be started while awaiting the test results.

LONG-TERM THERAPY: LMWH OR WARFARIN

The ACCP and the NCCN guidelines recommend LMWH monotherapy for extended treatment of VTE in patients with active malignancy, when appropriate.20,21 However, if long-term LMWH is not appropriate, then oral anticoagulation with a vitamin K antagonist, such as the coumarin derivative warfarin (Coumadin), is an alternative and should be started on the same day as the heparin. The heparin and the warfarin therapy must overlap for a minimum of 4 or 5 days and until a stable, therapeutic level of anticoagulation is achieved, ie, an international normalized ratio (INR) of 2 to 3 for 2 consecutive days.20

The duration of anticoagulant therapy depends on comorbidities and the patient’s underlying predisposition for VTE. In patients with limited disease, the guidelines recommend continuing anticoagulation for a minimum of 3 to 6 months for deep venous thrombosis and pulmonary embolism.20–21 Patients with active malignancy, ongoing treatment for the cancer, or continued risk factors may need indefinite treatment. In some circumstances, such as catheter-associated deep venous thrombosis, anticoagulation should continue for as long as the catheter is in place and for 1 to 3 months after its removal.21

WARFARIN CAN BE DIFFICULT TO USE

In 1954, the US Food and Drug Administration (FDA) approved the vitamin K antagonist warfarin for medical use in humans. Experience has shown it to be effective in preventing and treating VTE. However, it can be somewhat difficult to use, for several reasons:

  • A narrow therapeutic window
  • Genetic polymorphisms and variability in dose response
  • Drug interactions and dietary considerations
  • The need for laboratory monitoring and dose adjustment
  • Patient noncompliance or miscommunication between the patient and physician.22

In cancer patients, the response to warfarin may be unpredictable because of poor nutrition, interactions with chemotherapy and antibiotics, and comorbid conditions.22 Furthermore, its onset of action can be delayed and its clearance may be prolonged, further increasing the risk of complications, especially in patients prone to developing chemotherapy-related anemia or thrombocytopenia.22 Bleeding risk is the highest in the first 3 months of therapy. In addition, the risk of bleeding is higher in older patients, women, and patients with a history of gastrointestinal bleeding, stroke, recent myocardial infarction, diabetes, renal insufficiency, malignancy, or anemia.23,24

 

 

ADVANTAGES AND DISADVANTAGES OF LMWH

The advantages of the LMWHs over unfractionated heparin include a lower risk of heparin-induced thrombocytopenia, greater bioavailability when given subcutaneously (which also permits once-daily or twice-daily dosing), and no need for laboratory monitoring in most patients. LMWHs have a short half-life, so omitting one or two doses will adequately interrupt therapy. Also, LMWHs have been shown to be as safe and effective as unfractionated heparin in treating VTE. They can be given safely at home, thus enhancing quality of life.25–31

On the other hand, these drugs cost more than unfractionated heparin or warfarin, their dosage must be adjusted in patients with renal insufficiency, their anticoagulant effect can be reversed only to a limited extent, and their dose must be adjusted according to weight in morbidly obese or in very thin patients.32,33

LMWHs are expensive, but may be worth it

As initial therapy, the LMWHs are cost-effective compared with unfractionated heparin in patients with VTE.34,35 However, they cost more with extended use. A cost-effectiveness analysis comparing 6 months of LMWH therapy to standard warfarin concluded that LMWH therapy was more costly.35 However, the impact of fewer hospitalizations, probably fewer bleeding complications, and better quality of life are difficult to analyze in this decision model and should also be considered when deciding about therapy for an individual patient.35

LMWHs are cleared by the kidney

All LMWHs are renally cleared, so patients with significant renal insufficiency (creatinine clearance < 30 mL/min) are at greater risk of bleeding complications. The rate below which clearance is impaired varies among the different LMWHs. Only enoxaparin has approved dosing regimens for use in patients with renal impairment.

If the patient has renal insufficiency, the ACCP guidelines suggest using unfractionated heparin, or if using LMWH, monitoring anti-factor Xa levels to avoid drug accumulation and increased bleeding risk.25 If bleeding occurs, LMWHs have limited reversibility with protamine sulfate, which is estimated to neutralize about 60% of the anti-factor Xa activity of LMWHs.25

Adjusting LMWHs for body weight

In the Registro Informatizado de la Enfermedad Tromboembólica (RIETE),33 patients weighing less than 50 kg had a higher risk of bleeding than patients weighing 50 to 100 kg, so in thinner patients the risk of bleeding from LMWH vs oral anticoagulation must be considered carefully and monitored prudently.

Although there is little evidence to suggest a higher bleeding risk in morbidly obese patients (> 150 kg), they may be at risk of subtherapeutic treatment, and monitoring with anti-factor Xa assays is recommended.25,32,33

LMWH VS WARFARIN FOR VTE IN CANCER PATIENTS

LMWHs are the first-line treatment for VTE in cancer patients.20,21 Several randomized controlled trials compared the efficacy of LMWH vs warfarin in patients with cancer.

Meyer et al36 randomized patients to receive either warfarin for 3 months at an INR between 2 and 3, or enoxaparin 1.5 mg/kg subcutaneously daily. Seventy-one patients received warfarin and 67 received enoxaparin. Fifteen (21%, 95% confidence interval [CI] 12%–32%) of the 71 patients assigned to warfarin experienced one major outcome event, defined as major bleeding or recurrent VTE, compared with 7 (10.5%) of the 67 patients assigned to receive enoxaparin (95% CI 4%–20%, P = .09). Six patients in the warfarin group died of bleeding vs none of the patients in the enoxaparin group. Overall, the warfarin group had a higher rate of bleeding, although this did not reach statistical significance. Despite weekly INR measurements, only 41% of the measured values were within the therapeutic range during the 3 months of treatment.36

Lee et al37 randomized cancer patients with deep venous thrombosis, pulmonary embolism, or both to receive 6 months of dalteparin alone, dosed at 200 IU/kg daily for 1 month, then decreased to 75% to 80% of the original dose (150 IU/kg) daily for the duration of therapy, or dalteparin followed by warfarin. During the 6-month follow-up, 17.4% of patients in the warfarin group had a recurrent thromboembolic event vs 8.8% in the dalteparin group (P = .0017). No statistically significant difference was noted in rates of major bleeding, minor bleeding, or death.37

Hull et al38 reported statistically significantly fewer episodes of recurrent VTE at 12 months in cancer patients treated with once-daily tinzaparin vs warfarin. In the tinzaparin group the recurrence rate was 7%, vs 16% in the warfarin group (P = .044). No difference in rates of bleeding or death were found.

Deitcher et al39 compared enoxaparin with long-term warfarin in 102 patients. While this trial did not have the power to detect clinical differences in recurrent thromboembolic events or bleeding complications, at 180 days they noted 97% compliance with once-daily or twice-daily enoxaparin therapy.

Noble and Finlay,40 in another small study, found LMWH therapy to be qualitatively more acceptable for palliative-care cancer patients than oral therapy.

In general, long-term therapy with once-daily or twice-daily LMWH is well tolerated. Currently, dalteparin is the only LMWH approved by the FDA for extended monotherapy in cancer-related VTE.

 

 

DO LMWHS AFFECT CANCER?

In vitro and animal studies indicate that LMWH may have antimetastatic and antiangiogenic properties.41–44

Altinbas et al45 reported significantly better chemotherapy-induced tumor response rates and survival rates in patients with small cell lung cancer randomized to receive combination chemotherapy plus prophylactic dalteparin 5,000 IU daily compared with combination chemotherapy alone. However, as provocative as these results may be, we need to test the effects of LWMHs on different cancer types in a prospective clinical trial. For now, this area remains controversial.

It has been suggested that anticoagulants may improve survival in patients with nonmetastatic cancer. Supporting this observation, a post hoc analysis of the trial by Lee et al37 found a statistically significantly lower cancer-specific mortality rate in nonmetastatic cancer patients treated with dalteparin vs oral therapy with a coumarin derivative. In patients without metastatic disease, the death rate at 12 months was 36% in patients treated with oral therapy vs 20% in patients treated with dalteparin (P = .03).46

These findings are consistent with those of the Fragmin Advanced Malignancy Outcome Study (FAMOUS),47 the first randomized, placebo-controlled trial of dalteparin 5,000 IU daily in patients with advanced solid tumors and without evidence of underlying thrombosis. Overall, dalteparin prophylaxis did not increase survival. However, in a subgroup of patients with a better prognosis and who were alive 17 months after diagnosis, survival was statistically significantly longer in patients treated with dalteparin.

Another small trial showed similar survival benefits in cancer patients without VTE.48 The results may suggest a long-term favorable effect of LMWH on tumor cell biology, which could translate into a favorable outcome in some patients. It is important to note, however, that not all trials have shown this same clinical benefit.49

In general, the growing body of laboratory and clinical data indicates that LMWHs may suppress tumor growth and metastasis. However, definitive conclusions about these effects are not yet possible because of variations in study design, tumor type, and patient populations. Further investigations into the role of LMWHs in the treatment of VTE and in cancer progression are ongoing.

THE EVIDENCE IN PERSPECTIVE

Illness and the recurrence of VTE in patients with cancer depend on the location and extent of the underlying cancer. Rates of death are higher in VTE patients with cancer than in VTE patients without cancer. Patients with limited or localized disease may not die of the cancer itself but of complications of acute pulmonary embolism. Therefore, it is important to recognize the different options for and the potential side effects of treating VTE.

If patients are hospitalized for an acute thromboembolic event and unfractionated heparin is chosen as the initial anticoagulant, using a weight-based nomogram has been shown to achieve therapeutic levels within 24 hours and reduce the rates of recurrence of thromboembolic events.50

Warfarin treatment may pose a particular challenge for both cancer patients and physicians, since multiple drug interactions, anorexia, and comorbid conditions contribute to an unpredictable response.

The risk of bleeding is higher in cancer patients than in the general population, and the decision to start anticoagulants should be based on an individualized risk-benefit profile. Several trials have shown LMWH to be more effective and safer than warfarin in cancer patients.

These considerations, along with the other advantages of LMWHs (ease of use, less need for laboratory monitoring, and better patient tolerance), make LMWHs a good choice for initial therapy. Extended LMWH therapy is currently favored for initial management in patients with cancer. Trials are under way to further assess the antitumor properties and potential survival benefit in patients with selected solid tumors.

Venous thromboembolism (VTE) has various differing causes, so its treatment is not necessarily the same in all cases. Most cases of VTE are related to an easily identified risk factor. In patients with an apparently idiopathic event, identifying an underlying cause may alter therapy. In particular, identification of a malignancy may affect the choice of therapy and the duration of treatment.

In this review, we explore the role of cancer screening in patients with idiopathic VTE, then highlight the treatment for VTE in patients with cancer.

‘IDIOPATHIC’ VTE CAN BE DUE TO CANCER

Most patients with venous thrombosis have one of the components of Virchow’s triad: a hypercoagulable state, venous injury, or venous stasis. Those without identifiable risk factors for VTE are considered to have idiopathic VTE. In these patients, a search for a contributing factor may be indicated.

In 1861, the astute clinician Dr. Armand Trousseau noted a link between deep venous thrombosis and pancreatic cancer, stating that if cancer of an internal organ is suspected but the diagnosis cannot be verified, the diagnosis may be confirmed by the sudden, spontaneous appearance of thrombophlebitis in a large vein.1

Today, from 2% to 25% of patients with idiopathic VTE are found to have cancer within 24 months of the diagnosis of VTE.2–11 The goals of cancer screening in idiopathic VTE are to detect cancer at an early, treatable stage and to optimize the VTE therapy to decrease the risks of recurrence and anticoagulation-associated complications in patients who are found to have cancer. However, several questions must be considered first:

  • What are the risks and costs of the screening?
  • Will discovering the cancer sooner benefit the patient in terms of survival?
  • If cancer is found, what are the possible complications or risks of the additional procedures, interventions, or treatments required?
  • What is the psychological impact of the screening?

EVIDENCE SUPPORTING CANCER SCREENING AFTER IDIOPATHIC VTE

Piccioli et al12 recently performed a randomized, controlled trial comparing cancer-related death rates in 99 patients with idiopathic VTE screened for malignancy vs 102 patients with idiopathic VTE who were not screened.

The screened group underwent:

  • Abdominal and pelvic ultrasonography and computed tomography (CT)
  • Gastroscopy or double-contrast barium-swallow evaluation
  • Colonoscopy or sigmoidoscopy followed by barium enema
  • Testing for fecal occult blood
  • Sputum cytology
  • Measurement of carcinoembryonic antigen, alpha-fetoprotein, and cancer antigen 125.
  • Mammography and Papanicolaou smears (women)
  • Ultrasonography of the prostate and prostate-specific antigen testing (men).

Patients were followed for 2 years. The screening uncovered cancer in 13 patients. Cancer developed in one other patient in the screening group during follow-up; in the control group, 10 patients developed symptomatic cancer during follow-up. Overall, the time to cancer diagnosis was 11.6 months in the unscreened group vs 1 month in the screened group (P < .001). Nine of the 14 patients with cancer in the screened group had T1 or T2 disease without local or distant metastasis vs 2 of the 10 control patients with cancer (P = .047). Unfortunately, this study did not have adequate power to detect the effect of screening on survival.

Di Nisio et al13 used data from this trial to perform a decision analysis for cancer screening. They calculated that abdominal and pelvic CT, with or without mammography and with or without sputum cytologic testing, would cost the least per life-year gained and would harm the fewest number of patients. They also suggested that substituting CT of the chest for sputum cytology may provide additional diagnostic benefit.

However, this strategy has not been clinically tested. Given the limited number of patients and the short follow-up in this initial trial, larger trials are needed to look at the cost-effectiveness of this screening model and whether it increases survival.

Our recommendations

Because the data are limited, our approach to looking for an early, treatable malignancy in patients with idiopathic VTE follows the current consensus:

  • A thorough history and physical, including an extensive review of systems
  • Basic laboratory testing with a complete blood cell count, comprehensive metabolic profile, and urinalysis
  • Chest radiography
  • Other age- and sex-specific cancer screening tests.

Adding CT of the abdomen, pelvis, or chest to this evaluation may be considered. However, tumor marker testing, which typically has high false-positive rates, is not routinely warranted.13 Additional investigation should be considered if abnormalities are detected during the initial evaluation or in patients with recurrent VTE during therapy.

While this strategy may be most cost-effective, Monreal et al14 suggest that it may miss up to half of cancers ultimately discovered.

 

 

MANAGING VTE IN PATIENTS WITH KNOWN CANCER

Managing VTE is far more complex in cancer patients than in patients without cancer. Also, cancer patients with VTE have lower rates of survival than cancer patients without VTE and are at greater risk of adverse outcomes such as anticoagulant-associated bleeding and recurrent venous thrombotic events.15–17

Up to 21.5% of patients with VTE have another event within 5 years,18 but the risk is two to three times higher if they also have cancer.16,18 The risk of recurrence may be linked to the location of the thrombus and to the extent of the malignancy.

In one study, the 3-month rate of recurrence was up to 5.1% if the clot was in the popliteal vein, 5.3% if in the femoral vein, and 11.8% if in the iliac vein.19

Prandoni et al16 found that the risks of VTE recurrence and bleeding were higher in patients with extensive cancer than in those with less-extensive cancer. In this study, major bleeding was documented in 12.4% of patients with cancer vs 4.9% of patients without cancer. Compared with patients without cancer, the hazard ratio for a major bleeding event was 4.8 in patients with extensive cancer and 0.5 in patients with less-extensive cancer.

In addition, not all patients with bleeding had excessive levels of anticoagulation, and not all patients with recurrent events had subtherapeutic levels.16,17 Therefore, treatment of venous thrombosis in cancer patients requires a careful, individualized risk-to-benefit decision analysis.

ACUTE THERAPY FOR VTE: PARENTERAL AGENTS

Treatment in the first several hours or days after a thromboembolic event is with short-acting parenteral agents: unfractionated heparin; one of the low-molecular-weight heparins (LMWHs), ie, dalteparin (Fragmin), enoxaparin (Lovenox), or tinzaparin (Innohep); or fondaparinux (Arixtra).

Before starting anticoagulation, consider:

  • Does the patient have severe chronic kidney disease (ie, a creatinine clearance < 30 mL/min)? If so, unfractionated heparin may be better than an LMWH or fondaparinux, which are cleared by the kidney.
  • Does he or she need inpatient care? If not, LMWH therapy at home may be appropriate.
  • Are there concerns about the ease of anticoagulation administration (ie, whether the patient can give the injections or have a family member do it), the cost of the drugs, or the ability to reverse the anticoagulant effect, if necessary? If so, unfractionated heparin may be more appropriate.

For acute treatment, the 2008 guidelines of the American College of Chest Physicians20 (ACCP) recommend using an LMWH in a weight-based dose; unfractionated heparin given intravenously; unfractionated heparin given subcutaneously with monitoring and dosing adjustments; unfractionated heparin given subcutaneously at a fixed dose; or fondaparinux (grade 1A recommendation). The 2007 National Comprehensive Cancer Network (NCCN) guidelines21 recommend an LMWH, fondaparinux, or unfractionated heparin. Treatment should start promptly after the diagnosis of VTE is confirmed. However, if VTE is strongly suspected and a delay in diagnostic testing is anticipated, therapy should be started while awaiting the test results.

LONG-TERM THERAPY: LMWH OR WARFARIN

The ACCP and the NCCN guidelines recommend LMWH monotherapy for extended treatment of VTE in patients with active malignancy, when appropriate.20,21 However, if long-term LMWH is not appropriate, then oral anticoagulation with a vitamin K antagonist, such as the coumarin derivative warfarin (Coumadin), is an alternative and should be started on the same day as the heparin. The heparin and the warfarin therapy must overlap for a minimum of 4 or 5 days and until a stable, therapeutic level of anticoagulation is achieved, ie, an international normalized ratio (INR) of 2 to 3 for 2 consecutive days.20

The duration of anticoagulant therapy depends on comorbidities and the patient’s underlying predisposition for VTE. In patients with limited disease, the guidelines recommend continuing anticoagulation for a minimum of 3 to 6 months for deep venous thrombosis and pulmonary embolism.20–21 Patients with active malignancy, ongoing treatment for the cancer, or continued risk factors may need indefinite treatment. In some circumstances, such as catheter-associated deep venous thrombosis, anticoagulation should continue for as long as the catheter is in place and for 1 to 3 months after its removal.21

WARFARIN CAN BE DIFFICULT TO USE

In 1954, the US Food and Drug Administration (FDA) approved the vitamin K antagonist warfarin for medical use in humans. Experience has shown it to be effective in preventing and treating VTE. However, it can be somewhat difficult to use, for several reasons:

  • A narrow therapeutic window
  • Genetic polymorphisms and variability in dose response
  • Drug interactions and dietary considerations
  • The need for laboratory monitoring and dose adjustment
  • Patient noncompliance or miscommunication between the patient and physician.22

In cancer patients, the response to warfarin may be unpredictable because of poor nutrition, interactions with chemotherapy and antibiotics, and comorbid conditions.22 Furthermore, its onset of action can be delayed and its clearance may be prolonged, further increasing the risk of complications, especially in patients prone to developing chemotherapy-related anemia or thrombocytopenia.22 Bleeding risk is the highest in the first 3 months of therapy. In addition, the risk of bleeding is higher in older patients, women, and patients with a history of gastrointestinal bleeding, stroke, recent myocardial infarction, diabetes, renal insufficiency, malignancy, or anemia.23,24

 

 

ADVANTAGES AND DISADVANTAGES OF LMWH

The advantages of the LMWHs over unfractionated heparin include a lower risk of heparin-induced thrombocytopenia, greater bioavailability when given subcutaneously (which also permits once-daily or twice-daily dosing), and no need for laboratory monitoring in most patients. LMWHs have a short half-life, so omitting one or two doses will adequately interrupt therapy. Also, LMWHs have been shown to be as safe and effective as unfractionated heparin in treating VTE. They can be given safely at home, thus enhancing quality of life.25–31

On the other hand, these drugs cost more than unfractionated heparin or warfarin, their dosage must be adjusted in patients with renal insufficiency, their anticoagulant effect can be reversed only to a limited extent, and their dose must be adjusted according to weight in morbidly obese or in very thin patients.32,33

LMWHs are expensive, but may be worth it

As initial therapy, the LMWHs are cost-effective compared with unfractionated heparin in patients with VTE.34,35 However, they cost more with extended use. A cost-effectiveness analysis comparing 6 months of LMWH therapy to standard warfarin concluded that LMWH therapy was more costly.35 However, the impact of fewer hospitalizations, probably fewer bleeding complications, and better quality of life are difficult to analyze in this decision model and should also be considered when deciding about therapy for an individual patient.35

LMWHs are cleared by the kidney

All LMWHs are renally cleared, so patients with significant renal insufficiency (creatinine clearance < 30 mL/min) are at greater risk of bleeding complications. The rate below which clearance is impaired varies among the different LMWHs. Only enoxaparin has approved dosing regimens for use in patients with renal impairment.

If the patient has renal insufficiency, the ACCP guidelines suggest using unfractionated heparin, or if using LMWH, monitoring anti-factor Xa levels to avoid drug accumulation and increased bleeding risk.25 If bleeding occurs, LMWHs have limited reversibility with protamine sulfate, which is estimated to neutralize about 60% of the anti-factor Xa activity of LMWHs.25

Adjusting LMWHs for body weight

In the Registro Informatizado de la Enfermedad Tromboembólica (RIETE),33 patients weighing less than 50 kg had a higher risk of bleeding than patients weighing 50 to 100 kg, so in thinner patients the risk of bleeding from LMWH vs oral anticoagulation must be considered carefully and monitored prudently.

Although there is little evidence to suggest a higher bleeding risk in morbidly obese patients (> 150 kg), they may be at risk of subtherapeutic treatment, and monitoring with anti-factor Xa assays is recommended.25,32,33

LMWH VS WARFARIN FOR VTE IN CANCER PATIENTS

LMWHs are the first-line treatment for VTE in cancer patients.20,21 Several randomized controlled trials compared the efficacy of LMWH vs warfarin in patients with cancer.

Meyer et al36 randomized patients to receive either warfarin for 3 months at an INR between 2 and 3, or enoxaparin 1.5 mg/kg subcutaneously daily. Seventy-one patients received warfarin and 67 received enoxaparin. Fifteen (21%, 95% confidence interval [CI] 12%–32%) of the 71 patients assigned to warfarin experienced one major outcome event, defined as major bleeding or recurrent VTE, compared with 7 (10.5%) of the 67 patients assigned to receive enoxaparin (95% CI 4%–20%, P = .09). Six patients in the warfarin group died of bleeding vs none of the patients in the enoxaparin group. Overall, the warfarin group had a higher rate of bleeding, although this did not reach statistical significance. Despite weekly INR measurements, only 41% of the measured values were within the therapeutic range during the 3 months of treatment.36

Lee et al37 randomized cancer patients with deep venous thrombosis, pulmonary embolism, or both to receive 6 months of dalteparin alone, dosed at 200 IU/kg daily for 1 month, then decreased to 75% to 80% of the original dose (150 IU/kg) daily for the duration of therapy, or dalteparin followed by warfarin. During the 6-month follow-up, 17.4% of patients in the warfarin group had a recurrent thromboembolic event vs 8.8% in the dalteparin group (P = .0017). No statistically significant difference was noted in rates of major bleeding, minor bleeding, or death.37

Hull et al38 reported statistically significantly fewer episodes of recurrent VTE at 12 months in cancer patients treated with once-daily tinzaparin vs warfarin. In the tinzaparin group the recurrence rate was 7%, vs 16% in the warfarin group (P = .044). No difference in rates of bleeding or death were found.

Deitcher et al39 compared enoxaparin with long-term warfarin in 102 patients. While this trial did not have the power to detect clinical differences in recurrent thromboembolic events or bleeding complications, at 180 days they noted 97% compliance with once-daily or twice-daily enoxaparin therapy.

Noble and Finlay,40 in another small study, found LMWH therapy to be qualitatively more acceptable for palliative-care cancer patients than oral therapy.

In general, long-term therapy with once-daily or twice-daily LMWH is well tolerated. Currently, dalteparin is the only LMWH approved by the FDA for extended monotherapy in cancer-related VTE.

 

 

DO LMWHS AFFECT CANCER?

In vitro and animal studies indicate that LMWH may have antimetastatic and antiangiogenic properties.41–44

Altinbas et al45 reported significantly better chemotherapy-induced tumor response rates and survival rates in patients with small cell lung cancer randomized to receive combination chemotherapy plus prophylactic dalteparin 5,000 IU daily compared with combination chemotherapy alone. However, as provocative as these results may be, we need to test the effects of LWMHs on different cancer types in a prospective clinical trial. For now, this area remains controversial.

It has been suggested that anticoagulants may improve survival in patients with nonmetastatic cancer. Supporting this observation, a post hoc analysis of the trial by Lee et al37 found a statistically significantly lower cancer-specific mortality rate in nonmetastatic cancer patients treated with dalteparin vs oral therapy with a coumarin derivative. In patients without metastatic disease, the death rate at 12 months was 36% in patients treated with oral therapy vs 20% in patients treated with dalteparin (P = .03).46

These findings are consistent with those of the Fragmin Advanced Malignancy Outcome Study (FAMOUS),47 the first randomized, placebo-controlled trial of dalteparin 5,000 IU daily in patients with advanced solid tumors and without evidence of underlying thrombosis. Overall, dalteparin prophylaxis did not increase survival. However, in a subgroup of patients with a better prognosis and who were alive 17 months after diagnosis, survival was statistically significantly longer in patients treated with dalteparin.

Another small trial showed similar survival benefits in cancer patients without VTE.48 The results may suggest a long-term favorable effect of LMWH on tumor cell biology, which could translate into a favorable outcome in some patients. It is important to note, however, that not all trials have shown this same clinical benefit.49

In general, the growing body of laboratory and clinical data indicates that LMWHs may suppress tumor growth and metastasis. However, definitive conclusions about these effects are not yet possible because of variations in study design, tumor type, and patient populations. Further investigations into the role of LMWHs in the treatment of VTE and in cancer progression are ongoing.

THE EVIDENCE IN PERSPECTIVE

Illness and the recurrence of VTE in patients with cancer depend on the location and extent of the underlying cancer. Rates of death are higher in VTE patients with cancer than in VTE patients without cancer. Patients with limited or localized disease may not die of the cancer itself but of complications of acute pulmonary embolism. Therefore, it is important to recognize the different options for and the potential side effects of treating VTE.

If patients are hospitalized for an acute thromboembolic event and unfractionated heparin is chosen as the initial anticoagulant, using a weight-based nomogram has been shown to achieve therapeutic levels within 24 hours and reduce the rates of recurrence of thromboembolic events.50

Warfarin treatment may pose a particular challenge for both cancer patients and physicians, since multiple drug interactions, anorexia, and comorbid conditions contribute to an unpredictable response.

The risk of bleeding is higher in cancer patients than in the general population, and the decision to start anticoagulants should be based on an individualized risk-benefit profile. Several trials have shown LMWH to be more effective and safer than warfarin in cancer patients.

These considerations, along with the other advantages of LMWHs (ease of use, less need for laboratory monitoring, and better patient tolerance), make LMWHs a good choice for initial therapy. Extended LMWH therapy is currently favored for initial management in patients with cancer. Trials are under way to further assess the antitumor properties and potential survival benefit in patients with selected solid tumors.

References
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  3. Baron JA, Gridley G, Weiderpass E, Nyrén O, Linet M. Venous thromboembolism and cancer. Lancet 1998; 351:10771080.
  4. Schulman S, Lindmarker P. Incidence of cancer after prophylaxis with warfarin against recurrent venous thromboembolism. Duration of Anticoagulation Trial. N Engl J Med 2000; 342:19531958.
  5. Sørensen HT, Mellemkjaer L, Steffensen FH, Olsen JH, Nielsen GL. The risk of a diagnosis of cancer after primary deep venous thrombosis or pulmonary embolism. N Engl J Med 1998; 338:11691173.
  6. Monreal M, Lafoz E, Casals A, et al. Occult cancer in patients with deep venous thrombosis. A systematic approach. Cancer 1991; 67:541545.
  7. Nordström M, Lindblad B, Anderson H, Bergqvist D, Kjellström T. Deep venous thrombosis and occult malignancy: an epidemiological study. BMJ 1994; 308:891894.
  8. Prandoni P, Lensing AW, Büller HR, et al. Deep-vein thrombosis and the incidence of subsequent symptomatic cancer. N Engl J Med 1992; 327:11281133.
  9. Cornuz J, Pearson SD, Creager MA, Cook EF, Goldman L. Importance of findings on the initial evaluation for cancer in patients with symptomatic idiopathic deep venous thrombosis. Ann Intern Med 1996; 125:785793.
  10. Fennerty T. Screening for cancer in venous thromboembolic disease. BMJ 2001; 323:704705.
  11. Bastounis EA, Karayiannakis AJ, Makri GG, Alexiou D, Papalambros EL. The incidence of occult cancer in patients with deep venous thrombosis: a prospective study. J Intern Med 1996; 239:153156.
  12. Piccioli A, Lensing AW, Prins MH, et al. Extensive screening for occult malignant disease in idiopathic venous thromboembolism: a prospective randomized clinical trial. J Thromb Haemost 2004; 2:884889.
  13. Di Nisio M, Otten HM, Piccioli A, et al. Decision analysis for cancer screening in idiopathic venous thromboembolism. J Thromb Haemost 2005; 3:23912396.
  14. Monreal M, Lensing AW, Prins MH, et al. Screening for occult cancer in patients with acute deep vein thrombosis or pulmonary embolism. J Thromb Haemost 2004; 2:876881.
  15. Sørensen HT, Mellemkjaer L, Olsen JH, Baron JA. Prognosis of cancers associated with venous thromboembolism. N Engl J Med 2000; 343:18461850.
  16. Prandoni P, Lensing AW, Piccioli A, et al. Recurrent venous thromboembolism and bleeding complications during anticoagulant treatment in patients with cancer and venous thrombosis. Blood 2002; 100:34843488.
  17. Hutten BA, Prins MH, Gent M, Ginsberg J, Tijssen JG, Büller HR. Incidence of recurrent thromboembolic and bleeding complications among patients with venous thromboembolism in relation to both malignancy and achieved international normalized ratio: a retrospective analysis. J Clin Oncol 2000; 18:30783083.
  18. Hansson PO, Sörbo J, Eriksson H. Recurrent venous thromboembolism after deep vein thrombosis: incidence and risk factors. Arch Intern Med 2000; 160:769774.
  19. Douketis JD, Crowther MA, Foster GA, Ginsberg JS. Does the location of thrombosis determine the risk of disease recurrence in patients with proximal deep vein thrombosis? Am J Med 2001; 110:515519.
  20. Kearon C, Kahn SR, Agnelli G, Goldhaber S, Raskob GE, Comerota AJ. Antithrombotic therapy for venous thromboembolic disease: American College of Chest Physicians Evidence-based Clinical Practice Guidelines, 8th Edition. Chest 2008; 133 suppl 6:454S545S.
  21. National Comprehensive Cancer Network. Venous Thromboembolic Disease Clinical Practice Guidelines in Oncology (V.1.2007). Available at www.nccn.org/professionals/physician_gls/PDF/vte.pdf. Accessed 01/02/2008.
  22. Ansell J, Hirsh J, Poller L, Bussey H, Jacobson A, Hylek E. The pharmacology and management of the vitamin K antagonists: the Seventh ACCP Conference on Antithrombotic and Thrombolytic Therapy. Chest 2004; 126 suppl 3:204S233S.
  23. Beyth RJ, Quinn LM, Landefeld CS. Prospective evaluation of an index for predicting the risk of major bleeding in outpatients treated with warfarin. Am J Med 1998; 105:9199.
  24. Kuijer PM, Hutten BA, Prins MH, Büller HR. Prediction of the risk of bleeding during anticoagulant treatment for venous thromboembolism. Arch Intern Med 1999; 159:457460.
  25. Hirsh J, Raschke R. Heparin and low-molecular-weight heparin: the Seventh ACCP Conference on Antithrombotic and Thrombolytic therapy. Chest 2004; 126 suppl 3:188S203S.
  26. Levine M, Gent M, Hirsh J, et al. A comparison of low-molecular-weight heparin administered primarily at home with unfractionated heparin administered in the hospital for proximal deep-vein thrombosis. N Engl J Med 1996; 334:677681.
  27. Koopman MM, Prandoni P, Piovella F, et al. Treatment of venous thrombosis with intravenous unfractionated heparin administered in the hospital as compared with subcutaneous low-molecular-weight heparin administered at home. The Tasman Study Group. N Engl J Med 1996; 334:682687.
  28. Hettiarachchi RJ, Prins MH, Lensing AW, Büller HR. Low molecular weight heparin versus unfractionated heparin in the initial treatment of venous thromboembolism. Curr Opin Pulm Med 1998; 4:220225.
  29. Gould MK, Dembitzer AD, Doyle RL, Hastie TJ, Garber AM. Low-molecular-weight heparins compared with unfractionated heparin for treatment of acute deep venous thrombosis. A meta-analysis of randomized, controlled trials. Ann Intern Med 1999; 130:800809.
  30. Dolovich LR, Ginsberg JS, Douketis JD, Holbrook AM, Cheah G. A meta-analysis comparing low-molecular-weight heparins with un-fractionated heparin in the treatment of venous thromboembolism: examining some unanswered questions regarding location of treatment, product type, and dosing frequency. Arch Intern Med 2000; 160:181188.
  31. van Dongen CJ, van den Belt AG, Prins MH, Lensing AW. Fixed dose subcutaneous low molecular weight heparins versus adjusted dose unfractionated heparin for venous thromboembolism. Cochrane Database Syst Rev 2004; 4:CD001100.
  32. Cook LM, Kahn SR, Goodwin J, Kovacs MJ. Frequency of renal impairment, advanced age, obesity, and cancer in venous thromboembolism patients in clinical practice. J Thromb Haemost 2007; 5:937941.
  33. Barba R, Marco J, Martin-Alvarez H, et al. The influence of extreme body weight on clinical outcome of patients with venous thromboembolism: findings from a prospective registry (RIETE). J Thromb Haemost 2005; 3:856862.
  34. Segal JB, Strieff MB, Hofmann LV, Thornton K, Bass EB. Management of venous thromboembolism: a systematic review for a practice guideline. Ann Intern Med 2007; 146:211222.
  35. Aujesky D, Smith KJ, Cornuz J, Roberts MS. Cost-effectiveness of low-molecular-weight heparin for secondary prophylaxis of cancer-related venous thromboembolism. Thromb Haemost 2005; 93:592599.
  36. Meyer G, Marjanovic Z, Valcke J, et al. Comparison of low-molecular-weight heparin and warfarin for the secondary prevention of venous thromboembolism in patients with cancer: a randomized controlled study. Arch Intern Med 2002; 162:17291735.
  37. Lee AY, Levine MN, Baker RI, et al. Low-molecular-weight heparin versus a coumarin for the prevention of recurrent venous thromboembolism in patients with cancer. N Engl J Med 2003; 349:146153.
  38. Hull RD, Pineo GF, Brant RF, et al. Long-term low-molecular-weight heparin versus usual care in proximal-vein thrombosis patients with cancer. Am J Med 2006; 119:10621072.
  39. Deitcher SR, Kessler CM, Merli G, Rigas JR, Lyons RM, Fareed J ON-CENOX investigators. Secondary prevention of venous thromboembolic events in patients with active cancer: enoxaparin alone versus initial enoxaparin followed by warfarin for a 180-day period. Clin Appl Thromb Hemost 2006; 12:389396.
  40. Noble SI, Finlay IG. Is long-term low-molecular-weight heparin acceptable to palliative care patients in the treatment of cancer related venous thromboembolism? A qualitative study. Palliat Med 2005; 19:197201.
  41. Amirkhosravi A, Mousa SA, Amaya M, Francis JL. Antimetastatic effect of tinzaparin, a low-molecular-weight heparin. J Thromb Haemost 2003; 1:19721976.
  42. Kragh M, Binderup L, Vig Hjarnaa PJ, Bramm E, Johansen KB, Frimundt Petersen C. Non-anti-coagulant heparin inhibits metastasis but not primary tumor growth. Oncol Rep 2005; 14:99104.
  43. Mousa SA, Mohamed S. Anti-angiogenic mechanisms and efficacy of the low molecular weight heparin, tinzaparin: anti-cancer efficacy. Oncol Rep 2004; 12:683688.
  44. Bobek V, Kovarik J. Antitumor and antimetastatic effect of warfarin and heparins. Biomed Pharmacother 2004; 58:213219.
  45. Altinbas M, Coskun HS, Er O, et al. A randomized clinical trial of combination chemotherapy with and without low-molecular-weight heparin in small cell lung cancer. J Thromb Haemost 2004; 2:12661271.
  46. Lee AY, Rickles FR, Julian JA, et al. Randomized comparison of low molecular weight heparin and coumarin derivatives on the survival of patients with cancer and venous thromboembolism. J Clin Oncol 2005; 23:21232129.
  47. Kakkar AK, Levine MN, Kadziola Z, et al. Low molecular weight heparin, therapy with dalteparin, and survival in advanced cancer: the Fragmin Advanced Malignancy Outcome Study (FAMOUS). J Clin Oncol 2004; 22:19441948.
  48. Klerk CP, Smorenburg SM, Otten HM, et al. The effect of low molecular weight heparin on survival in patients with advanced malignancy. J Clin Oncol 2005; 23:21302135.
  49. Sideras K, Schaefer PL, Okuno SH, et al. Low-molecular-weight heparin in patients with advanced cancer: a phase 3 clinical trial. Mayo Clin Proc 2006; 81:758767.
  50. Bernardi E, Piccioli A, Oliboni G, Zuin R, Girolami A, Prandoni P. Nomograms for the administration of unfractionated heparin in the initial treatment of acute thromboembolism—an overview. Thromb Haemost 2000; 84:2226.
References
  1. Aron E. The 100th anniversary of the death of A. Trousseau. Presse Med 1967; 75:14291430.
  2. Hettiarachchi RJ, Lok J, Prins MH, Büller HR, Prandoni P. Undiagnosed malignancy in patients with deep vein thrombosis: incidence, risk indicators, and diagnosis. Cancer 1998; 83:180185.
  3. Baron JA, Gridley G, Weiderpass E, Nyrén O, Linet M. Venous thromboembolism and cancer. Lancet 1998; 351:10771080.
  4. Schulman S, Lindmarker P. Incidence of cancer after prophylaxis with warfarin against recurrent venous thromboembolism. Duration of Anticoagulation Trial. N Engl J Med 2000; 342:19531958.
  5. Sørensen HT, Mellemkjaer L, Steffensen FH, Olsen JH, Nielsen GL. The risk of a diagnosis of cancer after primary deep venous thrombosis or pulmonary embolism. N Engl J Med 1998; 338:11691173.
  6. Monreal M, Lafoz E, Casals A, et al. Occult cancer in patients with deep venous thrombosis. A systematic approach. Cancer 1991; 67:541545.
  7. Nordström M, Lindblad B, Anderson H, Bergqvist D, Kjellström T. Deep venous thrombosis and occult malignancy: an epidemiological study. BMJ 1994; 308:891894.
  8. Prandoni P, Lensing AW, Büller HR, et al. Deep-vein thrombosis and the incidence of subsequent symptomatic cancer. N Engl J Med 1992; 327:11281133.
  9. Cornuz J, Pearson SD, Creager MA, Cook EF, Goldman L. Importance of findings on the initial evaluation for cancer in patients with symptomatic idiopathic deep venous thrombosis. Ann Intern Med 1996; 125:785793.
  10. Fennerty T. Screening for cancer in venous thromboembolic disease. BMJ 2001; 323:704705.
  11. Bastounis EA, Karayiannakis AJ, Makri GG, Alexiou D, Papalambros EL. The incidence of occult cancer in patients with deep venous thrombosis: a prospective study. J Intern Med 1996; 239:153156.
  12. Piccioli A, Lensing AW, Prins MH, et al. Extensive screening for occult malignant disease in idiopathic venous thromboembolism: a prospective randomized clinical trial. J Thromb Haemost 2004; 2:884889.
  13. Di Nisio M, Otten HM, Piccioli A, et al. Decision analysis for cancer screening in idiopathic venous thromboembolism. J Thromb Haemost 2005; 3:23912396.
  14. Monreal M, Lensing AW, Prins MH, et al. Screening for occult cancer in patients with acute deep vein thrombosis or pulmonary embolism. J Thromb Haemost 2004; 2:876881.
  15. Sørensen HT, Mellemkjaer L, Olsen JH, Baron JA. Prognosis of cancers associated with venous thromboembolism. N Engl J Med 2000; 343:18461850.
  16. Prandoni P, Lensing AW, Piccioli A, et al. Recurrent venous thromboembolism and bleeding complications during anticoagulant treatment in patients with cancer and venous thrombosis. Blood 2002; 100:34843488.
  17. Hutten BA, Prins MH, Gent M, Ginsberg J, Tijssen JG, Büller HR. Incidence of recurrent thromboembolic and bleeding complications among patients with venous thromboembolism in relation to both malignancy and achieved international normalized ratio: a retrospective analysis. J Clin Oncol 2000; 18:30783083.
  18. Hansson PO, Sörbo J, Eriksson H. Recurrent venous thromboembolism after deep vein thrombosis: incidence and risk factors. Arch Intern Med 2000; 160:769774.
  19. Douketis JD, Crowther MA, Foster GA, Ginsberg JS. Does the location of thrombosis determine the risk of disease recurrence in patients with proximal deep vein thrombosis? Am J Med 2001; 110:515519.
  20. Kearon C, Kahn SR, Agnelli G, Goldhaber S, Raskob GE, Comerota AJ. Antithrombotic therapy for venous thromboembolic disease: American College of Chest Physicians Evidence-based Clinical Practice Guidelines, 8th Edition. Chest 2008; 133 suppl 6:454S545S.
  21. National Comprehensive Cancer Network. Venous Thromboembolic Disease Clinical Practice Guidelines in Oncology (V.1.2007). Available at www.nccn.org/professionals/physician_gls/PDF/vte.pdf. Accessed 01/02/2008.
  22. Ansell J, Hirsh J, Poller L, Bussey H, Jacobson A, Hylek E. The pharmacology and management of the vitamin K antagonists: the Seventh ACCP Conference on Antithrombotic and Thrombolytic Therapy. Chest 2004; 126 suppl 3:204S233S.
  23. Beyth RJ, Quinn LM, Landefeld CS. Prospective evaluation of an index for predicting the risk of major bleeding in outpatients treated with warfarin. Am J Med 1998; 105:9199.
  24. Kuijer PM, Hutten BA, Prins MH, Büller HR. Prediction of the risk of bleeding during anticoagulant treatment for venous thromboembolism. Arch Intern Med 1999; 159:457460.
  25. Hirsh J, Raschke R. Heparin and low-molecular-weight heparin: the Seventh ACCP Conference on Antithrombotic and Thrombolytic therapy. Chest 2004; 126 suppl 3:188S203S.
  26. Levine M, Gent M, Hirsh J, et al. A comparison of low-molecular-weight heparin administered primarily at home with unfractionated heparin administered in the hospital for proximal deep-vein thrombosis. N Engl J Med 1996; 334:677681.
  27. Koopman MM, Prandoni P, Piovella F, et al. Treatment of venous thrombosis with intravenous unfractionated heparin administered in the hospital as compared with subcutaneous low-molecular-weight heparin administered at home. The Tasman Study Group. N Engl J Med 1996; 334:682687.
  28. Hettiarachchi RJ, Prins MH, Lensing AW, Büller HR. Low molecular weight heparin versus unfractionated heparin in the initial treatment of venous thromboembolism. Curr Opin Pulm Med 1998; 4:220225.
  29. Gould MK, Dembitzer AD, Doyle RL, Hastie TJ, Garber AM. Low-molecular-weight heparins compared with unfractionated heparin for treatment of acute deep venous thrombosis. A meta-analysis of randomized, controlled trials. Ann Intern Med 1999; 130:800809.
  30. Dolovich LR, Ginsberg JS, Douketis JD, Holbrook AM, Cheah G. A meta-analysis comparing low-molecular-weight heparins with un-fractionated heparin in the treatment of venous thromboembolism: examining some unanswered questions regarding location of treatment, product type, and dosing frequency. Arch Intern Med 2000; 160:181188.
  31. van Dongen CJ, van den Belt AG, Prins MH, Lensing AW. Fixed dose subcutaneous low molecular weight heparins versus adjusted dose unfractionated heparin for venous thromboembolism. Cochrane Database Syst Rev 2004; 4:CD001100.
  32. Cook LM, Kahn SR, Goodwin J, Kovacs MJ. Frequency of renal impairment, advanced age, obesity, and cancer in venous thromboembolism patients in clinical practice. J Thromb Haemost 2007; 5:937941.
  33. Barba R, Marco J, Martin-Alvarez H, et al. The influence of extreme body weight on clinical outcome of patients with venous thromboembolism: findings from a prospective registry (RIETE). J Thromb Haemost 2005; 3:856862.
  34. Segal JB, Strieff MB, Hofmann LV, Thornton K, Bass EB. Management of venous thromboembolism: a systematic review for a practice guideline. Ann Intern Med 2007; 146:211222.
  35. Aujesky D, Smith KJ, Cornuz J, Roberts MS. Cost-effectiveness of low-molecular-weight heparin for secondary prophylaxis of cancer-related venous thromboembolism. Thromb Haemost 2005; 93:592599.
  36. Meyer G, Marjanovic Z, Valcke J, et al. Comparison of low-molecular-weight heparin and warfarin for the secondary prevention of venous thromboembolism in patients with cancer: a randomized controlled study. Arch Intern Med 2002; 162:17291735.
  37. Lee AY, Levine MN, Baker RI, et al. Low-molecular-weight heparin versus a coumarin for the prevention of recurrent venous thromboembolism in patients with cancer. N Engl J Med 2003; 349:146153.
  38. Hull RD, Pineo GF, Brant RF, et al. Long-term low-molecular-weight heparin versus usual care in proximal-vein thrombosis patients with cancer. Am J Med 2006; 119:10621072.
  39. Deitcher SR, Kessler CM, Merli G, Rigas JR, Lyons RM, Fareed J ON-CENOX investigators. Secondary prevention of venous thromboembolic events in patients with active cancer: enoxaparin alone versus initial enoxaparin followed by warfarin for a 180-day period. Clin Appl Thromb Hemost 2006; 12:389396.
  40. Noble SI, Finlay IG. Is long-term low-molecular-weight heparin acceptable to palliative care patients in the treatment of cancer related venous thromboembolism? A qualitative study. Palliat Med 2005; 19:197201.
  41. Amirkhosravi A, Mousa SA, Amaya M, Francis JL. Antimetastatic effect of tinzaparin, a low-molecular-weight heparin. J Thromb Haemost 2003; 1:19721976.
  42. Kragh M, Binderup L, Vig Hjarnaa PJ, Bramm E, Johansen KB, Frimundt Petersen C. Non-anti-coagulant heparin inhibits metastasis but not primary tumor growth. Oncol Rep 2005; 14:99104.
  43. Mousa SA, Mohamed S. Anti-angiogenic mechanisms and efficacy of the low molecular weight heparin, tinzaparin: anti-cancer efficacy. Oncol Rep 2004; 12:683688.
  44. Bobek V, Kovarik J. Antitumor and antimetastatic effect of warfarin and heparins. Biomed Pharmacother 2004; 58:213219.
  45. Altinbas M, Coskun HS, Er O, et al. A randomized clinical trial of combination chemotherapy with and without low-molecular-weight heparin in small cell lung cancer. J Thromb Haemost 2004; 2:12661271.
  46. Lee AY, Rickles FR, Julian JA, et al. Randomized comparison of low molecular weight heparin and coumarin derivatives on the survival of patients with cancer and venous thromboembolism. J Clin Oncol 2005; 23:21232129.
  47. Kakkar AK, Levine MN, Kadziola Z, et al. Low molecular weight heparin, therapy with dalteparin, and survival in advanced cancer: the Fragmin Advanced Malignancy Outcome Study (FAMOUS). J Clin Oncol 2004; 22:19441948.
  48. Klerk CP, Smorenburg SM, Otten HM, et al. The effect of low molecular weight heparin on survival in patients with advanced malignancy. J Clin Oncol 2005; 23:21302135.
  49. Sideras K, Schaefer PL, Okuno SH, et al. Low-molecular-weight heparin in patients with advanced cancer: a phase 3 clinical trial. Mayo Clin Proc 2006; 81:758767.
  50. Bernardi E, Piccioli A, Oliboni G, Zuin R, Girolami A, Prandoni P. Nomograms for the administration of unfractionated heparin in the initial treatment of acute thromboembolism—an overview. Thromb Haemost 2000; 84:2226.
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Cleveland Clinic Journal of Medicine - 76(2)
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Cleveland Clinic Journal of Medicine - 76(2)
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Cancer and clots: All cases of venous thromboembolism are not treated the same
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KEY POINTS

  • We recommend judiciously screening for cancer with age- and sex-specific tests in patients with idiopathic VTE.
  • Patients with VTE and cancer have a higher risk of both VTE recurrence and bleeding complications of anticoagulant therapy than do VTE patients without cancer.
  • Either unfractionated heparin or a low-molecular-weight heparin (LMWH) should be started as soon as VTE is confirmed or even strongly suspected, while still awaiting confirmation.
  • The current (grade 1A) recommendations for treating VTE in cancer patients are to use LMWH monotherapy for at least 3 to 6 months. Anticoagulation is necessary indefinitely when there is ongoing cancer treatment or persistent risk of VTE.
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Anticoagulants and pregnancy: When are they safe?

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Anticoagulants and pregnancy: When are they safe?

Anticoagulation is essential in a wide variety of conditions in women of child-bearing age. Some, such as venous thromboembolism, occur more often during pregnancy. Others, such as recurrent fetal loss in the setting of antiphospholipid antibodies, are specific to pregnancy.

While anticoagulants are useful in many circumstances, their use during pregnancy increases the risk of hemorrhage and other adverse effects on the mother and the fetus. Treatment with anticoagulants during pregnancy must therefore be carefully considered, with judicious selection of the agent, and with reflection on the physiologic changes of pregnancy to ensure appropriate dosing. In this article, we review these issues.

WHY IS THROMBOTIC RISK HIGHER DURING PREGNANCY?

Venous thromboembolism is among the leading causes of maternal death in developed countries.1–3 Modern care has dramatically reduced the risk of maternal death from hemorrhage, infection, and hypertension, but rates of morbidity and death from thrombosis have remained stable or increased in recent years.4

Pregnancy is a period of increased risk of thrombotic complications (Table 1), owing to hypercoagulability, venous stasis, and vascular damage—the three elements of Virchow’s triad.5 Several changes to the maternal coagulation system increase clotting risk:

  • Much higher levels of fibrinogen and factors VII, VIII, IX, and X
  • Lower levels of protein S and increased resistance to activated protein C
  • Impaired fibrinolysis, due to inhibitors derived from the placenta.

Acquired antithrombin deficiency may also occur in high-proteinuric states such as nephrotic syndrome or preeclampsia, further increasing thrombotic risk. Pooling of venous blood, caused by progesterone-mediated venous dilation and compounded by compression of the inferior vena cava by the uterus in later pregnancy, also increases thrombotic risk. And endothelial disruption of the pelvic vessels may occur during delivery, particularly during cesarean section.

Additional factors that increase thrombotic risk include immobilization, such as bed rest for pregnancy complications; surgery, including cesarean section; ovarian hyperstimulation during gonadotropin use for in vitro fertilization; trauma; malignancy; and hereditary or acquired hypercoagulable states.6 These hypercoagulable states include deficiencies of antithrombin or the intrinsic anticoagulant proteins C or S; resistance to activated protein C, usually due to the factor V Leiden mutation; the PT20210A mutation of the prothrombin gene; hyperhomocystinemia due to mutation of the methyltetrahydrofolate reductase (MTHFR) gene; and the sustained presence of antiphospholipid antibodies, including lupus anticoagulant antibodies, sometimes also with moderately high titers of anticardiolipin or beta-2-glycoprotein I antibodies.

Other conditions that increase thrombotic risk include hyperemesis gravidarum, obesity, inflammatory bowel disease, infection, smoking, and indwelling intravenous catheters.6 Given the multitude of risk factors, pregnant women have a risk of thrombotic complications three to five times higher than nonpregnant women.7

HEPARIN USE DURING PREGNANCY

Low-molecular-weight heparins (LMWHs)8 and unfractionated heparin bind to anti-thrombin and thus change the shape of the antithrombin molecule, dramatically increasing its interaction with the clotting factors Xa and prothrombin (factor II). The enhanced clearance of these procoagulant proteins leads to the anticoagulant effect. Unfractionated heparin has roughly equivalent interaction with factors Xa and II and prolongs the activated partial thromboplastin time (aPTT), which is therefore used to monitor the intensity of anticoagulation.

LMWHs, on the other hand, interact relatively little with factor II and do not predictably prolong the aPTT. Monitoring their effect is therefore more difficult and requires direct measurement of anti-factor-Xa activity. This test is widely available, but it is time-consuming (it takes several hours and results may not be available within 24 hours if the test is requested “after hours”), and therefore it is of limited use in the acute clinical setting. While weight-based dosing of LMWHs is reliable and safe in nonpregnant patients, it has not yet been validated for pregnant women.

Unfractionated heparin has been used for decades for many indications during pregnancy. It is a large molecule, so it does not cross the placenta and thus, in contrast to the coumarin derivatives, does not cause teratogenesis or toxic fetal effects. Its main limitations in pregnancy are its inconvenient dosing (at least twice daily when given subcutaneously) and its potential maternal adverse effects (mainly osteoporosis and heparin-induced thrombocytopenia).

Over the last 10 years LMWHs have become the preferred anticoagulants for treating and preventing thromboembolism in all patients. They are equivalent or superior to unfractionated heparin in efficacy and safety in the initial treatment of acute deep venous thrombosis9,10 and pulmonary embolism11,12 outside of pregnancy. While comparative data are much less robust in pregnant patients, several series have confirmed the safety and efficacy of LMWHs in pregnancy.13–15 LMWHs do not cross the placenta15–17 and thus have a fetal safety profile equivalent to that of unfractionated heparin.

 

 

Pregnancy alters metabolism of LMWHs

The physiologic changes of pregnancy alter the metabolism of LMWH, resulting in lower peak levels and a higher rate of clearance,18,19 and so a pregnant woman may need higher doses or more frequent dosing.

Recent evidence suggests that thromboprophylaxis can be done with lower, fixed, once-daily doses of LMWH throughout pregnancy,20 although some clinicians still prefer twice-daily dosing (particularly during the latter half of pregnancy).

For therapeutic anticoagulation, however, the dose of LMWH required to achieve the desired level of anti-factor-Xa activity appears to change significantly over the course of pregnancy in many women.18 Therapeutic dosing of LMWH may also require twice-daily dosing, depending on the agent used (Table 2).

Pending more research on weight-based dosing of LMWH in pregnancy, anti-factor- Xa activity levels should be measured after treatment is started and every 1 to 3 months thereafter during pregnancy.21 Doses should be adjusted to keep the peak anti-Xa level (ie, 4 hours after the dose) at 0.5 to 1.2 U/mL.22

Heparin-induced thrombocytopenia

Type-2 heparin-induced thrombocytopenia is an uncommon but serious adverse effect of unfractionated heparin therapy (and, less commonly of LMWH), caused by heparin-dependent immunoglobulin G (IgG) antibodies that activate platelets via their Fc receptors, potentially precipitating life-threatening arterial or venous thrombosis.

In a trial in nonpregnant orthopedic patients,23 clinical heparin-induced thrombocytopenia occurred in 2.7% of patients receiving unfractionated heparin vs 0% of those receiving LMWH; heparin-dependent IgG was present in 7.8% vs 2.2%, respectively.

Fortunately, heparin-induced thrombocytopenia seems to be very rare in pregnancy: two recent prospective series evaluating prolonged LMWH use in pregnancy13,15 revealed no episodes of this disease. Nonetheless, it is reasonable to measure the platelet count once or twice weekly during the first few weeks of LMWH use and less often thereafter, unless symptoms of heparin-induced thrombocytopenia develop. In pregnant women with heparin-induced thrombocytopenia or heparin-related skin reactions, other anticoagulants must be considered24 (see discussion later).

Heparin-induced osteoporosis

Heparin-induced osteoporosis, a potential effect of prolonged heparin therapy, is of concern, given the prolonged duration and high doses of unfractionated heparin often needed to treat venous thromboembolism during pregnancy. Several studies found significant loss of bone mineral density in the proximal femur25 and lumbar spine26 during extended use of unfractionated heparin in pregnancy.

Fortunately, LMWH appears to be much safer with respect to bone loss. Three recent studies27–30 evaluated the use of LMWH for extended periods during pregnancy, and none found any greater loss of bone mineral density than that seen in normal pregnant controls. Giving supplemental calcium (1,000–1,500 mg/day) and vitamin D (400–1,000 IU/day) concomitantly with unfractionated heparin or LMWH in pregnancy is advisable to further reduce the risk.

Interrupt heparin to permit regional anesthesia

Heparin therapy should be temporarily stopped during the immediate peripartum interval to minimize the risk of hemorrhage and to permit regional anesthesia. Because of the theoretical risk of paraspinal hemorrhage in women receiving heparin who undergo epidural or spinal anesthesia, many anesthetists will not perform neuraxial regional anesthesia in women who have recently received heparin.

Since unfractionated heparin has a relatively short duration of action, the American Society of Regional Anesthesia states that subcutaneous unfractionated heparin prophylaxis is not a contraindication to neuraxial regional anesthesia.31 However, LMWHs should be stopped for at least 12 to 24 hours before regional anesthesia can be considered safe. This issue is discussed in more detail in the section on peripartum and postpartum management of anticoagulation, below.

In summary, LMWH during pregnancy offers a number of advantages over unfractionated heparin: equivalent efficacy, once- or twice-daily dosing, lower risk of heparin-induced thrombocytopenia and osteoporosis, and less-intensive monitoring. Unfractionated heparin can be offered to women who cannot afford LMWH (which costs four to five times more), and it may be used peripartum to reduce hemorrhagic risk and to permit regional anesthesia.

COUMARINS

Coumarins are the mainstay of anticoagulant therapy in most nonpregnant women beyond the immediate thrombotic period.

Warfarin (Coumadin) is the most widely used coumarin because it has a predictable onset and duration of action and excellent bioavailability.32 Others, such as acenocoumarol (Sintrom) and phenprocoumon (Marcoumar), are used more outside the United States but can be ordered or brought into the United States.

Coumarins interfere with vitamin K metabolism, inhibiting the generation of vitamin-K-dependent procoagulant proteins (factors II, VII, IX, and X) and thereby preventing clotting. They also inhibit the formation of the vitamin-K-dependent intrinsic anticoagulant proteins C and S.

Major bleeding is the most significant side effect of coumarin therapy, occurring at a rate of 4% to 6% over 3 months when the prothrombin time is maintained at an international normalized ratio (INR) of 2 to 3,33 and more often if the INR is higher.

Other issues with warfarin are the effect of variations in dietary vitamin K intake on anticoagulation and potential drug interactions that may alter the anticoagulant effect. Thus, the INR needs to be monitored closely.

 

 

Risks to the fetus and the mother

Unlike the heparins, coumarins freely cross the placenta and thus pose a risk of teratogenicity. A cluster of fetal malformations including “warfarin embryopathy” (nasal bone hypoplasia and chondrodysplasia punctata) can occur when the drug is used between 6 and 12 weeks of gestation. Warfarin embryopathy may be avoided by stopping warfarin prior to 6 weeks from the onset of the last menstrual period (ie, 6-week “menstrual age” or 4-week gestational age34).

Later in pregnancy, warfarin is associated with potential fetal bleeding complications leading to central nervous system abnormalities, increased rates of intrauterine fetal death, and pregnancy loss. In pregnant women with mechanical cardiac valve prostheses who received oral anticoagulants throughout pregnancy, the incidence of congenital anomalies was 6.4% to 10.2%.35 Fetal demise (spontaneous abortion, stillbirth, neonatal death) was also very common (29.7% to 33.6% of pregnancies) in coumarin-treated women.

Severe maternal hemorrhage may also occur in pregnant women on oral anticoagulants, particularly those who remain fully anticoagulated around the time of labor and delivery.

General caveats to warfarin in pregnancy

Because of the many maternal and fetal concerns, oral anticoagulant use in pregnancy is largely restricted to women with older-generation prosthetic heart valves in whom the very high maternal thrombotic risk may outweigh the risk of maternal and fetal side effects.

While there are limited data on warfarin use in pregnant women with antiphospholipid syndrome,36 warfarin use in such patients should be considered only for those at highest risk and with careful informed consent. These issues are discussed further below in the section on mechanical heart valve prostheses.

ANTIPLATELET DRUGS

Aspirin is an antiplatelet agent rather than an anticoagulant. Although considered inadequate for preventing venous thrombosis in high-risk groups when used alone, aspirin can moderately reduce the risk of deep venous thrombosis and pulmonary embolism in nonpregnant patients.37 It also has a well-accepted role in preventing arterial thrombotic events, ie, coronary artery disease and stroke.38

Low-dose aspirin (≤ 100 mg/day) has been extensively evaluated during pregnancy39–41 and has been shown to be safe and effective in reducing the risk of preeclampsia in high-risk women39 and in treating women with antiphospholipid antibodies and recurrent pregnancy loss42 (in conjunction with prophylactic doses of heparin). Although higher doses of aspirin and other nonsteroidal anti-inflammatory drugs can be toxic to the fetus, low doses have been shown to be safe throughout pregnancy.43

Dipyridamole (Persantine) has been studied extensively in pregnancy, and while it appears to be safe, it has not found a well-defined therapeutic role.

Other antiplatelet drugs have been only rarely used, and data on their safety and efficacy during pregnancy are limited to case reports, for example, on ticlopidine44 (Ticlid) and clopidogrel45,46 (Plavix) given during pregnancy in women with cardiac disease. These drugs do not appear to be major teratogens or to cause specific fetal harm. Their use may be reasonable in some high-risk situations, such as recurrent thrombotic stroke despite aspirin therapy. They may be used alone or with other anticoagulants in women with a coronary or other vascular stent if fetal safety is uncertain or if there is an increased risk of maternal bleeding.

NEWER ANTICOAGULANTS

Several newer anticoagulants can be used in pregnancy (Table 3).47–50

Danaparoid

The heparinoid danaparoid (Orgaran) is an LMWH, a combination of heparan, dermatan, and chondroitin sulfate. Since it is derived from heparin, in theory it can cross-react with antiheparin antibodies, but this is generally not a problem. Danaparoid inhibits factor Xa, and monitoring is via measurement of anti-factor-Xa activity levels. It has been shown to be safe and effective in nonpregnant patients with heparin-induced thrombocytopenia.51

Although no controlled study has been published on danaparoid in pregnancy, at least 51 pregnancies in 49 patients treated with danaparoid have been reported.52 Thirty-two of the patients received danaparoid because of heparin-induced thrombocytopenia and 19 because of heparin-induced skin intolerance. These reports suggest that danaparoid does not cross the placenta53 and that it may be effective and safe during pregnancy.54 For this reason, it is probably the preferred anticoagulant in pregnant patients with heparin-induced thrombocytopenia or other serious reactions to heparin.

Unfortunately, danaparoid has two major disadvantages. First, it has a prolonged half-life and no effective reversing agent, which makes its use problematic close to the time of delivery. Second, and perhaps more relevant to this discussion, it is not readily available in the United States; it was removed from the market by its manufacturer in April 2002 for business reasons rather than because of concerns over toxicity. It is still available in Canada and Europe, and it can be obtained in special circumstances in the United States via the US Food and Drug Administration (FDA); this may be worthwhile in pregnant patients who require a nonurgent alternative to heparin.

Direct thrombin inhibitors

Lepirudin (Refludan), bivalirudin (Angiomax), and argatroban are direct thrombin inhibitors and exert their anticoagulant effect independently of antithrombin. They are given by continuous intravenous infusion, and they have a very short half-life.

Lepirudin and argatroban are typically monitored via the aPTT. Bivalirudin can be monitored with the activated clotting time, partial thromboplastin time, or INR, depending on the circumstances. None of these agents generates or cross-reacts with antibodies generated in heparin-induced thrombocytopenia. None has an antidote, but the short half-life usually obviates the need for one.

Unfortunately, pregnancy data are very sparse for all three of these new agents. Argatroban has a low molecular weight and likely crosses the placenta. Also, because these agents are given intravenously, they are not practical for long-term use in pregnancy.

Fondaparinux

Fondaparinux (Arixtra), a direct factor Xa inhibitor, binds to antithrombin, causing an irreversible conformational change that increases antithrombin’s ability to inactivate factor Xa (as do the heparins). It has no effect on factor IIa (thrombin) and does not predictably affect the aPTT. Its half-life is 17 hours, and no agent is known to reverse its anticoagulant effect, although some experts would recommend a trial of high-dose recombinant factor VIIa (Novo-Seven) in uncontrolled hemorrhage.

While not FDA-approved for treating heparin-induced thrombocytopenia, it has been used for this in some patients.55–58 Animal studies and in vitro human placental perfusion studies suggest that fondaparinux does not cross the placenta in significant amounts.49 Since danaparoid is not available in the United States, fondaparinux would likely be the first choice among the newer anticoagulants when treating heparin-induced thrombocytopenia in pregnancy.

 

 

INDICATIONS FOR ANTICOAGULANTS DURING PREGNANCY

Acute deep venous thrombosis and pulmonary embolism

If acute deep venous thrombosis or pulmonary embolism is confirmed or strongly suspected in a pregnant woman, therapeutic anticoagulation should be started promptly (Table 4). In most cases, the woman should probably be hospitalized, given the complex maternal and fetal concerns that include adequate maternal dosing and the potential for fetal harm in the setting of significant hypoxia.

Anticoagulant therapy should begin as full doses of either LMWH or intravenous unfractionated heparin. We prefer starting with LMWH, as it can be started rapidly with less need for nursing care (eg, no need to start and maintain an intravenous line and monitor the aPTT) and has excellent safety. If LMWH is selected, initial dosing should be based on the current weight (Table 2). Subsequent monitoring of the peak anti-factor-Xa activity levels (ie, 4 hours after the dose) is recommended, with the first level drawn in the first few days of treatment, and repeat levels every 1 to 3 months for the rest of treatment. As mentioned earlier, weight-based dosing has not been systematically evaluated in pregnancy.

If unfractionated heparin is the initial agent, it should be given as a bolus followed by a continuous infusion, ideally utilizing a weight-based nomogram to estimate required doses, with adjustment of the infusion rate to maintain the aPTT at 1.5 to 2.5 times the baseline value (obtained during pregnancy). After several days, the heparin may be switched to LMWH in therapeutic doses (Table 2).

Alternatively, in women approaching term or who cannot afford LMWH, anticoagulation may be continued as adjusted-dose subcutaneous unfractionated heparin, ie, two or three large daily doses of subcutaneous heparin to provide therapeutic levels of anticoagulation. The starting dose can be calculated as the total units of heparin required to maintain full anticoagulation intravenously over 24 hours, given as two or three divided doses (Table 2). The aPTT at the mid-dosing interval (eg, 6 hours after the subcutaneous dose during every-12-hour dosing) should be monitored and the dose adjusted to maintain the aPTT at 1.5 to 2.5 times the baseline value.

A therapeutic level of anticoagulation should be maintained for at least 3 months after an acute thrombotic event during pregnancy, though many physicians prefer to continue full anticoagulation for a total of 6 months. Beyond this interval, if the woman is still pregnant, the anticoagulation may be reduced in intensity, perhaps even to a prophylactic level for the duration of the pregnancy (see discussion below on prior venous thromboembolic events) (Table 2). Peripartum and postpartum anticoagulation are discussed further below.

PRIOR VENOUS THROMBOEMBOLIC EVENT

While all pregnant women are at higher risk of venous thrombosis, the overall incidence of thromboembolism is only about one event per 1,000 pregnancies. Routine thromboprophylaxis in all pregnant women is therefore not justified. However, women who have previously had a venous thromboembolic event are at a substantially higher risk of recurrent thrombosis and should be considered for thromboprophylaxis in all subsequent high-risk situations, including pregnancy.

For women on indefinite therapeutic anticoagulation (ie, because of recurrent thrombosis), full therapeutic anticoagulation with LMWH or adjusted-dose unfractionated heparin should be maintained throughout pregnancy, as described above.

Which other women should receive prophylactic anticoagulation is a topic of ongoing debate and controversy.

How great is the risk of recurrent thromboembolism?

A small observational study59 examined the risk of recurrent venous thromboembolism during subsequent pregnancies in women with a prior thrombotic event. Anticoagulation was withheld during the antepartum period and restarted briefly after delivery. Among the 125 women enrolled, recurrent venous thromboembolism occurred in 4.8%, with half of the events occurring during the antepartum period. Among those with underlying thrombophilia, the rate of recurrent venous thromboembolism was 13% (95% confidence interval [CI] 1.7%–40.5%) to 20% (95% CI 2.5%–56.5%), and those with a prior idiopathic clot without thrombophilia had an event rate of 7.7% (95% CI 0.01%–25.1%). The subgroup with a prior reversible risk factor (at the time of their initial venous thromboembolic event) and without detectable thrombophilia had no recurrent events.

This study suggests that women with prior venous thromboembolism and thrombophilia or a prior idiopathic thrombotic event are at a substantial risk of recurrent thrombotic events during pregnancy. And other data confirm the high risk of recurrent venous thromboembolism in thrombophilic pregnant women.60 These women should all be offered active antepartum and postpartum thromboprophylaxis with LMWH or unfractionated heparin (Tables 2 and 4). Women without thrombophilia but with a history of venous thromboembolism related to pregnancy or oral contraceptive use also have a substantial risk of recurrent venous thrombosis and should be offered antepartum and postpartum thromboprophylaxis.61 In contrast, women with a prior “secondary” clot, no thrombophilia, and no additional current risk factors (Table 1) appear to be at low risk of recurrent venous thromboembolism.

The risks should be discussed with these women, with an option for close clinical surveillance during pregnancy (Table 4), but with a low threshold to investigate any worrisome symptoms. Such women may also elect to take LMWH or unfractionated heparin during pregnancy.

 

 

Which heparin to use?

Prophylactic anticoagulation during pregnancy can be with either LMWH or unfractionated heparin. For most women this involves “prophylactic” dosing with the goal of maintaining a mid-interval anti-factor-Xa activity level of approximately 0.05 to 0.2 U/mL. Thromboprophylaxis with LMWH can be with lower, fixed, once-daily doses throughout pregnancy20 (Table 2), although some clinicians still prefer twice-daily dosing. The heparin should be started as soon as pregnancy is confirmed, as the pregnancy-associated increase in thrombotic risk begins by the middle of the first trimester.

To maintain effective prophylactic levels, the dose of unfractionated heparin should be increased sequentially over the trimesters62,63: approximately 5,000 units subcutaneously twice daily in the first trimester, then 7,500 units twice daily in the second trimester, and 10,000 units twice daily in the third trimester for a woman of average size.

When to add low-dose aspirin

Women with antiphospholipid antibodies, particularly those with prior recurrent pregnancy loss or fetal demise, should receive aspirin 81 mg/day in addition to heparin.39 The aspirin may be started prior to conception or when pregnancy is confirmed.

Other measures

Women on anticoagulant therapy who are at risk of recurrent venous thromboembolism should be encouraged to wear elastic compression stockings. Intermittent pneumatic compression of the legs via automated devices may be considered for women hospitalized for any reason or on bedrest.

Whichever measures are used, a high index of suspicion and a low threshold for investigating for recurrent thrombosis should be maintained throughout pregnancy and the puerperium.

PERIPARTUM AND POSTPARTUM MANAGEMENT OF ANTICOAGULATION

Heparin therapy must be interrupted temporarily during the immediate peripartum interval to minimize the risk of hemorrhage and to allow for the option of regional anesthesia. As mentioned earlier, because of the theoretical risk of paraspinal hemorrhage in women receiving heparin who undergo epidural or spinal anesthesia, the American Society of Regional Anesthesia guidelines advise waiting to insert the needle at least 10 to 12 hours after the last prophylactic dose of LMWH, and at least 24 hours after the last therapeutic dose.31

The guidelines state that neuraxial anesthesia is not contraindicated in patients on prophylactic unfractionated heparin.31

To facilitate use of regional anesthesia in these women, therefore, options include:

  • Electively stopping LMWH 24 hours before planned induction of labor
  • Electively stopping prophylactic-dose LMWH or unfractionated heparin at about 38 weeks of gestation, to await spontaneous labor, or
  • Switching therapeutic or prophylactic LMWH to unfractionated heparin at about 36 weeks of gestation, with instructions to discontinue the injections in the earliest stages of spontaneous labor. This aims to shorten the heparin-free period required before neuraxial anesthesia while minimizing maternal thrombotic risk.

Additional advantages to using unfractionated heparin peripartum include the option of obtaining a rapid aPTT measurement to confirm the absence of a significant ongoing heparin effect prior to regional anesthesia or delivery, and the ability to completely reverse the heparin effect with protamine sulfate if major bleeding occurs. LMWHs are only partially reversible.64

Interrupting anticoagulation after an initial thrombotic event

If therapeutic anticoagulation must be interrupted for labor within 1 month of the initial thrombotic event, the risk of recurrent thrombotic complications is high65; these women must be observed very carefully and may benefit from intravenous heparin before and after delivery. They may even merit placement of a temporary vena cava filter (particularly if less than 2 weeks have elapsed since the venous thromboembolic event and in women with a large deep venous clot burden), a procedure that has been used safely but little studied in pregnant women.66

Fluoroscopic guidance may be needed for filter placement. This exposes the fetus to radiation, but the low-level exposure at this late gestational age is unlikely to pose a significant risk. The filter may be removed within 1 to 2 weeks postpartum, assuming there are no ongoing contraindications to anticoagulation.

In the rare woman with antithrombin deficiency and a recent or prior thrombotic event, giving antithrombin concentrate during the peripartum (heparin-free) interval has been described and may be considered under the guidance of a hematologist.67

Ongoing anticoagulation is essential postpartum, as the puerperium is the period of highest day-to-day risk of thromboembolic events: about one-third of pregnancy-associated events occur during these 6 to 12 weeks.2 Heparin should be resumed 6 to 12 hours after delivery, once hemostasis is confirmed.

Options for women requiring ongoing therapeutic anticoagulation include intravenous heparin started without a bolus, to minimize bleeding risk, with aPTT measured 12 hours later, or an initial prophylactic dose of LMWH 6 to 12 hours postpartum, with therapeutic dosing resumed on postpartum day 1. If prophylactic dosing is desired, unfractionated heparin or LMWH may be given subcutaneously starting at about 6 hours postpartum.

Warfarin in the puerperium

Women may subsequently be maintained on either LMWH or unfractionated heparin, or switched to an oral anticoagulant such as warfarin. Although warfarin may appear in minute amounts in breast milk, it has not been associated with adverse events in newborns and is considered compatible with breastfeeding.68 Heparin should be continued during the initial days of warfarin therapy, until the INR is at a therapeutic level for 24 hours. Some physicians prefer to delay warfarin for several days, giving LMWH alone in the immediate postpartum period, to allow wound-healing and to reduce bleeding risk.

Postpartum, anticoagulation should be continued for at least 6 to 12 weeks, at which point the physiologic changes in the coagulation system related to pregnancy will have returned to normal.

 

 

THROMBOPHILIA WITHOUT A PREVIOUS THROMBOEMBOLIC EVENT

Over the last 5 to 10 years, practitioners have been seeing many more young women with genetic or acquired thrombophilias who have never had a venous thromboembolic event. Physicians must advise these women about their risk of thromboembolic events during pregnancy and about the appropriateness of anticoagulant use.

Thrombophilias are often detected in women who develop venous thrombosis during pregnancy,69–71 but they are also very common in the general population (around 15%). While women with thrombophilia are at above-average risk of venous thromboembolism during pregnancy, the magnitude of risk in an individual patient is often difficult to estimate.

Data suggest that some types of thrombophilia confer greater thrombotic risk than others. McColl et al72 derived risk estimates for a primary event in women with several of the disorders: 0.23% in women heterozygous for the factor V Leiden mutation, 0.88% in women with protein C deficiency, and 2.4% to 35.7% in women with antithrombin deficiency. A case-control study70 found that all thrombophilic states were more common in women with pregnancy-associated venous thromboembolism than in healthy pregnant controls, except those with the MTHFR mutation and protein S deficiency. The estimated risk during pregnancy was 0.03% in women with no defect, 0.1% in women with protein C deficiency, 0.25% in women with the factor V Leiden mutation, 0.4% in those with antithrombin deficiency, 0.5% in those with the prothrombin gene mutation, and 4.6% in those with both factor V Leiden and prothrombin gene mutations.

Routine anticoagulation not advised in pregnant thrombophilic women

Because the risk of a primary venous thromboembolic event is less than 1% for most thrombophilic women, routine anticoagulant therapy does not seem prudent for this indication. Given the low absolute risk of venous thromboembolism, the cost and potential side effects of anticoagulant use are difficult to justify.

The women who seem at higher risk and in whom anticoagulation should be considered include those with antithrombin deficiency; those with high-titer anticardiolipin antibodies or a lupus anticoagulant antibody (treat with heparin and low-dose aspirin); those with combined thrombophilic defects or who are homozygotes for the factor V Leiden or prothrombin gene mutations; and those with multiple other current risk factors for venous thromboembolism (Table 1).

Since anticoagulants for primary prevention of adverse pregnancy outcomes in thrombophilic women have not yet been shown to have a definitive benefit, they are not recommended for this purpose.

ADVERSE PREGNANCY OUTCOMES IN WOMEN WITH THROMBOPHILIAS

Women with antiphospholipid antibodies and a previous poor obstetric outcome are clearly at increased risk of recurrent adverse pregnancy outcomes such as recurrent spontaneous abortion, unexplained fetal death, placental insufficiency, and early or severe preeclampsia. In such women who have both antiphospholipid antibodies and a history of venous thromboembolism or adverse pregnancy outcome, treatment during subsequent pregnancy with low-dose aspirin and prophylactic-dose LMWH or unfractionated heparin improves pregnancy outcomes.36–42 Women with antiphospholipid antibodies without previous thrombosis or pregnancy complications may also be at increased risk, but it is unclear whether thromboprophylaxis improves their outcomes.

Recent epidemiologic data reveal that women with other thrombophilic conditions also are at increased risk of early, severe preeclampsia73 as well as other pregnancy complications, including recurrent pregnancy loss, placental abruption, fetal growth restriction, and stillbirth.74 A recent meta-analysis75 looked at individual thrombophilias and found that factor V Leiden and prothrombin gene mutations were associated with recurrent fetal loss, stillbirth, and preeclampsia; that protein S deficiency was associated with recurrent fetal loss and stillbirth; that antiphospholipid antibodies were associated with recurrent pregnancy loss, preeclampsia, and intrauterine growth restriction; that the MTHFR mutation (homozygous) was associated with preeclampsia; and that protein C and antithrombin deficiencies were not significantly associated with adverse pregnancy outcomes. Data were scant for some of the rarer thrombophilias.75

Several recent small studies76–78 suggest that anticoagulants may improve pregnancy outcomes in women with genetic thrombophilias and recurrent pregnancy loss. These findings have not yet been confirmed in high-quality clinical trials, but such trials are under way. It is still unclear whether anticoagulants also reduce the risk of other adverse pregnancy outcomes associated with thrombophilias.

The current American College of Chest Physicians guidelines recommend testing of women with adverse pregnancy outcomes (recurrent pregnancy loss, prior severe or recurrent preeclampsia, abruptions, or otherwise unexplained intrauterine death) for congenital thrombophilias and antiphospholipid antibodies, and offering treatment to such women, if thrombophilic, with low-dose aspirin plus prophylactic heparin (unfractionated or LMWH).22 The authors of the guidelines admit that the evidence for this recommendation is weak, but they argue that the heparin will also serve as thromboprophylaxis in this high-risk group. Hopefully, the randomized clinical trials currently under way will provide clearer guidance regarding the most appropriate therapy in this difficult clinical situation.

MECHANICAL HEART VALVES

Internists may occasionally encounter a woman with a mechanical heart valve prosthesis who is either pregnant or is planning a pregnancy and therefore needs advice regarding optimal anticoagulant management. This should generally be undertaken in a multi-disciplinary fashion, with input from cardiology, hematology, and maternal-fetal medicine. The substantial maternal and fetal risks and the lack of definitive data on which to base treatment decisions make it a treacherous and stressful undertaking. Nonetheless, all internists should have a basic understanding of the complex issues regarding this management.

Outside of pregnancy, oral anticoagulants are the mainstay of therapy for patients with mechanical heart valves. Unfortunately, as discussed above, the use of these agents during pregnancy carries a risk of teratogenicity and toxic fetal effects and increases the risk of pregnancy loss and maternal hemorrhage. Heparins have been used in this setting for many years, but data on their efficacy and safety are very limited, and there are numerous reports of catastrophic maternal thrombotic complications.79,80

A systematic review of anticoagulation in pregnant women with prosthetic heart valves34 found very limited data on heparin use throughout pregnancy. Women maintained on warfarin vs heparin between pregnancy weeks 6 and 12 had higher rates of congenital anomalies (6.4% with warfarin vs 3.4% with heparin) and total fetal wastage (33.6% vs 26.5%). The warfarin group had fewer maternal thromboembolic complications (3.9% vs 9.2%), however, and a slightly lower rate of maternal death (1.8% vs 4.2%). Most of the women had higher-risk older-generation valves in the mitral position.

Recent data on LMWH consist mainly of case reports and case series,81 with a likely bias to publication of worse outcomes. Controlled trials in this area will be difficult to conduct. Still, aggressive anticoagulation with LMWH or unfractionated heparin, with close monitoring of the intensity of anticoagulation, may be safe and effective for pregnant women with newer-generation mechanical heart valves.82 A recent consensus statement22 suggested several regimens for pregnant women with mechanical heart valves:

  • Twice-daily LMWH throughout pregnancy, with the dose adjusted either by weight, or to keep the 4-hour postinjection anti-factor-Xa activity level around 1.0 to 1.2 U/mL
  • Aggressive adjusted-dose unfractionated heparin throughout pregnancy, given subcutaneously every 12 hours and adjusted to keep the mid-interval aPTT at least twice the control value or to attain a mid-interval anti-factor-Xa activity level of 0.35 to 0.70 U/mL
  • Unfractionated heparin or LMWH (as above) until gestation week 13, then warfarin until the middle of the third trimester, and then heparin again.22

The authors also recommended adding low-dose aspirin (75–162 mg/day) in high-risk women.22

These options all seem reasonable, given our current knowledge, though warfarin use during pregnancy should be restricted to very-high-risk situations, such as women with older-generation mitral prostheses. LM-WHs may become the preferred therapy for this indication once further controlled data regarding their efficacy and safety become available.

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  42. Rai R, Cohen H, Dave M, Regan L. Randomised controlled trial of aspirin and aspirin plus heparin in pregnant women with recurrent miscarriage associated with phospholipid antibodies (or antiphospholipid antibodies). BMJ 1997; 314:253257.
  43. Kozer E, Nikfar S, Costei A, Boskovic R, Nulman I, Koren G. Aspirin consumption during the first trimester of pregnancy and congenital anomalies: a meta-analysis. Am J Obstet Gynecol 2002; 187:16231630.
  44. Sebastian C, Scherlag M, Kugelmass A, Schechter E. Primary stent implantation for acute myocardial infarction during pregnancy: use of abciximab, ticlopidine, and aspirin. Cathet Cardiovasc Diagn 1998; 45:275249.
  45. Wilson AM, Boyle AJ, Fox P. Management of ischaemic heart disease in women of child-bearing age. Intern Med J 2004; 34:694697.
  46. Klinzing P, Markert UR, Liesaus K, Peiker G. Case report: successful pregnancy and delivery after myocardial infarction and essential thrombocythemia treated with clopidogrel. Clin Exp Obstet Gynecol 2001; 28:215216.
  47. Danhof M, de Boer A, Magnani HN, Stiekema JC. Pharmacokinetic considerations on Orgaran (Org 10172) therapy. Haemostasis 1992; 22:7384.
  48. Tardy-Poncet B, Tardy B, Reynaud J, et al. Efficacy and safety of danaparoid sodium (ORG 10172) in critically ill patients with heparin-associated thrombocytopenia. Chest 1999; 115:16161620.
  49. Lagrange F, Vergnes C, Brun JL, et al. Absence of placental transfer of pentasaccharide (fondaparinux, Arixtra) in the dually perfused human cotyledon in vitro. Thromb Haemost 2002; 87:831835.
  50. Dempfle CE. Minor transplacental passge of fondapinux in vivo. N Engl J Med 2004; 350:1914.
  51. Magnani HN. Heparin-induced thrombocytopenia (HIT): an overview of 230 patients treated with orgaran (Org 10172). Thromb Haemost 1993; 70:554561.
  52. Lindhoff-Last E, Kreutzenbeck HJ, Magnani HN. Treatment of 51 pregnancies with danaparoid because of heparin intolerance. Thromb Haemost 2005; 93:6369.
  53. Greinacher A, Eckhardt T, Mussmann J, Mueller-Eckhardt C. Pregnancy complicated by heparin associated thrombocytopenia: management by a prospectively in vitro selected heparinoid (Org 10172). Thromb Res 1993; 71:123126.
  54. Schindewolf M, Mosch G, Bauersachs RM, Lindhoff-Last E. Safe anticoagulation with danaparoid in pregnancy and lactation. Thromb Haemost 2004; 92:211.
  55. Harenberg J. Treatment of a woman with lupus and thromboembolism and cutaneous intolerance to heparins using fondaparinux during pregnancy. Thromb Res 2007; 119:385388.
  56. Wijesiriwardana A, Lees DA, Lush C. Fondaparinux as anticoagulant in a pregnant woman with heparin allergy. Blood Coagul Fibrinolysis 2006; 17:147149.
  57. Mazzolai L, Hohlfeld P, Spertini F, Hayoz D, Schapira M, Duchosal MA. Fondaparinux is a safe alternative in case of heparin intolerance during pregnancy. Blood 2006; 108:15691570.
  58. Hawkins D, Evans J. Minimizing the risk of heparin-induced osteoporosis during pregnancy. Expert Opin Drug Saf 2005; 4:583590.
  59. Brill-Edwards P, Ginsberg JS, Gent M, et al. Safety of withholding heparin in pregnant women with a history of venous thromboembolism. Recurrence of clot in this pregnancy study group. N Engl J Med 2000; 343:14391444.
  60. Martinelli I, Legnani C, Bucciarelli P, Grandone E, De Stefano V, Mannucci PM. Risk of pregnancy-related venous thrombosis in carriers of severe inherited thrombophilia. Thromb Haemost 2001; 86:800803.
  61. De Stefano V, Martinelli I, Rossi E, Battaglioli T, Za T, Mannucci PM, Leone G. The risk of recurrent venous thromboembolism in pregnancy and puerperium without antithrombotic prophylaxis. Br J Haematol 2006; 135:386391.
  62. Barbour LA, Smith JM, Marlar RA. Heparin levels to guide thromboembolism prophylaxis during pregnancy. Am J Obstet Gynecol 1995; 173:18691873.
  63. Ensom MH, Stephenson MD. Pharmacokinetics of low molecular weight heparin and unfractionated heparin in pregnancy. J Soc Gynecol Investig 2004; 11:377383.
  64. Crowther MA, Berry LR, Monagle PT, Chan AK. Mechanisms responsible for the failure of protamine to inactivate low-molecular-weight heparin. Br J Haematol 2002; 116:178186.
  65. Kearon C, Hirsh J. Management of anticoagulation before and after elective surgery. N Engl J Med 1997; 336:15061511.
  66. Thomas LA, Summers RR, Cardwell MS. Use of Greenfield filters in pregnant women at risk for pulmonary embolism. South Med J 1997; 90:215217.
  67. Maclean PS, Tait RC. Hereditary and acquired antithrombin deficiency: epidemiology, pathogenesis and treatment options. Drugs 2007; 67:14291440.
  68. Information from LactMed: http://toxnet.nlm.nih.gov/cgi-bin/sis/htmlgen?LACT, LactMed Record Number: 279. Accessed 11/26/2008.
  69. Gerhardt A, Scharf RE, Beckmann MW, et al. Prothrombin and factor V mutations in women with a history of thrombosis during pregnancy and the puerperium. N Engl J Med 2000; 342:374380.
  70. Hirsch DR, Mikkola KM, Marks PW, et al. Pulmonary embolism and deep venous thrombosis during pregnancy or oral contraceptive use: prevalence of factor V Leiden. Am Heart J 1996; 131:11451148.
  71. Dizon-Townson DS, Nelson LM, Jang H, Varner MW, Ward K. The incidence of the factor V Leiden mutation in an obstetric population and its relationship to deep vein thrombosis. Am J Obstet Gynecol 1997; 176:883886.
  72. McColl MD, Ramsay JE, Tait RC, et al. Risk factors for pregnancy associated venous thromboembolism. Thromb Haemost 1997; 78:11831188.
  73. Kupferminc MJ, Fait G, Many A, Gordon D, Eldor A, Lessing JB. Severe preeclampsia and high frequency of genetic thrombophilic mutations. Obstet Gynecol 2000; 96:4549.
  74. Kupferminc MJ, Eldor A, Steinman N, et al. Increased frequency of genetic thrombophilia in women with complications of pregnancy. N Engl J Med 1999; 340:913.
  75. Robertson L, Wu O, Langhorne P, et al. Thrombophilia in pregnancy: a systematic review. Br J Haematol 2006; 132:171196.
  76. Brenner B, Hoffman R, Blumenfeld Z, Weiner Z, Younis JS. Gestational outcome in thrombophilic women with recurrent pregnancy loss treated by enoxaparin. Thromb Haemost 2000; 83:693697.
  77. Carp H, Dolitzky M, Inbal A. Thromboprophylaxis improves the live birth rate in women with consecutive recurrent miscarriages and hereditary thrombophilia. J Thromb Haemost 2003; 1:433438.
  78. Gris JC, Mercier E, Quere I, et al. Low-molecular-weight heparin versus low-dose aspirin in women with one fetal loss and a constitutional thrombophilic disorder. Blood 2004; 103:36953699.
  79. Salazar E, Izaguirre R, Verdejo J, Mutchinick O. Failure of adjusted doses of subcutaneous heparin to prevent thromboembolic phenomena in pregnant patients with mechanical cardiac valve prostheses. J Am Coll Cardiol 1996; 27:16981703.
  80. Iturbe-Alessio I, Fonseca MC, Mutchinik O, Santos MA, Zajarias A, Salazar E. Risks of anticoagulant therapy in pregnant women with artificial heart valves. N Engl J Med 1986; 315:13901393.
  81. Rowan JA, McCowan LM, Raudkivi PJ, North RA. Enoxaparin treatment in women with mechanical heart valves during pregnancy. Am J Obstet Gynecol 2001; 185:633637.
  82. Oran B, Lee-Parritz A, Ansell J. Low molecular weight heparin for the prophylaxis of thromboembolism in women with prosthetic mechanical heart valves during pregnancy. Thromb Haemost 2004; 92:747751.
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Address: Paul S. Gibson, MD, HSC-1443, 3330 Hospital Drive NW, Calgary,
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Related Articles

Anticoagulation is essential in a wide variety of conditions in women of child-bearing age. Some, such as venous thromboembolism, occur more often during pregnancy. Others, such as recurrent fetal loss in the setting of antiphospholipid antibodies, are specific to pregnancy.

While anticoagulants are useful in many circumstances, their use during pregnancy increases the risk of hemorrhage and other adverse effects on the mother and the fetus. Treatment with anticoagulants during pregnancy must therefore be carefully considered, with judicious selection of the agent, and with reflection on the physiologic changes of pregnancy to ensure appropriate dosing. In this article, we review these issues.

WHY IS THROMBOTIC RISK HIGHER DURING PREGNANCY?

Venous thromboembolism is among the leading causes of maternal death in developed countries.1–3 Modern care has dramatically reduced the risk of maternal death from hemorrhage, infection, and hypertension, but rates of morbidity and death from thrombosis have remained stable or increased in recent years.4

Pregnancy is a period of increased risk of thrombotic complications (Table 1), owing to hypercoagulability, venous stasis, and vascular damage—the three elements of Virchow’s triad.5 Several changes to the maternal coagulation system increase clotting risk:

  • Much higher levels of fibrinogen and factors VII, VIII, IX, and X
  • Lower levels of protein S and increased resistance to activated protein C
  • Impaired fibrinolysis, due to inhibitors derived from the placenta.

Acquired antithrombin deficiency may also occur in high-proteinuric states such as nephrotic syndrome or preeclampsia, further increasing thrombotic risk. Pooling of venous blood, caused by progesterone-mediated venous dilation and compounded by compression of the inferior vena cava by the uterus in later pregnancy, also increases thrombotic risk. And endothelial disruption of the pelvic vessels may occur during delivery, particularly during cesarean section.

Additional factors that increase thrombotic risk include immobilization, such as bed rest for pregnancy complications; surgery, including cesarean section; ovarian hyperstimulation during gonadotropin use for in vitro fertilization; trauma; malignancy; and hereditary or acquired hypercoagulable states.6 These hypercoagulable states include deficiencies of antithrombin or the intrinsic anticoagulant proteins C or S; resistance to activated protein C, usually due to the factor V Leiden mutation; the PT20210A mutation of the prothrombin gene; hyperhomocystinemia due to mutation of the methyltetrahydrofolate reductase (MTHFR) gene; and the sustained presence of antiphospholipid antibodies, including lupus anticoagulant antibodies, sometimes also with moderately high titers of anticardiolipin or beta-2-glycoprotein I antibodies.

Other conditions that increase thrombotic risk include hyperemesis gravidarum, obesity, inflammatory bowel disease, infection, smoking, and indwelling intravenous catheters.6 Given the multitude of risk factors, pregnant women have a risk of thrombotic complications three to five times higher than nonpregnant women.7

HEPARIN USE DURING PREGNANCY

Low-molecular-weight heparins (LMWHs)8 and unfractionated heparin bind to anti-thrombin and thus change the shape of the antithrombin molecule, dramatically increasing its interaction with the clotting factors Xa and prothrombin (factor II). The enhanced clearance of these procoagulant proteins leads to the anticoagulant effect. Unfractionated heparin has roughly equivalent interaction with factors Xa and II and prolongs the activated partial thromboplastin time (aPTT), which is therefore used to monitor the intensity of anticoagulation.

LMWHs, on the other hand, interact relatively little with factor II and do not predictably prolong the aPTT. Monitoring their effect is therefore more difficult and requires direct measurement of anti-factor-Xa activity. This test is widely available, but it is time-consuming (it takes several hours and results may not be available within 24 hours if the test is requested “after hours”), and therefore it is of limited use in the acute clinical setting. While weight-based dosing of LMWHs is reliable and safe in nonpregnant patients, it has not yet been validated for pregnant women.

Unfractionated heparin has been used for decades for many indications during pregnancy. It is a large molecule, so it does not cross the placenta and thus, in contrast to the coumarin derivatives, does not cause teratogenesis or toxic fetal effects. Its main limitations in pregnancy are its inconvenient dosing (at least twice daily when given subcutaneously) and its potential maternal adverse effects (mainly osteoporosis and heparin-induced thrombocytopenia).

Over the last 10 years LMWHs have become the preferred anticoagulants for treating and preventing thromboembolism in all patients. They are equivalent or superior to unfractionated heparin in efficacy and safety in the initial treatment of acute deep venous thrombosis9,10 and pulmonary embolism11,12 outside of pregnancy. While comparative data are much less robust in pregnant patients, several series have confirmed the safety and efficacy of LMWHs in pregnancy.13–15 LMWHs do not cross the placenta15–17 and thus have a fetal safety profile equivalent to that of unfractionated heparin.

 

 

Pregnancy alters metabolism of LMWHs

The physiologic changes of pregnancy alter the metabolism of LMWH, resulting in lower peak levels and a higher rate of clearance,18,19 and so a pregnant woman may need higher doses or more frequent dosing.

Recent evidence suggests that thromboprophylaxis can be done with lower, fixed, once-daily doses of LMWH throughout pregnancy,20 although some clinicians still prefer twice-daily dosing (particularly during the latter half of pregnancy).

For therapeutic anticoagulation, however, the dose of LMWH required to achieve the desired level of anti-factor-Xa activity appears to change significantly over the course of pregnancy in many women.18 Therapeutic dosing of LMWH may also require twice-daily dosing, depending on the agent used (Table 2).

Pending more research on weight-based dosing of LMWH in pregnancy, anti-factor- Xa activity levels should be measured after treatment is started and every 1 to 3 months thereafter during pregnancy.21 Doses should be adjusted to keep the peak anti-Xa level (ie, 4 hours after the dose) at 0.5 to 1.2 U/mL.22

Heparin-induced thrombocytopenia

Type-2 heparin-induced thrombocytopenia is an uncommon but serious adverse effect of unfractionated heparin therapy (and, less commonly of LMWH), caused by heparin-dependent immunoglobulin G (IgG) antibodies that activate platelets via their Fc receptors, potentially precipitating life-threatening arterial or venous thrombosis.

In a trial in nonpregnant orthopedic patients,23 clinical heparin-induced thrombocytopenia occurred in 2.7% of patients receiving unfractionated heparin vs 0% of those receiving LMWH; heparin-dependent IgG was present in 7.8% vs 2.2%, respectively.

Fortunately, heparin-induced thrombocytopenia seems to be very rare in pregnancy: two recent prospective series evaluating prolonged LMWH use in pregnancy13,15 revealed no episodes of this disease. Nonetheless, it is reasonable to measure the platelet count once or twice weekly during the first few weeks of LMWH use and less often thereafter, unless symptoms of heparin-induced thrombocytopenia develop. In pregnant women with heparin-induced thrombocytopenia or heparin-related skin reactions, other anticoagulants must be considered24 (see discussion later).

Heparin-induced osteoporosis

Heparin-induced osteoporosis, a potential effect of prolonged heparin therapy, is of concern, given the prolonged duration and high doses of unfractionated heparin often needed to treat venous thromboembolism during pregnancy. Several studies found significant loss of bone mineral density in the proximal femur25 and lumbar spine26 during extended use of unfractionated heparin in pregnancy.

Fortunately, LMWH appears to be much safer with respect to bone loss. Three recent studies27–30 evaluated the use of LMWH for extended periods during pregnancy, and none found any greater loss of bone mineral density than that seen in normal pregnant controls. Giving supplemental calcium (1,000–1,500 mg/day) and vitamin D (400–1,000 IU/day) concomitantly with unfractionated heparin or LMWH in pregnancy is advisable to further reduce the risk.

Interrupt heparin to permit regional anesthesia

Heparin therapy should be temporarily stopped during the immediate peripartum interval to minimize the risk of hemorrhage and to permit regional anesthesia. Because of the theoretical risk of paraspinal hemorrhage in women receiving heparin who undergo epidural or spinal anesthesia, many anesthetists will not perform neuraxial regional anesthesia in women who have recently received heparin.

Since unfractionated heparin has a relatively short duration of action, the American Society of Regional Anesthesia states that subcutaneous unfractionated heparin prophylaxis is not a contraindication to neuraxial regional anesthesia.31 However, LMWHs should be stopped for at least 12 to 24 hours before regional anesthesia can be considered safe. This issue is discussed in more detail in the section on peripartum and postpartum management of anticoagulation, below.

In summary, LMWH during pregnancy offers a number of advantages over unfractionated heparin: equivalent efficacy, once- or twice-daily dosing, lower risk of heparin-induced thrombocytopenia and osteoporosis, and less-intensive monitoring. Unfractionated heparin can be offered to women who cannot afford LMWH (which costs four to five times more), and it may be used peripartum to reduce hemorrhagic risk and to permit regional anesthesia.

COUMARINS

Coumarins are the mainstay of anticoagulant therapy in most nonpregnant women beyond the immediate thrombotic period.

Warfarin (Coumadin) is the most widely used coumarin because it has a predictable onset and duration of action and excellent bioavailability.32 Others, such as acenocoumarol (Sintrom) and phenprocoumon (Marcoumar), are used more outside the United States but can be ordered or brought into the United States.

Coumarins interfere with vitamin K metabolism, inhibiting the generation of vitamin-K-dependent procoagulant proteins (factors II, VII, IX, and X) and thereby preventing clotting. They also inhibit the formation of the vitamin-K-dependent intrinsic anticoagulant proteins C and S.

Major bleeding is the most significant side effect of coumarin therapy, occurring at a rate of 4% to 6% over 3 months when the prothrombin time is maintained at an international normalized ratio (INR) of 2 to 3,33 and more often if the INR is higher.

Other issues with warfarin are the effect of variations in dietary vitamin K intake on anticoagulation and potential drug interactions that may alter the anticoagulant effect. Thus, the INR needs to be monitored closely.

 

 

Risks to the fetus and the mother

Unlike the heparins, coumarins freely cross the placenta and thus pose a risk of teratogenicity. A cluster of fetal malformations including “warfarin embryopathy” (nasal bone hypoplasia and chondrodysplasia punctata) can occur when the drug is used between 6 and 12 weeks of gestation. Warfarin embryopathy may be avoided by stopping warfarin prior to 6 weeks from the onset of the last menstrual period (ie, 6-week “menstrual age” or 4-week gestational age34).

Later in pregnancy, warfarin is associated with potential fetal bleeding complications leading to central nervous system abnormalities, increased rates of intrauterine fetal death, and pregnancy loss. In pregnant women with mechanical cardiac valve prostheses who received oral anticoagulants throughout pregnancy, the incidence of congenital anomalies was 6.4% to 10.2%.35 Fetal demise (spontaneous abortion, stillbirth, neonatal death) was also very common (29.7% to 33.6% of pregnancies) in coumarin-treated women.

Severe maternal hemorrhage may also occur in pregnant women on oral anticoagulants, particularly those who remain fully anticoagulated around the time of labor and delivery.

General caveats to warfarin in pregnancy

Because of the many maternal and fetal concerns, oral anticoagulant use in pregnancy is largely restricted to women with older-generation prosthetic heart valves in whom the very high maternal thrombotic risk may outweigh the risk of maternal and fetal side effects.

While there are limited data on warfarin use in pregnant women with antiphospholipid syndrome,36 warfarin use in such patients should be considered only for those at highest risk and with careful informed consent. These issues are discussed further below in the section on mechanical heart valve prostheses.

ANTIPLATELET DRUGS

Aspirin is an antiplatelet agent rather than an anticoagulant. Although considered inadequate for preventing venous thrombosis in high-risk groups when used alone, aspirin can moderately reduce the risk of deep venous thrombosis and pulmonary embolism in nonpregnant patients.37 It also has a well-accepted role in preventing arterial thrombotic events, ie, coronary artery disease and stroke.38

Low-dose aspirin (≤ 100 mg/day) has been extensively evaluated during pregnancy39–41 and has been shown to be safe and effective in reducing the risk of preeclampsia in high-risk women39 and in treating women with antiphospholipid antibodies and recurrent pregnancy loss42 (in conjunction with prophylactic doses of heparin). Although higher doses of aspirin and other nonsteroidal anti-inflammatory drugs can be toxic to the fetus, low doses have been shown to be safe throughout pregnancy.43

Dipyridamole (Persantine) has been studied extensively in pregnancy, and while it appears to be safe, it has not found a well-defined therapeutic role.

Other antiplatelet drugs have been only rarely used, and data on their safety and efficacy during pregnancy are limited to case reports, for example, on ticlopidine44 (Ticlid) and clopidogrel45,46 (Plavix) given during pregnancy in women with cardiac disease. These drugs do not appear to be major teratogens or to cause specific fetal harm. Their use may be reasonable in some high-risk situations, such as recurrent thrombotic stroke despite aspirin therapy. They may be used alone or with other anticoagulants in women with a coronary or other vascular stent if fetal safety is uncertain or if there is an increased risk of maternal bleeding.

NEWER ANTICOAGULANTS

Several newer anticoagulants can be used in pregnancy (Table 3).47–50

Danaparoid

The heparinoid danaparoid (Orgaran) is an LMWH, a combination of heparan, dermatan, and chondroitin sulfate. Since it is derived from heparin, in theory it can cross-react with antiheparin antibodies, but this is generally not a problem. Danaparoid inhibits factor Xa, and monitoring is via measurement of anti-factor-Xa activity levels. It has been shown to be safe and effective in nonpregnant patients with heparin-induced thrombocytopenia.51

Although no controlled study has been published on danaparoid in pregnancy, at least 51 pregnancies in 49 patients treated with danaparoid have been reported.52 Thirty-two of the patients received danaparoid because of heparin-induced thrombocytopenia and 19 because of heparin-induced skin intolerance. These reports suggest that danaparoid does not cross the placenta53 and that it may be effective and safe during pregnancy.54 For this reason, it is probably the preferred anticoagulant in pregnant patients with heparin-induced thrombocytopenia or other serious reactions to heparin.

Unfortunately, danaparoid has two major disadvantages. First, it has a prolonged half-life and no effective reversing agent, which makes its use problematic close to the time of delivery. Second, and perhaps more relevant to this discussion, it is not readily available in the United States; it was removed from the market by its manufacturer in April 2002 for business reasons rather than because of concerns over toxicity. It is still available in Canada and Europe, and it can be obtained in special circumstances in the United States via the US Food and Drug Administration (FDA); this may be worthwhile in pregnant patients who require a nonurgent alternative to heparin.

Direct thrombin inhibitors

Lepirudin (Refludan), bivalirudin (Angiomax), and argatroban are direct thrombin inhibitors and exert their anticoagulant effect independently of antithrombin. They are given by continuous intravenous infusion, and they have a very short half-life.

Lepirudin and argatroban are typically monitored via the aPTT. Bivalirudin can be monitored with the activated clotting time, partial thromboplastin time, or INR, depending on the circumstances. None of these agents generates or cross-reacts with antibodies generated in heparin-induced thrombocytopenia. None has an antidote, but the short half-life usually obviates the need for one.

Unfortunately, pregnancy data are very sparse for all three of these new agents. Argatroban has a low molecular weight and likely crosses the placenta. Also, because these agents are given intravenously, they are not practical for long-term use in pregnancy.

Fondaparinux

Fondaparinux (Arixtra), a direct factor Xa inhibitor, binds to antithrombin, causing an irreversible conformational change that increases antithrombin’s ability to inactivate factor Xa (as do the heparins). It has no effect on factor IIa (thrombin) and does not predictably affect the aPTT. Its half-life is 17 hours, and no agent is known to reverse its anticoagulant effect, although some experts would recommend a trial of high-dose recombinant factor VIIa (Novo-Seven) in uncontrolled hemorrhage.

While not FDA-approved for treating heparin-induced thrombocytopenia, it has been used for this in some patients.55–58 Animal studies and in vitro human placental perfusion studies suggest that fondaparinux does not cross the placenta in significant amounts.49 Since danaparoid is not available in the United States, fondaparinux would likely be the first choice among the newer anticoagulants when treating heparin-induced thrombocytopenia in pregnancy.

 

 

INDICATIONS FOR ANTICOAGULANTS DURING PREGNANCY

Acute deep venous thrombosis and pulmonary embolism

If acute deep venous thrombosis or pulmonary embolism is confirmed or strongly suspected in a pregnant woman, therapeutic anticoagulation should be started promptly (Table 4). In most cases, the woman should probably be hospitalized, given the complex maternal and fetal concerns that include adequate maternal dosing and the potential for fetal harm in the setting of significant hypoxia.

Anticoagulant therapy should begin as full doses of either LMWH or intravenous unfractionated heparin. We prefer starting with LMWH, as it can be started rapidly with less need for nursing care (eg, no need to start and maintain an intravenous line and monitor the aPTT) and has excellent safety. If LMWH is selected, initial dosing should be based on the current weight (Table 2). Subsequent monitoring of the peak anti-factor-Xa activity levels (ie, 4 hours after the dose) is recommended, with the first level drawn in the first few days of treatment, and repeat levels every 1 to 3 months for the rest of treatment. As mentioned earlier, weight-based dosing has not been systematically evaluated in pregnancy.

If unfractionated heparin is the initial agent, it should be given as a bolus followed by a continuous infusion, ideally utilizing a weight-based nomogram to estimate required doses, with adjustment of the infusion rate to maintain the aPTT at 1.5 to 2.5 times the baseline value (obtained during pregnancy). After several days, the heparin may be switched to LMWH in therapeutic doses (Table 2).

Alternatively, in women approaching term or who cannot afford LMWH, anticoagulation may be continued as adjusted-dose subcutaneous unfractionated heparin, ie, two or three large daily doses of subcutaneous heparin to provide therapeutic levels of anticoagulation. The starting dose can be calculated as the total units of heparin required to maintain full anticoagulation intravenously over 24 hours, given as two or three divided doses (Table 2). The aPTT at the mid-dosing interval (eg, 6 hours after the subcutaneous dose during every-12-hour dosing) should be monitored and the dose adjusted to maintain the aPTT at 1.5 to 2.5 times the baseline value.

A therapeutic level of anticoagulation should be maintained for at least 3 months after an acute thrombotic event during pregnancy, though many physicians prefer to continue full anticoagulation for a total of 6 months. Beyond this interval, if the woman is still pregnant, the anticoagulation may be reduced in intensity, perhaps even to a prophylactic level for the duration of the pregnancy (see discussion below on prior venous thromboembolic events) (Table 2). Peripartum and postpartum anticoagulation are discussed further below.

PRIOR VENOUS THROMBOEMBOLIC EVENT

While all pregnant women are at higher risk of venous thrombosis, the overall incidence of thromboembolism is only about one event per 1,000 pregnancies. Routine thromboprophylaxis in all pregnant women is therefore not justified. However, women who have previously had a venous thromboembolic event are at a substantially higher risk of recurrent thrombosis and should be considered for thromboprophylaxis in all subsequent high-risk situations, including pregnancy.

For women on indefinite therapeutic anticoagulation (ie, because of recurrent thrombosis), full therapeutic anticoagulation with LMWH or adjusted-dose unfractionated heparin should be maintained throughout pregnancy, as described above.

Which other women should receive prophylactic anticoagulation is a topic of ongoing debate and controversy.

How great is the risk of recurrent thromboembolism?

A small observational study59 examined the risk of recurrent venous thromboembolism during subsequent pregnancies in women with a prior thrombotic event. Anticoagulation was withheld during the antepartum period and restarted briefly after delivery. Among the 125 women enrolled, recurrent venous thromboembolism occurred in 4.8%, with half of the events occurring during the antepartum period. Among those with underlying thrombophilia, the rate of recurrent venous thromboembolism was 13% (95% confidence interval [CI] 1.7%–40.5%) to 20% (95% CI 2.5%–56.5%), and those with a prior idiopathic clot without thrombophilia had an event rate of 7.7% (95% CI 0.01%–25.1%). The subgroup with a prior reversible risk factor (at the time of their initial venous thromboembolic event) and without detectable thrombophilia had no recurrent events.

This study suggests that women with prior venous thromboembolism and thrombophilia or a prior idiopathic thrombotic event are at a substantial risk of recurrent thrombotic events during pregnancy. And other data confirm the high risk of recurrent venous thromboembolism in thrombophilic pregnant women.60 These women should all be offered active antepartum and postpartum thromboprophylaxis with LMWH or unfractionated heparin (Tables 2 and 4). Women without thrombophilia but with a history of venous thromboembolism related to pregnancy or oral contraceptive use also have a substantial risk of recurrent venous thrombosis and should be offered antepartum and postpartum thromboprophylaxis.61 In contrast, women with a prior “secondary” clot, no thrombophilia, and no additional current risk factors (Table 1) appear to be at low risk of recurrent venous thromboembolism.

The risks should be discussed with these women, with an option for close clinical surveillance during pregnancy (Table 4), but with a low threshold to investigate any worrisome symptoms. Such women may also elect to take LMWH or unfractionated heparin during pregnancy.

 

 

Which heparin to use?

Prophylactic anticoagulation during pregnancy can be with either LMWH or unfractionated heparin. For most women this involves “prophylactic” dosing with the goal of maintaining a mid-interval anti-factor-Xa activity level of approximately 0.05 to 0.2 U/mL. Thromboprophylaxis with LMWH can be with lower, fixed, once-daily doses throughout pregnancy20 (Table 2), although some clinicians still prefer twice-daily dosing. The heparin should be started as soon as pregnancy is confirmed, as the pregnancy-associated increase in thrombotic risk begins by the middle of the first trimester.

To maintain effective prophylactic levels, the dose of unfractionated heparin should be increased sequentially over the trimesters62,63: approximately 5,000 units subcutaneously twice daily in the first trimester, then 7,500 units twice daily in the second trimester, and 10,000 units twice daily in the third trimester for a woman of average size.

When to add low-dose aspirin

Women with antiphospholipid antibodies, particularly those with prior recurrent pregnancy loss or fetal demise, should receive aspirin 81 mg/day in addition to heparin.39 The aspirin may be started prior to conception or when pregnancy is confirmed.

Other measures

Women on anticoagulant therapy who are at risk of recurrent venous thromboembolism should be encouraged to wear elastic compression stockings. Intermittent pneumatic compression of the legs via automated devices may be considered for women hospitalized for any reason or on bedrest.

Whichever measures are used, a high index of suspicion and a low threshold for investigating for recurrent thrombosis should be maintained throughout pregnancy and the puerperium.

PERIPARTUM AND POSTPARTUM MANAGEMENT OF ANTICOAGULATION

Heparin therapy must be interrupted temporarily during the immediate peripartum interval to minimize the risk of hemorrhage and to allow for the option of regional anesthesia. As mentioned earlier, because of the theoretical risk of paraspinal hemorrhage in women receiving heparin who undergo epidural or spinal anesthesia, the American Society of Regional Anesthesia guidelines advise waiting to insert the needle at least 10 to 12 hours after the last prophylactic dose of LMWH, and at least 24 hours after the last therapeutic dose.31

The guidelines state that neuraxial anesthesia is not contraindicated in patients on prophylactic unfractionated heparin.31

To facilitate use of regional anesthesia in these women, therefore, options include:

  • Electively stopping LMWH 24 hours before planned induction of labor
  • Electively stopping prophylactic-dose LMWH or unfractionated heparin at about 38 weeks of gestation, to await spontaneous labor, or
  • Switching therapeutic or prophylactic LMWH to unfractionated heparin at about 36 weeks of gestation, with instructions to discontinue the injections in the earliest stages of spontaneous labor. This aims to shorten the heparin-free period required before neuraxial anesthesia while minimizing maternal thrombotic risk.

Additional advantages to using unfractionated heparin peripartum include the option of obtaining a rapid aPTT measurement to confirm the absence of a significant ongoing heparin effect prior to regional anesthesia or delivery, and the ability to completely reverse the heparin effect with protamine sulfate if major bleeding occurs. LMWHs are only partially reversible.64

Interrupting anticoagulation after an initial thrombotic event

If therapeutic anticoagulation must be interrupted for labor within 1 month of the initial thrombotic event, the risk of recurrent thrombotic complications is high65; these women must be observed very carefully and may benefit from intravenous heparin before and after delivery. They may even merit placement of a temporary vena cava filter (particularly if less than 2 weeks have elapsed since the venous thromboembolic event and in women with a large deep venous clot burden), a procedure that has been used safely but little studied in pregnant women.66

Fluoroscopic guidance may be needed for filter placement. This exposes the fetus to radiation, but the low-level exposure at this late gestational age is unlikely to pose a significant risk. The filter may be removed within 1 to 2 weeks postpartum, assuming there are no ongoing contraindications to anticoagulation.

In the rare woman with antithrombin deficiency and a recent or prior thrombotic event, giving antithrombin concentrate during the peripartum (heparin-free) interval has been described and may be considered under the guidance of a hematologist.67

Ongoing anticoagulation is essential postpartum, as the puerperium is the period of highest day-to-day risk of thromboembolic events: about one-third of pregnancy-associated events occur during these 6 to 12 weeks.2 Heparin should be resumed 6 to 12 hours after delivery, once hemostasis is confirmed.

Options for women requiring ongoing therapeutic anticoagulation include intravenous heparin started without a bolus, to minimize bleeding risk, with aPTT measured 12 hours later, or an initial prophylactic dose of LMWH 6 to 12 hours postpartum, with therapeutic dosing resumed on postpartum day 1. If prophylactic dosing is desired, unfractionated heparin or LMWH may be given subcutaneously starting at about 6 hours postpartum.

Warfarin in the puerperium

Women may subsequently be maintained on either LMWH or unfractionated heparin, or switched to an oral anticoagulant such as warfarin. Although warfarin may appear in minute amounts in breast milk, it has not been associated with adverse events in newborns and is considered compatible with breastfeeding.68 Heparin should be continued during the initial days of warfarin therapy, until the INR is at a therapeutic level for 24 hours. Some physicians prefer to delay warfarin for several days, giving LMWH alone in the immediate postpartum period, to allow wound-healing and to reduce bleeding risk.

Postpartum, anticoagulation should be continued for at least 6 to 12 weeks, at which point the physiologic changes in the coagulation system related to pregnancy will have returned to normal.

 

 

THROMBOPHILIA WITHOUT A PREVIOUS THROMBOEMBOLIC EVENT

Over the last 5 to 10 years, practitioners have been seeing many more young women with genetic or acquired thrombophilias who have never had a venous thromboembolic event. Physicians must advise these women about their risk of thromboembolic events during pregnancy and about the appropriateness of anticoagulant use.

Thrombophilias are often detected in women who develop venous thrombosis during pregnancy,69–71 but they are also very common in the general population (around 15%). While women with thrombophilia are at above-average risk of venous thromboembolism during pregnancy, the magnitude of risk in an individual patient is often difficult to estimate.

Data suggest that some types of thrombophilia confer greater thrombotic risk than others. McColl et al72 derived risk estimates for a primary event in women with several of the disorders: 0.23% in women heterozygous for the factor V Leiden mutation, 0.88% in women with protein C deficiency, and 2.4% to 35.7% in women with antithrombin deficiency. A case-control study70 found that all thrombophilic states were more common in women with pregnancy-associated venous thromboembolism than in healthy pregnant controls, except those with the MTHFR mutation and protein S deficiency. The estimated risk during pregnancy was 0.03% in women with no defect, 0.1% in women with protein C deficiency, 0.25% in women with the factor V Leiden mutation, 0.4% in those with antithrombin deficiency, 0.5% in those with the prothrombin gene mutation, and 4.6% in those with both factor V Leiden and prothrombin gene mutations.

Routine anticoagulation not advised in pregnant thrombophilic women

Because the risk of a primary venous thromboembolic event is less than 1% for most thrombophilic women, routine anticoagulant therapy does not seem prudent for this indication. Given the low absolute risk of venous thromboembolism, the cost and potential side effects of anticoagulant use are difficult to justify.

The women who seem at higher risk and in whom anticoagulation should be considered include those with antithrombin deficiency; those with high-titer anticardiolipin antibodies or a lupus anticoagulant antibody (treat with heparin and low-dose aspirin); those with combined thrombophilic defects or who are homozygotes for the factor V Leiden or prothrombin gene mutations; and those with multiple other current risk factors for venous thromboembolism (Table 1).

Since anticoagulants for primary prevention of adverse pregnancy outcomes in thrombophilic women have not yet been shown to have a definitive benefit, they are not recommended for this purpose.

ADVERSE PREGNANCY OUTCOMES IN WOMEN WITH THROMBOPHILIAS

Women with antiphospholipid antibodies and a previous poor obstetric outcome are clearly at increased risk of recurrent adverse pregnancy outcomes such as recurrent spontaneous abortion, unexplained fetal death, placental insufficiency, and early or severe preeclampsia. In such women who have both antiphospholipid antibodies and a history of venous thromboembolism or adverse pregnancy outcome, treatment during subsequent pregnancy with low-dose aspirin and prophylactic-dose LMWH or unfractionated heparin improves pregnancy outcomes.36–42 Women with antiphospholipid antibodies without previous thrombosis or pregnancy complications may also be at increased risk, but it is unclear whether thromboprophylaxis improves their outcomes.

Recent epidemiologic data reveal that women with other thrombophilic conditions also are at increased risk of early, severe preeclampsia73 as well as other pregnancy complications, including recurrent pregnancy loss, placental abruption, fetal growth restriction, and stillbirth.74 A recent meta-analysis75 looked at individual thrombophilias and found that factor V Leiden and prothrombin gene mutations were associated with recurrent fetal loss, stillbirth, and preeclampsia; that protein S deficiency was associated with recurrent fetal loss and stillbirth; that antiphospholipid antibodies were associated with recurrent pregnancy loss, preeclampsia, and intrauterine growth restriction; that the MTHFR mutation (homozygous) was associated with preeclampsia; and that protein C and antithrombin deficiencies were not significantly associated with adverse pregnancy outcomes. Data were scant for some of the rarer thrombophilias.75

Several recent small studies76–78 suggest that anticoagulants may improve pregnancy outcomes in women with genetic thrombophilias and recurrent pregnancy loss. These findings have not yet been confirmed in high-quality clinical trials, but such trials are under way. It is still unclear whether anticoagulants also reduce the risk of other adverse pregnancy outcomes associated with thrombophilias.

The current American College of Chest Physicians guidelines recommend testing of women with adverse pregnancy outcomes (recurrent pregnancy loss, prior severe or recurrent preeclampsia, abruptions, or otherwise unexplained intrauterine death) for congenital thrombophilias and antiphospholipid antibodies, and offering treatment to such women, if thrombophilic, with low-dose aspirin plus prophylactic heparin (unfractionated or LMWH).22 The authors of the guidelines admit that the evidence for this recommendation is weak, but they argue that the heparin will also serve as thromboprophylaxis in this high-risk group. Hopefully, the randomized clinical trials currently under way will provide clearer guidance regarding the most appropriate therapy in this difficult clinical situation.

MECHANICAL HEART VALVES

Internists may occasionally encounter a woman with a mechanical heart valve prosthesis who is either pregnant or is planning a pregnancy and therefore needs advice regarding optimal anticoagulant management. This should generally be undertaken in a multi-disciplinary fashion, with input from cardiology, hematology, and maternal-fetal medicine. The substantial maternal and fetal risks and the lack of definitive data on which to base treatment decisions make it a treacherous and stressful undertaking. Nonetheless, all internists should have a basic understanding of the complex issues regarding this management.

Outside of pregnancy, oral anticoagulants are the mainstay of therapy for patients with mechanical heart valves. Unfortunately, as discussed above, the use of these agents during pregnancy carries a risk of teratogenicity and toxic fetal effects and increases the risk of pregnancy loss and maternal hemorrhage. Heparins have been used in this setting for many years, but data on their efficacy and safety are very limited, and there are numerous reports of catastrophic maternal thrombotic complications.79,80

A systematic review of anticoagulation in pregnant women with prosthetic heart valves34 found very limited data on heparin use throughout pregnancy. Women maintained on warfarin vs heparin between pregnancy weeks 6 and 12 had higher rates of congenital anomalies (6.4% with warfarin vs 3.4% with heparin) and total fetal wastage (33.6% vs 26.5%). The warfarin group had fewer maternal thromboembolic complications (3.9% vs 9.2%), however, and a slightly lower rate of maternal death (1.8% vs 4.2%). Most of the women had higher-risk older-generation valves in the mitral position.

Recent data on LMWH consist mainly of case reports and case series,81 with a likely bias to publication of worse outcomes. Controlled trials in this area will be difficult to conduct. Still, aggressive anticoagulation with LMWH or unfractionated heparin, with close monitoring of the intensity of anticoagulation, may be safe and effective for pregnant women with newer-generation mechanical heart valves.82 A recent consensus statement22 suggested several regimens for pregnant women with mechanical heart valves:

  • Twice-daily LMWH throughout pregnancy, with the dose adjusted either by weight, or to keep the 4-hour postinjection anti-factor-Xa activity level around 1.0 to 1.2 U/mL
  • Aggressive adjusted-dose unfractionated heparin throughout pregnancy, given subcutaneously every 12 hours and adjusted to keep the mid-interval aPTT at least twice the control value or to attain a mid-interval anti-factor-Xa activity level of 0.35 to 0.70 U/mL
  • Unfractionated heparin or LMWH (as above) until gestation week 13, then warfarin until the middle of the third trimester, and then heparin again.22

The authors also recommended adding low-dose aspirin (75–162 mg/day) in high-risk women.22

These options all seem reasonable, given our current knowledge, though warfarin use during pregnancy should be restricted to very-high-risk situations, such as women with older-generation mitral prostheses. LM-WHs may become the preferred therapy for this indication once further controlled data regarding their efficacy and safety become available.

Anticoagulation is essential in a wide variety of conditions in women of child-bearing age. Some, such as venous thromboembolism, occur more often during pregnancy. Others, such as recurrent fetal loss in the setting of antiphospholipid antibodies, are specific to pregnancy.

While anticoagulants are useful in many circumstances, their use during pregnancy increases the risk of hemorrhage and other adverse effects on the mother and the fetus. Treatment with anticoagulants during pregnancy must therefore be carefully considered, with judicious selection of the agent, and with reflection on the physiologic changes of pregnancy to ensure appropriate dosing. In this article, we review these issues.

WHY IS THROMBOTIC RISK HIGHER DURING PREGNANCY?

Venous thromboembolism is among the leading causes of maternal death in developed countries.1–3 Modern care has dramatically reduced the risk of maternal death from hemorrhage, infection, and hypertension, but rates of morbidity and death from thrombosis have remained stable or increased in recent years.4

Pregnancy is a period of increased risk of thrombotic complications (Table 1), owing to hypercoagulability, venous stasis, and vascular damage—the three elements of Virchow’s triad.5 Several changes to the maternal coagulation system increase clotting risk:

  • Much higher levels of fibrinogen and factors VII, VIII, IX, and X
  • Lower levels of protein S and increased resistance to activated protein C
  • Impaired fibrinolysis, due to inhibitors derived from the placenta.

Acquired antithrombin deficiency may also occur in high-proteinuric states such as nephrotic syndrome or preeclampsia, further increasing thrombotic risk. Pooling of venous blood, caused by progesterone-mediated venous dilation and compounded by compression of the inferior vena cava by the uterus in later pregnancy, also increases thrombotic risk. And endothelial disruption of the pelvic vessels may occur during delivery, particularly during cesarean section.

Additional factors that increase thrombotic risk include immobilization, such as bed rest for pregnancy complications; surgery, including cesarean section; ovarian hyperstimulation during gonadotropin use for in vitro fertilization; trauma; malignancy; and hereditary or acquired hypercoagulable states.6 These hypercoagulable states include deficiencies of antithrombin or the intrinsic anticoagulant proteins C or S; resistance to activated protein C, usually due to the factor V Leiden mutation; the PT20210A mutation of the prothrombin gene; hyperhomocystinemia due to mutation of the methyltetrahydrofolate reductase (MTHFR) gene; and the sustained presence of antiphospholipid antibodies, including lupus anticoagulant antibodies, sometimes also with moderately high titers of anticardiolipin or beta-2-glycoprotein I antibodies.

Other conditions that increase thrombotic risk include hyperemesis gravidarum, obesity, inflammatory bowel disease, infection, smoking, and indwelling intravenous catheters.6 Given the multitude of risk factors, pregnant women have a risk of thrombotic complications three to five times higher than nonpregnant women.7

HEPARIN USE DURING PREGNANCY

Low-molecular-weight heparins (LMWHs)8 and unfractionated heparin bind to anti-thrombin and thus change the shape of the antithrombin molecule, dramatically increasing its interaction with the clotting factors Xa and prothrombin (factor II). The enhanced clearance of these procoagulant proteins leads to the anticoagulant effect. Unfractionated heparin has roughly equivalent interaction with factors Xa and II and prolongs the activated partial thromboplastin time (aPTT), which is therefore used to monitor the intensity of anticoagulation.

LMWHs, on the other hand, interact relatively little with factor II and do not predictably prolong the aPTT. Monitoring their effect is therefore more difficult and requires direct measurement of anti-factor-Xa activity. This test is widely available, but it is time-consuming (it takes several hours and results may not be available within 24 hours if the test is requested “after hours”), and therefore it is of limited use in the acute clinical setting. While weight-based dosing of LMWHs is reliable and safe in nonpregnant patients, it has not yet been validated for pregnant women.

Unfractionated heparin has been used for decades for many indications during pregnancy. It is a large molecule, so it does not cross the placenta and thus, in contrast to the coumarin derivatives, does not cause teratogenesis or toxic fetal effects. Its main limitations in pregnancy are its inconvenient dosing (at least twice daily when given subcutaneously) and its potential maternal adverse effects (mainly osteoporosis and heparin-induced thrombocytopenia).

Over the last 10 years LMWHs have become the preferred anticoagulants for treating and preventing thromboembolism in all patients. They are equivalent or superior to unfractionated heparin in efficacy and safety in the initial treatment of acute deep venous thrombosis9,10 and pulmonary embolism11,12 outside of pregnancy. While comparative data are much less robust in pregnant patients, several series have confirmed the safety and efficacy of LMWHs in pregnancy.13–15 LMWHs do not cross the placenta15–17 and thus have a fetal safety profile equivalent to that of unfractionated heparin.

 

 

Pregnancy alters metabolism of LMWHs

The physiologic changes of pregnancy alter the metabolism of LMWH, resulting in lower peak levels and a higher rate of clearance,18,19 and so a pregnant woman may need higher doses or more frequent dosing.

Recent evidence suggests that thromboprophylaxis can be done with lower, fixed, once-daily doses of LMWH throughout pregnancy,20 although some clinicians still prefer twice-daily dosing (particularly during the latter half of pregnancy).

For therapeutic anticoagulation, however, the dose of LMWH required to achieve the desired level of anti-factor-Xa activity appears to change significantly over the course of pregnancy in many women.18 Therapeutic dosing of LMWH may also require twice-daily dosing, depending on the agent used (Table 2).

Pending more research on weight-based dosing of LMWH in pregnancy, anti-factor- Xa activity levels should be measured after treatment is started and every 1 to 3 months thereafter during pregnancy.21 Doses should be adjusted to keep the peak anti-Xa level (ie, 4 hours after the dose) at 0.5 to 1.2 U/mL.22

Heparin-induced thrombocytopenia

Type-2 heparin-induced thrombocytopenia is an uncommon but serious adverse effect of unfractionated heparin therapy (and, less commonly of LMWH), caused by heparin-dependent immunoglobulin G (IgG) antibodies that activate platelets via their Fc receptors, potentially precipitating life-threatening arterial or venous thrombosis.

In a trial in nonpregnant orthopedic patients,23 clinical heparin-induced thrombocytopenia occurred in 2.7% of patients receiving unfractionated heparin vs 0% of those receiving LMWH; heparin-dependent IgG was present in 7.8% vs 2.2%, respectively.

Fortunately, heparin-induced thrombocytopenia seems to be very rare in pregnancy: two recent prospective series evaluating prolonged LMWH use in pregnancy13,15 revealed no episodes of this disease. Nonetheless, it is reasonable to measure the platelet count once or twice weekly during the first few weeks of LMWH use and less often thereafter, unless symptoms of heparin-induced thrombocytopenia develop. In pregnant women with heparin-induced thrombocytopenia or heparin-related skin reactions, other anticoagulants must be considered24 (see discussion later).

Heparin-induced osteoporosis

Heparin-induced osteoporosis, a potential effect of prolonged heparin therapy, is of concern, given the prolonged duration and high doses of unfractionated heparin often needed to treat venous thromboembolism during pregnancy. Several studies found significant loss of bone mineral density in the proximal femur25 and lumbar spine26 during extended use of unfractionated heparin in pregnancy.

Fortunately, LMWH appears to be much safer with respect to bone loss. Three recent studies27–30 evaluated the use of LMWH for extended periods during pregnancy, and none found any greater loss of bone mineral density than that seen in normal pregnant controls. Giving supplemental calcium (1,000–1,500 mg/day) and vitamin D (400–1,000 IU/day) concomitantly with unfractionated heparin or LMWH in pregnancy is advisable to further reduce the risk.

Interrupt heparin to permit regional anesthesia

Heparin therapy should be temporarily stopped during the immediate peripartum interval to minimize the risk of hemorrhage and to permit regional anesthesia. Because of the theoretical risk of paraspinal hemorrhage in women receiving heparin who undergo epidural or spinal anesthesia, many anesthetists will not perform neuraxial regional anesthesia in women who have recently received heparin.

Since unfractionated heparin has a relatively short duration of action, the American Society of Regional Anesthesia states that subcutaneous unfractionated heparin prophylaxis is not a contraindication to neuraxial regional anesthesia.31 However, LMWHs should be stopped for at least 12 to 24 hours before regional anesthesia can be considered safe. This issue is discussed in more detail in the section on peripartum and postpartum management of anticoagulation, below.

In summary, LMWH during pregnancy offers a number of advantages over unfractionated heparin: equivalent efficacy, once- or twice-daily dosing, lower risk of heparin-induced thrombocytopenia and osteoporosis, and less-intensive monitoring. Unfractionated heparin can be offered to women who cannot afford LMWH (which costs four to five times more), and it may be used peripartum to reduce hemorrhagic risk and to permit regional anesthesia.

COUMARINS

Coumarins are the mainstay of anticoagulant therapy in most nonpregnant women beyond the immediate thrombotic period.

Warfarin (Coumadin) is the most widely used coumarin because it has a predictable onset and duration of action and excellent bioavailability.32 Others, such as acenocoumarol (Sintrom) and phenprocoumon (Marcoumar), are used more outside the United States but can be ordered or brought into the United States.

Coumarins interfere with vitamin K metabolism, inhibiting the generation of vitamin-K-dependent procoagulant proteins (factors II, VII, IX, and X) and thereby preventing clotting. They also inhibit the formation of the vitamin-K-dependent intrinsic anticoagulant proteins C and S.

Major bleeding is the most significant side effect of coumarin therapy, occurring at a rate of 4% to 6% over 3 months when the prothrombin time is maintained at an international normalized ratio (INR) of 2 to 3,33 and more often if the INR is higher.

Other issues with warfarin are the effect of variations in dietary vitamin K intake on anticoagulation and potential drug interactions that may alter the anticoagulant effect. Thus, the INR needs to be monitored closely.

 

 

Risks to the fetus and the mother

Unlike the heparins, coumarins freely cross the placenta and thus pose a risk of teratogenicity. A cluster of fetal malformations including “warfarin embryopathy” (nasal bone hypoplasia and chondrodysplasia punctata) can occur when the drug is used between 6 and 12 weeks of gestation. Warfarin embryopathy may be avoided by stopping warfarin prior to 6 weeks from the onset of the last menstrual period (ie, 6-week “menstrual age” or 4-week gestational age34).

Later in pregnancy, warfarin is associated with potential fetal bleeding complications leading to central nervous system abnormalities, increased rates of intrauterine fetal death, and pregnancy loss. In pregnant women with mechanical cardiac valve prostheses who received oral anticoagulants throughout pregnancy, the incidence of congenital anomalies was 6.4% to 10.2%.35 Fetal demise (spontaneous abortion, stillbirth, neonatal death) was also very common (29.7% to 33.6% of pregnancies) in coumarin-treated women.

Severe maternal hemorrhage may also occur in pregnant women on oral anticoagulants, particularly those who remain fully anticoagulated around the time of labor and delivery.

General caveats to warfarin in pregnancy

Because of the many maternal and fetal concerns, oral anticoagulant use in pregnancy is largely restricted to women with older-generation prosthetic heart valves in whom the very high maternal thrombotic risk may outweigh the risk of maternal and fetal side effects.

While there are limited data on warfarin use in pregnant women with antiphospholipid syndrome,36 warfarin use in such patients should be considered only for those at highest risk and with careful informed consent. These issues are discussed further below in the section on mechanical heart valve prostheses.

ANTIPLATELET DRUGS

Aspirin is an antiplatelet agent rather than an anticoagulant. Although considered inadequate for preventing venous thrombosis in high-risk groups when used alone, aspirin can moderately reduce the risk of deep venous thrombosis and pulmonary embolism in nonpregnant patients.37 It also has a well-accepted role in preventing arterial thrombotic events, ie, coronary artery disease and stroke.38

Low-dose aspirin (≤ 100 mg/day) has been extensively evaluated during pregnancy39–41 and has been shown to be safe and effective in reducing the risk of preeclampsia in high-risk women39 and in treating women with antiphospholipid antibodies and recurrent pregnancy loss42 (in conjunction with prophylactic doses of heparin). Although higher doses of aspirin and other nonsteroidal anti-inflammatory drugs can be toxic to the fetus, low doses have been shown to be safe throughout pregnancy.43

Dipyridamole (Persantine) has been studied extensively in pregnancy, and while it appears to be safe, it has not found a well-defined therapeutic role.

Other antiplatelet drugs have been only rarely used, and data on their safety and efficacy during pregnancy are limited to case reports, for example, on ticlopidine44 (Ticlid) and clopidogrel45,46 (Plavix) given during pregnancy in women with cardiac disease. These drugs do not appear to be major teratogens or to cause specific fetal harm. Their use may be reasonable in some high-risk situations, such as recurrent thrombotic stroke despite aspirin therapy. They may be used alone or with other anticoagulants in women with a coronary or other vascular stent if fetal safety is uncertain or if there is an increased risk of maternal bleeding.

NEWER ANTICOAGULANTS

Several newer anticoagulants can be used in pregnancy (Table 3).47–50

Danaparoid

The heparinoid danaparoid (Orgaran) is an LMWH, a combination of heparan, dermatan, and chondroitin sulfate. Since it is derived from heparin, in theory it can cross-react with antiheparin antibodies, but this is generally not a problem. Danaparoid inhibits factor Xa, and monitoring is via measurement of anti-factor-Xa activity levels. It has been shown to be safe and effective in nonpregnant patients with heparin-induced thrombocytopenia.51

Although no controlled study has been published on danaparoid in pregnancy, at least 51 pregnancies in 49 patients treated with danaparoid have been reported.52 Thirty-two of the patients received danaparoid because of heparin-induced thrombocytopenia and 19 because of heparin-induced skin intolerance. These reports suggest that danaparoid does not cross the placenta53 and that it may be effective and safe during pregnancy.54 For this reason, it is probably the preferred anticoagulant in pregnant patients with heparin-induced thrombocytopenia or other serious reactions to heparin.

Unfortunately, danaparoid has two major disadvantages. First, it has a prolonged half-life and no effective reversing agent, which makes its use problematic close to the time of delivery. Second, and perhaps more relevant to this discussion, it is not readily available in the United States; it was removed from the market by its manufacturer in April 2002 for business reasons rather than because of concerns over toxicity. It is still available in Canada and Europe, and it can be obtained in special circumstances in the United States via the US Food and Drug Administration (FDA); this may be worthwhile in pregnant patients who require a nonurgent alternative to heparin.

Direct thrombin inhibitors

Lepirudin (Refludan), bivalirudin (Angiomax), and argatroban are direct thrombin inhibitors and exert their anticoagulant effect independently of antithrombin. They are given by continuous intravenous infusion, and they have a very short half-life.

Lepirudin and argatroban are typically monitored via the aPTT. Bivalirudin can be monitored with the activated clotting time, partial thromboplastin time, or INR, depending on the circumstances. None of these agents generates or cross-reacts with antibodies generated in heparin-induced thrombocytopenia. None has an antidote, but the short half-life usually obviates the need for one.

Unfortunately, pregnancy data are very sparse for all three of these new agents. Argatroban has a low molecular weight and likely crosses the placenta. Also, because these agents are given intravenously, they are not practical for long-term use in pregnancy.

Fondaparinux

Fondaparinux (Arixtra), a direct factor Xa inhibitor, binds to antithrombin, causing an irreversible conformational change that increases antithrombin’s ability to inactivate factor Xa (as do the heparins). It has no effect on factor IIa (thrombin) and does not predictably affect the aPTT. Its half-life is 17 hours, and no agent is known to reverse its anticoagulant effect, although some experts would recommend a trial of high-dose recombinant factor VIIa (Novo-Seven) in uncontrolled hemorrhage.

While not FDA-approved for treating heparin-induced thrombocytopenia, it has been used for this in some patients.55–58 Animal studies and in vitro human placental perfusion studies suggest that fondaparinux does not cross the placenta in significant amounts.49 Since danaparoid is not available in the United States, fondaparinux would likely be the first choice among the newer anticoagulants when treating heparin-induced thrombocytopenia in pregnancy.

 

 

INDICATIONS FOR ANTICOAGULANTS DURING PREGNANCY

Acute deep venous thrombosis and pulmonary embolism

If acute deep venous thrombosis or pulmonary embolism is confirmed or strongly suspected in a pregnant woman, therapeutic anticoagulation should be started promptly (Table 4). In most cases, the woman should probably be hospitalized, given the complex maternal and fetal concerns that include adequate maternal dosing and the potential for fetal harm in the setting of significant hypoxia.

Anticoagulant therapy should begin as full doses of either LMWH or intravenous unfractionated heparin. We prefer starting with LMWH, as it can be started rapidly with less need for nursing care (eg, no need to start and maintain an intravenous line and monitor the aPTT) and has excellent safety. If LMWH is selected, initial dosing should be based on the current weight (Table 2). Subsequent monitoring of the peak anti-factor-Xa activity levels (ie, 4 hours after the dose) is recommended, with the first level drawn in the first few days of treatment, and repeat levels every 1 to 3 months for the rest of treatment. As mentioned earlier, weight-based dosing has not been systematically evaluated in pregnancy.

If unfractionated heparin is the initial agent, it should be given as a bolus followed by a continuous infusion, ideally utilizing a weight-based nomogram to estimate required doses, with adjustment of the infusion rate to maintain the aPTT at 1.5 to 2.5 times the baseline value (obtained during pregnancy). After several days, the heparin may be switched to LMWH in therapeutic doses (Table 2).

Alternatively, in women approaching term or who cannot afford LMWH, anticoagulation may be continued as adjusted-dose subcutaneous unfractionated heparin, ie, two or three large daily doses of subcutaneous heparin to provide therapeutic levels of anticoagulation. The starting dose can be calculated as the total units of heparin required to maintain full anticoagulation intravenously over 24 hours, given as two or three divided doses (Table 2). The aPTT at the mid-dosing interval (eg, 6 hours after the subcutaneous dose during every-12-hour dosing) should be monitored and the dose adjusted to maintain the aPTT at 1.5 to 2.5 times the baseline value.

A therapeutic level of anticoagulation should be maintained for at least 3 months after an acute thrombotic event during pregnancy, though many physicians prefer to continue full anticoagulation for a total of 6 months. Beyond this interval, if the woman is still pregnant, the anticoagulation may be reduced in intensity, perhaps even to a prophylactic level for the duration of the pregnancy (see discussion below on prior venous thromboembolic events) (Table 2). Peripartum and postpartum anticoagulation are discussed further below.

PRIOR VENOUS THROMBOEMBOLIC EVENT

While all pregnant women are at higher risk of venous thrombosis, the overall incidence of thromboembolism is only about one event per 1,000 pregnancies. Routine thromboprophylaxis in all pregnant women is therefore not justified. However, women who have previously had a venous thromboembolic event are at a substantially higher risk of recurrent thrombosis and should be considered for thromboprophylaxis in all subsequent high-risk situations, including pregnancy.

For women on indefinite therapeutic anticoagulation (ie, because of recurrent thrombosis), full therapeutic anticoagulation with LMWH or adjusted-dose unfractionated heparin should be maintained throughout pregnancy, as described above.

Which other women should receive prophylactic anticoagulation is a topic of ongoing debate and controversy.

How great is the risk of recurrent thromboembolism?

A small observational study59 examined the risk of recurrent venous thromboembolism during subsequent pregnancies in women with a prior thrombotic event. Anticoagulation was withheld during the antepartum period and restarted briefly after delivery. Among the 125 women enrolled, recurrent venous thromboembolism occurred in 4.8%, with half of the events occurring during the antepartum period. Among those with underlying thrombophilia, the rate of recurrent venous thromboembolism was 13% (95% confidence interval [CI] 1.7%–40.5%) to 20% (95% CI 2.5%–56.5%), and those with a prior idiopathic clot without thrombophilia had an event rate of 7.7% (95% CI 0.01%–25.1%). The subgroup with a prior reversible risk factor (at the time of their initial venous thromboembolic event) and without detectable thrombophilia had no recurrent events.

This study suggests that women with prior venous thromboembolism and thrombophilia or a prior idiopathic thrombotic event are at a substantial risk of recurrent thrombotic events during pregnancy. And other data confirm the high risk of recurrent venous thromboembolism in thrombophilic pregnant women.60 These women should all be offered active antepartum and postpartum thromboprophylaxis with LMWH or unfractionated heparin (Tables 2 and 4). Women without thrombophilia but with a history of venous thromboembolism related to pregnancy or oral contraceptive use also have a substantial risk of recurrent venous thrombosis and should be offered antepartum and postpartum thromboprophylaxis.61 In contrast, women with a prior “secondary” clot, no thrombophilia, and no additional current risk factors (Table 1) appear to be at low risk of recurrent venous thromboembolism.

The risks should be discussed with these women, with an option for close clinical surveillance during pregnancy (Table 4), but with a low threshold to investigate any worrisome symptoms. Such women may also elect to take LMWH or unfractionated heparin during pregnancy.

 

 

Which heparin to use?

Prophylactic anticoagulation during pregnancy can be with either LMWH or unfractionated heparin. For most women this involves “prophylactic” dosing with the goal of maintaining a mid-interval anti-factor-Xa activity level of approximately 0.05 to 0.2 U/mL. Thromboprophylaxis with LMWH can be with lower, fixed, once-daily doses throughout pregnancy20 (Table 2), although some clinicians still prefer twice-daily dosing. The heparin should be started as soon as pregnancy is confirmed, as the pregnancy-associated increase in thrombotic risk begins by the middle of the first trimester.

To maintain effective prophylactic levels, the dose of unfractionated heparin should be increased sequentially over the trimesters62,63: approximately 5,000 units subcutaneously twice daily in the first trimester, then 7,500 units twice daily in the second trimester, and 10,000 units twice daily in the third trimester for a woman of average size.

When to add low-dose aspirin

Women with antiphospholipid antibodies, particularly those with prior recurrent pregnancy loss or fetal demise, should receive aspirin 81 mg/day in addition to heparin.39 The aspirin may be started prior to conception or when pregnancy is confirmed.

Other measures

Women on anticoagulant therapy who are at risk of recurrent venous thromboembolism should be encouraged to wear elastic compression stockings. Intermittent pneumatic compression of the legs via automated devices may be considered for women hospitalized for any reason or on bedrest.

Whichever measures are used, a high index of suspicion and a low threshold for investigating for recurrent thrombosis should be maintained throughout pregnancy and the puerperium.

PERIPARTUM AND POSTPARTUM MANAGEMENT OF ANTICOAGULATION

Heparin therapy must be interrupted temporarily during the immediate peripartum interval to minimize the risk of hemorrhage and to allow for the option of regional anesthesia. As mentioned earlier, because of the theoretical risk of paraspinal hemorrhage in women receiving heparin who undergo epidural or spinal anesthesia, the American Society of Regional Anesthesia guidelines advise waiting to insert the needle at least 10 to 12 hours after the last prophylactic dose of LMWH, and at least 24 hours after the last therapeutic dose.31

The guidelines state that neuraxial anesthesia is not contraindicated in patients on prophylactic unfractionated heparin.31

To facilitate use of regional anesthesia in these women, therefore, options include:

  • Electively stopping LMWH 24 hours before planned induction of labor
  • Electively stopping prophylactic-dose LMWH or unfractionated heparin at about 38 weeks of gestation, to await spontaneous labor, or
  • Switching therapeutic or prophylactic LMWH to unfractionated heparin at about 36 weeks of gestation, with instructions to discontinue the injections in the earliest stages of spontaneous labor. This aims to shorten the heparin-free period required before neuraxial anesthesia while minimizing maternal thrombotic risk.

Additional advantages to using unfractionated heparin peripartum include the option of obtaining a rapid aPTT measurement to confirm the absence of a significant ongoing heparin effect prior to regional anesthesia or delivery, and the ability to completely reverse the heparin effect with protamine sulfate if major bleeding occurs. LMWHs are only partially reversible.64

Interrupting anticoagulation after an initial thrombotic event

If therapeutic anticoagulation must be interrupted for labor within 1 month of the initial thrombotic event, the risk of recurrent thrombotic complications is high65; these women must be observed very carefully and may benefit from intravenous heparin before and after delivery. They may even merit placement of a temporary vena cava filter (particularly if less than 2 weeks have elapsed since the venous thromboembolic event and in women with a large deep venous clot burden), a procedure that has been used safely but little studied in pregnant women.66

Fluoroscopic guidance may be needed for filter placement. This exposes the fetus to radiation, but the low-level exposure at this late gestational age is unlikely to pose a significant risk. The filter may be removed within 1 to 2 weeks postpartum, assuming there are no ongoing contraindications to anticoagulation.

In the rare woman with antithrombin deficiency and a recent or prior thrombotic event, giving antithrombin concentrate during the peripartum (heparin-free) interval has been described and may be considered under the guidance of a hematologist.67

Ongoing anticoagulation is essential postpartum, as the puerperium is the period of highest day-to-day risk of thromboembolic events: about one-third of pregnancy-associated events occur during these 6 to 12 weeks.2 Heparin should be resumed 6 to 12 hours after delivery, once hemostasis is confirmed.

Options for women requiring ongoing therapeutic anticoagulation include intravenous heparin started without a bolus, to minimize bleeding risk, with aPTT measured 12 hours later, or an initial prophylactic dose of LMWH 6 to 12 hours postpartum, with therapeutic dosing resumed on postpartum day 1. If prophylactic dosing is desired, unfractionated heparin or LMWH may be given subcutaneously starting at about 6 hours postpartum.

Warfarin in the puerperium

Women may subsequently be maintained on either LMWH or unfractionated heparin, or switched to an oral anticoagulant such as warfarin. Although warfarin may appear in minute amounts in breast milk, it has not been associated with adverse events in newborns and is considered compatible with breastfeeding.68 Heparin should be continued during the initial days of warfarin therapy, until the INR is at a therapeutic level for 24 hours. Some physicians prefer to delay warfarin for several days, giving LMWH alone in the immediate postpartum period, to allow wound-healing and to reduce bleeding risk.

Postpartum, anticoagulation should be continued for at least 6 to 12 weeks, at which point the physiologic changes in the coagulation system related to pregnancy will have returned to normal.

 

 

THROMBOPHILIA WITHOUT A PREVIOUS THROMBOEMBOLIC EVENT

Over the last 5 to 10 years, practitioners have been seeing many more young women with genetic or acquired thrombophilias who have never had a venous thromboembolic event. Physicians must advise these women about their risk of thromboembolic events during pregnancy and about the appropriateness of anticoagulant use.

Thrombophilias are often detected in women who develop venous thrombosis during pregnancy,69–71 but they are also very common in the general population (around 15%). While women with thrombophilia are at above-average risk of venous thromboembolism during pregnancy, the magnitude of risk in an individual patient is often difficult to estimate.

Data suggest that some types of thrombophilia confer greater thrombotic risk than others. McColl et al72 derived risk estimates for a primary event in women with several of the disorders: 0.23% in women heterozygous for the factor V Leiden mutation, 0.88% in women with protein C deficiency, and 2.4% to 35.7% in women with antithrombin deficiency. A case-control study70 found that all thrombophilic states were more common in women with pregnancy-associated venous thromboembolism than in healthy pregnant controls, except those with the MTHFR mutation and protein S deficiency. The estimated risk during pregnancy was 0.03% in women with no defect, 0.1% in women with protein C deficiency, 0.25% in women with the factor V Leiden mutation, 0.4% in those with antithrombin deficiency, 0.5% in those with the prothrombin gene mutation, and 4.6% in those with both factor V Leiden and prothrombin gene mutations.

Routine anticoagulation not advised in pregnant thrombophilic women

Because the risk of a primary venous thromboembolic event is less than 1% for most thrombophilic women, routine anticoagulant therapy does not seem prudent for this indication. Given the low absolute risk of venous thromboembolism, the cost and potential side effects of anticoagulant use are difficult to justify.

The women who seem at higher risk and in whom anticoagulation should be considered include those with antithrombin deficiency; those with high-titer anticardiolipin antibodies or a lupus anticoagulant antibody (treat with heparin and low-dose aspirin); those with combined thrombophilic defects or who are homozygotes for the factor V Leiden or prothrombin gene mutations; and those with multiple other current risk factors for venous thromboembolism (Table 1).

Since anticoagulants for primary prevention of adverse pregnancy outcomes in thrombophilic women have not yet been shown to have a definitive benefit, they are not recommended for this purpose.

ADVERSE PREGNANCY OUTCOMES IN WOMEN WITH THROMBOPHILIAS

Women with antiphospholipid antibodies and a previous poor obstetric outcome are clearly at increased risk of recurrent adverse pregnancy outcomes such as recurrent spontaneous abortion, unexplained fetal death, placental insufficiency, and early or severe preeclampsia. In such women who have both antiphospholipid antibodies and a history of venous thromboembolism or adverse pregnancy outcome, treatment during subsequent pregnancy with low-dose aspirin and prophylactic-dose LMWH or unfractionated heparin improves pregnancy outcomes.36–42 Women with antiphospholipid antibodies without previous thrombosis or pregnancy complications may also be at increased risk, but it is unclear whether thromboprophylaxis improves their outcomes.

Recent epidemiologic data reveal that women with other thrombophilic conditions also are at increased risk of early, severe preeclampsia73 as well as other pregnancy complications, including recurrent pregnancy loss, placental abruption, fetal growth restriction, and stillbirth.74 A recent meta-analysis75 looked at individual thrombophilias and found that factor V Leiden and prothrombin gene mutations were associated with recurrent fetal loss, stillbirth, and preeclampsia; that protein S deficiency was associated with recurrent fetal loss and stillbirth; that antiphospholipid antibodies were associated with recurrent pregnancy loss, preeclampsia, and intrauterine growth restriction; that the MTHFR mutation (homozygous) was associated with preeclampsia; and that protein C and antithrombin deficiencies were not significantly associated with adverse pregnancy outcomes. Data were scant for some of the rarer thrombophilias.75

Several recent small studies76–78 suggest that anticoagulants may improve pregnancy outcomes in women with genetic thrombophilias and recurrent pregnancy loss. These findings have not yet been confirmed in high-quality clinical trials, but such trials are under way. It is still unclear whether anticoagulants also reduce the risk of other adverse pregnancy outcomes associated with thrombophilias.

The current American College of Chest Physicians guidelines recommend testing of women with adverse pregnancy outcomes (recurrent pregnancy loss, prior severe or recurrent preeclampsia, abruptions, or otherwise unexplained intrauterine death) for congenital thrombophilias and antiphospholipid antibodies, and offering treatment to such women, if thrombophilic, with low-dose aspirin plus prophylactic heparin (unfractionated or LMWH).22 The authors of the guidelines admit that the evidence for this recommendation is weak, but they argue that the heparin will also serve as thromboprophylaxis in this high-risk group. Hopefully, the randomized clinical trials currently under way will provide clearer guidance regarding the most appropriate therapy in this difficult clinical situation.

MECHANICAL HEART VALVES

Internists may occasionally encounter a woman with a mechanical heart valve prosthesis who is either pregnant or is planning a pregnancy and therefore needs advice regarding optimal anticoagulant management. This should generally be undertaken in a multi-disciplinary fashion, with input from cardiology, hematology, and maternal-fetal medicine. The substantial maternal and fetal risks and the lack of definitive data on which to base treatment decisions make it a treacherous and stressful undertaking. Nonetheless, all internists should have a basic understanding of the complex issues regarding this management.

Outside of pregnancy, oral anticoagulants are the mainstay of therapy for patients with mechanical heart valves. Unfortunately, as discussed above, the use of these agents during pregnancy carries a risk of teratogenicity and toxic fetal effects and increases the risk of pregnancy loss and maternal hemorrhage. Heparins have been used in this setting for many years, but data on their efficacy and safety are very limited, and there are numerous reports of catastrophic maternal thrombotic complications.79,80

A systematic review of anticoagulation in pregnant women with prosthetic heart valves34 found very limited data on heparin use throughout pregnancy. Women maintained on warfarin vs heparin between pregnancy weeks 6 and 12 had higher rates of congenital anomalies (6.4% with warfarin vs 3.4% with heparin) and total fetal wastage (33.6% vs 26.5%). The warfarin group had fewer maternal thromboembolic complications (3.9% vs 9.2%), however, and a slightly lower rate of maternal death (1.8% vs 4.2%). Most of the women had higher-risk older-generation valves in the mitral position.

Recent data on LMWH consist mainly of case reports and case series,81 with a likely bias to publication of worse outcomes. Controlled trials in this area will be difficult to conduct. Still, aggressive anticoagulation with LMWH or unfractionated heparin, with close monitoring of the intensity of anticoagulation, may be safe and effective for pregnant women with newer-generation mechanical heart valves.82 A recent consensus statement22 suggested several regimens for pregnant women with mechanical heart valves:

  • Twice-daily LMWH throughout pregnancy, with the dose adjusted either by weight, or to keep the 4-hour postinjection anti-factor-Xa activity level around 1.0 to 1.2 U/mL
  • Aggressive adjusted-dose unfractionated heparin throughout pregnancy, given subcutaneously every 12 hours and adjusted to keep the mid-interval aPTT at least twice the control value or to attain a mid-interval anti-factor-Xa activity level of 0.35 to 0.70 U/mL
  • Unfractionated heparin or LMWH (as above) until gestation week 13, then warfarin until the middle of the third trimester, and then heparin again.22

The authors also recommended adding low-dose aspirin (75–162 mg/day) in high-risk women.22

These options all seem reasonable, given our current knowledge, though warfarin use during pregnancy should be restricted to very-high-risk situations, such as women with older-generation mitral prostheses. LM-WHs may become the preferred therapy for this indication once further controlled data regarding their efficacy and safety become available.

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  3. Health Canada. Special Report on Maternal Mortality and Severe Morbidity in Canada—Enhanced Surveillance: The Path to Prevention. Ottawa: Minister of Public Works and Government Services Canada, 2004. www.phac-aspc.gc.ca/rhs-ssg/srmm-rsmm/page1-eng.php. Accessed 11/26/2008.
  4. Stein PD, Hull RD, Kayali F, et al. Venous thromboembolism in pregnancy: 21-year trends. Am J Med 2004; 117:121125.
  5. Greer IA. Thrombosis in pregnancy: maternal and fetal issues. Lancet 1999; 353:12581265.
  6. Rosendaal FR. Venous thrombosis: a multicausal disease. Lancet 1999; 353:11671173.
  7. Gherman RB, Goodwin TM, Leung B, et al. Incidence, clinical characteristics, and timing of objectively diagnosed venous thromboembolism during pregnancy. Obstet Gynecol 1999; 94:730734.
  8. Weitz JI. Low-molecular-weight heparins. N Engl J Med 1997; 337:688698.
  9. Levine M, Gent M, Hirsh J, et al. A comparison of low-molecular-weight heparin administered primarily at home with unfractionated heparin administered in the hospital for proximal deep-vein thrombosis. N Engl J Med 1996; 334:677681.
  10. Koopman MM, Prandoni P, Piovella F, et al. Treatment of venous thrombosis with intravenous unfractionated heparin administered in the hospital as compared with subcutaneous low-molecular-weight heparin administered at home. The Tasman Study Group. N Engl J Med 1996; 334:682687.
  11. Simonneau G, Sors H, Charbonnier B, et al. A comparison of low-molecular-weight heparin with unfractionated heparin for acute pulmonary embolism. The THESEE Study Group. Tinzaparine ou Heparine Standard: Evaluations dans l’Embolie Pulmonaire. N Engl J Med 1997; 337:663669.
  12. Hull RD, Raskob GE, Brant RF, et al. Low-molecular-weight heparin vs heparin in the treatment of patients with pulmonary embolism. American-Canadian Thrombosis Study Group. Arch Intern Med 2000; 160:229236.
  13. Sanson BJ, Lensing AW, Prins MH, et al. Safety of low-molecular-weight heparin in pregnancy: a systematic review. Thromb Haemost 1999; 81:668672.
  14. Greer IA, Nelson-Piercy C. Low-molecular-weight heparins for thromboprophylaxis and treatment of venous thromboembolism in pregnancy: a systematic review of safety and efficacy. Blood 2005; 106:401407.
  15. Melissari E, Parker CJ, Wilson NV, et al. Use of low molecular weight heparin in pregnancy. Thromb Haemost 1992; 68:652656.
  16. Forestier F, Daffos F, Capella-Pavlovsky M. Low molecular weight heparin (PK 10169) does not cross the placenta during the second trimester of pregnancy study by direct fetal blood sampling under ultrasound. Thromb Res 1984; 34:557560.
  17. Forestier F, Daffos F, Rainaut M, Toulemonde F. Low molecular weight heparin (CY 216) does not cross the placenta during the third trimester of pregnancy. Thromb Haemost 1987; 57:234.
  18. Barbour LA, Oja JL, Schultz LK. A prospective trial that demonstrates that dalteparin requirements increase in pregnancy to maintain therapeutic levels of anticoagulation. Am J Obstet Gynecol 2004; 191:10241029.
  19. Smith MP, Norris LA, Steer PJ, Savidge GF, Bonnar J. Tinzaparin sodium for thrombosis treatment and prevention during pregnancy. Am J Obstet Gynecol 2004; 190:495501.
  20. Ellison J, Walker ID, Greer IA. Antenatal use of enoxaparin for prevention and treatment of thromboembolism in pregnancy. BJOG 2000; 107:11161121.
  21. Sarig G, Brenner B. Monitoring of low molecular weight heparin (LMWH) in pregnancy. Thromb Res 2005; 115 suppl 1:8486.
  22. Bates SM, Greer IA, Hirsh J, Ginsberg JS. Use of antithrombotic agents during pregnancy: the seventh ACCP conference on antithrombotic and thrombolytic therapy. Chest 2004; 126 suppl 3:627S644S.
  23. Warkentin TE, Levine MN, Hirsh J, et al. Heparin-induced thrombocytopenia in patients treated with low-molecular-weight heparin or unfractionated heparin. N Engl J Med 1995; 332:13301335.
  24. Hassell K. The management of patients with heparin-induced thrombocytopenia who require anticoagulant therapy. Chest 2005; 127 suppl 2:1S8S.
  25. Barbour LA, Kick SD, Steiner JF, et al. A prospective study of heparin-induced osteoporosis in pregnancy using bone densitometry. Am J Obst Gynecol 1994; 170:862869.
  26. Douketis JD, Ginsberg JS, Burrows RF, Duku EK, Webber CE, Brill-Edwards P. The effects of long-term heparin therapy during pregnancy on bone density. A prospective matched cohort study. Thromb Haemost 1996; 75:254257.
  27. Pettila V, Leinonen P, Markkola A, Hiilesmaa V, Kaaja R. Postpartum bone mineral density in women treated for thromboprophylaxis with unfractionated heparin or LMW heparin. Thromb Haemost 2002; 87:182186.
  28. Carlin AJ, Farquharson RG, Quenby SM, Topping J, Fraser WD. Prospective observational study of bone mineral density during pregnancy: low molecular weight heparin versus control. Hum Reprod 2004; 19:12111214.
  29. Casele HL, Laifer SA. Prospective evaluation of bone density in pregnant women receiving the low molecular weight heparin enoxaparin sodium. J Matern Fetal Med 2000; 9:122125.
  30. Casele H, Haney EI, James A, Rosene-Montella K, Carson M. Bone density changes in women who receive thromboprophylaxis in pregnancy. Am J Obstet Gynecol 2006; 195:11091113.
  31. Horlocker TT, Wedel DJ, Benzon H, et al. Regional anesthesia in the anticoagulated patient: defining the risks (the second ASRA Consensus Conference on Neuraxial Anesthesia and Anticoagulation). Reg Anesth Pain Med 2003; 28:172197.
  32. Hirsh J, Dalen JE, Anderson DR, et al. Oral anticoagulants: mechanism of action, clinical effectiveness, and optimal therapeutic range. Chest 2001; 119 suppl 1:8S21S.
  33. Levine MN, Raskob G, Beyth RJ, Kearon C, Schulman S. Hemorrhagic complications of anticoagulant treatment: the seventh ACCP conference on antithrombotic and thrombolytic therapy. Chest 2004; 126 suppl 3:287S310S.
  34. Holmes LB. Teratogen-induced limb defects. Am J Med Genet 2002; 112:297303.
  35. Chan WS, Anand S, Ginsberg JS. Anticoagulation of pregnant women with mechanical heart valves: a systematic review of the literature. Arch Intern Med 2000; 160:191196.
  36. Pauzner R, Dulitzki M, Langevitz P, Livneh A, Kenett R, Many A. Low molecular weight heparin and warfarin in the treatment of patients with antiphospholipid syndrome during pregnancy. Thromb Haemost 2001; 86:13791384.
  37. Pulmonary Embolism Prevention (PEP) Trial Collaborative Group. Prevention of pulmonary embolism and deep vein thrombosis with low dose aspirin: Pulmonary Embolism Prevention (PEP) trial. Lancet 2000; 355:12951302.
  38. Patrono C, Coller B, FitzGerald GA, Hirsh J, Roth G. Platelet-active drugs: the relationships among dose, effectiveness, and side effects: the Seventh ACCP Conference on Antithrombotic and Thrombolytic Therapy. Chest 2004; 126 suppl 3:234S264S.
  39. Duley L, Henderson-Smart DJ, Knight M, King JF. Antiplatelet agents for preventing preeclampsia and its complications. Cochrane Database Syst Rev. 2004; ( 1):CD004659.
  40. Coomarasamy A, Honest H, Papaioannou S, Gee H, Khan KS. Aspirin for prevention of preeclampsia in women with historical risk factors: a systematic review. Obstet Gynecol 2003; 101:13191332.
  41. Caritis SN, Sibai BM, Hauth J, et al, and the National Institute of Child Health and Human Development Network of Maternal Fetal Medicine Units. Low-dose aspirin to prevent preeclampsia in women at high risk. N Engl J Med 1998; 338:701705.
  42. Rai R, Cohen H, Dave M, Regan L. Randomised controlled trial of aspirin and aspirin plus heparin in pregnant women with recurrent miscarriage associated with phospholipid antibodies (or antiphospholipid antibodies). BMJ 1997; 314:253257.
  43. Kozer E, Nikfar S, Costei A, Boskovic R, Nulman I, Koren G. Aspirin consumption during the first trimester of pregnancy and congenital anomalies: a meta-analysis. Am J Obstet Gynecol 2002; 187:16231630.
  44. Sebastian C, Scherlag M, Kugelmass A, Schechter E. Primary stent implantation for acute myocardial infarction during pregnancy: use of abciximab, ticlopidine, and aspirin. Cathet Cardiovasc Diagn 1998; 45:275249.
  45. Wilson AM, Boyle AJ, Fox P. Management of ischaemic heart disease in women of child-bearing age. Intern Med J 2004; 34:694697.
  46. Klinzing P, Markert UR, Liesaus K, Peiker G. Case report: successful pregnancy and delivery after myocardial infarction and essential thrombocythemia treated with clopidogrel. Clin Exp Obstet Gynecol 2001; 28:215216.
  47. Danhof M, de Boer A, Magnani HN, Stiekema JC. Pharmacokinetic considerations on Orgaran (Org 10172) therapy. Haemostasis 1992; 22:7384.
  48. Tardy-Poncet B, Tardy B, Reynaud J, et al. Efficacy and safety of danaparoid sodium (ORG 10172) in critically ill patients with heparin-associated thrombocytopenia. Chest 1999; 115:16161620.
  49. Lagrange F, Vergnes C, Brun JL, et al. Absence of placental transfer of pentasaccharide (fondaparinux, Arixtra) in the dually perfused human cotyledon in vitro. Thromb Haemost 2002; 87:831835.
  50. Dempfle CE. Minor transplacental passge of fondapinux in vivo. N Engl J Med 2004; 350:1914.
  51. Magnani HN. Heparin-induced thrombocytopenia (HIT): an overview of 230 patients treated with orgaran (Org 10172). Thromb Haemost 1993; 70:554561.
  52. Lindhoff-Last E, Kreutzenbeck HJ, Magnani HN. Treatment of 51 pregnancies with danaparoid because of heparin intolerance. Thromb Haemost 2005; 93:6369.
  53. Greinacher A, Eckhardt T, Mussmann J, Mueller-Eckhardt C. Pregnancy complicated by heparin associated thrombocytopenia: management by a prospectively in vitro selected heparinoid (Org 10172). Thromb Res 1993; 71:123126.
  54. Schindewolf M, Mosch G, Bauersachs RM, Lindhoff-Last E. Safe anticoagulation with danaparoid in pregnancy and lactation. Thromb Haemost 2004; 92:211.
  55. Harenberg J. Treatment of a woman with lupus and thromboembolism and cutaneous intolerance to heparins using fondaparinux during pregnancy. Thromb Res 2007; 119:385388.
  56. Wijesiriwardana A, Lees DA, Lush C. Fondaparinux as anticoagulant in a pregnant woman with heparin allergy. Blood Coagul Fibrinolysis 2006; 17:147149.
  57. Mazzolai L, Hohlfeld P, Spertini F, Hayoz D, Schapira M, Duchosal MA. Fondaparinux is a safe alternative in case of heparin intolerance during pregnancy. Blood 2006; 108:15691570.
  58. Hawkins D, Evans J. Minimizing the risk of heparin-induced osteoporosis during pregnancy. Expert Opin Drug Saf 2005; 4:583590.
  59. Brill-Edwards P, Ginsberg JS, Gent M, et al. Safety of withholding heparin in pregnant women with a history of venous thromboembolism. Recurrence of clot in this pregnancy study group. N Engl J Med 2000; 343:14391444.
  60. Martinelli I, Legnani C, Bucciarelli P, Grandone E, De Stefano V, Mannucci PM. Risk of pregnancy-related venous thrombosis in carriers of severe inherited thrombophilia. Thromb Haemost 2001; 86:800803.
  61. De Stefano V, Martinelli I, Rossi E, Battaglioli T, Za T, Mannucci PM, Leone G. The risk of recurrent venous thromboembolism in pregnancy and puerperium without antithrombotic prophylaxis. Br J Haematol 2006; 135:386391.
  62. Barbour LA, Smith JM, Marlar RA. Heparin levels to guide thromboembolism prophylaxis during pregnancy. Am J Obstet Gynecol 1995; 173:18691873.
  63. Ensom MH, Stephenson MD. Pharmacokinetics of low molecular weight heparin and unfractionated heparin in pregnancy. J Soc Gynecol Investig 2004; 11:377383.
  64. Crowther MA, Berry LR, Monagle PT, Chan AK. Mechanisms responsible for the failure of protamine to inactivate low-molecular-weight heparin. Br J Haematol 2002; 116:178186.
  65. Kearon C, Hirsh J. Management of anticoagulation before and after elective surgery. N Engl J Med 1997; 336:15061511.
  66. Thomas LA, Summers RR, Cardwell MS. Use of Greenfield filters in pregnant women at risk for pulmonary embolism. South Med J 1997; 90:215217.
  67. Maclean PS, Tait RC. Hereditary and acquired antithrombin deficiency: epidemiology, pathogenesis and treatment options. Drugs 2007; 67:14291440.
  68. Information from LactMed: http://toxnet.nlm.nih.gov/cgi-bin/sis/htmlgen?LACT, LactMed Record Number: 279. Accessed 11/26/2008.
  69. Gerhardt A, Scharf RE, Beckmann MW, et al. Prothrombin and factor V mutations in women with a history of thrombosis during pregnancy and the puerperium. N Engl J Med 2000; 342:374380.
  70. Hirsch DR, Mikkola KM, Marks PW, et al. Pulmonary embolism and deep venous thrombosis during pregnancy or oral contraceptive use: prevalence of factor V Leiden. Am Heart J 1996; 131:11451148.
  71. Dizon-Townson DS, Nelson LM, Jang H, Varner MW, Ward K. The incidence of the factor V Leiden mutation in an obstetric population and its relationship to deep vein thrombosis. Am J Obstet Gynecol 1997; 176:883886.
  72. McColl MD, Ramsay JE, Tait RC, et al. Risk factors for pregnancy associated venous thromboembolism. Thromb Haemost 1997; 78:11831188.
  73. Kupferminc MJ, Fait G, Many A, Gordon D, Eldor A, Lessing JB. Severe preeclampsia and high frequency of genetic thrombophilic mutations. Obstet Gynecol 2000; 96:4549.
  74. Kupferminc MJ, Eldor A, Steinman N, et al. Increased frequency of genetic thrombophilia in women with complications of pregnancy. N Engl J Med 1999; 340:913.
  75. Robertson L, Wu O, Langhorne P, et al. Thrombophilia in pregnancy: a systematic review. Br J Haematol 2006; 132:171196.
  76. Brenner B, Hoffman R, Blumenfeld Z, Weiner Z, Younis JS. Gestational outcome in thrombophilic women with recurrent pregnancy loss treated by enoxaparin. Thromb Haemost 2000; 83:693697.
  77. Carp H, Dolitzky M, Inbal A. Thromboprophylaxis improves the live birth rate in women with consecutive recurrent miscarriages and hereditary thrombophilia. J Thromb Haemost 2003; 1:433438.
  78. Gris JC, Mercier E, Quere I, et al. Low-molecular-weight heparin versus low-dose aspirin in women with one fetal loss and a constitutional thrombophilic disorder. Blood 2004; 103:36953699.
  79. Salazar E, Izaguirre R, Verdejo J, Mutchinick O. Failure of adjusted doses of subcutaneous heparin to prevent thromboembolic phenomena in pregnant patients with mechanical cardiac valve prostheses. J Am Coll Cardiol 1996; 27:16981703.
  80. Iturbe-Alessio I, Fonseca MC, Mutchinik O, Santos MA, Zajarias A, Salazar E. Risks of anticoagulant therapy in pregnant women with artificial heart valves. N Engl J Med 1986; 315:13901393.
  81. Rowan JA, McCowan LM, Raudkivi PJ, North RA. Enoxaparin treatment in women with mechanical heart valves during pregnancy. Am J Obstet Gynecol 2001; 185:633637.
  82. Oran B, Lee-Parritz A, Ansell J. Low molecular weight heparin for the prophylaxis of thromboembolism in women with prosthetic mechanical heart valves during pregnancy. Thromb Haemost 2004; 92:747751.
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KEY POINTS

  • Pregnancy is a hypercoagulable state. Thrombotic risk in an individual pregnancy depends on many maternal and situational factors.
  • When indicated, careful anticoagulation can proceed with minimal risk to the mother and fetus.
  • Heparins, especially LMWHs, are the main anticoagulants used in pregnancy. Dosing depends on the clinical indications and on the agent selected.
  • If anticoagulation is absolutely necessary and LMWH is contraindicated, a newer, alternative anticoagulant should be considered.
  • Warfarin should not be used in pregnancy in any but the highest-risk situations.
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An error occurred in Table 2 of the article Elgouhari HM, Abu-Rajab Tamimi, Carey W. Hepatitis B: A strategy for evaluation and management. Cleve Clin J Med 2009; 76:19–35. In the lamivudine column, the information on drug resistance, pregnancy risk category, and cost was incorrect. The corrected table is reproduced below and online. Also, the bulleted text in the first column of page 24 should read: “Chronic inactive carriers who have no e antigen, persistently normal ALT levels, and very low or undetectable levels of HBV DNA without evidence of significant liver injury.”

 

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An error occurred in Table 2 of the article Elgouhari HM, Abu-Rajab Tamimi, Carey W. Hepatitis B: A strategy for evaluation and management. Cleve Clin J Med 2009; 76:19–35. In the lamivudine column, the information on drug resistance, pregnancy risk category, and cost was incorrect. The corrected table is reproduced below and online. Also, the bulleted text in the first column of page 24 should read: “Chronic inactive carriers who have no e antigen, persistently normal ALT levels, and very low or undetectable levels of HBV DNA without evidence of significant liver injury.”

 

An error occurred in Table 2 of the article Elgouhari HM, Abu-Rajab Tamimi, Carey W. Hepatitis B: A strategy for evaluation and management. Cleve Clin J Med 2009; 76:19–35. In the lamivudine column, the information on drug resistance, pregnancy risk category, and cost was incorrect. The corrected table is reproduced below and online. Also, the bulleted text in the first column of page 24 should read: “Chronic inactive carriers who have no e antigen, persistently normal ALT levels, and very low or undetectable levels of HBV DNA without evidence of significant liver injury.”

 

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Depression and heart disease: What do we know, and where are we headed?

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Depression is a risk factor for heart disease, and in patients with heart disease, it is a risk factor for complications and death. Unfortunately, in the trials performed to date, treating depression in cardiac patients did not lead to lower rates of recurrent cardiovascular events or death. Nevertheless, we recommend that clinicians systematically screen for it in their heart patients, in view of the benefits of antidepressant therapy.

In this article we review key epidemiologic and psychosocial studies, the mechanistic links between depression and heart disease, and recent intervention trials. We also offer practical management advice and address the continued need for guidelines and risk stratification in the treatment of depressed cardiac patients.

After we submitted our review article, the American Heart Association (AHA)1 released a consensus document recommending that health care providers screen for and treat depression in patients with coronary heart disease. We will discuss the same screening tests that have been recommended by the AHA.

DEPRESSION AND HEART DISEASE: COMMON AND LINKED

Depression and heart disease are very common and often coexist: the prevalence of depression in various heart conditions ranges from 15% to 20%.1–3 According to data from the World Health Organization, by the year 2020 depression will be the second-leading cause of disability in developed countries (after heart disease).4

The World Health Survey5 showed that depression worsens health more than angina, arthritis, asthma, or diabetes. Furthermore, patients with severe mental illness have a higher risk of dying from heart disease and stroke.6

SOME HEART DISEASE RISK FACTORS ARE PSYCHOSOCIAL

In the 1980s, the “type A” personality (ambitious, aggressive, hostile, and competitive, with a chronic sense of urgency) was linked to heart disease.7 Later studies differed as to whether the entire set of features is valid as a collective risk factor for progressive heart disease,8 but hostility remains a validated risk factor and a focus of behavior modification.9,10

Other psychosocial risk factors have been implicated,11,12 one of which is social isolation.9,13 Another is the “type D” personality, which includes a tendency to experience negative emotions across time and situations coupled with social inhibition and which is believed to be more valid than the type A personality as a risk factor for cardiac disease.14,15

The INTERHEART study16 gathered data about attributable risk in the development of myocardial infarction (MI) in 52 countries in a case-control fashion. Psychosocial factors including stress, low generalized locus of control (ie, the perceived inability to control one’s life), and depression accounted for 32.5% of the attributable risk for an MI.17 This would mean that they account for slightly less attributable risk than that of lifetime smoking but more than that of hypertension and obesity.

Job stress increases the risk of initial coronary heart disease18 and also the risk of recurrent cardiac events after a first MI.19 Even though numerous psychosocial risk factors have been associated with coronary heart disease, including anxiety,20,21 depression is perhaps the best studied.

PROSPECTIVE STUDIES OF DEPRESSION AND HEART DISEASE

To examine the impact of depression in coronary heart disease, prospective studies have been done in healthy people and in patients with established cardiovascular disease who develop depression.22

In healthy people, depression increases the risk of coronary disease

The 1996 Epidemiologic Catchment Area study23 found that people with major depression had a risk of MI four times higher than the norm, and people with 2 weeks of sadness or dysphoria had a risk two times higher.

A subsequent meta-analysis of 11 studies,24 which included 36,000 patients, found that the overall relative risk of developing heart disease in depressed but healthy people was 1.64.

A meta-analysis by Van der Kooy et al25 of 28 epidemiologic studies with nearly 80,000 patients showed depression to be an independent risk factor for cardiovascular disease.

Wulsin and Singal26 performed a systematic review to see if depression increases the risk of coronary disease. In 10 studies with a follow-up of more than 4 years, the relative risk in people with depression was 1.64, which was less than that in active smokers (2.5) but more than that in passive smokers (1.25).

Depression can also exacerbate the classic risk factors for coronary disease, such as smoking, diabetes, obesity, and physical inactivity. 27

A 2007 study from Sweden28 prospectively followed patients who were hospitalized for depression. The odds ratio of developing an acute MI was 2.9, and the risk persisted for decades after the initial hospitalization.

A prospective United Kingdom cohort study of people initially free of heart disease revealed major depression to be associated with a higher rate of death from ischemic heart disease.29 Specifically, patients who had depression currently or in the past 12 months had a 2.7 times higher risk of dying than those who had never had depression or who had had it more than 12 months previously.

In existing heart disease, depression predicts recurrent events, death

Carney et el30 found that patients with major depressive disorder had a higher incidence of new cardiac events in the 12 months after undergoing cardiac catheterization than those without major depressive disorder.

Frasure-Smith et al,31 in a landmark study, showed that patients who were depressed at 1 week after an MI were three to four times more likely to die in the next 6 months than nondepressed post-MI patients. Even after 18 months, depression remained an independent risk factor for cardiac-related death.32

In longer studies (with up to 19.4 years of follow-up), depression was associated with higher rates of death from cardiac and all causes in patients with coronary artery disease.33 Lespérance et al34 found that in MI patients, the higher the Beck Depression Inventory score at the time of hospital admission, the higher the 5-year death rate.

Using meta-analysis, Barth et al35 found the risk of dying in the first 2 years after initial assessment to be twice as high in depressed cardiac patients as in nondepressed cardiac patients (odds ratio 2.24).

Van Melle et al36 reviewed 22 studies and found that in the 2 years after an MI, depressed patients had a 2 to 2.5 times higher risk of dying of a cardiac or any other cause than did nondepressed patients.

Depression also predicts higher morbidity and mortality rates in patients undergoing coronary artery bypass grafting,37,38 patients with congestive heart failure,39 and heart transplant recipients.40

 

 

MEDICAL ILLNESS CAN PREDISPOSE TO DEPRESSION, AND VICE VERSA

Medical illnesses can predispose a patient to develop depression. Specifically, compared with healthy people, cardiac patients appear to be at greater risk of developing depression for many years after the initial medical diagnosis is made.41

Katon et al42 reviewed 31 studies involving 16,922 patients, that assessed the impact of depression and anxiety in chronic medical illnesses such as heart disease, diabetes, pulmonary disease, and arthritis. After the severity of the medical disorder was controlled for, patients with depression and anxiety reported a higher number of medical symptoms.

DEPRESSION WORSENS QUALITY OF LIFE AND ADHERENCE TO TREATMENT

Depressed patients perceive their health status and quality of life negatively. In the Heart and Soul study,43 depressive symptoms and low exercise capacity—but not low ejection fraction or ischemia—were significantly associated with perceived deterioration of health in patients with coronary artery disease.

After an MI, patients who take their cardiac drugs properly have a better chance of survival.44,45 Clinical depression can worsen compliance with cardiac medication regimens,46 and reducing depression increases medication adherence overall.47 Not surprisingly, depressed patients also adhere less well to other recommendations,48 including modifying the diet, exercising, stopping smoking, and attending cardiac rehabilitation programs. 49

PLAUSIBLE MECHANISMS LINK DEPRESSION AND HEART DISEASE

Traditional cardiac risk factors such as smoking, high cholesterol, hypertension, diabetes, and obesity tend to cluster in depressed patients. 50 Other mechanisms linking depression and heart disease are reviewed below.51,52

Autonomic imbalance

Excessive sympathetic stimulation or diminished vagal stimulation or both are associated with higher rates of morbidity and death.53

Lack of variability in the heart rate reflects a sympathetic-vagal imbalance and is a risk factor for ventricular arrhythmias and sudden cardiac death in patients with cardiovascular disease.54 Carney et al55 reported that patients with coronary artery disease and depression had significantly less heart rate variability than nondepressed cardiac patients. Similarly, after an MI, depressed patients had significantly less heart rate variability than nondepressed patients,56 implying that low heart rate variability may mediate the adverse effect of depression on survival after an MI.57

In the Heart and Soul study, Gehi et al58 found no distinct relationship between heart rate variability and depression. However, in the same study, de Jong et al59 did find specific somatic symptoms of depression to be associated with lower heart rate variability, although cognitive symptoms were not.

Platelet activation, endothelial dysfunction

Depressed patients have been found to have exaggerated platelet reactivity.60 Plasma levels of platelet factor IV and beta-thromboglobulin, markers of platelet activation, are higher in depressed patients with ischemic heart disease than in nondepressed patients with ischemic heart disease and in control patients.61 This activation of platelets can lead to vascular damage and thrombosis.

In a subset study of the Sertraline Anti-Depressant Heart Attack Randomized Trial (SADHART), depressed MI patients were treated with sertraline (Zoloft), a selective serotonin reuptake inhibitor (SSRI), and had substantially less platelet and endothelial biomarker release.62

Depressed cardiac patients also have impaired flow-mediated dilation of the brachial artery, a sign of endothelial dysfunction.63 Although a recent study did not find coronary endothelial dysfunction in depressed patients who did not have cardiac disease, these patients had more clustering of other cardiac risk factors.64

Hypothalamic-pituitary-adrenocortical and sympathetic adrenal medullary activation

High cortisol levels can accelerate the development of hypertension and atherosclerosis and result in endothelial vascular injury. Sympathoadrenal activation in turn can lead to higher levels of catecholamines, predisposing to vasoconstriction, a rapid heart rate, and platelet activation. Depressed patients have more activation of the hypothalamic-pituitary-adrenocortical and sympathetic adrenal medullary systems,51,65 yet another plausible mechanism for worse clinical outcomes in depressed cardiac patients.

Sudden emotional stress can cause transient left ventricular dysfunction, even in people without coronary disease, an effect that may be mediated by elevated plasma catecholamine levels.66

Inflammatory cytokines

Inflammatory cytokines play a key role in the development of atherosclerosis.67 C-reactive protein, an acute-phase reactant produced in hepatocytes, can be induced by cytokines such as interleukin 6. Damage to endothelial tissues leads to the release of inflammatory cytokines, including interleukin 1, interleukin 6, and tumor tumor necrosis factor alpha.

Depressed patients have higher levels of these inflammatory markers.68,69 A prospective study reported direct correlations between depression scores and C-reactive protein levels in post-MI patients.70 The Heart and Soul study, however, did not confirm that coronary patients have more inflammation if they have depression,71 indicating that the relationship is complex and is perhaps more evident in specific types of depression.72

Anticholinergic inflammatory pathway

Tracey73 proposed a theory that vagal tone inhibits the release of inflammatory cytokines. This has important implications for treatment, as exercise, biofeedback, and meditation can stimulate the vagus nerve and therefore have beneficial anti-inflammatory effects.74

Polymorphism in the serotonin transport promoter region gene

Research is focusing on the serotonin transport promoter region gene (5-HTTLPR).75 The gene exists in two forms, a long one and a less-effective short one that appears to predispose to depression.76

Nakatani et al77 showed that MI patients were more likely to become depressed and to have subsequent cardiac events if one or both of their alleles of this gene were short. Otte et al,78 using Heart and Soul study data, found that patients with a short allele had a higher likelihood of depression, higher perceived levels of stress, and higher urinary norepinephrine secretion. However, the long allele genotype may be associated with a higher risk of developing an MI.79

Our knowledge of the genetic interplay of depression and cardiovascular disease is still in its infancy, and further studies are needed to clarify these findings.

 

 

IN TRIALS, LESS DEPRESSION BUT NO EFFECT ON DEATHS, RECURRENT MI

Major behavioral and drug trials conducted in the last 15 years have focused on how to best treat depression in cardiac patients.80–85

The Montreal Heart Attack Readjustment Trial (MHART)81 used telephone calls and home nursing visits to explore and monitor psychological distress for up to 1 year after an MI. The overall trial did not show these interventions to have any impact on survival compared with usual care. In fact, in women receiving the telephone intervention, there was a trend toward higher rates of cardiac and all-cause death, which was quite unexpected. Uncovering stresses and problems without resolving them, rather than encouraging patients to place these on the “back burner,” may partially explain these results.

SADHART82 studied the safety of sertraline in depressed post-MI patients. No major differences in cardiac function were noted between the sertraline and placebo groups, showing that sertraline was safe for these patients. The sertraline group had fewer cardiovascular events, but the difference was not statistically significant.

The Enhancing Recovery in Coronary Heart Disease (ENRICHD) study83 was primarily designed to see whether a psychosocial intervention would decrease deaths in depressed cardiac patients. Much to the chagrin of behavioral medicine, the group undergoing cognitive behavioral therapy did not have a higher rate of event-free survival, although the intervention had a favorable impact on depression and social support.

The Myocardial Infarction Depression Intervention Trial (MIND-IT)84 looked at whether the antidepressant mirtazapine (Remeron) would improve long-term depression and cardiovascular outcomes in depressed post-MI patients. In 18 months of follow-up, neither objective was obtained.

The Cardiac Randomized Evaluation of Antidepressant and Psychotherapy Efficacy (CREATE) trial85 tested the efficacy of the SSRI citalopram (Celexa) and interpersonal therapy in a short-term intervention. Here, the antidepressant was superior to placebo in the primary outcome of treating depression, but interpersonal therapy had no advantage over “clinical management,” ie, a shorter, 20-minute supportive intervention.

Common threads in these studies.

  • In ENRICHD and MIND-IT, patients whose depression did not respond to treatment were at higher risk of cardiac events during follow-up.86–88
  • In SADHART and CREATE, which used drug treatment, the antidepressant response was more robust in patients with a history of depression before their heart attacks, suggesting that a patient with recurrent depression at the time of a cardiac event should receive medication for it.85,89

CLINICAL RECOMMENDATIONS

Use a depression screening tool

Ziegelstein et al90 recently studied the ability of clinical personnel to detect depression in hospitalized MI patients. If a screening tool was not used, the results were abysmal, indicating the need to use formal screening for symptoms of depression in acute MI patients.

Many self-rating scales are available, among which are the Beck Depression Inventory (BDI) and the Hospital Anxiety and Depression Scale (HADS). Others are:

The Patient Health Questionnaire (PHQ-9) is a nine-item tool, easy to administer and score (Table 1). It has been well studied in both screening for and follow-up of depression in primary care.91,92 It was used in the Heart and Soul study and the Prospective Registry Evaluating Outcomes After Myocardial Infarction: Events and Recovery (PREMIER) study.3 It has also been used to identify and document depressive symptoms in patients with acute coronary syndrome.94 A cut-off score of 10 or higher on the PHQ-9 is diagnostic of depression.95

The PHQ-2 consists of the two first questions of the PHQ-9, which deal with mood and lack of pleasure. A cut-off score of 3 or higher has a sensitivity of 83% and a specificity of 92%,96 fulfilling the need for a quick and reliable depression screening tool. The clinician can also ask for a yes-or-no answer to the two questions of the PHQ-2 (Table 1). A yes to either of the two questions is up to 90% sensitive and 75% specific.92,97

When to suspect depression in cardiac patients

Cardiac patients may not realize they have the classic symptoms of depression, since they often ascribe somatic symptoms to their heart disease and overlook emotional associations. Lespérance and colleagues98 suggest that certain clues should make us suspect depression in cardiac patients (Table 2).

Which type of psychotherapy is best?

The negative results of psychosocial interventions (phone calls and home visits from a nurse) in MHART and of cognitive behavioral therapy in ENRICHD raise questions about which type of psychotherapy is best for depression in heart disease. CREATE found that 50-minute weekly sessions of interpersonal psychotherapy were no more beneficial than clinical management, ie, 20-minute weekly sessions that focused on compliance with treatment and education about depression and overall management. Perhaps a type of therapy akin to “clinical management” in this study or the brief behavior-based and targeted therapy used in the Improving Mood Promoting Access to Collaborative Care Treatment (IMPACT) trials of depression in primary care99 could be designed specifically to treat depression in cardiac disease. However, it is also quite possible that treatments that focus on uncovering stresses or problems may not be timely for these patients.

Which therapy is best for women is another area of consideration. In MHART, even after 5 years of follow-up,100 women who received the psychosocial support intervention did marginally worse. In the ENRICHD study, women did not experience a benefit from cognitive behavioral therapy. Further studies must address sex differences in response to different therapies.

 

 

SSRIs seem to be better than other antidepressants for cardiac patients

Before SSRIs were available, tricyclic antidepressants were the mainstays. Subsequent analysis showed the tricyclics to have an unfavorable risk-benefit profile in cardiac patients,101 and since other types of antidepressants are available, tricyclics should be avoided altogether in cardiac patients.102

Whether the SSRIs actually decrease one’s risk of death in heart disease is still an issue of debate, but there are encouraging signs. In SADHART, the rate of death and recurrent nonfatal MI was 20% lower in the patients randomized to receive sertraline, although the difference was not statistically significant.82 In ENRICHD, patients who did not respond to cognitive behavioral treatment or had severe depression could receive sertraline or other antidepressant drugs on a nonrandomized basis, and those who did had a 42% lower incidence of death or recurrent MI.103

The SADHART and CREATE trials provide convincing evidence of the cardiac safety and antidepressant efficacy of two SSRIs (sertraline and citalopram) in depressed cardiac patients. Mirtazapine, studied in MIND-IT, was not effective in treating depression in cardiac patients, although it had a better adverse effect and safety profile than tricyclic antidepressants. 104

Clinical observations indicate that SSRIs are associated with less risk of MI than non-SSRI drugs.105,106 During hospitalization for acute coronary syndromes, patients on SSRIs had lower rates of recurrent ischemia and heart failure but higher bleeding rates than patients not taking SSRIs.107 In a retrospective study of patients undergoing coronary artery bypass grafting, those on an SSRI before surgery had higher rates of death and rehospitalization.108 Being on antidepressant medication could be interpreted as a surrogate marker of having more severe depression before surgery; this issue clearly requires further study.

Given current observations and recent data from interventional trials coupled with the safe drug-interaction profile of sertraline and citalopram, these two SSRIs are recommended for treating depression in cardiac patients. If the patient is also receiving an anticoagulant, one should monitor for bleeding, as all SSRIs are associated with a prolonged bleeding time. Monitoring for rare cases of hyponatremia and bradycardia should also be part of early follow-up.

Do cardiac drugs have psychiatric effects?

Some concerns have arisen about cardiovascular drugs causing or aggravating psychiatric conditions.

Statins were once suspected of causing clinical depression or even suicide. However, subsequent studies have not substantiated this.109,110 In fact, long-term statin use has been associated with improved psychological wellbeing. 111 Whether the favorable psychological profile is due to an improved lifestyle, a direct noncholesterol effect, or an immunomodulatory effect has yet to be determined.

Beta-blockers have been suspected of increasing depression and fatigue. Robust metaanalyses have shown no increased risk of depressive symptoms but a small increased risk of fatigue and sexual dysfunction.112 Observational trials in the first year post-MI have shown no differences between beta-blocker users and nonusers in depressive symptoms or depressive disorders.113

Statins and beta-blockers offer both immense cardiac benefit and low risk, and both may be prescribed with confidence in depressed cardiac patients.

Refer patients for cardiac rehabilitation

The American Association of Cardiovascular and Pulmonary Rehabilitation strongly recommends screening cardiac patients for depression and referring them to cardiac rehabilitation programs.114 Typical programs run 12 weeks, affording an opportunity to further listen to and assess the patient and to promote general wellness via nutrition, stress management, and exercise.

These interventions by themselves can favorably affect depression. Blumenthal and colleagues,115 in the Standard Medical Intervention and Long-Term Exercise (SMILE) study, found that exercise was as effective as drug treatment in reducing depression. In addition, stress management as a psychosocial treatment in cardiac rehabilitation can reduce death rates in cardiac patients.116

Unfortunately, many patients who are eligible for cardiac rehabilitation programs do not avail themselves of them.117

Our algorithm

Figure 2. Our algorithm for detecting and treating depression in cardiac patients.
In view of the data outlined in this review, we propose an algorithm for use in depressed cardiac patients (Figure 2), which is similar to the algorithm proposed by the AHA committee,1 but which we developed independently.

FUTURE DIRECTIONS FOR RESEARCH

Can we predict the course of depression?

We need to identify better which patients will have a spontaneous remission of their depressive symptoms after a cardiac event, which patients will linger with depression, and which patients will best respond to treatment. Risk stratification, using the psychiatric history, symptoms and severity of depression, and genetic predisposition118 might allow improved targeted therapies.

Does depression cause cardiac disease?

The link between depression and heart disease can be seen as merely an association. In the interventional trials performed to date, we have not yet seen a reduction in cardiac deaths when depression was treated, challenging any assumption of a causal relationship between depression and heart disease. The debate about association vs cause is germane to behavioral medicine,119 and the better we understand the mechanistic pathways, the better we can advise patients and treat depression comorbid with heart disease.

Behavioral medicine is currently measuring the aspects of depression associated with cardiac disease, including the spectrum of somatic (body) and affective (mood) symptoms120 and specific areas such as sympathetic arousal and early morning insomnia.121 If we can determine the depression subtype that carries a worse cardiac prognosis, we may untangle the biobehavioral links that bidirectionally bridge clinical depression and cardiac disease.

Another area of interest, emotional vitality (a positive state associated with interest, enthusiasm, excitement, and energy for living) has been shown to protect against coronary heart disease122 and holds much promise.

In the plenary lecture of the Academy of Psychosomatic Medicine in 2006, Frasure-Smith spoke of the “pleiotropism” of our antidepressant interventions on the various risk factors in depressed cardiac patients.123 We need behavioral medicine studies that elucidate these mechanisms, guiding more precise treatments as well as novel therapies. Omega-3 fatty acids, which benefit heart disease and clinical depression,124 will be used in a randomized controlled trial by Lespérance and colleagues.125 We await the results of this exciting research.

 

 

Will treating depression help in other types of heart disease?

The SADHART-CHF trial is examining whether 12 weeks of sertraline therapy is better than placebo in preventing death and improving cardiac outcomes in patients with chronic heart failure and comorbid major depressive disorder. It was to be completed in the fall of 2008. The results and experience of this study will help in designing future interventional trials to reduce the risk of depression in cardiovascular diseases.

We also await the results of a National Heart, Lung, and Blood Institute (NHLBI) trial, “Bypassing the Blues,” which is studying the treatment of depression after cardiac bypass surgery. This study should provide further insights into management of the depressed cardiac patient. Further prognostic studies in cardiac patients are also needed using the PHQ-9 and its shorter version, PHQ-2.

Current and future guidelines

For years our European colleagues have been ahead of us in recognizing depression screening and stress management as key to cardiac disease-prevention strategies.126 The NHLBI nicely outlined recommendations on the assessment and treatment of depression in cardiovascular patients.127 The just-published AHA Science Advisory should further encourage clinicians to screen and treat depression in the patient population.1 As our knowledge grows, we look forward to future evidence-based guidelines for depressed cardiac patients.

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  106. Sauer WH, Berlin JA, Kimmel SE. Effect of antidepressants and their relative affinity for the serotonin transporter on the risk of myocardial infarction. Circulation 2003; 108:3236.
  107. Ziegelstein RC, Meuchel J, Kim TJ, et al. Selective serotonin reuptake inhibitor use by patients with acute coronary syndromes. Am J Med 2007; 120:525530.
  108. Xiong GL, Jiang W, Clare R, et al. Prognosis of patients taking selective serotonin reuptake inhibitors before coronary artery bypass grafting. Am J Cardiol 2006; 98:4247.
  109. Yang C-C, Jick SS, Jick H. Lipid-lowering drugs and the risk of depression and suicidal behavior. Arch Intern Med 2003; 163:19261932.
  110. Callreus T, Agerskov Andersen U, Hallas J, Andersen M. Cardiovascular drugs and the risk of suicide: a nested case-control study. Eur J Clin Pharmacol 2007; 63:591596.
  111. Young-Xu Y, Chan KA, Liao JK, Ravid S, Blatt CM. Long-term statin use and psychological well-being. J Am Coll Cardiol 2003; 42:690697.
  112. Ko DT, Hebert PR, Coffey CS, Sedrakyan A, Curtis JP, Krumholz HM. Beta-blocker therapy and symptoms of depression, fatigue, and sexual dysfunction. JAMA 2002; 288:351357.
  113. van Melle JP, Verbeek D, van den Berg MP, Ormel J, van der Line MR, de Jonge P. Beta-blockers and depression after myocardial infarction. J Am Coll Cardiol 2006; 48:22092214.
  114. Thomas RJ, King M, Lui K, et al. AACVPR/ACC/AHA 2007 performance measures on cardiac rehabilitation for referral to and delivery of cardiac rehabilitation/secondary prevention services. J Am Coll Cardiol 2007; 50:14001433.
  115. Blumenthal JA, Babyak MA, Doraiswamy PM, et al. Exercise and pharmacotherapy in the treatment of major depressive disorder. Psychosom Med 2007; 69:587596.
  116. Linden W, Phillips MJ, Leclerc J. Psychological treatment of cardiac patients: a meta-analysis. Eur Heart J 2007; 28:29722984.
  117. Centers for Disease Control and Prevention. Receipt of outpatient cardiac rehabilitation among heart attack survivors—United States, 2005. JAMA 2008; 299:15341536.
  118. Williams RB. Treating depression after myocardial infarction: can selecting patients on the basis of genetic susceptibility improve psychiatric and medical outcomes? Am Heart J 2005; 150:617619.
  119. Schneiderman N, Williams RB. The great debate editorial, revisited. Psychosom Med 2006; 68:636638.
  120. de Jonge P, Ormel J, van den Brink RHS, et al. Symptom dimensions of depression following myocardial infarction and their relationship with somatic health status and cardiovascular prognosis. Am J Psychiatry 2006; 163:138144.
  121. Fraguas R, Iosifescu DV, Alpert J, et al. Major depressive disorder and comorbid cardiac disease: is there a depressive subtype with greater cardiovascular morbidity? Results from the STAR*D Study. Psychosomatics 2007; 48:418425.
  122. Kubzansky LD, Thurston RC. Emotional vitality and incident coronary heart disease: benefits of healthy psychological functioning. Arch Gen Psychiatry 2007; 64:13931401.
  123. Frasure-Smith N. Reflections on depression as a cardiac risk factor Academy of Psychosomatic Medicine, 53rd Annual Meeting, Tucson, Arizona, 2006.
  124. Frasure-Smith N, Lespérance F. Major depression is associated with lower omega-3 fatty acid levels in patients with recent acute coronary syndromes. Biol Psychiatry 2004; 55:891896.
  125. Lespérance F. Annual Research Award Lecture Academy of Psychosomatic Medicine, Amelia Island, Florida, 2007.
  126. Graham I, Atar D, Borch-Johnsen K, et al. European guidelines on cardiovascular disease prevention in clinical practice: executive summary. Eur Heart J 2007; 28:23752414.
  127. Davidson KW, Kupfer DJ, Bigger JT, et al. Assessment and treatment of depression in patients with cardiovascular disease: National Heart, Lung, and Blood Institute Working Group Report. Psychosom Med 2006; 68:645650.
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George Tesar, MD
Chairman, Department of Psychiatry and Psychology, Cleveland Clinic

Jianping Zhang, MD, PhD
Department of Psychiatry, Zucker Hillside Hospital, North Shore Long Island Jewish Health System, Glen Oaks, NY

Marc Penn, MD, PhD
Director, Bakken Heart-Brain Institute; Director, Cardiac Intensive Care Unit; Department of Stem Cell Biology and Regenerative Medicine; and Department of Biomedical Engineering, Cleveland Clinic

Kathleen Franco, MD
Department of Psychiatry and Psychology, Cleveland Clinic; Associate Dean, Cleveland Clinic Lerner College of Medicine of Case Western Reserve University, Cleveland, OH

Wei Jiang, MD
Associate Professor, Medicine, Psychiatry, and Behavioral Sciences, Duke University Medical Center, Durham, NC; Investigator, Sertraline AntiDepressant Heart Attack Randomized Trial (SADHART)-CHF study

Address: Leopoldo Pozuelo, MD, Department of Psychiatry and Psychology, P57, Cleveland Clinic, 9500 Euclid Avenue, Cleveland, OH 44195; e-mail [email protected]

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George Tesar, MD
Chairman, Department of Psychiatry and Psychology, Cleveland Clinic

Jianping Zhang, MD, PhD
Department of Psychiatry, Zucker Hillside Hospital, North Shore Long Island Jewish Health System, Glen Oaks, NY

Marc Penn, MD, PhD
Director, Bakken Heart-Brain Institute; Director, Cardiac Intensive Care Unit; Department of Stem Cell Biology and Regenerative Medicine; and Department of Biomedical Engineering, Cleveland Clinic

Kathleen Franco, MD
Department of Psychiatry and Psychology, Cleveland Clinic; Associate Dean, Cleveland Clinic Lerner College of Medicine of Case Western Reserve University, Cleveland, OH

Wei Jiang, MD
Associate Professor, Medicine, Psychiatry, and Behavioral Sciences, Duke University Medical Center, Durham, NC; Investigator, Sertraline AntiDepressant Heart Attack Randomized Trial (SADHART)-CHF study

Address: Leopoldo Pozuelo, MD, Department of Psychiatry and Psychology, P57, Cleveland Clinic, 9500 Euclid Avenue, Cleveland, OH 44195; e-mail [email protected]

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Section Head, Consultation Psychiatry, Department of Psychiatry and Psychology; Associate Director, Bakken Heart-Brain Institute; and Department of Cardiovascular Medicine, Cleveland Clinic

George Tesar, MD
Chairman, Department of Psychiatry and Psychology, Cleveland Clinic

Jianping Zhang, MD, PhD
Department of Psychiatry, Zucker Hillside Hospital, North Shore Long Island Jewish Health System, Glen Oaks, NY

Marc Penn, MD, PhD
Director, Bakken Heart-Brain Institute; Director, Cardiac Intensive Care Unit; Department of Stem Cell Biology and Regenerative Medicine; and Department of Biomedical Engineering, Cleveland Clinic

Kathleen Franco, MD
Department of Psychiatry and Psychology, Cleveland Clinic; Associate Dean, Cleveland Clinic Lerner College of Medicine of Case Western Reserve University, Cleveland, OH

Wei Jiang, MD
Associate Professor, Medicine, Psychiatry, and Behavioral Sciences, Duke University Medical Center, Durham, NC; Investigator, Sertraline AntiDepressant Heart Attack Randomized Trial (SADHART)-CHF study

Address: Leopoldo Pozuelo, MD, Department of Psychiatry and Psychology, P57, Cleveland Clinic, 9500 Euclid Avenue, Cleveland, OH 44195; e-mail [email protected]

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Depression is a risk factor for heart disease, and in patients with heart disease, it is a risk factor for complications and death. Unfortunately, in the trials performed to date, treating depression in cardiac patients did not lead to lower rates of recurrent cardiovascular events or death. Nevertheless, we recommend that clinicians systematically screen for it in their heart patients, in view of the benefits of antidepressant therapy.

In this article we review key epidemiologic and psychosocial studies, the mechanistic links between depression and heart disease, and recent intervention trials. We also offer practical management advice and address the continued need for guidelines and risk stratification in the treatment of depressed cardiac patients.

After we submitted our review article, the American Heart Association (AHA)1 released a consensus document recommending that health care providers screen for and treat depression in patients with coronary heart disease. We will discuss the same screening tests that have been recommended by the AHA.

DEPRESSION AND HEART DISEASE: COMMON AND LINKED

Depression and heart disease are very common and often coexist: the prevalence of depression in various heart conditions ranges from 15% to 20%.1–3 According to data from the World Health Organization, by the year 2020 depression will be the second-leading cause of disability in developed countries (after heart disease).4

The World Health Survey5 showed that depression worsens health more than angina, arthritis, asthma, or diabetes. Furthermore, patients with severe mental illness have a higher risk of dying from heart disease and stroke.6

SOME HEART DISEASE RISK FACTORS ARE PSYCHOSOCIAL

In the 1980s, the “type A” personality (ambitious, aggressive, hostile, and competitive, with a chronic sense of urgency) was linked to heart disease.7 Later studies differed as to whether the entire set of features is valid as a collective risk factor for progressive heart disease,8 but hostility remains a validated risk factor and a focus of behavior modification.9,10

Other psychosocial risk factors have been implicated,11,12 one of which is social isolation.9,13 Another is the “type D” personality, which includes a tendency to experience negative emotions across time and situations coupled with social inhibition and which is believed to be more valid than the type A personality as a risk factor for cardiac disease.14,15

The INTERHEART study16 gathered data about attributable risk in the development of myocardial infarction (MI) in 52 countries in a case-control fashion. Psychosocial factors including stress, low generalized locus of control (ie, the perceived inability to control one’s life), and depression accounted for 32.5% of the attributable risk for an MI.17 This would mean that they account for slightly less attributable risk than that of lifetime smoking but more than that of hypertension and obesity.

Job stress increases the risk of initial coronary heart disease18 and also the risk of recurrent cardiac events after a first MI.19 Even though numerous psychosocial risk factors have been associated with coronary heart disease, including anxiety,20,21 depression is perhaps the best studied.

PROSPECTIVE STUDIES OF DEPRESSION AND HEART DISEASE

To examine the impact of depression in coronary heart disease, prospective studies have been done in healthy people and in patients with established cardiovascular disease who develop depression.22

In healthy people, depression increases the risk of coronary disease

The 1996 Epidemiologic Catchment Area study23 found that people with major depression had a risk of MI four times higher than the norm, and people with 2 weeks of sadness or dysphoria had a risk two times higher.

A subsequent meta-analysis of 11 studies,24 which included 36,000 patients, found that the overall relative risk of developing heart disease in depressed but healthy people was 1.64.

A meta-analysis by Van der Kooy et al25 of 28 epidemiologic studies with nearly 80,000 patients showed depression to be an independent risk factor for cardiovascular disease.

Wulsin and Singal26 performed a systematic review to see if depression increases the risk of coronary disease. In 10 studies with a follow-up of more than 4 years, the relative risk in people with depression was 1.64, which was less than that in active smokers (2.5) but more than that in passive smokers (1.25).

Depression can also exacerbate the classic risk factors for coronary disease, such as smoking, diabetes, obesity, and physical inactivity. 27

A 2007 study from Sweden28 prospectively followed patients who were hospitalized for depression. The odds ratio of developing an acute MI was 2.9, and the risk persisted for decades after the initial hospitalization.

A prospective United Kingdom cohort study of people initially free of heart disease revealed major depression to be associated with a higher rate of death from ischemic heart disease.29 Specifically, patients who had depression currently or in the past 12 months had a 2.7 times higher risk of dying than those who had never had depression or who had had it more than 12 months previously.

In existing heart disease, depression predicts recurrent events, death

Carney et el30 found that patients with major depressive disorder had a higher incidence of new cardiac events in the 12 months after undergoing cardiac catheterization than those without major depressive disorder.

Frasure-Smith et al,31 in a landmark study, showed that patients who were depressed at 1 week after an MI were three to four times more likely to die in the next 6 months than nondepressed post-MI patients. Even after 18 months, depression remained an independent risk factor for cardiac-related death.32

In longer studies (with up to 19.4 years of follow-up), depression was associated with higher rates of death from cardiac and all causes in patients with coronary artery disease.33 Lespérance et al34 found that in MI patients, the higher the Beck Depression Inventory score at the time of hospital admission, the higher the 5-year death rate.

Using meta-analysis, Barth et al35 found the risk of dying in the first 2 years after initial assessment to be twice as high in depressed cardiac patients as in nondepressed cardiac patients (odds ratio 2.24).

Van Melle et al36 reviewed 22 studies and found that in the 2 years after an MI, depressed patients had a 2 to 2.5 times higher risk of dying of a cardiac or any other cause than did nondepressed patients.

Depression also predicts higher morbidity and mortality rates in patients undergoing coronary artery bypass grafting,37,38 patients with congestive heart failure,39 and heart transplant recipients.40

 

 

MEDICAL ILLNESS CAN PREDISPOSE TO DEPRESSION, AND VICE VERSA

Medical illnesses can predispose a patient to develop depression. Specifically, compared with healthy people, cardiac patients appear to be at greater risk of developing depression for many years after the initial medical diagnosis is made.41

Katon et al42 reviewed 31 studies involving 16,922 patients, that assessed the impact of depression and anxiety in chronic medical illnesses such as heart disease, diabetes, pulmonary disease, and arthritis. After the severity of the medical disorder was controlled for, patients with depression and anxiety reported a higher number of medical symptoms.

DEPRESSION WORSENS QUALITY OF LIFE AND ADHERENCE TO TREATMENT

Depressed patients perceive their health status and quality of life negatively. In the Heart and Soul study,43 depressive symptoms and low exercise capacity—but not low ejection fraction or ischemia—were significantly associated with perceived deterioration of health in patients with coronary artery disease.

After an MI, patients who take their cardiac drugs properly have a better chance of survival.44,45 Clinical depression can worsen compliance with cardiac medication regimens,46 and reducing depression increases medication adherence overall.47 Not surprisingly, depressed patients also adhere less well to other recommendations,48 including modifying the diet, exercising, stopping smoking, and attending cardiac rehabilitation programs. 49

PLAUSIBLE MECHANISMS LINK DEPRESSION AND HEART DISEASE

Traditional cardiac risk factors such as smoking, high cholesterol, hypertension, diabetes, and obesity tend to cluster in depressed patients. 50 Other mechanisms linking depression and heart disease are reviewed below.51,52

Autonomic imbalance

Excessive sympathetic stimulation or diminished vagal stimulation or both are associated with higher rates of morbidity and death.53

Lack of variability in the heart rate reflects a sympathetic-vagal imbalance and is a risk factor for ventricular arrhythmias and sudden cardiac death in patients with cardiovascular disease.54 Carney et al55 reported that patients with coronary artery disease and depression had significantly less heart rate variability than nondepressed cardiac patients. Similarly, after an MI, depressed patients had significantly less heart rate variability than nondepressed patients,56 implying that low heart rate variability may mediate the adverse effect of depression on survival after an MI.57

In the Heart and Soul study, Gehi et al58 found no distinct relationship between heart rate variability and depression. However, in the same study, de Jong et al59 did find specific somatic symptoms of depression to be associated with lower heart rate variability, although cognitive symptoms were not.

Platelet activation, endothelial dysfunction

Depressed patients have been found to have exaggerated platelet reactivity.60 Plasma levels of platelet factor IV and beta-thromboglobulin, markers of platelet activation, are higher in depressed patients with ischemic heart disease than in nondepressed patients with ischemic heart disease and in control patients.61 This activation of platelets can lead to vascular damage and thrombosis.

In a subset study of the Sertraline Anti-Depressant Heart Attack Randomized Trial (SADHART), depressed MI patients were treated with sertraline (Zoloft), a selective serotonin reuptake inhibitor (SSRI), and had substantially less platelet and endothelial biomarker release.62

Depressed cardiac patients also have impaired flow-mediated dilation of the brachial artery, a sign of endothelial dysfunction.63 Although a recent study did not find coronary endothelial dysfunction in depressed patients who did not have cardiac disease, these patients had more clustering of other cardiac risk factors.64

Hypothalamic-pituitary-adrenocortical and sympathetic adrenal medullary activation

High cortisol levels can accelerate the development of hypertension and atherosclerosis and result in endothelial vascular injury. Sympathoadrenal activation in turn can lead to higher levels of catecholamines, predisposing to vasoconstriction, a rapid heart rate, and platelet activation. Depressed patients have more activation of the hypothalamic-pituitary-adrenocortical and sympathetic adrenal medullary systems,51,65 yet another plausible mechanism for worse clinical outcomes in depressed cardiac patients.

Sudden emotional stress can cause transient left ventricular dysfunction, even in people without coronary disease, an effect that may be mediated by elevated plasma catecholamine levels.66

Inflammatory cytokines

Inflammatory cytokines play a key role in the development of atherosclerosis.67 C-reactive protein, an acute-phase reactant produced in hepatocytes, can be induced by cytokines such as interleukin 6. Damage to endothelial tissues leads to the release of inflammatory cytokines, including interleukin 1, interleukin 6, and tumor tumor necrosis factor alpha.

Depressed patients have higher levels of these inflammatory markers.68,69 A prospective study reported direct correlations between depression scores and C-reactive protein levels in post-MI patients.70 The Heart and Soul study, however, did not confirm that coronary patients have more inflammation if they have depression,71 indicating that the relationship is complex and is perhaps more evident in specific types of depression.72

Anticholinergic inflammatory pathway

Tracey73 proposed a theory that vagal tone inhibits the release of inflammatory cytokines. This has important implications for treatment, as exercise, biofeedback, and meditation can stimulate the vagus nerve and therefore have beneficial anti-inflammatory effects.74

Polymorphism in the serotonin transport promoter region gene

Research is focusing on the serotonin transport promoter region gene (5-HTTLPR).75 The gene exists in two forms, a long one and a less-effective short one that appears to predispose to depression.76

Nakatani et al77 showed that MI patients were more likely to become depressed and to have subsequent cardiac events if one or both of their alleles of this gene were short. Otte et al,78 using Heart and Soul study data, found that patients with a short allele had a higher likelihood of depression, higher perceived levels of stress, and higher urinary norepinephrine secretion. However, the long allele genotype may be associated with a higher risk of developing an MI.79

Our knowledge of the genetic interplay of depression and cardiovascular disease is still in its infancy, and further studies are needed to clarify these findings.

 

 

IN TRIALS, LESS DEPRESSION BUT NO EFFECT ON DEATHS, RECURRENT MI

Major behavioral and drug trials conducted in the last 15 years have focused on how to best treat depression in cardiac patients.80–85

The Montreal Heart Attack Readjustment Trial (MHART)81 used telephone calls and home nursing visits to explore and monitor psychological distress for up to 1 year after an MI. The overall trial did not show these interventions to have any impact on survival compared with usual care. In fact, in women receiving the telephone intervention, there was a trend toward higher rates of cardiac and all-cause death, which was quite unexpected. Uncovering stresses and problems without resolving them, rather than encouraging patients to place these on the “back burner,” may partially explain these results.

SADHART82 studied the safety of sertraline in depressed post-MI patients. No major differences in cardiac function were noted between the sertraline and placebo groups, showing that sertraline was safe for these patients. The sertraline group had fewer cardiovascular events, but the difference was not statistically significant.

The Enhancing Recovery in Coronary Heart Disease (ENRICHD) study83 was primarily designed to see whether a psychosocial intervention would decrease deaths in depressed cardiac patients. Much to the chagrin of behavioral medicine, the group undergoing cognitive behavioral therapy did not have a higher rate of event-free survival, although the intervention had a favorable impact on depression and social support.

The Myocardial Infarction Depression Intervention Trial (MIND-IT)84 looked at whether the antidepressant mirtazapine (Remeron) would improve long-term depression and cardiovascular outcomes in depressed post-MI patients. In 18 months of follow-up, neither objective was obtained.

The Cardiac Randomized Evaluation of Antidepressant and Psychotherapy Efficacy (CREATE) trial85 tested the efficacy of the SSRI citalopram (Celexa) and interpersonal therapy in a short-term intervention. Here, the antidepressant was superior to placebo in the primary outcome of treating depression, but interpersonal therapy had no advantage over “clinical management,” ie, a shorter, 20-minute supportive intervention.

Common threads in these studies.

  • In ENRICHD and MIND-IT, patients whose depression did not respond to treatment were at higher risk of cardiac events during follow-up.86–88
  • In SADHART and CREATE, which used drug treatment, the antidepressant response was more robust in patients with a history of depression before their heart attacks, suggesting that a patient with recurrent depression at the time of a cardiac event should receive medication for it.85,89

CLINICAL RECOMMENDATIONS

Use a depression screening tool

Ziegelstein et al90 recently studied the ability of clinical personnel to detect depression in hospitalized MI patients. If a screening tool was not used, the results were abysmal, indicating the need to use formal screening for symptoms of depression in acute MI patients.

Many self-rating scales are available, among which are the Beck Depression Inventory (BDI) and the Hospital Anxiety and Depression Scale (HADS). Others are:

The Patient Health Questionnaire (PHQ-9) is a nine-item tool, easy to administer and score (Table 1). It has been well studied in both screening for and follow-up of depression in primary care.91,92 It was used in the Heart and Soul study and the Prospective Registry Evaluating Outcomes After Myocardial Infarction: Events and Recovery (PREMIER) study.3 It has also been used to identify and document depressive symptoms in patients with acute coronary syndrome.94 A cut-off score of 10 or higher on the PHQ-9 is diagnostic of depression.95

The PHQ-2 consists of the two first questions of the PHQ-9, which deal with mood and lack of pleasure. A cut-off score of 3 or higher has a sensitivity of 83% and a specificity of 92%,96 fulfilling the need for a quick and reliable depression screening tool. The clinician can also ask for a yes-or-no answer to the two questions of the PHQ-2 (Table 1). A yes to either of the two questions is up to 90% sensitive and 75% specific.92,97

When to suspect depression in cardiac patients

Cardiac patients may not realize they have the classic symptoms of depression, since they often ascribe somatic symptoms to their heart disease and overlook emotional associations. Lespérance and colleagues98 suggest that certain clues should make us suspect depression in cardiac patients (Table 2).

Which type of psychotherapy is best?

The negative results of psychosocial interventions (phone calls and home visits from a nurse) in MHART and of cognitive behavioral therapy in ENRICHD raise questions about which type of psychotherapy is best for depression in heart disease. CREATE found that 50-minute weekly sessions of interpersonal psychotherapy were no more beneficial than clinical management, ie, 20-minute weekly sessions that focused on compliance with treatment and education about depression and overall management. Perhaps a type of therapy akin to “clinical management” in this study or the brief behavior-based and targeted therapy used in the Improving Mood Promoting Access to Collaborative Care Treatment (IMPACT) trials of depression in primary care99 could be designed specifically to treat depression in cardiac disease. However, it is also quite possible that treatments that focus on uncovering stresses or problems may not be timely for these patients.

Which therapy is best for women is another area of consideration. In MHART, even after 5 years of follow-up,100 women who received the psychosocial support intervention did marginally worse. In the ENRICHD study, women did not experience a benefit from cognitive behavioral therapy. Further studies must address sex differences in response to different therapies.

 

 

SSRIs seem to be better than other antidepressants for cardiac patients

Before SSRIs were available, tricyclic antidepressants were the mainstays. Subsequent analysis showed the tricyclics to have an unfavorable risk-benefit profile in cardiac patients,101 and since other types of antidepressants are available, tricyclics should be avoided altogether in cardiac patients.102

Whether the SSRIs actually decrease one’s risk of death in heart disease is still an issue of debate, but there are encouraging signs. In SADHART, the rate of death and recurrent nonfatal MI was 20% lower in the patients randomized to receive sertraline, although the difference was not statistically significant.82 In ENRICHD, patients who did not respond to cognitive behavioral treatment or had severe depression could receive sertraline or other antidepressant drugs on a nonrandomized basis, and those who did had a 42% lower incidence of death or recurrent MI.103

The SADHART and CREATE trials provide convincing evidence of the cardiac safety and antidepressant efficacy of two SSRIs (sertraline and citalopram) in depressed cardiac patients. Mirtazapine, studied in MIND-IT, was not effective in treating depression in cardiac patients, although it had a better adverse effect and safety profile than tricyclic antidepressants. 104

Clinical observations indicate that SSRIs are associated with less risk of MI than non-SSRI drugs.105,106 During hospitalization for acute coronary syndromes, patients on SSRIs had lower rates of recurrent ischemia and heart failure but higher bleeding rates than patients not taking SSRIs.107 In a retrospective study of patients undergoing coronary artery bypass grafting, those on an SSRI before surgery had higher rates of death and rehospitalization.108 Being on antidepressant medication could be interpreted as a surrogate marker of having more severe depression before surgery; this issue clearly requires further study.

Given current observations and recent data from interventional trials coupled with the safe drug-interaction profile of sertraline and citalopram, these two SSRIs are recommended for treating depression in cardiac patients. If the patient is also receiving an anticoagulant, one should monitor for bleeding, as all SSRIs are associated with a prolonged bleeding time. Monitoring for rare cases of hyponatremia and bradycardia should also be part of early follow-up.

Do cardiac drugs have psychiatric effects?

Some concerns have arisen about cardiovascular drugs causing or aggravating psychiatric conditions.

Statins were once suspected of causing clinical depression or even suicide. However, subsequent studies have not substantiated this.109,110 In fact, long-term statin use has been associated with improved psychological wellbeing. 111 Whether the favorable psychological profile is due to an improved lifestyle, a direct noncholesterol effect, or an immunomodulatory effect has yet to be determined.

Beta-blockers have been suspected of increasing depression and fatigue. Robust metaanalyses have shown no increased risk of depressive symptoms but a small increased risk of fatigue and sexual dysfunction.112 Observational trials in the first year post-MI have shown no differences between beta-blocker users and nonusers in depressive symptoms or depressive disorders.113

Statins and beta-blockers offer both immense cardiac benefit and low risk, and both may be prescribed with confidence in depressed cardiac patients.

Refer patients for cardiac rehabilitation

The American Association of Cardiovascular and Pulmonary Rehabilitation strongly recommends screening cardiac patients for depression and referring them to cardiac rehabilitation programs.114 Typical programs run 12 weeks, affording an opportunity to further listen to and assess the patient and to promote general wellness via nutrition, stress management, and exercise.

These interventions by themselves can favorably affect depression. Blumenthal and colleagues,115 in the Standard Medical Intervention and Long-Term Exercise (SMILE) study, found that exercise was as effective as drug treatment in reducing depression. In addition, stress management as a psychosocial treatment in cardiac rehabilitation can reduce death rates in cardiac patients.116

Unfortunately, many patients who are eligible for cardiac rehabilitation programs do not avail themselves of them.117

Our algorithm

Figure 2. Our algorithm for detecting and treating depression in cardiac patients.
In view of the data outlined in this review, we propose an algorithm for use in depressed cardiac patients (Figure 2), which is similar to the algorithm proposed by the AHA committee,1 but which we developed independently.

FUTURE DIRECTIONS FOR RESEARCH

Can we predict the course of depression?

We need to identify better which patients will have a spontaneous remission of their depressive symptoms after a cardiac event, which patients will linger with depression, and which patients will best respond to treatment. Risk stratification, using the psychiatric history, symptoms and severity of depression, and genetic predisposition118 might allow improved targeted therapies.

Does depression cause cardiac disease?

The link between depression and heart disease can be seen as merely an association. In the interventional trials performed to date, we have not yet seen a reduction in cardiac deaths when depression was treated, challenging any assumption of a causal relationship between depression and heart disease. The debate about association vs cause is germane to behavioral medicine,119 and the better we understand the mechanistic pathways, the better we can advise patients and treat depression comorbid with heart disease.

Behavioral medicine is currently measuring the aspects of depression associated with cardiac disease, including the spectrum of somatic (body) and affective (mood) symptoms120 and specific areas such as sympathetic arousal and early morning insomnia.121 If we can determine the depression subtype that carries a worse cardiac prognosis, we may untangle the biobehavioral links that bidirectionally bridge clinical depression and cardiac disease.

Another area of interest, emotional vitality (a positive state associated with interest, enthusiasm, excitement, and energy for living) has been shown to protect against coronary heart disease122 and holds much promise.

In the plenary lecture of the Academy of Psychosomatic Medicine in 2006, Frasure-Smith spoke of the “pleiotropism” of our antidepressant interventions on the various risk factors in depressed cardiac patients.123 We need behavioral medicine studies that elucidate these mechanisms, guiding more precise treatments as well as novel therapies. Omega-3 fatty acids, which benefit heart disease and clinical depression,124 will be used in a randomized controlled trial by Lespérance and colleagues.125 We await the results of this exciting research.

 

 

Will treating depression help in other types of heart disease?

The SADHART-CHF trial is examining whether 12 weeks of sertraline therapy is better than placebo in preventing death and improving cardiac outcomes in patients with chronic heart failure and comorbid major depressive disorder. It was to be completed in the fall of 2008. The results and experience of this study will help in designing future interventional trials to reduce the risk of depression in cardiovascular diseases.

We also await the results of a National Heart, Lung, and Blood Institute (NHLBI) trial, “Bypassing the Blues,” which is studying the treatment of depression after cardiac bypass surgery. This study should provide further insights into management of the depressed cardiac patient. Further prognostic studies in cardiac patients are also needed using the PHQ-9 and its shorter version, PHQ-2.

Current and future guidelines

For years our European colleagues have been ahead of us in recognizing depression screening and stress management as key to cardiac disease-prevention strategies.126 The NHLBI nicely outlined recommendations on the assessment and treatment of depression in cardiovascular patients.127 The just-published AHA Science Advisory should further encourage clinicians to screen and treat depression in the patient population.1 As our knowledge grows, we look forward to future evidence-based guidelines for depressed cardiac patients.

Depression is a risk factor for heart disease, and in patients with heart disease, it is a risk factor for complications and death. Unfortunately, in the trials performed to date, treating depression in cardiac patients did not lead to lower rates of recurrent cardiovascular events or death. Nevertheless, we recommend that clinicians systematically screen for it in their heart patients, in view of the benefits of antidepressant therapy.

In this article we review key epidemiologic and psychosocial studies, the mechanistic links between depression and heart disease, and recent intervention trials. We also offer practical management advice and address the continued need for guidelines and risk stratification in the treatment of depressed cardiac patients.

After we submitted our review article, the American Heart Association (AHA)1 released a consensus document recommending that health care providers screen for and treat depression in patients with coronary heart disease. We will discuss the same screening tests that have been recommended by the AHA.

DEPRESSION AND HEART DISEASE: COMMON AND LINKED

Depression and heart disease are very common and often coexist: the prevalence of depression in various heart conditions ranges from 15% to 20%.1–3 According to data from the World Health Organization, by the year 2020 depression will be the second-leading cause of disability in developed countries (after heart disease).4

The World Health Survey5 showed that depression worsens health more than angina, arthritis, asthma, or diabetes. Furthermore, patients with severe mental illness have a higher risk of dying from heart disease and stroke.6

SOME HEART DISEASE RISK FACTORS ARE PSYCHOSOCIAL

In the 1980s, the “type A” personality (ambitious, aggressive, hostile, and competitive, with a chronic sense of urgency) was linked to heart disease.7 Later studies differed as to whether the entire set of features is valid as a collective risk factor for progressive heart disease,8 but hostility remains a validated risk factor and a focus of behavior modification.9,10

Other psychosocial risk factors have been implicated,11,12 one of which is social isolation.9,13 Another is the “type D” personality, which includes a tendency to experience negative emotions across time and situations coupled with social inhibition and which is believed to be more valid than the type A personality as a risk factor for cardiac disease.14,15

The INTERHEART study16 gathered data about attributable risk in the development of myocardial infarction (MI) in 52 countries in a case-control fashion. Psychosocial factors including stress, low generalized locus of control (ie, the perceived inability to control one’s life), and depression accounted for 32.5% of the attributable risk for an MI.17 This would mean that they account for slightly less attributable risk than that of lifetime smoking but more than that of hypertension and obesity.

Job stress increases the risk of initial coronary heart disease18 and also the risk of recurrent cardiac events after a first MI.19 Even though numerous psychosocial risk factors have been associated with coronary heart disease, including anxiety,20,21 depression is perhaps the best studied.

PROSPECTIVE STUDIES OF DEPRESSION AND HEART DISEASE

To examine the impact of depression in coronary heart disease, prospective studies have been done in healthy people and in patients with established cardiovascular disease who develop depression.22

In healthy people, depression increases the risk of coronary disease

The 1996 Epidemiologic Catchment Area study23 found that people with major depression had a risk of MI four times higher than the norm, and people with 2 weeks of sadness or dysphoria had a risk two times higher.

A subsequent meta-analysis of 11 studies,24 which included 36,000 patients, found that the overall relative risk of developing heart disease in depressed but healthy people was 1.64.

A meta-analysis by Van der Kooy et al25 of 28 epidemiologic studies with nearly 80,000 patients showed depression to be an independent risk factor for cardiovascular disease.

Wulsin and Singal26 performed a systematic review to see if depression increases the risk of coronary disease. In 10 studies with a follow-up of more than 4 years, the relative risk in people with depression was 1.64, which was less than that in active smokers (2.5) but more than that in passive smokers (1.25).

Depression can also exacerbate the classic risk factors for coronary disease, such as smoking, diabetes, obesity, and physical inactivity. 27

A 2007 study from Sweden28 prospectively followed patients who were hospitalized for depression. The odds ratio of developing an acute MI was 2.9, and the risk persisted for decades after the initial hospitalization.

A prospective United Kingdom cohort study of people initially free of heart disease revealed major depression to be associated with a higher rate of death from ischemic heart disease.29 Specifically, patients who had depression currently or in the past 12 months had a 2.7 times higher risk of dying than those who had never had depression or who had had it more than 12 months previously.

In existing heart disease, depression predicts recurrent events, death

Carney et el30 found that patients with major depressive disorder had a higher incidence of new cardiac events in the 12 months after undergoing cardiac catheterization than those without major depressive disorder.

Frasure-Smith et al,31 in a landmark study, showed that patients who were depressed at 1 week after an MI were three to four times more likely to die in the next 6 months than nondepressed post-MI patients. Even after 18 months, depression remained an independent risk factor for cardiac-related death.32

In longer studies (with up to 19.4 years of follow-up), depression was associated with higher rates of death from cardiac and all causes in patients with coronary artery disease.33 Lespérance et al34 found that in MI patients, the higher the Beck Depression Inventory score at the time of hospital admission, the higher the 5-year death rate.

Using meta-analysis, Barth et al35 found the risk of dying in the first 2 years after initial assessment to be twice as high in depressed cardiac patients as in nondepressed cardiac patients (odds ratio 2.24).

Van Melle et al36 reviewed 22 studies and found that in the 2 years after an MI, depressed patients had a 2 to 2.5 times higher risk of dying of a cardiac or any other cause than did nondepressed patients.

Depression also predicts higher morbidity and mortality rates in patients undergoing coronary artery bypass grafting,37,38 patients with congestive heart failure,39 and heart transplant recipients.40

 

 

MEDICAL ILLNESS CAN PREDISPOSE TO DEPRESSION, AND VICE VERSA

Medical illnesses can predispose a patient to develop depression. Specifically, compared with healthy people, cardiac patients appear to be at greater risk of developing depression for many years after the initial medical diagnosis is made.41

Katon et al42 reviewed 31 studies involving 16,922 patients, that assessed the impact of depression and anxiety in chronic medical illnesses such as heart disease, diabetes, pulmonary disease, and arthritis. After the severity of the medical disorder was controlled for, patients with depression and anxiety reported a higher number of medical symptoms.

DEPRESSION WORSENS QUALITY OF LIFE AND ADHERENCE TO TREATMENT

Depressed patients perceive their health status and quality of life negatively. In the Heart and Soul study,43 depressive symptoms and low exercise capacity—but not low ejection fraction or ischemia—were significantly associated with perceived deterioration of health in patients with coronary artery disease.

After an MI, patients who take their cardiac drugs properly have a better chance of survival.44,45 Clinical depression can worsen compliance with cardiac medication regimens,46 and reducing depression increases medication adherence overall.47 Not surprisingly, depressed patients also adhere less well to other recommendations,48 including modifying the diet, exercising, stopping smoking, and attending cardiac rehabilitation programs. 49

PLAUSIBLE MECHANISMS LINK DEPRESSION AND HEART DISEASE

Traditional cardiac risk factors such as smoking, high cholesterol, hypertension, diabetes, and obesity tend to cluster in depressed patients. 50 Other mechanisms linking depression and heart disease are reviewed below.51,52

Autonomic imbalance

Excessive sympathetic stimulation or diminished vagal stimulation or both are associated with higher rates of morbidity and death.53

Lack of variability in the heart rate reflects a sympathetic-vagal imbalance and is a risk factor for ventricular arrhythmias and sudden cardiac death in patients with cardiovascular disease.54 Carney et al55 reported that patients with coronary artery disease and depression had significantly less heart rate variability than nondepressed cardiac patients. Similarly, after an MI, depressed patients had significantly less heart rate variability than nondepressed patients,56 implying that low heart rate variability may mediate the adverse effect of depression on survival after an MI.57

In the Heart and Soul study, Gehi et al58 found no distinct relationship between heart rate variability and depression. However, in the same study, de Jong et al59 did find specific somatic symptoms of depression to be associated with lower heart rate variability, although cognitive symptoms were not.

Platelet activation, endothelial dysfunction

Depressed patients have been found to have exaggerated platelet reactivity.60 Plasma levels of platelet factor IV and beta-thromboglobulin, markers of platelet activation, are higher in depressed patients with ischemic heart disease than in nondepressed patients with ischemic heart disease and in control patients.61 This activation of platelets can lead to vascular damage and thrombosis.

In a subset study of the Sertraline Anti-Depressant Heart Attack Randomized Trial (SADHART), depressed MI patients were treated with sertraline (Zoloft), a selective serotonin reuptake inhibitor (SSRI), and had substantially less platelet and endothelial biomarker release.62

Depressed cardiac patients also have impaired flow-mediated dilation of the brachial artery, a sign of endothelial dysfunction.63 Although a recent study did not find coronary endothelial dysfunction in depressed patients who did not have cardiac disease, these patients had more clustering of other cardiac risk factors.64

Hypothalamic-pituitary-adrenocortical and sympathetic adrenal medullary activation

High cortisol levels can accelerate the development of hypertension and atherosclerosis and result in endothelial vascular injury. Sympathoadrenal activation in turn can lead to higher levels of catecholamines, predisposing to vasoconstriction, a rapid heart rate, and platelet activation. Depressed patients have more activation of the hypothalamic-pituitary-adrenocortical and sympathetic adrenal medullary systems,51,65 yet another plausible mechanism for worse clinical outcomes in depressed cardiac patients.

Sudden emotional stress can cause transient left ventricular dysfunction, even in people without coronary disease, an effect that may be mediated by elevated plasma catecholamine levels.66

Inflammatory cytokines

Inflammatory cytokines play a key role in the development of atherosclerosis.67 C-reactive protein, an acute-phase reactant produced in hepatocytes, can be induced by cytokines such as interleukin 6. Damage to endothelial tissues leads to the release of inflammatory cytokines, including interleukin 1, interleukin 6, and tumor tumor necrosis factor alpha.

Depressed patients have higher levels of these inflammatory markers.68,69 A prospective study reported direct correlations between depression scores and C-reactive protein levels in post-MI patients.70 The Heart and Soul study, however, did not confirm that coronary patients have more inflammation if they have depression,71 indicating that the relationship is complex and is perhaps more evident in specific types of depression.72

Anticholinergic inflammatory pathway

Tracey73 proposed a theory that vagal tone inhibits the release of inflammatory cytokines. This has important implications for treatment, as exercise, biofeedback, and meditation can stimulate the vagus nerve and therefore have beneficial anti-inflammatory effects.74

Polymorphism in the serotonin transport promoter region gene

Research is focusing on the serotonin transport promoter region gene (5-HTTLPR).75 The gene exists in two forms, a long one and a less-effective short one that appears to predispose to depression.76

Nakatani et al77 showed that MI patients were more likely to become depressed and to have subsequent cardiac events if one or both of their alleles of this gene were short. Otte et al,78 using Heart and Soul study data, found that patients with a short allele had a higher likelihood of depression, higher perceived levels of stress, and higher urinary norepinephrine secretion. However, the long allele genotype may be associated with a higher risk of developing an MI.79

Our knowledge of the genetic interplay of depression and cardiovascular disease is still in its infancy, and further studies are needed to clarify these findings.

 

 

IN TRIALS, LESS DEPRESSION BUT NO EFFECT ON DEATHS, RECURRENT MI

Major behavioral and drug trials conducted in the last 15 years have focused on how to best treat depression in cardiac patients.80–85

The Montreal Heart Attack Readjustment Trial (MHART)81 used telephone calls and home nursing visits to explore and monitor psychological distress for up to 1 year after an MI. The overall trial did not show these interventions to have any impact on survival compared with usual care. In fact, in women receiving the telephone intervention, there was a trend toward higher rates of cardiac and all-cause death, which was quite unexpected. Uncovering stresses and problems without resolving them, rather than encouraging patients to place these on the “back burner,” may partially explain these results.

SADHART82 studied the safety of sertraline in depressed post-MI patients. No major differences in cardiac function were noted between the sertraline and placebo groups, showing that sertraline was safe for these patients. The sertraline group had fewer cardiovascular events, but the difference was not statistically significant.

The Enhancing Recovery in Coronary Heart Disease (ENRICHD) study83 was primarily designed to see whether a psychosocial intervention would decrease deaths in depressed cardiac patients. Much to the chagrin of behavioral medicine, the group undergoing cognitive behavioral therapy did not have a higher rate of event-free survival, although the intervention had a favorable impact on depression and social support.

The Myocardial Infarction Depression Intervention Trial (MIND-IT)84 looked at whether the antidepressant mirtazapine (Remeron) would improve long-term depression and cardiovascular outcomes in depressed post-MI patients. In 18 months of follow-up, neither objective was obtained.

The Cardiac Randomized Evaluation of Antidepressant and Psychotherapy Efficacy (CREATE) trial85 tested the efficacy of the SSRI citalopram (Celexa) and interpersonal therapy in a short-term intervention. Here, the antidepressant was superior to placebo in the primary outcome of treating depression, but interpersonal therapy had no advantage over “clinical management,” ie, a shorter, 20-minute supportive intervention.

Common threads in these studies.

  • In ENRICHD and MIND-IT, patients whose depression did not respond to treatment were at higher risk of cardiac events during follow-up.86–88
  • In SADHART and CREATE, which used drug treatment, the antidepressant response was more robust in patients with a history of depression before their heart attacks, suggesting that a patient with recurrent depression at the time of a cardiac event should receive medication for it.85,89

CLINICAL RECOMMENDATIONS

Use a depression screening tool

Ziegelstein et al90 recently studied the ability of clinical personnel to detect depression in hospitalized MI patients. If a screening tool was not used, the results were abysmal, indicating the need to use formal screening for symptoms of depression in acute MI patients.

Many self-rating scales are available, among which are the Beck Depression Inventory (BDI) and the Hospital Anxiety and Depression Scale (HADS). Others are:

The Patient Health Questionnaire (PHQ-9) is a nine-item tool, easy to administer and score (Table 1). It has been well studied in both screening for and follow-up of depression in primary care.91,92 It was used in the Heart and Soul study and the Prospective Registry Evaluating Outcomes After Myocardial Infarction: Events and Recovery (PREMIER) study.3 It has also been used to identify and document depressive symptoms in patients with acute coronary syndrome.94 A cut-off score of 10 or higher on the PHQ-9 is diagnostic of depression.95

The PHQ-2 consists of the two first questions of the PHQ-9, which deal with mood and lack of pleasure. A cut-off score of 3 or higher has a sensitivity of 83% and a specificity of 92%,96 fulfilling the need for a quick and reliable depression screening tool. The clinician can also ask for a yes-or-no answer to the two questions of the PHQ-2 (Table 1). A yes to either of the two questions is up to 90% sensitive and 75% specific.92,97

When to suspect depression in cardiac patients

Cardiac patients may not realize they have the classic symptoms of depression, since they often ascribe somatic symptoms to their heart disease and overlook emotional associations. Lespérance and colleagues98 suggest that certain clues should make us suspect depression in cardiac patients (Table 2).

Which type of psychotherapy is best?

The negative results of psychosocial interventions (phone calls and home visits from a nurse) in MHART and of cognitive behavioral therapy in ENRICHD raise questions about which type of psychotherapy is best for depression in heart disease. CREATE found that 50-minute weekly sessions of interpersonal psychotherapy were no more beneficial than clinical management, ie, 20-minute weekly sessions that focused on compliance with treatment and education about depression and overall management. Perhaps a type of therapy akin to “clinical management” in this study or the brief behavior-based and targeted therapy used in the Improving Mood Promoting Access to Collaborative Care Treatment (IMPACT) trials of depression in primary care99 could be designed specifically to treat depression in cardiac disease. However, it is also quite possible that treatments that focus on uncovering stresses or problems may not be timely for these patients.

Which therapy is best for women is another area of consideration. In MHART, even after 5 years of follow-up,100 women who received the psychosocial support intervention did marginally worse. In the ENRICHD study, women did not experience a benefit from cognitive behavioral therapy. Further studies must address sex differences in response to different therapies.

 

 

SSRIs seem to be better than other antidepressants for cardiac patients

Before SSRIs were available, tricyclic antidepressants were the mainstays. Subsequent analysis showed the tricyclics to have an unfavorable risk-benefit profile in cardiac patients,101 and since other types of antidepressants are available, tricyclics should be avoided altogether in cardiac patients.102

Whether the SSRIs actually decrease one’s risk of death in heart disease is still an issue of debate, but there are encouraging signs. In SADHART, the rate of death and recurrent nonfatal MI was 20% lower in the patients randomized to receive sertraline, although the difference was not statistically significant.82 In ENRICHD, patients who did not respond to cognitive behavioral treatment or had severe depression could receive sertraline or other antidepressant drugs on a nonrandomized basis, and those who did had a 42% lower incidence of death or recurrent MI.103

The SADHART and CREATE trials provide convincing evidence of the cardiac safety and antidepressant efficacy of two SSRIs (sertraline and citalopram) in depressed cardiac patients. Mirtazapine, studied in MIND-IT, was not effective in treating depression in cardiac patients, although it had a better adverse effect and safety profile than tricyclic antidepressants. 104

Clinical observations indicate that SSRIs are associated with less risk of MI than non-SSRI drugs.105,106 During hospitalization for acute coronary syndromes, patients on SSRIs had lower rates of recurrent ischemia and heart failure but higher bleeding rates than patients not taking SSRIs.107 In a retrospective study of patients undergoing coronary artery bypass grafting, those on an SSRI before surgery had higher rates of death and rehospitalization.108 Being on antidepressant medication could be interpreted as a surrogate marker of having more severe depression before surgery; this issue clearly requires further study.

Given current observations and recent data from interventional trials coupled with the safe drug-interaction profile of sertraline and citalopram, these two SSRIs are recommended for treating depression in cardiac patients. If the patient is also receiving an anticoagulant, one should monitor for bleeding, as all SSRIs are associated with a prolonged bleeding time. Monitoring for rare cases of hyponatremia and bradycardia should also be part of early follow-up.

Do cardiac drugs have psychiatric effects?

Some concerns have arisen about cardiovascular drugs causing or aggravating psychiatric conditions.

Statins were once suspected of causing clinical depression or even suicide. However, subsequent studies have not substantiated this.109,110 In fact, long-term statin use has been associated with improved psychological wellbeing. 111 Whether the favorable psychological profile is due to an improved lifestyle, a direct noncholesterol effect, or an immunomodulatory effect has yet to be determined.

Beta-blockers have been suspected of increasing depression and fatigue. Robust metaanalyses have shown no increased risk of depressive symptoms but a small increased risk of fatigue and sexual dysfunction.112 Observational trials in the first year post-MI have shown no differences between beta-blocker users and nonusers in depressive symptoms or depressive disorders.113

Statins and beta-blockers offer both immense cardiac benefit and low risk, and both may be prescribed with confidence in depressed cardiac patients.

Refer patients for cardiac rehabilitation

The American Association of Cardiovascular and Pulmonary Rehabilitation strongly recommends screening cardiac patients for depression and referring them to cardiac rehabilitation programs.114 Typical programs run 12 weeks, affording an opportunity to further listen to and assess the patient and to promote general wellness via nutrition, stress management, and exercise.

These interventions by themselves can favorably affect depression. Blumenthal and colleagues,115 in the Standard Medical Intervention and Long-Term Exercise (SMILE) study, found that exercise was as effective as drug treatment in reducing depression. In addition, stress management as a psychosocial treatment in cardiac rehabilitation can reduce death rates in cardiac patients.116

Unfortunately, many patients who are eligible for cardiac rehabilitation programs do not avail themselves of them.117

Our algorithm

Figure 2. Our algorithm for detecting and treating depression in cardiac patients.
In view of the data outlined in this review, we propose an algorithm for use in depressed cardiac patients (Figure 2), which is similar to the algorithm proposed by the AHA committee,1 but which we developed independently.

FUTURE DIRECTIONS FOR RESEARCH

Can we predict the course of depression?

We need to identify better which patients will have a spontaneous remission of their depressive symptoms after a cardiac event, which patients will linger with depression, and which patients will best respond to treatment. Risk stratification, using the psychiatric history, symptoms and severity of depression, and genetic predisposition118 might allow improved targeted therapies.

Does depression cause cardiac disease?

The link between depression and heart disease can be seen as merely an association. In the interventional trials performed to date, we have not yet seen a reduction in cardiac deaths when depression was treated, challenging any assumption of a causal relationship between depression and heart disease. The debate about association vs cause is germane to behavioral medicine,119 and the better we understand the mechanistic pathways, the better we can advise patients and treat depression comorbid with heart disease.

Behavioral medicine is currently measuring the aspects of depression associated with cardiac disease, including the spectrum of somatic (body) and affective (mood) symptoms120 and specific areas such as sympathetic arousal and early morning insomnia.121 If we can determine the depression subtype that carries a worse cardiac prognosis, we may untangle the biobehavioral links that bidirectionally bridge clinical depression and cardiac disease.

Another area of interest, emotional vitality (a positive state associated with interest, enthusiasm, excitement, and energy for living) has been shown to protect against coronary heart disease122 and holds much promise.

In the plenary lecture of the Academy of Psychosomatic Medicine in 2006, Frasure-Smith spoke of the “pleiotropism” of our antidepressant interventions on the various risk factors in depressed cardiac patients.123 We need behavioral medicine studies that elucidate these mechanisms, guiding more precise treatments as well as novel therapies. Omega-3 fatty acids, which benefit heart disease and clinical depression,124 will be used in a randomized controlled trial by Lespérance and colleagues.125 We await the results of this exciting research.

 

 

Will treating depression help in other types of heart disease?

The SADHART-CHF trial is examining whether 12 weeks of sertraline therapy is better than placebo in preventing death and improving cardiac outcomes in patients with chronic heart failure and comorbid major depressive disorder. It was to be completed in the fall of 2008. The results and experience of this study will help in designing future interventional trials to reduce the risk of depression in cardiovascular diseases.

We also await the results of a National Heart, Lung, and Blood Institute (NHLBI) trial, “Bypassing the Blues,” which is studying the treatment of depression after cardiac bypass surgery. This study should provide further insights into management of the depressed cardiac patient. Further prognostic studies in cardiac patients are also needed using the PHQ-9 and its shorter version, PHQ-2.

Current and future guidelines

For years our European colleagues have been ahead of us in recognizing depression screening and stress management as key to cardiac disease-prevention strategies.126 The NHLBI nicely outlined recommendations on the assessment and treatment of depression in cardiovascular patients.127 The just-published AHA Science Advisory should further encourage clinicians to screen and treat depression in the patient population.1 As our knowledge grows, we look forward to future evidence-based guidelines for depressed cardiac patients.

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  92. Löwe B, Unutzer J, Callahan CM, Perkins AJ, Kroenke K. Monitoring depression treatment outcomes with the Patient Health Questionnaire-9. Med Care 2004; 42:11941201.
  93. Parashar S, Rumsfeld JS, Spertus JA, et al. Time course of depression and outcome of myocardial infarction. Arch Intern Med 2006; 166:20352043.
  94. Amin AA, Jones AMH, Nugent K, Rumsfeld JS, Spertus JA. The prevalence of unrecognized depression in patients with acute coronary syndrome. Am Heart J 2006; 152:928934.
  95. McManus D, Pipkin SS, Whooley MA. Screening for depression in patients with coronary heart disease (data from the Heart and Soul Study). Am J Cardiol 2005; 96:10761081.
  96. Kroenke K, Spitzer RL, Williams JB. The Patient Health Questionnaire-2: validity of a two-item depression screener. Med Care 2003; 41:12841292.
  97. Spitzer RL, Williams JB, Kroenke K, et al. Utility of a new procedure for diagnosing mental disorders in primary care. The PRIME-MD 1000 study. JAMA 1994; 272:17491756.
  98. Lespérance F, Frasure-Smith N. Depression in patients with cardiac disease. J Psychosom Res 2000; 48:379391.
  99. Hunkeler EM, Katon W, Tang L, et al. Long term outcomes from the IMPACT randomised trial for depressed elderly patients in primary care. BMJ 2006; 332:259263.
  100. Frasure-Smith N, Lespérance F, Gravel G, Masson A, Juneau M, Bourassa MG. Long-term survival differences among low-anxious, high-anxious and repressive copers enrolled in the Montreal Heart Attack Readjustment Trial. Psychosom Med 2002; 64:571579.
  101. Glassman AH, Roose SP, Bigger JT. The safety of tricyclic antidepressants in cardiac patients: risk-benefit reconsidered. JAMA 1993; 269:26732675.
  102. Cohen HW, Gibson G, Alderman MH. Excess risk of myocardial infarction in patients treated with antidepressant medications: association with use of tricyclic agents. Am J Med 2000; 108:28.
  103. Taylor CB, Youngblood ME, Catellier D, et al. Effects of antidepressant medication on morbidity and mortality in depressed patients after myocardial infarction. Arch Gen Psychiatry 2005; 62:792798.
  104. Montgomery SA. Safety of mirtazapine: a review. Int Clin Psychopharmacol 1995; 10(suppl 4):3745.
  105. Sauer WH, Berlin JA, Kimmel SE. Selective serotonin reuptake inhibitors and myocardial infarction. Circulation 2001; 104:18941898.
  106. Sauer WH, Berlin JA, Kimmel SE. Effect of antidepressants and their relative affinity for the serotonin transporter on the risk of myocardial infarction. Circulation 2003; 108:3236.
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KEY POINTS

  • Depression is a risk factor for new cardiac disease and has a detrimental impact in established cardiac disease.
  • Numerous mechanistic pathways have been implicated.
  • In clinical trials, drug therapy and psychotherapy have not clearly decreased the rate of cardiac death in depressed cardiac patients, but they did improve depression, adherence to drug therapy, and quality of life.
  • Clinicians should routinely screen for depression in cardiac patients and should not hesitate to treat it.
  • Eligible patients should routinely be referred to cardiac rehabilitation programs.
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Alzheimer disease: Time to improve its diagnosis and treatment

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Alzheimer disease: Time to improve its diagnosis and treatment

The number of patients with Alzheimer disease, the most common cause of disability in the elderly, is about to rise dramatically. More than 5 million people in the United States are affected, and by 2050 this figure may rise to between 11 and 16 million.1 The prevalence doubles every 5 years from ages 65 to 85, so that Alzheimer disease affects 30% to 50% of all people at age 85.1,2

Primary care physicians bear the brunt of diagnosing and treating all these patients,3 requiring that they have the training to meet this critical public health problem.

But diagnosing this disease is not easy. In the early stages, it can be difficult to distinguish between the decline in certain cognitive functions due to normal aging (eg, name recall) and the mild cognitive impairment that often precedes Alzheimer disease.

Once a patient is diagnosed with Alzheimer disease, there needs to be a realistic discussion with the patient and family about what treatment with different drugs can—and cannot—accomplish.

ALZHEIMER DISEASE DIAGNOSIS: THE EARLIER, THE BETTER

While much has been accomplished in Alzheimer disease research in the last 20 years, a great deal remains to be done to improve its diagnosis and treatment. There is increasing evidence that early diagnosis of Alzheimer disease will be key to maximizing treatment benefits. But too often, patients are diagnosed in later stages of the disease, when disabling symptoms and neuropathologic changes have become well established.

Mild cognitive impairment: A predementia phase

The pathologic changes of Alzheimer disease typically begin many years before its clinical signs are apparent. Most patients pass through a predementia phase called mild cognitive impairment, with early memory loss but with relatively well-preserved activities of daily living.

From 6% to 25% of patients with mild cognitive impairment progress to dementia annually, a rate far higher than the incidence rate in the general population of 0.3% to 3.9% per year, depending on age.4,5 Therefore, patients with mild cognitive impairment are a good population in which to test interventions to prevent dementia.6,7

The concept of mild cognitive impairment is controversial because it is a transitional stage between normal aging and dementia rather than a distinct pathologic entity.8 Moreover, in some large community-based studies,9,10 a sizeable number of people with mild cognitive impairment reverted to normal cognitive function over 5 years, suggesting that mild cognitive impairment may be unstable over time.

Are other factors causing the dementia?

The Diagnostic and Statistical Manual IV-Text Revision11 defines dementia as memory loss and at least one other area of cognitive impairment, not due to delirium, that interferes with social and occupational functioning. Alzheimer disease is the most common cause of dementia in the United States.1

Still, Alzheimer disease does not typically exist in isolation. For example, while Alzheimer disease was the predominant cause of dementia in a recent postmortem series, 38% of dementia cases featured Alzheimer disease with lacunar infarction.12 Accordingly, clinicians must consider factors other than Alzheimer disease that could contribute to (or even fully account for) the complaints or observed deficits.

Is it Alzheimer disease or normal aging?

Although cognitive impairment and changes in behavior are common in the elderly, they are not a normal part of aging. Like other chronic disorders associated with aging, Alzheimer disease can be diagnosed and treated. Cognitive impairment may come to light when the patient or a family member reports a problem or the clinician asks about problems or observes signs of impairment in the office. The cognitive difficulties should be taken seriously, and their impact on daily functioning should be evaluated.

Certain cognitive functions such as mental flexibility and speed of processing decline in normal aging,13 and many older people report cognitive symptoms. Therefore, it is important to differentiate mild age-associated cognitive changes from the beginning of a cognitive disorder such as Alzheimer disease. This can be difficult because the cognitive complaints of normal aging overlap with the symptoms of early Alzheimer disease, and there are no clear rules for distinguishing the two.13

Clues that a more serious problem exists may come from details such as a history of decline in cognitive abilities, involvement of more than one domain, and the extent to which the problem disrupts daily functioning. 13 When evaluating the nature and severity of a cognitive disorder, one must take into account the patient’s level of education, premorbid intellectual and occupational functioning, and concurrent medical and psychiatric conditions. Clinicians must also consider the impact that medications, possible substance abuse, and language and culture of origin have on cognition.

The most common cognitive complaints in the elderly tend to be related to working memory (eg, recalling the name of a recent acquaintance or a telephone number that was just looked up).14 Other common complaints center on the speed of mental processing (eg, thinking quickly), memory (eg, recalling the name of an old acquaintance, or remembering where objects were placed or why one entered a room), executive function (eg, multitasking or planning a series of events), attention, and concentration.14

People with age-related cognitive changes can learn new information and recall previously learned information, although they may do so less rapidly and less efficiently. Furthermore, age-related cognitive change is not substantially progressive and does not significantly impair daily functioning.14 Nevertheless, complaints of cognitive changes should be monitored, since several studies showed that elderly people with cognitive complaints have an increased risk of developing dementia.15,16

 

 

Key warning signs

The Alzheimer’s Association17 lists 10 key warning signs of Alzheimer disease:

  • Memory loss
  • Difficulty performing familiar tasks
  • Problems with language
  • Disorientation to time and place
  • Poor or decreased judgment
  • Problems with abstract thought
  • Misplacing things
  • Changes in mood or behavior
  • Changes in personality
  • Loss of initiative.

As annotated on the Alzheimer’s Association Web site,17 the list also highlights key differences between normal aging and more serious symptoms of possible Alzheimer disease. For example, patients with Alzheimer disease are more likely to forget entire experiences and not remember them later, whereas normal elderly may forget parts of events and then recall the missing details later. Also, patients with Alzheimer disease are more likely to lose the ability to complete familiar tasks or to follow written or spoken directions. Additional signs that a more serious cognitive problem exists include misplacing items so often that it interferes with daily activities, frequently losing the thread of conversations, and repeating the same questions, stories, or comments within a short time without being aware of it.18

The key factor differentiating mild cognitive impairment from dementia is that the former does not significantly disrupt the ability to perform activities of daily living,4 although some mild degree of impairment in complex instrumental activities of daily living is likely present.19 Table 1 highlights some of the considerations discussed here for differentiating normal aging from mild cognitive impairment and Alzheimer disease.

Talk to a family member

Interviewing a reliable informant who knows the patient well is extremely helpful for determining the presence and extent of a cognitive problem. This is particularly important because even patients with mild cognitive impairment may have impaired awareness of their memory problems and may underestimate20 or overestimate21 the problem.

Ask the informant about symptoms such as being repetitive, misplacing items, or having trouble with finding words or names, remembering to take medication, managing finances, navigating while driving, or performing multiple tasks or all steps of a task. A change in behavior may be the first sign of a cognitive disorder, so the patient and informant should also be asked about signs of irritability, anxiety, increased social isolation, and decline in motivation.

Screening tests

Memory can be tested with a three- or four-word recall test during the physical examination, with the addition of a clock-drawing task,22 or can be assessed with a composite cognitive measure. For example:

The Mini-Mental State Exam (MMSE)23 can be given by the clinician or a trained member of the office staff. People with Alzheimer disease show progressive disability and a predictable rate of decline of approximately 2.8 points on the MMSE per year, with slower decline in the milder stages and faster decline in the moderate and severe stages of the illness.

The Montreal Cognitive Assessment Battery (MOCA, www.mocatest.org),24 is a new cognitive screening test with a 30-point format similar to that of the MMSE. It includes a five-word recall, clock-drawing, and executive and visuospatial items that make it more sensitive for mild cognitive impairment and vascular dementia.

The Alzheimer’s Disease 8 (AD8),25 a sensitive eight-question scale developed at Washington University, St. Louis, MO, can be completed by an informant in the waiting room.

New computerized screening measures are being developed that can be completed online or in the waiting room, and some simulate practical tasks such as using an automated teller machine and driving.

Care should be taken when interpreting performance on screening tests in patients who have very low or very high education levels, who are not tested in their native language, or who have physical or sensory deficits that might limit their performance.

Brain imaging and other tests

Patients with evidence of cognitive impairment should undergo a structural brain imaging test such as noncontrast computed tomography (CT) or magnetic resonance imaging (MRI) to evaluate for changes consistent with Alzheimer disease and to help rule out alternative causes of the cognitive impairment.26,27

Neuropsychologic testing can be done by a dementia specialist, who can also help with diagnosis and treatment.

Positron emission tomography (PET) using fluorodeoxyglucose shows patterns of brain metabolism and can help differentiate Alzheimer disease from non-Alzheimer dementia, as patients with the former typically show hypometabolism in the temporal and parietal cortices.28

Quantitative MRI and PET amyloid imaging are exciting new techniques currently being developed to diagnose Alzheimer disease earlier in clinical practice.29,30

Cerebrospinal fluid markers. A decrease in the amyloid beta 1–42 peptide and an increase in the tau and phosphotau proteins may be the earliest signs of Alzheimer disease.31,32 However, before these tests can be widely used in clinical practice, their sensitivity and specificity need to be established, people’s reluctance to undergo lumbar puncture will have to be overcome, and third-party reimbursement will have to be obtained.

Genetic factors also play an important role in the development of Alzheimer disease. The apolipoprotein E4 (ApoE4) allele is a marker for Alzheimer disease. People of European descent who possess one copy of the allele have three times the risk (with onset typically in their 70s), and individuals who are homozygous have 15 times the risk (with typical onset in their 60s), compared with people lacking ApoE4.33,34 This test is commercially available but is still considered a research tool.

 

 

CURRENT AND FUTURE TREATMENTS

Five drugs have been approved for treating Alzheimer disease: four cholinesterase inhibitors approved for mild to moderate disease and a glutamate N-methyl D-aspartate (NMDA) antagonist approved for moderate to severe disease.

Cholinesterase inhibitors for mild to moderate disease

The cholinesterase inhibitors tend to stabilize memory during the first year of treatment, and they may make the subsequent decline more gradual. The four current drugs have similar efficacy, so the choice is usually based on tolerability and ease of use.

Tacrine (Cognex) is rarely used because it must be taken four times a day, it can cause gastrointestinal adverse effects, and it can raise hepatic enzyme levels.

Donepezil (Aricept) is the drug most often prescribed because it can be taken once daily, a major benefit in older patients with memory loss. Also, its starting dose (5 mg) is a therapeutic dose. Donepezil was also recently approved for the treatment of severe Alzheimer disease on the basis of positive results in trials in patients with moderate to severe disease.35,36

Galantamine (Razadyne) comes in an extended-release formulation that can be taken once daily.

Rivastigmine (Exelon) is taken twice a day with food to reduce the risk of gastrointestinal adverse effects. It is also now available as a daily patch, which has a more favorable adverse-effect profile than oral rivastigmine.37

Memantine for moderate to severe disease

Memantine (Namenda), an NMDA antagonist, is approved for moderate to severe Alzheimer disease. The approval was based on a trial in which patients with advanced Alzheimer disease who received memantine monotherapy showed less decline in cognition and function after 6 months than those who received placebo,38 and another trial in which patients who received the combination of donepezil plus memantine showed more benefit than with donepezil alone.39

A treatment strategy

Recent guidelines recommend starting treatment with a cholinesterase inhibitor soon after Alzheimer disease is diagnosed and titrating the dose, as tolerated, to the high end of the therapeutic range.40 Once patients decline to the moderate stage of the illness, usually with an MMSE score of 10 to 20, memantine should be added and titrated upward to 10 mg twice a day. The medications should be continued as long as they are tolerated and the clinician feels there is some evidence they are helping.

The main benefit of the cholinesterase inhibitors in clinical trials is an attenuation of decline over time rather than an improvement in cognitive or behavioral symptoms. This should be considered when judging whether there has been a positive effect. It is also important to discuss this point with patients and their families, who may expect improvement rather than relative stability. Benefits of these drugs in later stages of the illness usually involve better recognition and engagement with family members and people around them and less severe behavioral disturbances, making care easier.36,41–43

Will drug therapy help in mild cognitive impairment?

Currently, no drugs are approved by the US Food and Drug Administration for patients with mild cognitive impairment, and the use of cholinesterase inhibitors in this population may not be reimbursed.

Six trials of cholinesterase inhibitors for mild cognitive impairment have been completed.44–47 On the whole, donepezil, rivastigmine, and galantamine had no effect on the primary end points in these trials, but they had some effects on some secondary ones.

In the Alzheimer Disease Cooperative Study,44 donepezil had no effect on the rate of progression from mild cognitive impairment to Alzheimer disease over the entire 3 years of the study, but it did reduce the rate in the first year of treatment. Moreover, the subgroup with one or two ApoE4 alleles benefitted over the entire 3 years.

A 24-week trial of donepezil in patients with mild cognitive impairment45 had negative results with regard to the selected study end points (two standardized tests), but there was evidence of cognitive benefit with donepezil on secondary measures such as the Alzheimer’s Disease Cognitive Assessment Scale-Cognitive Subscale,48 a widely used cognitive measure in Alzheimer disease trials, and in patients’ self-assessment of their memory.

One should discuss the risks and benefits of cholinesterase treatment with patients with mild cognitive impairment in whom underlying Alzheimer disease is strongly suspected.

Addressing behavioral problems

Behavioral problems are often the most disturbing symptoms in dementia, often leading to higher levels of care.

Apathy is the most common behavioral symptom in Alzheimer disease, increasing with disease severity.49 There is no approved treatment for these apathetic symptoms, though methylphenidate (Ritalin) and modafanil (Provigil) are being tested in small clinical trials.

Depression and irritability are common and may respond well to low doses of serotonin reuptake inhibitors.

Agitation and psychosis are distressing and are likely to overwhelm the caregiver’s ability to cope. Recent studies have raised concern about the safety and efficacy of atypical neuroleptics in patients with dementia and suggest that these drugs be used with careful monitoring.50

A safe, calm, predictable environment

Patients with Alzheimer disease function best in an environment that is safe, calm, and predictable, and their caregivers require ongoing support and education to develop realistic expectations throughout the course of the illness.

Behavioral treatments for problematic behaviors for which supportive evidence exists include reduction of environmental stressors and behavioral management of problematic behaviors.51–53 Such interventions typically include carefully observing and recording the problematic behavior, including its antecedents and situations under which it is most likely to occur, and then modifying the physical and interpersonal environment and schedule to reduce its occurrence.51

A challenge to the use of behavioral interventions in dementia is that the patient’s cognitive functioning is gradually declining, and this may require adjustments of interventions with time and in response to new behaviors that emerge.51 Referral to a behavioral specialist such as a geriatric psychiatrist may be helpful in managing disruptive and hard-to-treat behavioral problems.

 

 

Amyloid-lowering drugs are being tested

The cholinesterase inhibitors and memantine are symptomatic therapies that help maintain neuronal function but do not have a significant impact on the underlying disease process. Their benefits are mild, and treatments that modify the disease course are urgently needed.54,55

New disease-modifying agents are being tested to see if they delay disability, promote independence, and improve quality of life. Chief among these are compounds that reduce brain amyloid.

The amyloid cascade hypothesis is the current prevailing view of the pathogenesis of Alzheimer disease.56 Small molecules of extracellular amyloid are deposited in the brain early in the course of the disease. These oligomers of beta-amyloid gradually coalesce into fibrillar sheets that form the core of amyloid plaques. Amyloid invokes an immune response and stimulates the hyperphosphorylation of tau into intraneuronal neurofibrillary tangles. The accumulation of these tangles contributes to neuronal and synaptic loss, which correlates with dementia and disability.

The current disease-modifying strategies are designed to decrease the production of amyloid, inhibit fibrillogenesis, and promote clearance of the toxic amyloid beta 1–42 fragment. We should note, however, that the correlation between amyloid burden and clinical decline is not strong, and that lowering brain amyloid may not produce a measurable clinical benefit.57

Large-scale trials are being conducted with agents that modulate and inhibit gamma secretase, an enzyme involved in cleaving the amyloid precursor protein into the toxic fragment of beta amyloid.58 Early results show improvement in cognition and decreased amyloid levels in transgenic animals treated with these agents.

A recently completed phase III trial of tramiprosate, a glycosaminoglycan receptor inhibitor that interferes with fibrillization of amyloid, did not show positive results, but other antifibrillization agents are currently being tested.59,60

Exciting immunotherapeutic approaches that target the toxic fragment of beta amyloid have been developed. In the active vaccine approach, a small fragment of beta amyloid is injected to stimulate the production of beta amyloid antibodies to lower brain amyloid levels. However, although active vaccines are designed primarily to stimulate a B-cell response, they can cause adverse effects through unplanned stimulation of T cells.

Passive immunization with a monoclonal antibody against beta amyloid may be a safer strategy, and a number of compounds are undergoing clinical trials.61–63 Intravenous immune globulin contains antiamyloid antibodies and other immunomodulatory factors that may be useful in treating Alzheimer disease, and a phase III trial is being planned in view of positive results from earlier-phase studies.64

Future disease-modifying treatments

Treatments designed to prevent hyperphosphorylation of tau are also being pursued. Currently approved compounds such as lithium (Eskalith) and valproic acid (Depakene) have been shown to decrease the formation of neurofibrillary tangles in laboratory models. There is some retrospective epidemiologic evidence that statin treatment is associated with a lower incidence of Alzheimer disease and decreased amyloid deposition in in vitro preparations, and two large phase III trials of statins in addition to cholinesterase inhibitors are nearing completion.65,66

Aging is the strongest risk factor for Alzheimer disease, and future treatment targets will be derived from new insights into the biology of neuronal aging and senescence. Two recent phase III trials of xaliproden, a neurotrophin enhancer, were negative in patients with mild to moderate Alzheimer disease.67

Future mechanism-based treatments will be directed at reducing oxidative stress, promoting neurorestoration, and genetic modification. A summary of the disease-modifying strategies now being tested has recently been published (Table 3).

SOME RISK FACTORS ARE MODIFIABLE

Evidence is growing that nutritional factors (eg, dietary restriction, antioxidant intake, and the Mediterranean diet) and lifestyle factors (eg, social and mental activity and exercise) can promote healthy brain aging and delay the onset of Alzheimer disease.69,70

Animals on low-calorie diets live longer, and some epidemiologic studies have shown that people who consume fewer calories have a lower incidence of Alzheimer disease.69

Consuming fish two to three times per week appears to lower the incidence of Alzheimer disease, and a recent report in 2,254 elderly people followed for 4 years found that a Mediterranean diet of fish, olive oil, vegetables, and fruit had a protective effect.71

Resveratrol, a chemical found in red wine, is associated with longevity. A clinical trial of resveratrol to prevent Alzheimer disease is being planned.72–74 Compounds such as docosahexaenoic acid (an omega-3 fatty acid), a flavanoid found in green tea, and curcumin (a component of many curry dishes) are also associated with lowering levels of amyloid.75–77

Foods high in antioxidants may reduce the risk of Alzheimer disease.69,78 Daily folate supplements may have a protective effect, but antioxidants such as vitamin E and anti-inflammatory medications have shown disappointing results in preventing or treating Alzheimer disease and may have significant adverse effects.44,59,79,80

Evidence is also increasing that education, learning new skills, frequent socializing, and regularly engaging in physical exercise and mentally stimulating activities delay the onset of Alzheimer disease, and these pursuits should be encouraged.81–83 Also, treatment of cardiovascular risk factors such as hypertension and hyperlipidemia in mid-life and in older age may lower the rate of cognitive impairment in the elderly.84–86

ACKNOWLEDGMENT

The authors would like to thank Caroline O’Connor and Martha Dunlap for their assistance in preparing this manuscript.

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  41. Feldman H, Gauthier S, Hecker J, et al. Efficacy of donepezil on maintenance of activities of daily living in patients with moderate to severe Alzheimer’s disease and the effect on caregiver burden. J Am Geriatr Soc 2003; 51:737744.
  42. Cummings JL, Mackell J, Kaufer D. Behavioral effects of current Alzheimer’s disease treatment: a descriptive review. Alzheimers Dement 2008; 4:4960.
  43. Wilcock GK, Ballard CG, Cooper JA, Henrik L. Memantine for agitation/aggression and psychosis in moderately severe to severe Alzheimer’s disease: a pooled analysis of 3 studies. J Clin Psychiatry 2008; 69:341348.
  44. Petersen RC, Thomas RG, Grundman M, et al. Vitamin E and donepezil for the treatment of mild cognitive impairment. N Engl J Med 2005; 352:23792388.
  45. Salloway S, Ferris S, Kluger A, et al. Efficacy of donepezil in mild cognitive impairment: a randomized placebo-controlled trial. Neurology 2004; 63:651657.
  46. Feldman HH, Ferris S, Winblad B, et al. Effect of rivastigmine on delay to diagnosis of Alzheimer’s disease from mild cognitive impairment: the InDDEx study. Lancet Neurol 2007; 6:501512.
  47. Winblad B, Gauthier S, Scinto L, et al. Safety and efficacy of galantamine in subjects with mild cognitive impairment. Neurology 2008; 70:20242035.
  48. Mohs RC, Knopman D, Petersen RC, et al. Development of cognitive instruments for use in clinical trials of antidementia drugs: additions to the Alzheimer’s Disease Assessment Scale that broaden its scope. The Alzheimer’s Disease Cooperative Study. Alzheimer Dis Assoc Disord 1997; 11( suppl 2):S13S21.
  49. Mega MS, Cummings JL. Frontal-subcortical circuits and neuropsychiatric disorders. J Neuropsychiatry Clin Neurosci 1994; 6:358370.
  50. Schneider LS, Tariot PN, Dagerman KS, et al. Effectiveness of atypical antipsychotic drugs in patients with Alzheimer’s disease. N Engl J Med 2006; 355:15251538.
  51. Logsdon RG, McCurry SM, Teri L. Evidence-based psychological treatments for disruptive behaviors in individuals with dementia. Psychol Aging 2007; 22:2836.
  52. Overshott R, Byrne J, Burns A. Nonpharmacological and pharmacological interventions for symptoms in Alzheimer’s disease. Expert Rev Neurother 2004; 4:809821.
  53. Spira AP, Edelstein BA. Behavioral interventions for agitation in older adults with dementia: an evaluative review. Int Psychogeriatr 2006; 18:195225.
  54. Raina P, Santaguida P, Ismaila A, et al. Effectiveness of cholinesterase inhibitors and memantine for treating dementia: evidence review for a clinical practice guideline. Ann Intern Med 2008; 148:379397.
  55. Qaseem A, Snow V, Cross J, et al. Current pharmacologic treatment of dementia: a clinical practice guideline from the American College of Physicians and the American Academy of Family Physicians. Ann Intern Med 2008; 148:370378.
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  58. Geerts H. Drug evaluation: (R)-flurbiprofen—an enantiomer of flurbiprofen for the treatment of Alzheimer’s disease. IDrugs 2007; 10:121133.
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  60. Fenili D, Brown M, Rappaport R, McLaurin J. Properties of scylloinositol as a therapeutic treatment of AD-like pathology. J Mol Med 2007; 85:603611.
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  62. Masliah E, Hansen L, Adame A, et al. Abeta vaccination effects on plaque pathology in the absence of encephalitis in Alzheimer disease. Neurology 2005; 64:129131.
  63. Gilman S, Koller M, Black RS, et al. Clinical effects of Abeta immunization (AN1792) in patients with AD in an interrupted trial. Neurology 2005; 64:15531562.
  64. Dodel RC, Du Y, Depboylu C, et al. Intravenous immunoglobulins containing antibodies against beta-amyloid for the treatment of Alzheimer’s disease. J Neurol Neurosurg Psychiatry 2004; 75:14721474.
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Stephen Salloway, MD, MS
Professor of Clinical Neurosciences and Psychiatry, Alpert Medical School, Brown University; Director of Neurology and the Memory and Aging Program, Butler Hospital, Providence, RI

Stephen Correia, PhD
Assistant Professor of Psychiatry and Human Behavior, Alpert Medical School, Brown University; Veterans Administration Medical Center, Providence, RI

Address: Stephen Salloway, MD, MS, Department of Neurology, Butler Hospital, 345 Blackstone Boulevard, Providence, RI 02906; e-mail [email protected]

Dr. Salloway has received research support and honoraria from and has served as a consultant for Johnson and Johnson, Eisai, Pfizer, Forest, and Myriad Pharmaceuticals companies. He receives research support from Elan, Neurochem, and Cephalon companies and the National Institutes of Health. He is on the speaker panel for Novartis and Athena Diagnostics and has served as a consultant for sanofi-aventis and Merck companies.

Dr. Correia has received research support from the Alzheimer’s Association and the Rhode Island Foundation.

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Stephen Salloway, MD, MS
Professor of Clinical Neurosciences and Psychiatry, Alpert Medical School, Brown University; Director of Neurology and the Memory and Aging Program, Butler Hospital, Providence, RI

Stephen Correia, PhD
Assistant Professor of Psychiatry and Human Behavior, Alpert Medical School, Brown University; Veterans Administration Medical Center, Providence, RI

Address: Stephen Salloway, MD, MS, Department of Neurology, Butler Hospital, 345 Blackstone Boulevard, Providence, RI 02906; e-mail [email protected]

Dr. Salloway has received research support and honoraria from and has served as a consultant for Johnson and Johnson, Eisai, Pfizer, Forest, and Myriad Pharmaceuticals companies. He receives research support from Elan, Neurochem, and Cephalon companies and the National Institutes of Health. He is on the speaker panel for Novartis and Athena Diagnostics and has served as a consultant for sanofi-aventis and Merck companies.

Dr. Correia has received research support from the Alzheimer’s Association and the Rhode Island Foundation.

Author and Disclosure Information

Stephen Salloway, MD, MS
Professor of Clinical Neurosciences and Psychiatry, Alpert Medical School, Brown University; Director of Neurology and the Memory and Aging Program, Butler Hospital, Providence, RI

Stephen Correia, PhD
Assistant Professor of Psychiatry and Human Behavior, Alpert Medical School, Brown University; Veterans Administration Medical Center, Providence, RI

Address: Stephen Salloway, MD, MS, Department of Neurology, Butler Hospital, 345 Blackstone Boulevard, Providence, RI 02906; e-mail [email protected]

Dr. Salloway has received research support and honoraria from and has served as a consultant for Johnson and Johnson, Eisai, Pfizer, Forest, and Myriad Pharmaceuticals companies. He receives research support from Elan, Neurochem, and Cephalon companies and the National Institutes of Health. He is on the speaker panel for Novartis and Athena Diagnostics and has served as a consultant for sanofi-aventis and Merck companies.

Dr. Correia has received research support from the Alzheimer’s Association and the Rhode Island Foundation.

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The number of patients with Alzheimer disease, the most common cause of disability in the elderly, is about to rise dramatically. More than 5 million people in the United States are affected, and by 2050 this figure may rise to between 11 and 16 million.1 The prevalence doubles every 5 years from ages 65 to 85, so that Alzheimer disease affects 30% to 50% of all people at age 85.1,2

Primary care physicians bear the brunt of diagnosing and treating all these patients,3 requiring that they have the training to meet this critical public health problem.

But diagnosing this disease is not easy. In the early stages, it can be difficult to distinguish between the decline in certain cognitive functions due to normal aging (eg, name recall) and the mild cognitive impairment that often precedes Alzheimer disease.

Once a patient is diagnosed with Alzheimer disease, there needs to be a realistic discussion with the patient and family about what treatment with different drugs can—and cannot—accomplish.

ALZHEIMER DISEASE DIAGNOSIS: THE EARLIER, THE BETTER

While much has been accomplished in Alzheimer disease research in the last 20 years, a great deal remains to be done to improve its diagnosis and treatment. There is increasing evidence that early diagnosis of Alzheimer disease will be key to maximizing treatment benefits. But too often, patients are diagnosed in later stages of the disease, when disabling symptoms and neuropathologic changes have become well established.

Mild cognitive impairment: A predementia phase

The pathologic changes of Alzheimer disease typically begin many years before its clinical signs are apparent. Most patients pass through a predementia phase called mild cognitive impairment, with early memory loss but with relatively well-preserved activities of daily living.

From 6% to 25% of patients with mild cognitive impairment progress to dementia annually, a rate far higher than the incidence rate in the general population of 0.3% to 3.9% per year, depending on age.4,5 Therefore, patients with mild cognitive impairment are a good population in which to test interventions to prevent dementia.6,7

The concept of mild cognitive impairment is controversial because it is a transitional stage between normal aging and dementia rather than a distinct pathologic entity.8 Moreover, in some large community-based studies,9,10 a sizeable number of people with mild cognitive impairment reverted to normal cognitive function over 5 years, suggesting that mild cognitive impairment may be unstable over time.

Are other factors causing the dementia?

The Diagnostic and Statistical Manual IV-Text Revision11 defines dementia as memory loss and at least one other area of cognitive impairment, not due to delirium, that interferes with social and occupational functioning. Alzheimer disease is the most common cause of dementia in the United States.1

Still, Alzheimer disease does not typically exist in isolation. For example, while Alzheimer disease was the predominant cause of dementia in a recent postmortem series, 38% of dementia cases featured Alzheimer disease with lacunar infarction.12 Accordingly, clinicians must consider factors other than Alzheimer disease that could contribute to (or even fully account for) the complaints or observed deficits.

Is it Alzheimer disease or normal aging?

Although cognitive impairment and changes in behavior are common in the elderly, they are not a normal part of aging. Like other chronic disorders associated with aging, Alzheimer disease can be diagnosed and treated. Cognitive impairment may come to light when the patient or a family member reports a problem or the clinician asks about problems or observes signs of impairment in the office. The cognitive difficulties should be taken seriously, and their impact on daily functioning should be evaluated.

Certain cognitive functions such as mental flexibility and speed of processing decline in normal aging,13 and many older people report cognitive symptoms. Therefore, it is important to differentiate mild age-associated cognitive changes from the beginning of a cognitive disorder such as Alzheimer disease. This can be difficult because the cognitive complaints of normal aging overlap with the symptoms of early Alzheimer disease, and there are no clear rules for distinguishing the two.13

Clues that a more serious problem exists may come from details such as a history of decline in cognitive abilities, involvement of more than one domain, and the extent to which the problem disrupts daily functioning. 13 When evaluating the nature and severity of a cognitive disorder, one must take into account the patient’s level of education, premorbid intellectual and occupational functioning, and concurrent medical and psychiatric conditions. Clinicians must also consider the impact that medications, possible substance abuse, and language and culture of origin have on cognition.

The most common cognitive complaints in the elderly tend to be related to working memory (eg, recalling the name of a recent acquaintance or a telephone number that was just looked up).14 Other common complaints center on the speed of mental processing (eg, thinking quickly), memory (eg, recalling the name of an old acquaintance, or remembering where objects were placed or why one entered a room), executive function (eg, multitasking or planning a series of events), attention, and concentration.14

People with age-related cognitive changes can learn new information and recall previously learned information, although they may do so less rapidly and less efficiently. Furthermore, age-related cognitive change is not substantially progressive and does not significantly impair daily functioning.14 Nevertheless, complaints of cognitive changes should be monitored, since several studies showed that elderly people with cognitive complaints have an increased risk of developing dementia.15,16

 

 

Key warning signs

The Alzheimer’s Association17 lists 10 key warning signs of Alzheimer disease:

  • Memory loss
  • Difficulty performing familiar tasks
  • Problems with language
  • Disorientation to time and place
  • Poor or decreased judgment
  • Problems with abstract thought
  • Misplacing things
  • Changes in mood or behavior
  • Changes in personality
  • Loss of initiative.

As annotated on the Alzheimer’s Association Web site,17 the list also highlights key differences between normal aging and more serious symptoms of possible Alzheimer disease. For example, patients with Alzheimer disease are more likely to forget entire experiences and not remember them later, whereas normal elderly may forget parts of events and then recall the missing details later. Also, patients with Alzheimer disease are more likely to lose the ability to complete familiar tasks or to follow written or spoken directions. Additional signs that a more serious cognitive problem exists include misplacing items so often that it interferes with daily activities, frequently losing the thread of conversations, and repeating the same questions, stories, or comments within a short time without being aware of it.18

The key factor differentiating mild cognitive impairment from dementia is that the former does not significantly disrupt the ability to perform activities of daily living,4 although some mild degree of impairment in complex instrumental activities of daily living is likely present.19 Table 1 highlights some of the considerations discussed here for differentiating normal aging from mild cognitive impairment and Alzheimer disease.

Talk to a family member

Interviewing a reliable informant who knows the patient well is extremely helpful for determining the presence and extent of a cognitive problem. This is particularly important because even patients with mild cognitive impairment may have impaired awareness of their memory problems and may underestimate20 or overestimate21 the problem.

Ask the informant about symptoms such as being repetitive, misplacing items, or having trouble with finding words or names, remembering to take medication, managing finances, navigating while driving, or performing multiple tasks or all steps of a task. A change in behavior may be the first sign of a cognitive disorder, so the patient and informant should also be asked about signs of irritability, anxiety, increased social isolation, and decline in motivation.

Screening tests

Memory can be tested with a three- or four-word recall test during the physical examination, with the addition of a clock-drawing task,22 or can be assessed with a composite cognitive measure. For example:

The Mini-Mental State Exam (MMSE)23 can be given by the clinician or a trained member of the office staff. People with Alzheimer disease show progressive disability and a predictable rate of decline of approximately 2.8 points on the MMSE per year, with slower decline in the milder stages and faster decline in the moderate and severe stages of the illness.

The Montreal Cognitive Assessment Battery (MOCA, www.mocatest.org),24 is a new cognitive screening test with a 30-point format similar to that of the MMSE. It includes a five-word recall, clock-drawing, and executive and visuospatial items that make it more sensitive for mild cognitive impairment and vascular dementia.

The Alzheimer’s Disease 8 (AD8),25 a sensitive eight-question scale developed at Washington University, St. Louis, MO, can be completed by an informant in the waiting room.

New computerized screening measures are being developed that can be completed online or in the waiting room, and some simulate practical tasks such as using an automated teller machine and driving.

Care should be taken when interpreting performance on screening tests in patients who have very low or very high education levels, who are not tested in their native language, or who have physical or sensory deficits that might limit their performance.

Brain imaging and other tests

Patients with evidence of cognitive impairment should undergo a structural brain imaging test such as noncontrast computed tomography (CT) or magnetic resonance imaging (MRI) to evaluate for changes consistent with Alzheimer disease and to help rule out alternative causes of the cognitive impairment.26,27

Neuropsychologic testing can be done by a dementia specialist, who can also help with diagnosis and treatment.

Positron emission tomography (PET) using fluorodeoxyglucose shows patterns of brain metabolism and can help differentiate Alzheimer disease from non-Alzheimer dementia, as patients with the former typically show hypometabolism in the temporal and parietal cortices.28

Quantitative MRI and PET amyloid imaging are exciting new techniques currently being developed to diagnose Alzheimer disease earlier in clinical practice.29,30

Cerebrospinal fluid markers. A decrease in the amyloid beta 1–42 peptide and an increase in the tau and phosphotau proteins may be the earliest signs of Alzheimer disease.31,32 However, before these tests can be widely used in clinical practice, their sensitivity and specificity need to be established, people’s reluctance to undergo lumbar puncture will have to be overcome, and third-party reimbursement will have to be obtained.

Genetic factors also play an important role in the development of Alzheimer disease. The apolipoprotein E4 (ApoE4) allele is a marker for Alzheimer disease. People of European descent who possess one copy of the allele have three times the risk (with onset typically in their 70s), and individuals who are homozygous have 15 times the risk (with typical onset in their 60s), compared with people lacking ApoE4.33,34 This test is commercially available but is still considered a research tool.

 

 

CURRENT AND FUTURE TREATMENTS

Five drugs have been approved for treating Alzheimer disease: four cholinesterase inhibitors approved for mild to moderate disease and a glutamate N-methyl D-aspartate (NMDA) antagonist approved for moderate to severe disease.

Cholinesterase inhibitors for mild to moderate disease

The cholinesterase inhibitors tend to stabilize memory during the first year of treatment, and they may make the subsequent decline more gradual. The four current drugs have similar efficacy, so the choice is usually based on tolerability and ease of use.

Tacrine (Cognex) is rarely used because it must be taken four times a day, it can cause gastrointestinal adverse effects, and it can raise hepatic enzyme levels.

Donepezil (Aricept) is the drug most often prescribed because it can be taken once daily, a major benefit in older patients with memory loss. Also, its starting dose (5 mg) is a therapeutic dose. Donepezil was also recently approved for the treatment of severe Alzheimer disease on the basis of positive results in trials in patients with moderate to severe disease.35,36

Galantamine (Razadyne) comes in an extended-release formulation that can be taken once daily.

Rivastigmine (Exelon) is taken twice a day with food to reduce the risk of gastrointestinal adverse effects. It is also now available as a daily patch, which has a more favorable adverse-effect profile than oral rivastigmine.37

Memantine for moderate to severe disease

Memantine (Namenda), an NMDA antagonist, is approved for moderate to severe Alzheimer disease. The approval was based on a trial in which patients with advanced Alzheimer disease who received memantine monotherapy showed less decline in cognition and function after 6 months than those who received placebo,38 and another trial in which patients who received the combination of donepezil plus memantine showed more benefit than with donepezil alone.39

A treatment strategy

Recent guidelines recommend starting treatment with a cholinesterase inhibitor soon after Alzheimer disease is diagnosed and titrating the dose, as tolerated, to the high end of the therapeutic range.40 Once patients decline to the moderate stage of the illness, usually with an MMSE score of 10 to 20, memantine should be added and titrated upward to 10 mg twice a day. The medications should be continued as long as they are tolerated and the clinician feels there is some evidence they are helping.

The main benefit of the cholinesterase inhibitors in clinical trials is an attenuation of decline over time rather than an improvement in cognitive or behavioral symptoms. This should be considered when judging whether there has been a positive effect. It is also important to discuss this point with patients and their families, who may expect improvement rather than relative stability. Benefits of these drugs in later stages of the illness usually involve better recognition and engagement with family members and people around them and less severe behavioral disturbances, making care easier.36,41–43

Will drug therapy help in mild cognitive impairment?

Currently, no drugs are approved by the US Food and Drug Administration for patients with mild cognitive impairment, and the use of cholinesterase inhibitors in this population may not be reimbursed.

Six trials of cholinesterase inhibitors for mild cognitive impairment have been completed.44–47 On the whole, donepezil, rivastigmine, and galantamine had no effect on the primary end points in these trials, but they had some effects on some secondary ones.

In the Alzheimer Disease Cooperative Study,44 donepezil had no effect on the rate of progression from mild cognitive impairment to Alzheimer disease over the entire 3 years of the study, but it did reduce the rate in the first year of treatment. Moreover, the subgroup with one or two ApoE4 alleles benefitted over the entire 3 years.

A 24-week trial of donepezil in patients with mild cognitive impairment45 had negative results with regard to the selected study end points (two standardized tests), but there was evidence of cognitive benefit with donepezil on secondary measures such as the Alzheimer’s Disease Cognitive Assessment Scale-Cognitive Subscale,48 a widely used cognitive measure in Alzheimer disease trials, and in patients’ self-assessment of their memory.

One should discuss the risks and benefits of cholinesterase treatment with patients with mild cognitive impairment in whom underlying Alzheimer disease is strongly suspected.

Addressing behavioral problems

Behavioral problems are often the most disturbing symptoms in dementia, often leading to higher levels of care.

Apathy is the most common behavioral symptom in Alzheimer disease, increasing with disease severity.49 There is no approved treatment for these apathetic symptoms, though methylphenidate (Ritalin) and modafanil (Provigil) are being tested in small clinical trials.

Depression and irritability are common and may respond well to low doses of serotonin reuptake inhibitors.

Agitation and psychosis are distressing and are likely to overwhelm the caregiver’s ability to cope. Recent studies have raised concern about the safety and efficacy of atypical neuroleptics in patients with dementia and suggest that these drugs be used with careful monitoring.50

A safe, calm, predictable environment

Patients with Alzheimer disease function best in an environment that is safe, calm, and predictable, and their caregivers require ongoing support and education to develop realistic expectations throughout the course of the illness.

Behavioral treatments for problematic behaviors for which supportive evidence exists include reduction of environmental stressors and behavioral management of problematic behaviors.51–53 Such interventions typically include carefully observing and recording the problematic behavior, including its antecedents and situations under which it is most likely to occur, and then modifying the physical and interpersonal environment and schedule to reduce its occurrence.51

A challenge to the use of behavioral interventions in dementia is that the patient’s cognitive functioning is gradually declining, and this may require adjustments of interventions with time and in response to new behaviors that emerge.51 Referral to a behavioral specialist such as a geriatric psychiatrist may be helpful in managing disruptive and hard-to-treat behavioral problems.

 

 

Amyloid-lowering drugs are being tested

The cholinesterase inhibitors and memantine are symptomatic therapies that help maintain neuronal function but do not have a significant impact on the underlying disease process. Their benefits are mild, and treatments that modify the disease course are urgently needed.54,55

New disease-modifying agents are being tested to see if they delay disability, promote independence, and improve quality of life. Chief among these are compounds that reduce brain amyloid.

The amyloid cascade hypothesis is the current prevailing view of the pathogenesis of Alzheimer disease.56 Small molecules of extracellular amyloid are deposited in the brain early in the course of the disease. These oligomers of beta-amyloid gradually coalesce into fibrillar sheets that form the core of amyloid plaques. Amyloid invokes an immune response and stimulates the hyperphosphorylation of tau into intraneuronal neurofibrillary tangles. The accumulation of these tangles contributes to neuronal and synaptic loss, which correlates with dementia and disability.

The current disease-modifying strategies are designed to decrease the production of amyloid, inhibit fibrillogenesis, and promote clearance of the toxic amyloid beta 1–42 fragment. We should note, however, that the correlation between amyloid burden and clinical decline is not strong, and that lowering brain amyloid may not produce a measurable clinical benefit.57

Large-scale trials are being conducted with agents that modulate and inhibit gamma secretase, an enzyme involved in cleaving the amyloid precursor protein into the toxic fragment of beta amyloid.58 Early results show improvement in cognition and decreased amyloid levels in transgenic animals treated with these agents.

A recently completed phase III trial of tramiprosate, a glycosaminoglycan receptor inhibitor that interferes with fibrillization of amyloid, did not show positive results, but other antifibrillization agents are currently being tested.59,60

Exciting immunotherapeutic approaches that target the toxic fragment of beta amyloid have been developed. In the active vaccine approach, a small fragment of beta amyloid is injected to stimulate the production of beta amyloid antibodies to lower brain amyloid levels. However, although active vaccines are designed primarily to stimulate a B-cell response, they can cause adverse effects through unplanned stimulation of T cells.

Passive immunization with a monoclonal antibody against beta amyloid may be a safer strategy, and a number of compounds are undergoing clinical trials.61–63 Intravenous immune globulin contains antiamyloid antibodies and other immunomodulatory factors that may be useful in treating Alzheimer disease, and a phase III trial is being planned in view of positive results from earlier-phase studies.64

Future disease-modifying treatments

Treatments designed to prevent hyperphosphorylation of tau are also being pursued. Currently approved compounds such as lithium (Eskalith) and valproic acid (Depakene) have been shown to decrease the formation of neurofibrillary tangles in laboratory models. There is some retrospective epidemiologic evidence that statin treatment is associated with a lower incidence of Alzheimer disease and decreased amyloid deposition in in vitro preparations, and two large phase III trials of statins in addition to cholinesterase inhibitors are nearing completion.65,66

Aging is the strongest risk factor for Alzheimer disease, and future treatment targets will be derived from new insights into the biology of neuronal aging and senescence. Two recent phase III trials of xaliproden, a neurotrophin enhancer, were negative in patients with mild to moderate Alzheimer disease.67

Future mechanism-based treatments will be directed at reducing oxidative stress, promoting neurorestoration, and genetic modification. A summary of the disease-modifying strategies now being tested has recently been published (Table 3).

SOME RISK FACTORS ARE MODIFIABLE

Evidence is growing that nutritional factors (eg, dietary restriction, antioxidant intake, and the Mediterranean diet) and lifestyle factors (eg, social and mental activity and exercise) can promote healthy brain aging and delay the onset of Alzheimer disease.69,70

Animals on low-calorie diets live longer, and some epidemiologic studies have shown that people who consume fewer calories have a lower incidence of Alzheimer disease.69

Consuming fish two to three times per week appears to lower the incidence of Alzheimer disease, and a recent report in 2,254 elderly people followed for 4 years found that a Mediterranean diet of fish, olive oil, vegetables, and fruit had a protective effect.71

Resveratrol, a chemical found in red wine, is associated with longevity. A clinical trial of resveratrol to prevent Alzheimer disease is being planned.72–74 Compounds such as docosahexaenoic acid (an omega-3 fatty acid), a flavanoid found in green tea, and curcumin (a component of many curry dishes) are also associated with lowering levels of amyloid.75–77

Foods high in antioxidants may reduce the risk of Alzheimer disease.69,78 Daily folate supplements may have a protective effect, but antioxidants such as vitamin E and anti-inflammatory medications have shown disappointing results in preventing or treating Alzheimer disease and may have significant adverse effects.44,59,79,80

Evidence is also increasing that education, learning new skills, frequent socializing, and regularly engaging in physical exercise and mentally stimulating activities delay the onset of Alzheimer disease, and these pursuits should be encouraged.81–83 Also, treatment of cardiovascular risk factors such as hypertension and hyperlipidemia in mid-life and in older age may lower the rate of cognitive impairment in the elderly.84–86

ACKNOWLEDGMENT

The authors would like to thank Caroline O’Connor and Martha Dunlap for their assistance in preparing this manuscript.

The number of patients with Alzheimer disease, the most common cause of disability in the elderly, is about to rise dramatically. More than 5 million people in the United States are affected, and by 2050 this figure may rise to between 11 and 16 million.1 The prevalence doubles every 5 years from ages 65 to 85, so that Alzheimer disease affects 30% to 50% of all people at age 85.1,2

Primary care physicians bear the brunt of diagnosing and treating all these patients,3 requiring that they have the training to meet this critical public health problem.

But diagnosing this disease is not easy. In the early stages, it can be difficult to distinguish between the decline in certain cognitive functions due to normal aging (eg, name recall) and the mild cognitive impairment that often precedes Alzheimer disease.

Once a patient is diagnosed with Alzheimer disease, there needs to be a realistic discussion with the patient and family about what treatment with different drugs can—and cannot—accomplish.

ALZHEIMER DISEASE DIAGNOSIS: THE EARLIER, THE BETTER

While much has been accomplished in Alzheimer disease research in the last 20 years, a great deal remains to be done to improve its diagnosis and treatment. There is increasing evidence that early diagnosis of Alzheimer disease will be key to maximizing treatment benefits. But too often, patients are diagnosed in later stages of the disease, when disabling symptoms and neuropathologic changes have become well established.

Mild cognitive impairment: A predementia phase

The pathologic changes of Alzheimer disease typically begin many years before its clinical signs are apparent. Most patients pass through a predementia phase called mild cognitive impairment, with early memory loss but with relatively well-preserved activities of daily living.

From 6% to 25% of patients with mild cognitive impairment progress to dementia annually, a rate far higher than the incidence rate in the general population of 0.3% to 3.9% per year, depending on age.4,5 Therefore, patients with mild cognitive impairment are a good population in which to test interventions to prevent dementia.6,7

The concept of mild cognitive impairment is controversial because it is a transitional stage between normal aging and dementia rather than a distinct pathologic entity.8 Moreover, in some large community-based studies,9,10 a sizeable number of people with mild cognitive impairment reverted to normal cognitive function over 5 years, suggesting that mild cognitive impairment may be unstable over time.

Are other factors causing the dementia?

The Diagnostic and Statistical Manual IV-Text Revision11 defines dementia as memory loss and at least one other area of cognitive impairment, not due to delirium, that interferes with social and occupational functioning. Alzheimer disease is the most common cause of dementia in the United States.1

Still, Alzheimer disease does not typically exist in isolation. For example, while Alzheimer disease was the predominant cause of dementia in a recent postmortem series, 38% of dementia cases featured Alzheimer disease with lacunar infarction.12 Accordingly, clinicians must consider factors other than Alzheimer disease that could contribute to (or even fully account for) the complaints or observed deficits.

Is it Alzheimer disease or normal aging?

Although cognitive impairment and changes in behavior are common in the elderly, they are not a normal part of aging. Like other chronic disorders associated with aging, Alzheimer disease can be diagnosed and treated. Cognitive impairment may come to light when the patient or a family member reports a problem or the clinician asks about problems or observes signs of impairment in the office. The cognitive difficulties should be taken seriously, and their impact on daily functioning should be evaluated.

Certain cognitive functions such as mental flexibility and speed of processing decline in normal aging,13 and many older people report cognitive symptoms. Therefore, it is important to differentiate mild age-associated cognitive changes from the beginning of a cognitive disorder such as Alzheimer disease. This can be difficult because the cognitive complaints of normal aging overlap with the symptoms of early Alzheimer disease, and there are no clear rules for distinguishing the two.13

Clues that a more serious problem exists may come from details such as a history of decline in cognitive abilities, involvement of more than one domain, and the extent to which the problem disrupts daily functioning. 13 When evaluating the nature and severity of a cognitive disorder, one must take into account the patient’s level of education, premorbid intellectual and occupational functioning, and concurrent medical and psychiatric conditions. Clinicians must also consider the impact that medications, possible substance abuse, and language and culture of origin have on cognition.

The most common cognitive complaints in the elderly tend to be related to working memory (eg, recalling the name of a recent acquaintance or a telephone number that was just looked up).14 Other common complaints center on the speed of mental processing (eg, thinking quickly), memory (eg, recalling the name of an old acquaintance, or remembering where objects were placed or why one entered a room), executive function (eg, multitasking or planning a series of events), attention, and concentration.14

People with age-related cognitive changes can learn new information and recall previously learned information, although they may do so less rapidly and less efficiently. Furthermore, age-related cognitive change is not substantially progressive and does not significantly impair daily functioning.14 Nevertheless, complaints of cognitive changes should be monitored, since several studies showed that elderly people with cognitive complaints have an increased risk of developing dementia.15,16

 

 

Key warning signs

The Alzheimer’s Association17 lists 10 key warning signs of Alzheimer disease:

  • Memory loss
  • Difficulty performing familiar tasks
  • Problems with language
  • Disorientation to time and place
  • Poor or decreased judgment
  • Problems with abstract thought
  • Misplacing things
  • Changes in mood or behavior
  • Changes in personality
  • Loss of initiative.

As annotated on the Alzheimer’s Association Web site,17 the list also highlights key differences between normal aging and more serious symptoms of possible Alzheimer disease. For example, patients with Alzheimer disease are more likely to forget entire experiences and not remember them later, whereas normal elderly may forget parts of events and then recall the missing details later. Also, patients with Alzheimer disease are more likely to lose the ability to complete familiar tasks or to follow written or spoken directions. Additional signs that a more serious cognitive problem exists include misplacing items so often that it interferes with daily activities, frequently losing the thread of conversations, and repeating the same questions, stories, or comments within a short time without being aware of it.18

The key factor differentiating mild cognitive impairment from dementia is that the former does not significantly disrupt the ability to perform activities of daily living,4 although some mild degree of impairment in complex instrumental activities of daily living is likely present.19 Table 1 highlights some of the considerations discussed here for differentiating normal aging from mild cognitive impairment and Alzheimer disease.

Talk to a family member

Interviewing a reliable informant who knows the patient well is extremely helpful for determining the presence and extent of a cognitive problem. This is particularly important because even patients with mild cognitive impairment may have impaired awareness of their memory problems and may underestimate20 or overestimate21 the problem.

Ask the informant about symptoms such as being repetitive, misplacing items, or having trouble with finding words or names, remembering to take medication, managing finances, navigating while driving, or performing multiple tasks or all steps of a task. A change in behavior may be the first sign of a cognitive disorder, so the patient and informant should also be asked about signs of irritability, anxiety, increased social isolation, and decline in motivation.

Screening tests

Memory can be tested with a three- or four-word recall test during the physical examination, with the addition of a clock-drawing task,22 or can be assessed with a composite cognitive measure. For example:

The Mini-Mental State Exam (MMSE)23 can be given by the clinician or a trained member of the office staff. People with Alzheimer disease show progressive disability and a predictable rate of decline of approximately 2.8 points on the MMSE per year, with slower decline in the milder stages and faster decline in the moderate and severe stages of the illness.

The Montreal Cognitive Assessment Battery (MOCA, www.mocatest.org),24 is a new cognitive screening test with a 30-point format similar to that of the MMSE. It includes a five-word recall, clock-drawing, and executive and visuospatial items that make it more sensitive for mild cognitive impairment and vascular dementia.

The Alzheimer’s Disease 8 (AD8),25 a sensitive eight-question scale developed at Washington University, St. Louis, MO, can be completed by an informant in the waiting room.

New computerized screening measures are being developed that can be completed online or in the waiting room, and some simulate practical tasks such as using an automated teller machine and driving.

Care should be taken when interpreting performance on screening tests in patients who have very low or very high education levels, who are not tested in their native language, or who have physical or sensory deficits that might limit their performance.

Brain imaging and other tests

Patients with evidence of cognitive impairment should undergo a structural brain imaging test such as noncontrast computed tomography (CT) or magnetic resonance imaging (MRI) to evaluate for changes consistent with Alzheimer disease and to help rule out alternative causes of the cognitive impairment.26,27

Neuropsychologic testing can be done by a dementia specialist, who can also help with diagnosis and treatment.

Positron emission tomography (PET) using fluorodeoxyglucose shows patterns of brain metabolism and can help differentiate Alzheimer disease from non-Alzheimer dementia, as patients with the former typically show hypometabolism in the temporal and parietal cortices.28

Quantitative MRI and PET amyloid imaging are exciting new techniques currently being developed to diagnose Alzheimer disease earlier in clinical practice.29,30

Cerebrospinal fluid markers. A decrease in the amyloid beta 1–42 peptide and an increase in the tau and phosphotau proteins may be the earliest signs of Alzheimer disease.31,32 However, before these tests can be widely used in clinical practice, their sensitivity and specificity need to be established, people’s reluctance to undergo lumbar puncture will have to be overcome, and third-party reimbursement will have to be obtained.

Genetic factors also play an important role in the development of Alzheimer disease. The apolipoprotein E4 (ApoE4) allele is a marker for Alzheimer disease. People of European descent who possess one copy of the allele have three times the risk (with onset typically in their 70s), and individuals who are homozygous have 15 times the risk (with typical onset in their 60s), compared with people lacking ApoE4.33,34 This test is commercially available but is still considered a research tool.

 

 

CURRENT AND FUTURE TREATMENTS

Five drugs have been approved for treating Alzheimer disease: four cholinesterase inhibitors approved for mild to moderate disease and a glutamate N-methyl D-aspartate (NMDA) antagonist approved for moderate to severe disease.

Cholinesterase inhibitors for mild to moderate disease

The cholinesterase inhibitors tend to stabilize memory during the first year of treatment, and they may make the subsequent decline more gradual. The four current drugs have similar efficacy, so the choice is usually based on tolerability and ease of use.

Tacrine (Cognex) is rarely used because it must be taken four times a day, it can cause gastrointestinal adverse effects, and it can raise hepatic enzyme levels.

Donepezil (Aricept) is the drug most often prescribed because it can be taken once daily, a major benefit in older patients with memory loss. Also, its starting dose (5 mg) is a therapeutic dose. Donepezil was also recently approved for the treatment of severe Alzheimer disease on the basis of positive results in trials in patients with moderate to severe disease.35,36

Galantamine (Razadyne) comes in an extended-release formulation that can be taken once daily.

Rivastigmine (Exelon) is taken twice a day with food to reduce the risk of gastrointestinal adverse effects. It is also now available as a daily patch, which has a more favorable adverse-effect profile than oral rivastigmine.37

Memantine for moderate to severe disease

Memantine (Namenda), an NMDA antagonist, is approved for moderate to severe Alzheimer disease. The approval was based on a trial in which patients with advanced Alzheimer disease who received memantine monotherapy showed less decline in cognition and function after 6 months than those who received placebo,38 and another trial in which patients who received the combination of donepezil plus memantine showed more benefit than with donepezil alone.39

A treatment strategy

Recent guidelines recommend starting treatment with a cholinesterase inhibitor soon after Alzheimer disease is diagnosed and titrating the dose, as tolerated, to the high end of the therapeutic range.40 Once patients decline to the moderate stage of the illness, usually with an MMSE score of 10 to 20, memantine should be added and titrated upward to 10 mg twice a day. The medications should be continued as long as they are tolerated and the clinician feels there is some evidence they are helping.

The main benefit of the cholinesterase inhibitors in clinical trials is an attenuation of decline over time rather than an improvement in cognitive or behavioral symptoms. This should be considered when judging whether there has been a positive effect. It is also important to discuss this point with patients and their families, who may expect improvement rather than relative stability. Benefits of these drugs in later stages of the illness usually involve better recognition and engagement with family members and people around them and less severe behavioral disturbances, making care easier.36,41–43

Will drug therapy help in mild cognitive impairment?

Currently, no drugs are approved by the US Food and Drug Administration for patients with mild cognitive impairment, and the use of cholinesterase inhibitors in this population may not be reimbursed.

Six trials of cholinesterase inhibitors for mild cognitive impairment have been completed.44–47 On the whole, donepezil, rivastigmine, and galantamine had no effect on the primary end points in these trials, but they had some effects on some secondary ones.

In the Alzheimer Disease Cooperative Study,44 donepezil had no effect on the rate of progression from mild cognitive impairment to Alzheimer disease over the entire 3 years of the study, but it did reduce the rate in the first year of treatment. Moreover, the subgroup with one or two ApoE4 alleles benefitted over the entire 3 years.

A 24-week trial of donepezil in patients with mild cognitive impairment45 had negative results with regard to the selected study end points (two standardized tests), but there was evidence of cognitive benefit with donepezil on secondary measures such as the Alzheimer’s Disease Cognitive Assessment Scale-Cognitive Subscale,48 a widely used cognitive measure in Alzheimer disease trials, and in patients’ self-assessment of their memory.

One should discuss the risks and benefits of cholinesterase treatment with patients with mild cognitive impairment in whom underlying Alzheimer disease is strongly suspected.

Addressing behavioral problems

Behavioral problems are often the most disturbing symptoms in dementia, often leading to higher levels of care.

Apathy is the most common behavioral symptom in Alzheimer disease, increasing with disease severity.49 There is no approved treatment for these apathetic symptoms, though methylphenidate (Ritalin) and modafanil (Provigil) are being tested in small clinical trials.

Depression and irritability are common and may respond well to low doses of serotonin reuptake inhibitors.

Agitation and psychosis are distressing and are likely to overwhelm the caregiver’s ability to cope. Recent studies have raised concern about the safety and efficacy of atypical neuroleptics in patients with dementia and suggest that these drugs be used with careful monitoring.50

A safe, calm, predictable environment

Patients with Alzheimer disease function best in an environment that is safe, calm, and predictable, and their caregivers require ongoing support and education to develop realistic expectations throughout the course of the illness.

Behavioral treatments for problematic behaviors for which supportive evidence exists include reduction of environmental stressors and behavioral management of problematic behaviors.51–53 Such interventions typically include carefully observing and recording the problematic behavior, including its antecedents and situations under which it is most likely to occur, and then modifying the physical and interpersonal environment and schedule to reduce its occurrence.51

A challenge to the use of behavioral interventions in dementia is that the patient’s cognitive functioning is gradually declining, and this may require adjustments of interventions with time and in response to new behaviors that emerge.51 Referral to a behavioral specialist such as a geriatric psychiatrist may be helpful in managing disruptive and hard-to-treat behavioral problems.

 

 

Amyloid-lowering drugs are being tested

The cholinesterase inhibitors and memantine are symptomatic therapies that help maintain neuronal function but do not have a significant impact on the underlying disease process. Their benefits are mild, and treatments that modify the disease course are urgently needed.54,55

New disease-modifying agents are being tested to see if they delay disability, promote independence, and improve quality of life. Chief among these are compounds that reduce brain amyloid.

The amyloid cascade hypothesis is the current prevailing view of the pathogenesis of Alzheimer disease.56 Small molecules of extracellular amyloid are deposited in the brain early in the course of the disease. These oligomers of beta-amyloid gradually coalesce into fibrillar sheets that form the core of amyloid plaques. Amyloid invokes an immune response and stimulates the hyperphosphorylation of tau into intraneuronal neurofibrillary tangles. The accumulation of these tangles contributes to neuronal and synaptic loss, which correlates with dementia and disability.

The current disease-modifying strategies are designed to decrease the production of amyloid, inhibit fibrillogenesis, and promote clearance of the toxic amyloid beta 1–42 fragment. We should note, however, that the correlation between amyloid burden and clinical decline is not strong, and that lowering brain amyloid may not produce a measurable clinical benefit.57

Large-scale trials are being conducted with agents that modulate and inhibit gamma secretase, an enzyme involved in cleaving the amyloid precursor protein into the toxic fragment of beta amyloid.58 Early results show improvement in cognition and decreased amyloid levels in transgenic animals treated with these agents.

A recently completed phase III trial of tramiprosate, a glycosaminoglycan receptor inhibitor that interferes with fibrillization of amyloid, did not show positive results, but other antifibrillization agents are currently being tested.59,60

Exciting immunotherapeutic approaches that target the toxic fragment of beta amyloid have been developed. In the active vaccine approach, a small fragment of beta amyloid is injected to stimulate the production of beta amyloid antibodies to lower brain amyloid levels. However, although active vaccines are designed primarily to stimulate a B-cell response, they can cause adverse effects through unplanned stimulation of T cells.

Passive immunization with a monoclonal antibody against beta amyloid may be a safer strategy, and a number of compounds are undergoing clinical trials.61–63 Intravenous immune globulin contains antiamyloid antibodies and other immunomodulatory factors that may be useful in treating Alzheimer disease, and a phase III trial is being planned in view of positive results from earlier-phase studies.64

Future disease-modifying treatments

Treatments designed to prevent hyperphosphorylation of tau are also being pursued. Currently approved compounds such as lithium (Eskalith) and valproic acid (Depakene) have been shown to decrease the formation of neurofibrillary tangles in laboratory models. There is some retrospective epidemiologic evidence that statin treatment is associated with a lower incidence of Alzheimer disease and decreased amyloid deposition in in vitro preparations, and two large phase III trials of statins in addition to cholinesterase inhibitors are nearing completion.65,66

Aging is the strongest risk factor for Alzheimer disease, and future treatment targets will be derived from new insights into the biology of neuronal aging and senescence. Two recent phase III trials of xaliproden, a neurotrophin enhancer, were negative in patients with mild to moderate Alzheimer disease.67

Future mechanism-based treatments will be directed at reducing oxidative stress, promoting neurorestoration, and genetic modification. A summary of the disease-modifying strategies now being tested has recently been published (Table 3).

SOME RISK FACTORS ARE MODIFIABLE

Evidence is growing that nutritional factors (eg, dietary restriction, antioxidant intake, and the Mediterranean diet) and lifestyle factors (eg, social and mental activity and exercise) can promote healthy brain aging and delay the onset of Alzheimer disease.69,70

Animals on low-calorie diets live longer, and some epidemiologic studies have shown that people who consume fewer calories have a lower incidence of Alzheimer disease.69

Consuming fish two to three times per week appears to lower the incidence of Alzheimer disease, and a recent report in 2,254 elderly people followed for 4 years found that a Mediterranean diet of fish, olive oil, vegetables, and fruit had a protective effect.71

Resveratrol, a chemical found in red wine, is associated with longevity. A clinical trial of resveratrol to prevent Alzheimer disease is being planned.72–74 Compounds such as docosahexaenoic acid (an omega-3 fatty acid), a flavanoid found in green tea, and curcumin (a component of many curry dishes) are also associated with lowering levels of amyloid.75–77

Foods high in antioxidants may reduce the risk of Alzheimer disease.69,78 Daily folate supplements may have a protective effect, but antioxidants such as vitamin E and anti-inflammatory medications have shown disappointing results in preventing or treating Alzheimer disease and may have significant adverse effects.44,59,79,80

Evidence is also increasing that education, learning new skills, frequent socializing, and regularly engaging in physical exercise and mentally stimulating activities delay the onset of Alzheimer disease, and these pursuits should be encouraged.81–83 Also, treatment of cardiovascular risk factors such as hypertension and hyperlipidemia in mid-life and in older age may lower the rate of cognitive impairment in the elderly.84–86

ACKNOWLEDGMENT

The authors would like to thank Caroline O’Connor and Martha Dunlap for their assistance in preparing this manuscript.

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  47. Winblad B, Gauthier S, Scinto L, et al. Safety and efficacy of galantamine in subjects with mild cognitive impairment. Neurology 2008; 70:20242035.
  48. Mohs RC, Knopman D, Petersen RC, et al. Development of cognitive instruments for use in clinical trials of antidementia drugs: additions to the Alzheimer’s Disease Assessment Scale that broaden its scope. The Alzheimer’s Disease Cooperative Study. Alzheimer Dis Assoc Disord 1997; 11( suppl 2):S13S21.
  49. Mega MS, Cummings JL. Frontal-subcortical circuits and neuropsychiatric disorders. J Neuropsychiatry Clin Neurosci 1994; 6:358370.
  50. Schneider LS, Tariot PN, Dagerman KS, et al. Effectiveness of atypical antipsychotic drugs in patients with Alzheimer’s disease. N Engl J Med 2006; 355:15251538.
  51. Logsdon RG, McCurry SM, Teri L. Evidence-based psychological treatments for disruptive behaviors in individuals with dementia. Psychol Aging 2007; 22:2836.
  52. Overshott R, Byrne J, Burns A. Nonpharmacological and pharmacological interventions for symptoms in Alzheimer’s disease. Expert Rev Neurother 2004; 4:809821.
  53. Spira AP, Edelstein BA. Behavioral interventions for agitation in older adults with dementia: an evaluative review. Int Psychogeriatr 2006; 18:195225.
  54. Raina P, Santaguida P, Ismaila A, et al. Effectiveness of cholinesterase inhibitors and memantine for treating dementia: evidence review for a clinical practice guideline. Ann Intern Med 2008; 148:379397.
  55. Qaseem A, Snow V, Cross J, et al. Current pharmacologic treatment of dementia: a clinical practice guideline from the American College of Physicians and the American Academy of Family Physicians. Ann Intern Med 2008; 148:370378.
  56. Hardy J, Selkoe DJ. The amyloid hypothesis of Alzheimer’s disease: progress and problems on the road to therapeutics. Science 2002; 297:353356.
  57. Giannakopoulos P, Herrmann FR, Bussiere T, et al. Tangle and neuron numbers, but not amyloid load, predict cognitive status in Alzheimer’s disease. Neurology 2003; 60:14951500.
  58. Geerts H. Drug evaluation: (R)-flurbiprofen—an enantiomer of flurbiprofen for the treatment of Alzheimer’s disease. IDrugs 2007; 10:121133.
  59. Aisen PS, Schmeidler J, Pasinetti GM. Randomized pilot study of nimesulide treatment in Alzheimer’s disease. Neurology 2002; 58:10501054.
  60. Fenili D, Brown M, Rappaport R, McLaurin J. Properties of scylloinositol as a therapeutic treatment of AD-like pathology. J Mol Med 2007; 85:603611.
  61. Lee M, Bard F, Johnson-Wood K, Lee C, et al. Abeta42 immunization in Alzheimer’s disease generates Abeta N-terminal antibodies. Ann Neurol 2005; 58:430435.
  62. Masliah E, Hansen L, Adame A, et al. Abeta vaccination effects on plaque pathology in the absence of encephalitis in Alzheimer disease. Neurology 2005; 64:129131.
  63. Gilman S, Koller M, Black RS, et al. Clinical effects of Abeta immunization (AN1792) in patients with AD in an interrupted trial. Neurology 2005; 64:15531562.
  64. Dodel RC, Du Y, Depboylu C, et al. Intravenous immunoglobulins containing antibodies against beta-amyloid for the treatment of Alzheimer’s disease. J Neurol Neurosurg Psychiatry 2004; 75:14721474.
  65. Jick H, Zornberg GL, Jick SS, Seshadri S, Drachman DA. Statins and the risk of dementia. Lancet 2000; 356:16271631.
  66. Sparks DL, Sabbagh MN, Connor DJ, et al. Atorvastatin for the treatment of mild to moderate Alzheimer disease: preliminary results. Arch Neurol 2005; 62:753757.
  67. Labie C, Lafon C, Marmouget C, et al. Effect of the neuroprotective compound SR57746A on nerve growth factor synthesis in cultured astrocytes from neonatal rat cortex. Br J Pharmacol 1999; 127:139144.
  68. Salloway S, Mintzer J, Weiner MF, Cummings JL. Disease-modifying therapies in Alzheimer’s disease. Alzheimer Dement 2008; 4:6579.
  69. Burgener SC, Buettner L, Coen Buckwalter K, et al. Evidence supporting nutritional interventions for persons in early stage Alzheimer’s disease (AD). J Nutr Health Aging 2008; 12:1821.
  70. Kivipelto M, Solomon A. Alzheimer’s disease - the ways of prevention. J Nutr Health Aging 2008; 12:89S94S.
  71. Scarmeas N, Stern Y, Tang MX, Mayeux R, Luchsinger JA. Mediterranean diet and risk for Alzheimer’s disease. Ann Neurol 2006; 59:912921.
  72. Anekonda TS. Resveratrol—a boon for treating Alzheimer’s disease? Brain Res Rev 2006; 52:316326.
  73. Wang J, Ho L, Zhao Z, et al. Moderate consumption of Cabernet Sauvignon attenuates Abeta neuropathology in a mouse model of Alzheimer’s disease. FASEB J 2006; 20:23132320.
  74. Marambaud P, Zhao H, Davies P. Resveratrol promotes clearance of Alzheimer’s disease amyloid-beta peptides. J Biol Chem 2005; 280:3737737382.
  75. Cole GM, Frautschy SA. Docosahexaenoic acid protects from amyloid and dendritic pathology in an Alzheimer’s disease mouse model. Nutr Health 2006; 18:249259.
  76. Rezai-Zadeh K, Shytle D, Sun N, et al. Green tea epigallocatechin-3 gallate (EGCG) modulates amyloid precursor protein cleavage and reduces cerebral amyloidosis in Alzheimer transgenic mice. J Neurosci 2005; 25:88078814.
  77. Zhang L, Fiala M, Cashman J, et al. Curcuminoids enhance amyloid-beta uptake by macrophages of Alzheimer’s disease patients. J Alzheimers Dis 2006; 10:17.
  78. Frank B, Gupta S. A review of antioxidants and Alzheimer’s disease. Ann Clin Psychiatry 2005; 17:269286.
  79. Thal LJ, Ferris SH, Kirby L, et al. A randomized, double-blind, study of rofecoxib in patients with mild cognitive impairment. Neuropsychopharmacology 2005; 30:12041215.
  80. Hayden KM, Welsh-Bohmer KA, Wengreen HJ, Zandi PP, Lyketsos CG, Breitner JC. Risk of mortality with vitamin E supplements: the Cache County study. Am J Med 2007; 120:180184.
  81. Verghese J, Lipton RB, Katz MJ, et al. Leisure activities and the risk of dementia in the elderly. N Engl J Med 2003; 348:25082516.
  82. Larson EB, Wang L, Bowen JD, et al. Exercise is associated with reduced risk for incident dementia among persons 65 years of age and older. Ann Intern Med 2006; 144:7381.
  83. Lytle ME, Vander Bilt J, Pandav RS, Dodge HH, Ganguli M. Exercise level and cognitive decline: the MoVIES project. Alzheimer Dis Assoc Disord 2004; 18:5764.
  84. Forette F, Seux ML, Staessen JA, et al. The prevention of dementia with antihypertensive treatment: new evidence from the Systolic Hypertension in Europe (Syst-Eur) study. Arch Intern Med 2002; 162:20462052.
  85. Kivipelto M, Helkala EL, Hanninen T, et al. Midlife vascular risk factors and late-life mild cognitive impairment: a population-based study. Neurology 2001; 56:16831689.
  86. Launer LJ, Ross GW, Petrovitch H, et al. Midlife blood pressure and dementia: the Honolulu-Asia aging study. Neurobiol Aging 2000; 21:4955.
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  21. Kalbe E, Salmon E, Perani D, et al. Anosognosia in very mild Alzheimer’s disease but not in mild cognitive impairment. Dement Geriatr Cogn Disord 2005; 19:349356.
  22. Borson S, Scanlan JM, Chen P, Ganguli M. The Mini-Cog as a screen for dementia: validation in a population-based sample. J Am Geriatr Soc 2003; 51:14511454.
  23. Folstein MF, Folstein ES, McHugh PR. “Mini-Mental State”: a practical method for grading the cognitive status of patients for the clinician”. J Psychiatr Res 1975; 12:189198.
  24. Nasreddine ZS, Phillips NA, Bedirian V, et al. The Montreal Cognitive Assessment, MoCA: a brief screening tool for mild cognitive impairment. J Am Geriatr Soc 2005; 53:695699.
  25. Galvin JE, Roe CM, Powlishta KK, et al. The AD8: a brief informant interview to detect dementia. Neurology 2005; 65:559564.
  26. Doody RS, Stevens JC, Beck C, et al. Practice parameter: management of dementia (an evidence-based review). Report of the Quality Standards Subcommittee of the American Academy of Neurology. Neurology 2001; 56:11541166.
  27. Knopman DS, DeKosky ST, Cummings JL, et al. Practice parameter: diagnosis of dementia (an evidence-based review). Report of the Quality Standards Subcommittee of the American Academy of Neurology. Neurology 2001; 56:11431153.
  28. Jagust W, Reed B, Mungas D, Ellis W, Decarli C. What does fluorodeoxyglucose PET imaging add to a clinical diagnosis of dementia? Neurology 2007; 69:871877.
  29. Jack CR, Dickson DW, Parisi JE, et al. Antemortem MRI findings correlate with hippocampal neuropathology in typical aging and dementia. Neurology 2002; 58:750757.
  30. Klunk WE, Engler H, Nordberg A, et al. Imaging brain amyloid in Alzheimer’s disease with Pittsburgh Compound-B. Ann Neurol 2004; 55:306319.
  31. Sunderland T, Linker G, Mirza N, et al. Decreased beta-amyloid 1–42 and increased tau levels in cerebrospinal fluid of patients with Alzheimer disease. JAMA 2003; 289:20942103.
  32. Burger PC, Vogel FS. The development of the pathologic changes of Alzheimer’s disease and senile dementia in patients with Down’s syndrome. Am J Pathol 1973; 73:457476.
  33. Mayeux R, Saunders AM, Shea S, et al. Utility of the apolipoprotein E genotype in the diagnosis of Alzheimer’s disease. Alzheimer’s Disease Centers Consortium on Apolipoprotein E and Alzheimer’s Disease. N Engl J Med 1998; 338:506511.
  34. Farrer LA, Cupples LA, Haines JL, et al. Effects of age, sex, and ethnicity on the association between apolipoprotein E genotype and Alzheimer disease. A meta-analysis. APOE and Alzheimer Disease Meta Analysis Consortium. JAMA 1997; 278:13491356.
  35. Winblad B, Kilander L, Eriksson S, et al. Donepezil in patients with severe Alzheimer’s disease: double-blind, parallel-group, placebo-controlled study. Lancet 2006; 367:10571065.
  36. Black SE, Doody R, Li H, et al. Donepezil preserves cognition and global function in patients with severe Alzheimer disease. Neurology 2007; 69:459469.
  37. Winblad B, Cummings J, Andreasen N, et al. A six-month double-blind, randomized, placebo-controlled study of a transdermal patch in Alzheimer’s disease—rivastigmine patch versus capsule. Int J Geriatr Psychiatry 2007; 22:456467.
  38. Reisberg B, Doody R, Stoffler A, Schmitt F, Ferris S, Mobius HJ. Memantine in moderate-to-severe Alzheimer’s disease. N Engl J Med 2003; 348:13331341.
  39. Tariot PN, Farlow MR, Grossberg GT, Graham SM, McDonald S, Gergel I. Memantine treatment in patients with moderate to severe Alzheimer disease already receiving donepezil: a randomized controlled trial. JAMA 2004; 291:317324.
  40. Fillit HM, Doody RS, Binaso K, et al. Recommendations for best practices in the treatment of Alzheimer’s disease in managed care. Am J Geriatr Pharmacother 2006; 4( suppl A):S9S24.
  41. Feldman H, Gauthier S, Hecker J, et al. Efficacy of donepezil on maintenance of activities of daily living in patients with moderate to severe Alzheimer’s disease and the effect on caregiver burden. J Am Geriatr Soc 2003; 51:737744.
  42. Cummings JL, Mackell J, Kaufer D. Behavioral effects of current Alzheimer’s disease treatment: a descriptive review. Alzheimers Dement 2008; 4:4960.
  43. Wilcock GK, Ballard CG, Cooper JA, Henrik L. Memantine for agitation/aggression and psychosis in moderately severe to severe Alzheimer’s disease: a pooled analysis of 3 studies. J Clin Psychiatry 2008; 69:341348.
  44. Petersen RC, Thomas RG, Grundman M, et al. Vitamin E and donepezil for the treatment of mild cognitive impairment. N Engl J Med 2005; 352:23792388.
  45. Salloway S, Ferris S, Kluger A, et al. Efficacy of donepezil in mild cognitive impairment: a randomized placebo-controlled trial. Neurology 2004; 63:651657.
  46. Feldman HH, Ferris S, Winblad B, et al. Effect of rivastigmine on delay to diagnosis of Alzheimer’s disease from mild cognitive impairment: the InDDEx study. Lancet Neurol 2007; 6:501512.
  47. Winblad B, Gauthier S, Scinto L, et al. Safety and efficacy of galantamine in subjects with mild cognitive impairment. Neurology 2008; 70:20242035.
  48. Mohs RC, Knopman D, Petersen RC, et al. Development of cognitive instruments for use in clinical trials of antidementia drugs: additions to the Alzheimer’s Disease Assessment Scale that broaden its scope. The Alzheimer’s Disease Cooperative Study. Alzheimer Dis Assoc Disord 1997; 11( suppl 2):S13S21.
  49. Mega MS, Cummings JL. Frontal-subcortical circuits and neuropsychiatric disorders. J Neuropsychiatry Clin Neurosci 1994; 6:358370.
  50. Schneider LS, Tariot PN, Dagerman KS, et al. Effectiveness of atypical antipsychotic drugs in patients with Alzheimer’s disease. N Engl J Med 2006; 355:15251538.
  51. Logsdon RG, McCurry SM, Teri L. Evidence-based psychological treatments for disruptive behaviors in individuals with dementia. Psychol Aging 2007; 22:2836.
  52. Overshott R, Byrne J, Burns A. Nonpharmacological and pharmacological interventions for symptoms in Alzheimer’s disease. Expert Rev Neurother 2004; 4:809821.
  53. Spira AP, Edelstein BA. Behavioral interventions for agitation in older adults with dementia: an evaluative review. Int Psychogeriatr 2006; 18:195225.
  54. Raina P, Santaguida P, Ismaila A, et al. Effectiveness of cholinesterase inhibitors and memantine for treating dementia: evidence review for a clinical practice guideline. Ann Intern Med 2008; 148:379397.
  55. Qaseem A, Snow V, Cross J, et al. Current pharmacologic treatment of dementia: a clinical practice guideline from the American College of Physicians and the American Academy of Family Physicians. Ann Intern Med 2008; 148:370378.
  56. Hardy J, Selkoe DJ. The amyloid hypothesis of Alzheimer’s disease: progress and problems on the road to therapeutics. Science 2002; 297:353356.
  57. Giannakopoulos P, Herrmann FR, Bussiere T, et al. Tangle and neuron numbers, but not amyloid load, predict cognitive status in Alzheimer’s disease. Neurology 2003; 60:14951500.
  58. Geerts H. Drug evaluation: (R)-flurbiprofen—an enantiomer of flurbiprofen for the treatment of Alzheimer’s disease. IDrugs 2007; 10:121133.
  59. Aisen PS, Schmeidler J, Pasinetti GM. Randomized pilot study of nimesulide treatment in Alzheimer’s disease. Neurology 2002; 58:10501054.
  60. Fenili D, Brown M, Rappaport R, McLaurin J. Properties of scylloinositol as a therapeutic treatment of AD-like pathology. J Mol Med 2007; 85:603611.
  61. Lee M, Bard F, Johnson-Wood K, Lee C, et al. Abeta42 immunization in Alzheimer’s disease generates Abeta N-terminal antibodies. Ann Neurol 2005; 58:430435.
  62. Masliah E, Hansen L, Adame A, et al. Abeta vaccination effects on plaque pathology in the absence of encephalitis in Alzheimer disease. Neurology 2005; 64:129131.
  63. Gilman S, Koller M, Black RS, et al. Clinical effects of Abeta immunization (AN1792) in patients with AD in an interrupted trial. Neurology 2005; 64:15531562.
  64. Dodel RC, Du Y, Depboylu C, et al. Intravenous immunoglobulins containing antibodies against beta-amyloid for the treatment of Alzheimer’s disease. J Neurol Neurosurg Psychiatry 2004; 75:14721474.
  65. Jick H, Zornberg GL, Jick SS, Seshadri S, Drachman DA. Statins and the risk of dementia. Lancet 2000; 356:16271631.
  66. Sparks DL, Sabbagh MN, Connor DJ, et al. Atorvastatin for the treatment of mild to moderate Alzheimer disease: preliminary results. Arch Neurol 2005; 62:753757.
  67. Labie C, Lafon C, Marmouget C, et al. Effect of the neuroprotective compound SR57746A on nerve growth factor synthesis in cultured astrocytes from neonatal rat cortex. Br J Pharmacol 1999; 127:139144.
  68. Salloway S, Mintzer J, Weiner MF, Cummings JL. Disease-modifying therapies in Alzheimer’s disease. Alzheimer Dement 2008; 4:6579.
  69. Burgener SC, Buettner L, Coen Buckwalter K, et al. Evidence supporting nutritional interventions for persons in early stage Alzheimer’s disease (AD). J Nutr Health Aging 2008; 12:1821.
  70. Kivipelto M, Solomon A. Alzheimer’s disease - the ways of prevention. J Nutr Health Aging 2008; 12:89S94S.
  71. Scarmeas N, Stern Y, Tang MX, Mayeux R, Luchsinger JA. Mediterranean diet and risk for Alzheimer’s disease. Ann Neurol 2006; 59:912921.
  72. Anekonda TS. Resveratrol—a boon for treating Alzheimer’s disease? Brain Res Rev 2006; 52:316326.
  73. Wang J, Ho L, Zhao Z, et al. Moderate consumption of Cabernet Sauvignon attenuates Abeta neuropathology in a mouse model of Alzheimer’s disease. FASEB J 2006; 20:23132320.
  74. Marambaud P, Zhao H, Davies P. Resveratrol promotes clearance of Alzheimer’s disease amyloid-beta peptides. J Biol Chem 2005; 280:3737737382.
  75. Cole GM, Frautschy SA. Docosahexaenoic acid protects from amyloid and dendritic pathology in an Alzheimer’s disease mouse model. Nutr Health 2006; 18:249259.
  76. Rezai-Zadeh K, Shytle D, Sun N, et al. Green tea epigallocatechin-3 gallate (EGCG) modulates amyloid precursor protein cleavage and reduces cerebral amyloidosis in Alzheimer transgenic mice. J Neurosci 2005; 25:88078814.
  77. Zhang L, Fiala M, Cashman J, et al. Curcuminoids enhance amyloid-beta uptake by macrophages of Alzheimer’s disease patients. J Alzheimers Dis 2006; 10:17.
  78. Frank B, Gupta S. A review of antioxidants and Alzheimer’s disease. Ann Clin Psychiatry 2005; 17:269286.
  79. Thal LJ, Ferris SH, Kirby L, et al. A randomized, double-blind, study of rofecoxib in patients with mild cognitive impairment. Neuropsychopharmacology 2005; 30:12041215.
  80. Hayden KM, Welsh-Bohmer KA, Wengreen HJ, Zandi PP, Lyketsos CG, Breitner JC. Risk of mortality with vitamin E supplements: the Cache County study. Am J Med 2007; 120:180184.
  81. Verghese J, Lipton RB, Katz MJ, et al. Leisure activities and the risk of dementia in the elderly. N Engl J Med 2003; 348:25082516.
  82. Larson EB, Wang L, Bowen JD, et al. Exercise is associated with reduced risk for incident dementia among persons 65 years of age and older. Ann Intern Med 2006; 144:7381.
  83. Lytle ME, Vander Bilt J, Pandav RS, Dodge HH, Ganguli M. Exercise level and cognitive decline: the MoVIES project. Alzheimer Dis Assoc Disord 2004; 18:5764.
  84. Forette F, Seux ML, Staessen JA, et al. The prevention of dementia with antihypertensive treatment: new evidence from the Systolic Hypertension in Europe (Syst-Eur) study. Arch Intern Med 2002; 162:20462052.
  85. Kivipelto M, Helkala EL, Hanninen T, et al. Midlife vascular risk factors and late-life mild cognitive impairment: a population-based study. Neurology 2001; 56:16831689.
  86. Launer LJ, Ross GW, Petrovitch H, et al. Midlife blood pressure and dementia: the Honolulu-Asia aging study. Neurobiol Aging 2000; 21:4955.
Issue
Cleveland Clinic Journal of Medicine - 76(1)
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Cleveland Clinic Journal of Medicine - 76(1)
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Alzheimer disease: Time to improve its diagnosis and treatment
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Alzheimer disease: Time to improve its diagnosis and treatment
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KEY POINTS

  • Interpret screening tests carefully in patients who have very low or very high education levels, who are not tested in their native language, or who have deficits that might limit their performance.
  • Patients with Alzheimer disease function best in a safe, calm, and predictable environment. Their caregivers require ongoing support and education to develop realistic expectations throughout the course of the illness.
  • It is important that families be made aware that treatments for Alzheimer disease, such as cholinesterase inhibitors, attenuate decline over time rather than improve cognitive and behavioral symptoms.
  • Evidence is growing that nutritional factors (eg, dietary restriction, antioxidant intake, and the Mediterranean diet) and lifestyle factors (eg, social and mental activity and exercise) can delay the onset of Alzheimer disease.
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Who should receive the shingles vaccine?

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Who should receive the shingles vaccine?

The Advisory Committee on Immunization Practices (ACIP) recommends routinely giving a single dose of live zoster vaccine to immunocompetent patients age 60 and older at their first clinical encounter. The vaccine effectively prevents shingles and postherpetic neuralgia and their associated burden of illness. Although not all insurance companies pay for it yet, it should be offered to all patients for whom it is indicated to increase their health-related quality of life.

IMMUNITY WANES WITH AGE

Shingles, also known as zoster or herpes zoster, is caused by retrograde transport of the varicella zoster virus (VZV) from the ganglia to the skin in a host who had a primary varicella infection (chickenpox) in the past.1 Although shingles is not one of the diseases that must be reported to public health authorities, more than 1 million cases are estimated to occur each year in the United States. From 10% to 30% of people develop shingles during their lifetime.2,3

The elderly are at particular risk of shingles, because immunity to VZV wanes as a part of normal aging. As many as 50% of people who live to age 85 will have shingles at some point in their life.

Moreover, about 20% of patients with shingles develop postherpetic neuralgia,3,4 the pain and discomfort of which can be disabling and can diminish quality of life.5

Antiviral therapy reduces the severity and duration of an episode of shingles but does not prevent postherpetic neuralgia.2,6 Steroids provide additional relief of acute zoster pain, but they do not clearly prevent postherpetic neuralgia either and should be used only in combination with antiviral drugs. Preventing zoster and postherpetic neuralgia by routine vaccination should be a goal in our efforts to promote healthy aging, especially with the increasing number of elderly in our country.7

THE VACCINE IS EFFECTIVE: THE SHINGLES PREVENTION STUDY

The Shingles Prevention Study was a prospective, double-blind trial in more than 38,000 adults, median age 69 years (range 59–99), who were followed for a mean of 3.13 years (range 1 day to 4.9 years) after receiving the zoster vaccine or placebo.8–10

Zoster vaccination significantly reduced the herpes zoster burden of illness by 61% (P < .001), the incidence of zoster by 51% (P < .001), and the incidence of postherpetic neuralgia by 66% (Table 1). The burden of illness was measured by an index based on the incidence, severity, and duration of pain and discomfort from zoster.

The virus in the vaccine did not elicit shingles in any patient. After vaccination, if lesions did occur, they were from the patient’s native strain, not the vaccine strain.8

ZOSTAVAX

The US Food and Drug Administration approved the zoster vaccine in May 2006 for prevention of herpes zoster in people age 60 and older. Zostavax, licensed by Merck, is the only vaccine available for this purpose.11,12 Zoster vaccine is not indicated for treating episodes of shingles or postherpetic neuralgia or for preventing primary varicella infection (chickenpox).

Zostavax does not contain thimerosal, a mercury-based preservative used in other vaccines. Therefore, it must be kept frozen at an average temperature of –15°C (5°F) and should not be used if its temperature rises above –5°C (23°F).13,14 Just before it is given, the vaccine is reconstituted with the supplied diluents and then injected subcutaneously in the deltoid region.12

No booster dose is recommended at present. Also, many cases of herpes zoster occur in people under age 60, for whom there is no recommendation.11,15 Although the vaccine would probably be safe and effective in this younger group, data are insufficient to recommend vaccinating them.16

ZOSTER VACCINE (ZOSTAVAX) IS NOT CHICKENPOX VACCINE (VARIVAX)

Both Zostavax and the chickenpox vaccine (Varivax) are live, attenuated vaccines from the same Oka/Merck strain of the virus, but Zostavax is about 14 times more potent than Varivax (Zostavax contains 8,700–60,000 plaque-forming units of virus, whereas Varivax contains 1,350), and they should not be used interchangeably.14

GIVING ZOSTER VACCINE WITH OTHER VACCINES IN THE ELDERLY

Zostavax can be given either simultaneously with or at any time before or after any inactivated vaccine (such as tetanus toxoid, influenza, pneumococcus). However, each vaccine must be given in a separate syringe at a different anatomic site.17

VACCINATE EVEN IF THE PATIENT DOESN’T RECALL HAVING CHICKENPOX

Even in people who do not recall ever having chickenpox, the rate of VZV seropositivity is very high (> 95% in those over age 60 in the United States).18 The ACIP recommends vaccination whether or not the patient reports having had chickenpox. Serologic testing to determine varicella immunity is not needed before vaccination, nor was it required for entry in the Shingles Prevention Study.

Furthermore, in VZV-seronegative adults, giving the zoster vaccine is thought to provide at least partial protection against varicella, and no data indicate any excessive adverse effects in this population.

 

 

VACCINATE EVEN IF THE PATIENT HAS HAD SHINGLES

The ACIP says that people with a history of zoster can be vaccinated. Recurrent zoster has been confirmed in immunocompetent patients soon after a previous episode. There is no test to confirm prior zoster episodes, and if the patient is immunocompetent, no different safety concerns are anticipated with vaccination in this group.16

ADVERSE EFFECTS ARE MILD

No significant safety concerns have been noted with zoster vaccine. Mild local reactions (erythema, swelling, pain, pruritus) and headache are the most common adverse events. There have been no differences in the numbers and types of serious adverse events during the 42 days after receipt of vaccine or placebo.

CONTRAINDICATIONS

Contraindications to zoster vaccine are:

  • A history of anaphylactic or anaphylactoid reactions to gelatin, neomycin, or other components of the vaccine
  • Acquired or primary immune deficiency states, including AIDS
  • Cancer chemotherapy or radiotherapy
  • Leukemia
  • Lymphoma
  • Organ transplantation
  • Active untreated tuberculosis
  • Pregnancy or breast-feeding.

However, patients with leukemia in remission who have not received chemotherapy (eg, alkylating drugs or antimetabolites) or radiation for at least 3 months can receive zoster vaccine.

Although zoster vaccine is contraindicated in conditions of cellular immune deficiency, patients with humoral immunodeficiency (eg, hypogammaglobulinemia or dysgammaglobulinemia) can receive it.

Diabetes, hypertension, chronic renal failure, coronary artery disease, chronic lung disease, rheumatoid arthritis, and other medical conditions are not considered contraindications to the vaccine.

The ACIP does not recommend any upper age limit for the vaccine, and preventing zoster is particularly important in the oldest elderly because they have the highest incidence of zoster and postherpetic neuralgia.16

Do not vaccinate during immunosuppressive treatment

If immunosuppressive treatment is planned (eg, with corticosteroids or anti-tumor necrosis factor agents), the vaccine should be given at least 14 days (preferably 1 month) before immunosuppression begins.

The safety and efficacy of zoster vaccine is unknown in patients receiving recombinant human immune mediators and immune modulators, especially anti-tumor necrosis factor agents such as adalimumab (Humira), infliximab (Remicade), or etanercept (Enbrel). These patients should be vaccinated 1 month before starting the treatment or 1 month after stopping it.16

Patients on corticosteroids in doses equivalent to prednisone 20 mg/day or more for 2 or more weeks should not be vaccinated against zoster unless the steroids have been stopped for at least 1 month.11

Low doses of methotrexate (< 0.4 mg/kg/week), azathioprine (Azasan) (< 3.0 mg/kg/day), or 6-mercaptopurine (Purinethol, 6-MP) (< 1.5 mg/kg/day) for the treatment of rheumatoid arthritis, psoriasis, polymyositis, sarcoidosis, inflammatory bowel disease, and other conditions are not contraindications to zoster vaccination.

Medications against herpes, such as acyclovir (Zovirax), famciclovir (Famvir), or valacyclovir (Valtrex) should be discontinued at least 24 hours before zoster vaccination and should not be started until 14 days afterward.

COSTLY AND EFFECTIVE? OR COST-EFFECTIVE?

The average cost associated with an acute episode of zoster ranges from $112 to $287 if treated on an outpatient basis and $3,221 to $7,206 if the patient is hospitalized (costs in 2006).19

Zoster vaccine is relatively costly (bulk price $155 per dose) (Table 2), and most insurance companies do not cover it yet. It is covered by Medicare part D but not part B, and it is treated as a prescription drug. However, available evidence suggests that zoster vaccination is approximately as cost-effective as other public health interventions.20

Although pharmacists are licensed to administer influenza and pneumococcal vaccines, several states do not specifically allow them to administer zoster vaccine. Moreover, one usually cannot provide the vaccine out of the office stock and get reimbursed for it (except by some private insurance companies). Instead, the patient needs to take a prescription to a local pharmacy, where the vaccine is placed on ice and then brought back to the physician’s office for administration.

References
  1. Nagel MA, Gilden DH. The protean neurologic manifestations of varicella-zoster virus infection. Cleve Clin J Med 2007; 74:489504.
  2. Gnann JW, Whitley RJ. Clinical practice. Herpes zoster. N Engl J Med 2002; 347:340346.
  3. Katz J, Cooper EM, Walther RR, Sweeney EW, Dworkin RH. Acute pain in herpes zoster and its impact on health-related quality of life. Clin Infect Dis 2004; 39:342348.
  4. Hope-Simpson RE. The nature of herpes zoster: a long-term study and a new hypothesis. Proc R Soc Med 1965; 58:920.
  5. Lydick E, Epstein RS, Himmelberger D, White CJ. Herpes zoster and quality of life: a self-limited disease with severe impact. Neurology 1995; 45:S52S53.
  6. Kost RG, Straus SE. Postherpetic neuralgia—pathogenesis, treatment, and prevention. N Engl J Med 1996; 335:3242.
  7. Johnson R, McElhaney J, Pedalino B, Levin M. Prevention of herpes zoster and its painful and debilitating complications. Int J Infect Dis 2007; 11( suppl 2):S43S48.
  8. Oxman MN, Levin MJ, Johnson GR, et al. A vaccine to prevent herpes zoster and postherpetic neuralgia in older adults. N Engl J Med 2005; 352:22712284.
  9. Burke MS. Herpes zoster vaccine: clinical trial evidence and implications for medical practice. J Am Osteopath Assoc 2007; 107( suppl 1):S14S18.
  10. Betts RF. Vaccination strategies for the prevention of herpes zoster and postherpetic neuralgia. J Am Acad Dermatol 2007; 57( suppl):S143S147.
  11. Kroger AT, Atkinson WL, Marcuse EK, Pickering LK. General recommendations on immunization: recommendations of the Advisory Committee on Immunization Practices (ACIP). MMWR Recomm Rep 2006; 55:148.
  12. Merck. Zostavax zoster vaccine live suspension for subcutaneous injection. www.merck.com/product/usa/pi_circulars/z/zostavax_pi.pdf. Accessed 11/17/2008.
  13. Holodniy M. Prevention of shingles by varicella zoster virus vaccination. Expert Rev Vaccines 2006; 5:431443.
  14. Herpes zoster vaccine (Zostavax). Med Lett Drugs Ther 2006; 48:7374.
  15. Donahue JG, Choo PW, Manson JE, Platt R. The incidence of herpes zoster. Arch Intern Med 1995; 155:16051609.
  16. Harpaz R, Ortega-Sanchez IR, Seward JF. Prevention of herpes zoster: recommendations of the Advisory Committee on Immunization Practices (ACIP). MMWR Recomm Rep 2008; 57:130.
  17. Bader MS. Immunization for the elderly. Am J Med Sci 2007; 334:481486.
  18. Kilgore PE, Kruszon-Moran D, Seward JF, et al. Varicella in Americans from NHANES III: implications for control through routine immunization. J Med Virol 2003; 70( suppl 1):S111S118.
  19. Dworkin RH, White R, O’Connor AB, Baser O, Hawkins K. Healthcare costs of acute and chronic pain associated with a diagnosis of herpes zoster. J Am Geriatr Soc 2007; 55:11681175.
  20. Dworkin RH, White R, O’Connor AB, Hawkins K. Health care expenditure burden of persisting herpes zoster pain. Pain Med 2008; 9:348353.
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Division of Hospital Medicine, University of California San Francisco

Kristin Englund, MD
Department of Infectious Diseases, Cleveland Clinic, Cleveland, OH

Address: Kristin Englund, MD, Department of Infectious Diseases, S32, Cleveland Clinic, 9500 Euclid Avenue, Cleveland, OH 44195; e-mail [email protected]

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Division of Hospital Medicine, University of California San Francisco

Kristin Englund, MD
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Address: Kristin Englund, MD, Department of Infectious Diseases, S32, Cleveland Clinic, 9500 Euclid Avenue, Cleveland, OH 44195; e-mail [email protected]

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Related Articles

The Advisory Committee on Immunization Practices (ACIP) recommends routinely giving a single dose of live zoster vaccine to immunocompetent patients age 60 and older at their first clinical encounter. The vaccine effectively prevents shingles and postherpetic neuralgia and their associated burden of illness. Although not all insurance companies pay for it yet, it should be offered to all patients for whom it is indicated to increase their health-related quality of life.

IMMUNITY WANES WITH AGE

Shingles, also known as zoster or herpes zoster, is caused by retrograde transport of the varicella zoster virus (VZV) from the ganglia to the skin in a host who had a primary varicella infection (chickenpox) in the past.1 Although shingles is not one of the diseases that must be reported to public health authorities, more than 1 million cases are estimated to occur each year in the United States. From 10% to 30% of people develop shingles during their lifetime.2,3

The elderly are at particular risk of shingles, because immunity to VZV wanes as a part of normal aging. As many as 50% of people who live to age 85 will have shingles at some point in their life.

Moreover, about 20% of patients with shingles develop postherpetic neuralgia,3,4 the pain and discomfort of which can be disabling and can diminish quality of life.5

Antiviral therapy reduces the severity and duration of an episode of shingles but does not prevent postherpetic neuralgia.2,6 Steroids provide additional relief of acute zoster pain, but they do not clearly prevent postherpetic neuralgia either and should be used only in combination with antiviral drugs. Preventing zoster and postherpetic neuralgia by routine vaccination should be a goal in our efforts to promote healthy aging, especially with the increasing number of elderly in our country.7

THE VACCINE IS EFFECTIVE: THE SHINGLES PREVENTION STUDY

The Shingles Prevention Study was a prospective, double-blind trial in more than 38,000 adults, median age 69 years (range 59–99), who were followed for a mean of 3.13 years (range 1 day to 4.9 years) after receiving the zoster vaccine or placebo.8–10

Zoster vaccination significantly reduced the herpes zoster burden of illness by 61% (P < .001), the incidence of zoster by 51% (P < .001), and the incidence of postherpetic neuralgia by 66% (Table 1). The burden of illness was measured by an index based on the incidence, severity, and duration of pain and discomfort from zoster.

The virus in the vaccine did not elicit shingles in any patient. After vaccination, if lesions did occur, they were from the patient’s native strain, not the vaccine strain.8

ZOSTAVAX

The US Food and Drug Administration approved the zoster vaccine in May 2006 for prevention of herpes zoster in people age 60 and older. Zostavax, licensed by Merck, is the only vaccine available for this purpose.11,12 Zoster vaccine is not indicated for treating episodes of shingles or postherpetic neuralgia or for preventing primary varicella infection (chickenpox).

Zostavax does not contain thimerosal, a mercury-based preservative used in other vaccines. Therefore, it must be kept frozen at an average temperature of –15°C (5°F) and should not be used if its temperature rises above –5°C (23°F).13,14 Just before it is given, the vaccine is reconstituted with the supplied diluents and then injected subcutaneously in the deltoid region.12

No booster dose is recommended at present. Also, many cases of herpes zoster occur in people under age 60, for whom there is no recommendation.11,15 Although the vaccine would probably be safe and effective in this younger group, data are insufficient to recommend vaccinating them.16

ZOSTER VACCINE (ZOSTAVAX) IS NOT CHICKENPOX VACCINE (VARIVAX)

Both Zostavax and the chickenpox vaccine (Varivax) are live, attenuated vaccines from the same Oka/Merck strain of the virus, but Zostavax is about 14 times more potent than Varivax (Zostavax contains 8,700–60,000 plaque-forming units of virus, whereas Varivax contains 1,350), and they should not be used interchangeably.14

GIVING ZOSTER VACCINE WITH OTHER VACCINES IN THE ELDERLY

Zostavax can be given either simultaneously with or at any time before or after any inactivated vaccine (such as tetanus toxoid, influenza, pneumococcus). However, each vaccine must be given in a separate syringe at a different anatomic site.17

VACCINATE EVEN IF THE PATIENT DOESN’T RECALL HAVING CHICKENPOX

Even in people who do not recall ever having chickenpox, the rate of VZV seropositivity is very high (> 95% in those over age 60 in the United States).18 The ACIP recommends vaccination whether or not the patient reports having had chickenpox. Serologic testing to determine varicella immunity is not needed before vaccination, nor was it required for entry in the Shingles Prevention Study.

Furthermore, in VZV-seronegative adults, giving the zoster vaccine is thought to provide at least partial protection against varicella, and no data indicate any excessive adverse effects in this population.

 

 

VACCINATE EVEN IF THE PATIENT HAS HAD SHINGLES

The ACIP says that people with a history of zoster can be vaccinated. Recurrent zoster has been confirmed in immunocompetent patients soon after a previous episode. There is no test to confirm prior zoster episodes, and if the patient is immunocompetent, no different safety concerns are anticipated with vaccination in this group.16

ADVERSE EFFECTS ARE MILD

No significant safety concerns have been noted with zoster vaccine. Mild local reactions (erythema, swelling, pain, pruritus) and headache are the most common adverse events. There have been no differences in the numbers and types of serious adverse events during the 42 days after receipt of vaccine or placebo.

CONTRAINDICATIONS

Contraindications to zoster vaccine are:

  • A history of anaphylactic or anaphylactoid reactions to gelatin, neomycin, or other components of the vaccine
  • Acquired or primary immune deficiency states, including AIDS
  • Cancer chemotherapy or radiotherapy
  • Leukemia
  • Lymphoma
  • Organ transplantation
  • Active untreated tuberculosis
  • Pregnancy or breast-feeding.

However, patients with leukemia in remission who have not received chemotherapy (eg, alkylating drugs or antimetabolites) or radiation for at least 3 months can receive zoster vaccine.

Although zoster vaccine is contraindicated in conditions of cellular immune deficiency, patients with humoral immunodeficiency (eg, hypogammaglobulinemia or dysgammaglobulinemia) can receive it.

Diabetes, hypertension, chronic renal failure, coronary artery disease, chronic lung disease, rheumatoid arthritis, and other medical conditions are not considered contraindications to the vaccine.

The ACIP does not recommend any upper age limit for the vaccine, and preventing zoster is particularly important in the oldest elderly because they have the highest incidence of zoster and postherpetic neuralgia.16

Do not vaccinate during immunosuppressive treatment

If immunosuppressive treatment is planned (eg, with corticosteroids or anti-tumor necrosis factor agents), the vaccine should be given at least 14 days (preferably 1 month) before immunosuppression begins.

The safety and efficacy of zoster vaccine is unknown in patients receiving recombinant human immune mediators and immune modulators, especially anti-tumor necrosis factor agents such as adalimumab (Humira), infliximab (Remicade), or etanercept (Enbrel). These patients should be vaccinated 1 month before starting the treatment or 1 month after stopping it.16

Patients on corticosteroids in doses equivalent to prednisone 20 mg/day or more for 2 or more weeks should not be vaccinated against zoster unless the steroids have been stopped for at least 1 month.11

Low doses of methotrexate (< 0.4 mg/kg/week), azathioprine (Azasan) (< 3.0 mg/kg/day), or 6-mercaptopurine (Purinethol, 6-MP) (< 1.5 mg/kg/day) for the treatment of rheumatoid arthritis, psoriasis, polymyositis, sarcoidosis, inflammatory bowel disease, and other conditions are not contraindications to zoster vaccination.

Medications against herpes, such as acyclovir (Zovirax), famciclovir (Famvir), or valacyclovir (Valtrex) should be discontinued at least 24 hours before zoster vaccination and should not be started until 14 days afterward.

COSTLY AND EFFECTIVE? OR COST-EFFECTIVE?

The average cost associated with an acute episode of zoster ranges from $112 to $287 if treated on an outpatient basis and $3,221 to $7,206 if the patient is hospitalized (costs in 2006).19

Zoster vaccine is relatively costly (bulk price $155 per dose) (Table 2), and most insurance companies do not cover it yet. It is covered by Medicare part D but not part B, and it is treated as a prescription drug. However, available evidence suggests that zoster vaccination is approximately as cost-effective as other public health interventions.20

Although pharmacists are licensed to administer influenza and pneumococcal vaccines, several states do not specifically allow them to administer zoster vaccine. Moreover, one usually cannot provide the vaccine out of the office stock and get reimbursed for it (except by some private insurance companies). Instead, the patient needs to take a prescription to a local pharmacy, where the vaccine is placed on ice and then brought back to the physician’s office for administration.

The Advisory Committee on Immunization Practices (ACIP) recommends routinely giving a single dose of live zoster vaccine to immunocompetent patients age 60 and older at their first clinical encounter. The vaccine effectively prevents shingles and postherpetic neuralgia and their associated burden of illness. Although not all insurance companies pay for it yet, it should be offered to all patients for whom it is indicated to increase their health-related quality of life.

IMMUNITY WANES WITH AGE

Shingles, also known as zoster or herpes zoster, is caused by retrograde transport of the varicella zoster virus (VZV) from the ganglia to the skin in a host who had a primary varicella infection (chickenpox) in the past.1 Although shingles is not one of the diseases that must be reported to public health authorities, more than 1 million cases are estimated to occur each year in the United States. From 10% to 30% of people develop shingles during their lifetime.2,3

The elderly are at particular risk of shingles, because immunity to VZV wanes as a part of normal aging. As many as 50% of people who live to age 85 will have shingles at some point in their life.

Moreover, about 20% of patients with shingles develop postherpetic neuralgia,3,4 the pain and discomfort of which can be disabling and can diminish quality of life.5

Antiviral therapy reduces the severity and duration of an episode of shingles but does not prevent postherpetic neuralgia.2,6 Steroids provide additional relief of acute zoster pain, but they do not clearly prevent postherpetic neuralgia either and should be used only in combination with antiviral drugs. Preventing zoster and postherpetic neuralgia by routine vaccination should be a goal in our efforts to promote healthy aging, especially with the increasing number of elderly in our country.7

THE VACCINE IS EFFECTIVE: THE SHINGLES PREVENTION STUDY

The Shingles Prevention Study was a prospective, double-blind trial in more than 38,000 adults, median age 69 years (range 59–99), who were followed for a mean of 3.13 years (range 1 day to 4.9 years) after receiving the zoster vaccine or placebo.8–10

Zoster vaccination significantly reduced the herpes zoster burden of illness by 61% (P < .001), the incidence of zoster by 51% (P < .001), and the incidence of postherpetic neuralgia by 66% (Table 1). The burden of illness was measured by an index based on the incidence, severity, and duration of pain and discomfort from zoster.

The virus in the vaccine did not elicit shingles in any patient. After vaccination, if lesions did occur, they were from the patient’s native strain, not the vaccine strain.8

ZOSTAVAX

The US Food and Drug Administration approved the zoster vaccine in May 2006 for prevention of herpes zoster in people age 60 and older. Zostavax, licensed by Merck, is the only vaccine available for this purpose.11,12 Zoster vaccine is not indicated for treating episodes of shingles or postherpetic neuralgia or for preventing primary varicella infection (chickenpox).

Zostavax does not contain thimerosal, a mercury-based preservative used in other vaccines. Therefore, it must be kept frozen at an average temperature of –15°C (5°F) and should not be used if its temperature rises above –5°C (23°F).13,14 Just before it is given, the vaccine is reconstituted with the supplied diluents and then injected subcutaneously in the deltoid region.12

No booster dose is recommended at present. Also, many cases of herpes zoster occur in people under age 60, for whom there is no recommendation.11,15 Although the vaccine would probably be safe and effective in this younger group, data are insufficient to recommend vaccinating them.16

ZOSTER VACCINE (ZOSTAVAX) IS NOT CHICKENPOX VACCINE (VARIVAX)

Both Zostavax and the chickenpox vaccine (Varivax) are live, attenuated vaccines from the same Oka/Merck strain of the virus, but Zostavax is about 14 times more potent than Varivax (Zostavax contains 8,700–60,000 plaque-forming units of virus, whereas Varivax contains 1,350), and they should not be used interchangeably.14

GIVING ZOSTER VACCINE WITH OTHER VACCINES IN THE ELDERLY

Zostavax can be given either simultaneously with or at any time before or after any inactivated vaccine (such as tetanus toxoid, influenza, pneumococcus). However, each vaccine must be given in a separate syringe at a different anatomic site.17

VACCINATE EVEN IF THE PATIENT DOESN’T RECALL HAVING CHICKENPOX

Even in people who do not recall ever having chickenpox, the rate of VZV seropositivity is very high (> 95% in those over age 60 in the United States).18 The ACIP recommends vaccination whether or not the patient reports having had chickenpox. Serologic testing to determine varicella immunity is not needed before vaccination, nor was it required for entry in the Shingles Prevention Study.

Furthermore, in VZV-seronegative adults, giving the zoster vaccine is thought to provide at least partial protection against varicella, and no data indicate any excessive adverse effects in this population.

 

 

VACCINATE EVEN IF THE PATIENT HAS HAD SHINGLES

The ACIP says that people with a history of zoster can be vaccinated. Recurrent zoster has been confirmed in immunocompetent patients soon after a previous episode. There is no test to confirm prior zoster episodes, and if the patient is immunocompetent, no different safety concerns are anticipated with vaccination in this group.16

ADVERSE EFFECTS ARE MILD

No significant safety concerns have been noted with zoster vaccine. Mild local reactions (erythema, swelling, pain, pruritus) and headache are the most common adverse events. There have been no differences in the numbers and types of serious adverse events during the 42 days after receipt of vaccine or placebo.

CONTRAINDICATIONS

Contraindications to zoster vaccine are:

  • A history of anaphylactic or anaphylactoid reactions to gelatin, neomycin, or other components of the vaccine
  • Acquired or primary immune deficiency states, including AIDS
  • Cancer chemotherapy or radiotherapy
  • Leukemia
  • Lymphoma
  • Organ transplantation
  • Active untreated tuberculosis
  • Pregnancy or breast-feeding.

However, patients with leukemia in remission who have not received chemotherapy (eg, alkylating drugs or antimetabolites) or radiation for at least 3 months can receive zoster vaccine.

Although zoster vaccine is contraindicated in conditions of cellular immune deficiency, patients with humoral immunodeficiency (eg, hypogammaglobulinemia or dysgammaglobulinemia) can receive it.

Diabetes, hypertension, chronic renal failure, coronary artery disease, chronic lung disease, rheumatoid arthritis, and other medical conditions are not considered contraindications to the vaccine.

The ACIP does not recommend any upper age limit for the vaccine, and preventing zoster is particularly important in the oldest elderly because they have the highest incidence of zoster and postherpetic neuralgia.16

Do not vaccinate during immunosuppressive treatment

If immunosuppressive treatment is planned (eg, with corticosteroids or anti-tumor necrosis factor agents), the vaccine should be given at least 14 days (preferably 1 month) before immunosuppression begins.

The safety and efficacy of zoster vaccine is unknown in patients receiving recombinant human immune mediators and immune modulators, especially anti-tumor necrosis factor agents such as adalimumab (Humira), infliximab (Remicade), or etanercept (Enbrel). These patients should be vaccinated 1 month before starting the treatment or 1 month after stopping it.16

Patients on corticosteroids in doses equivalent to prednisone 20 mg/day or more for 2 or more weeks should not be vaccinated against zoster unless the steroids have been stopped for at least 1 month.11

Low doses of methotrexate (< 0.4 mg/kg/week), azathioprine (Azasan) (< 3.0 mg/kg/day), or 6-mercaptopurine (Purinethol, 6-MP) (< 1.5 mg/kg/day) for the treatment of rheumatoid arthritis, psoriasis, polymyositis, sarcoidosis, inflammatory bowel disease, and other conditions are not contraindications to zoster vaccination.

Medications against herpes, such as acyclovir (Zovirax), famciclovir (Famvir), or valacyclovir (Valtrex) should be discontinued at least 24 hours before zoster vaccination and should not be started until 14 days afterward.

COSTLY AND EFFECTIVE? OR COST-EFFECTIVE?

The average cost associated with an acute episode of zoster ranges from $112 to $287 if treated on an outpatient basis and $3,221 to $7,206 if the patient is hospitalized (costs in 2006).19

Zoster vaccine is relatively costly (bulk price $155 per dose) (Table 2), and most insurance companies do not cover it yet. It is covered by Medicare part D but not part B, and it is treated as a prescription drug. However, available evidence suggests that zoster vaccination is approximately as cost-effective as other public health interventions.20

Although pharmacists are licensed to administer influenza and pneumococcal vaccines, several states do not specifically allow them to administer zoster vaccine. Moreover, one usually cannot provide the vaccine out of the office stock and get reimbursed for it (except by some private insurance companies). Instead, the patient needs to take a prescription to a local pharmacy, where the vaccine is placed on ice and then brought back to the physician’s office for administration.

References
  1. Nagel MA, Gilden DH. The protean neurologic manifestations of varicella-zoster virus infection. Cleve Clin J Med 2007; 74:489504.
  2. Gnann JW, Whitley RJ. Clinical practice. Herpes zoster. N Engl J Med 2002; 347:340346.
  3. Katz J, Cooper EM, Walther RR, Sweeney EW, Dworkin RH. Acute pain in herpes zoster and its impact on health-related quality of life. Clin Infect Dis 2004; 39:342348.
  4. Hope-Simpson RE. The nature of herpes zoster: a long-term study and a new hypothesis. Proc R Soc Med 1965; 58:920.
  5. Lydick E, Epstein RS, Himmelberger D, White CJ. Herpes zoster and quality of life: a self-limited disease with severe impact. Neurology 1995; 45:S52S53.
  6. Kost RG, Straus SE. Postherpetic neuralgia—pathogenesis, treatment, and prevention. N Engl J Med 1996; 335:3242.
  7. Johnson R, McElhaney J, Pedalino B, Levin M. Prevention of herpes zoster and its painful and debilitating complications. Int J Infect Dis 2007; 11( suppl 2):S43S48.
  8. Oxman MN, Levin MJ, Johnson GR, et al. A vaccine to prevent herpes zoster and postherpetic neuralgia in older adults. N Engl J Med 2005; 352:22712284.
  9. Burke MS. Herpes zoster vaccine: clinical trial evidence and implications for medical practice. J Am Osteopath Assoc 2007; 107( suppl 1):S14S18.
  10. Betts RF. Vaccination strategies for the prevention of herpes zoster and postherpetic neuralgia. J Am Acad Dermatol 2007; 57( suppl):S143S147.
  11. Kroger AT, Atkinson WL, Marcuse EK, Pickering LK. General recommendations on immunization: recommendations of the Advisory Committee on Immunization Practices (ACIP). MMWR Recomm Rep 2006; 55:148.
  12. Merck. Zostavax zoster vaccine live suspension for subcutaneous injection. www.merck.com/product/usa/pi_circulars/z/zostavax_pi.pdf. Accessed 11/17/2008.
  13. Holodniy M. Prevention of shingles by varicella zoster virus vaccination. Expert Rev Vaccines 2006; 5:431443.
  14. Herpes zoster vaccine (Zostavax). Med Lett Drugs Ther 2006; 48:7374.
  15. Donahue JG, Choo PW, Manson JE, Platt R. The incidence of herpes zoster. Arch Intern Med 1995; 155:16051609.
  16. Harpaz R, Ortega-Sanchez IR, Seward JF. Prevention of herpes zoster: recommendations of the Advisory Committee on Immunization Practices (ACIP). MMWR Recomm Rep 2008; 57:130.
  17. Bader MS. Immunization for the elderly. Am J Med Sci 2007; 334:481486.
  18. Kilgore PE, Kruszon-Moran D, Seward JF, et al. Varicella in Americans from NHANES III: implications for control through routine immunization. J Med Virol 2003; 70( suppl 1):S111S118.
  19. Dworkin RH, White R, O’Connor AB, Baser O, Hawkins K. Healthcare costs of acute and chronic pain associated with a diagnosis of herpes zoster. J Am Geriatr Soc 2007; 55:11681175.
  20. Dworkin RH, White R, O’Connor AB, Hawkins K. Health care expenditure burden of persisting herpes zoster pain. Pain Med 2008; 9:348353.
References
  1. Nagel MA, Gilden DH. The protean neurologic manifestations of varicella-zoster virus infection. Cleve Clin J Med 2007; 74:489504.
  2. Gnann JW, Whitley RJ. Clinical practice. Herpes zoster. N Engl J Med 2002; 347:340346.
  3. Katz J, Cooper EM, Walther RR, Sweeney EW, Dworkin RH. Acute pain in herpes zoster and its impact on health-related quality of life. Clin Infect Dis 2004; 39:342348.
  4. Hope-Simpson RE. The nature of herpes zoster: a long-term study and a new hypothesis. Proc R Soc Med 1965; 58:920.
  5. Lydick E, Epstein RS, Himmelberger D, White CJ. Herpes zoster and quality of life: a self-limited disease with severe impact. Neurology 1995; 45:S52S53.
  6. Kost RG, Straus SE. Postherpetic neuralgia—pathogenesis, treatment, and prevention. N Engl J Med 1996; 335:3242.
  7. Johnson R, McElhaney J, Pedalino B, Levin M. Prevention of herpes zoster and its painful and debilitating complications. Int J Infect Dis 2007; 11( suppl 2):S43S48.
  8. Oxman MN, Levin MJ, Johnson GR, et al. A vaccine to prevent herpes zoster and postherpetic neuralgia in older adults. N Engl J Med 2005; 352:22712284.
  9. Burke MS. Herpes zoster vaccine: clinical trial evidence and implications for medical practice. J Am Osteopath Assoc 2007; 107( suppl 1):S14S18.
  10. Betts RF. Vaccination strategies for the prevention of herpes zoster and postherpetic neuralgia. J Am Acad Dermatol 2007; 57( suppl):S143S147.
  11. Kroger AT, Atkinson WL, Marcuse EK, Pickering LK. General recommendations on immunization: recommendations of the Advisory Committee on Immunization Practices (ACIP). MMWR Recomm Rep 2006; 55:148.
  12. Merck. Zostavax zoster vaccine live suspension for subcutaneous injection. www.merck.com/product/usa/pi_circulars/z/zostavax_pi.pdf. Accessed 11/17/2008.
  13. Holodniy M. Prevention of shingles by varicella zoster virus vaccination. Expert Rev Vaccines 2006; 5:431443.
  14. Herpes zoster vaccine (Zostavax). Med Lett Drugs Ther 2006; 48:7374.
  15. Donahue JG, Choo PW, Manson JE, Platt R. The incidence of herpes zoster. Arch Intern Med 1995; 155:16051609.
  16. Harpaz R, Ortega-Sanchez IR, Seward JF. Prevention of herpes zoster: recommendations of the Advisory Committee on Immunization Practices (ACIP). MMWR Recomm Rep 2008; 57:130.
  17. Bader MS. Immunization for the elderly. Am J Med Sci 2007; 334:481486.
  18. Kilgore PE, Kruszon-Moran D, Seward JF, et al. Varicella in Americans from NHANES III: implications for control through routine immunization. J Med Virol 2003; 70( suppl 1):S111S118.
  19. Dworkin RH, White R, O’Connor AB, Baser O, Hawkins K. Healthcare costs of acute and chronic pain associated with a diagnosis of herpes zoster. J Am Geriatr Soc 2007; 55:11681175.
  20. Dworkin RH, White R, O’Connor AB, Hawkins K. Health care expenditure burden of persisting herpes zoster pain. Pain Med 2008; 9:348353.
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Hepatitis b virus (HBV) infection is sometimes challenging to manage because the disease has several stages and many clinical scenarios. HBV-infected patients are a very heterogeneous group, and we cannot apply a single management approach to all.

An understanding of the natural history of HBV infection and its diagnosis, which we reviewed in last month’s issue of this Journal1, is critical to understanding how to manage HBV infection.

In this article, we will review the principles of HBV management in adults, including those on immunosuppressant therapy and pregnant women, and guidelines for HBV vaccination.

WORKUP FOR HBV INFECTION

Once the diagnosis of HBV infection is made,1 a full management strategy should be formulated, as outlined below.

History

When and how did the patient acquire HBV? This information is important to know when making treatment decisions. For example, most acute, adult-onset cases (eg, acquired recently via sexual contact or parenteral drug abuse) resolve spontaneously within a few months, whereas most chronic cases (defined as being positive for HBV surface antigen for more than 6 months) were acquired at birth or in early childhood. Therefore, we should try to determine if the patient’s mother, siblings, household contacts, and sexual partners are positive for HBV surface antigen or have risk factors for HBV infection1; those without infection or immunity to HBV should be vaccinated.

People at risk of HBV infection include:

  • Parenteral drug users
  • People with multiple sexual partners
  • Household contacts and sexual partners of people positive for HBV surface antigen
  • Infants born to HBV-infected mothers
  • Patients and staff in custodial institutions for the developmentally disabled
  • Recipients of certain plasma-derived products (including patients with congenital coagulation defects)
  • Hemodialysis patients
  • Health and public-safety workers who have contact with blood
  • People born in areas where HBV is endemic, and their children.1

Does the patient have risk factors for other infections? Especially look for risk factors for human immunodeficiency virus (HIV) infection (eg, intravenous drug users and men having sex with men) and hepatitis D virus (intravenous drug users and patients from countries where hepatitis D virus infection is common, particularly Eastern Europe, Mediterranean countries, and the Amazon basin).

Does the patient have other modifiable risk factors for progressive liver disease, particularly alcohol abuse and obesity?

Does the patient have symptoms or signs of cirrhosis or hepatocellular carcinoma? Symptoms and signs that involve multiple systems could be extrahepatic manifestations of HBV infection, such as polyarteritis nodosa, which causes abdominal pain, arthralgia, hypertension, and asymmetric polyneuropathy.

Baseline laboratory evaluation

At baseline we should obtain a complete blood count, blood urea nitrogen level, serum creatinine level, liver profile, prothrombin time, urinalysis, and HBV serologic markers. In addition, HBV DNA can be detected in the serum at levels as low as 60 IU/mL, and it should be measured in the initial evaluation to establish a baseline before starting antiviral therapy in patients with chronic HBV infection and subsequently to monitor the response.

All patients with chronic HBV infection should also be tested for serologic markers of hepatitis A and hepatitis C; patients at risk of HIV and hepatitis D should also be tested for these diseases.

Not all patients need liver biopsy

Liver biopsy is the most accurate tool for staging the degree of HBV-related hepatic fibrosis in patients who have no obvious clinical manifestations of cirrhosis.

Not all patients with HBV infection need a biopsy, however. In patients with acute HBV infection, liver biopsy has no benefit except if concomitant pathology (eg, iron overload, nonalcoholic steatohepatitis, or alcoholic steatohepatitis) is suspected. In patients with chronic hepatitis B, liver biopsy is helpful when the viral load alone does not provide sufficient guidance for treatment, eg, when the viral load is less than 2 × 104 IU/mL in a patient positive for hepatitis e antigen or less than 2 × 103 IU/mL in a patient negative for hepatitis e antigen. (The presence of e antigen is a marker of HBV replication and infectivity.1) Biopsy should also be considered in those who have been infected a long time (eg, more than 10 years), because they may have occult cirrhosis, and if they do they may need to undergo antiviral treatment, endoscopy to look for varices, and surveillance for liver cancer.

In some situations it is easy to decide whether antiviral therapy is indicated without resorting to liver biopsy.

We would treat:

  • A patient positive for HBV e antigen for more than 6 months, whose HBV DNA level is higher than 2 × 104 IU/mL and whose alanine aminotransferase (ALT) level is high
  • A patient with HBV for more than 6 months who is negative for e antigen and who has an HBV DNA level higher than 2 × 103 IU/mL and elevated ALT
  • A patient with compensated HBV cirrhosis and an HBV DNA level higher than 2 × 103 IU/mL
  • A patient with HBV cirrhosis with decompensation and any detectable HBV DNA.

We would not treat:

  • An HBV carrier with a normal ALT level and an HBV DNA level that is lower than 2 × 104 IU/mL or undetectable.

If a patient does not fit into one of these categories but has HBV DNA, a liver biopsy showing significant necroinflammation or fibrosis would be an indication for treatment.

 

 

ANTIVIRAL THERAPY

Below, we summarize the main principles of anti-HBV therapy, emphasizing whether to treat and with which agent. Treatment of HBV infection in patients who are also infected with HIV or hepatitis C virus and in those with resistant or refractory hepatitis B is not within the scope of this article.

Acute infection rarely needs treatment

Acute, adult-acquired HBV infection is self-limited in most cases,1 and antiviral therapy is not routinely indicated.

In the rare cases of acute liver failure related to acute HBV infection, use of a nucleoside or nucleotide analogue reverse transcriptase inhibitor (nucleoside/nucleotide analogues) has been recommended, although no properly designed studies have been done.2,3 This recommendation is based on anecdotal experience, the relative safety of the antiviral agents, the serious nature of acute liver failure, and the possible need for emergency liver transplantation that requires prophylaxis against recurrence.

The nucleoside/nucleotide analogues that have been recommended in acute liver failure are lamivudine (Epivir), telbivudine (Tyzeka), and entecavir (Baraclude)—but not adefovir (Hepsera), which has a slow action and potential nephrotoxicity. Interferon drugs are contraindicated because they frequently cause side effects and can worsen hepatitis.4

Patients with acute liver failure should be referred promptly to a liver transplant center, and other management measures should also be started in a timely fashion.

In chronic HBV infection, treatment decisions are individualized

In chronic hepatitis B (ie, lasting > 6 months), treatment decisions should be based on the patient’s clinical situation and test results. The route and duration of infection (if known), history of previous hepatitis flares, ALT levels, current and previous HBV serologic test results and DNA levels, findings on liver biopsy (if previously done), and clinically suspected cirrhosis are all important to consider when deciding whether antiviral therapy is needed.

Because the HBV DNA level has a major impact on the risk of cirrhosis and hepatocellular carcinoma, it is increasingly the main variable used for treatment decisions. These levels, however, differ according to the clinical stage of chronic HBV infection.4,5 Table 1 summarizes the common indications for anti-viral therapy in chronic HBV infection.

For many patients with chronic HBV infection, observation without antiviral therapy is warranted, eg:

  • Young patients (< 30 years old) who acquired HBV at birth and who have persistently normal ALT levels with no evidence of advanced liver disease, regardless of their HBV DNA level (immune tolerance phase)
  • Chronic inactive carriers who have no e antigen, persistently normal ALT levels, and very low or undetectable levels of HBV DNA without evidence of significant liver injury.

These patients can be managed by internists by close monitoring for hepatitis flares with serial ALT measurements along with other general management measures.

Antiviral agents for chronic HBV infection

An ideal agent for treating hepatitis B does not exist. Trade-offs are the essence of agent selection.

Interferons, the first drugs shown to be effective against HBV, can in some respects be considered the best available initial choice, especially in patients positive for hepatitis e antigen. Interferons have numerous side effects but, unlike all the other options, they have a well-defined duration of treatment (4–6 months in patients positive for e antigen). The principal goal of this therapy is disappearance of e antigen.

Interferon-based therapy is not recommended in patients with cirrhosis, however, because of the risk of hepatic decompensation associated with interferon-related flares of hepatitis.4

Nucleoside/nucleotide analogues are easy to use and therefore are usually the first-line therapy. Problems with these agents are that the optimal treatment duration is not known, and that drug resistance can emerge (Table 2, Table 3).

Of the analogues now available, we recommend tenofovir (Viread) or entecavir. These agents are less likely to result in emergence of resistant strains than the prototypical agent, lamivudine. Three other agents, clevudine, adefovir, and tenofovir with emtricitabine (Truvada), are also available or in late stages of clinical trials.

Although single-agent antiviral therapy may someday be replaced by a multidrug regimen, the data so far are not sufficiently robust to recommend multidrug regimens except possibly in cases of established drug resistance.

Adjunctive management

Vaccinations. All patients with chronic hepatitis B should be vaccinated against hepatitis A if serologic testing indicates they have no immunity to it. Influenza and pneumococcal vaccines are recommended for all patients with chronic liver disease.6

Alcohol rehabilitation. Patients who abuse alcohol should be counseled, and many need consultation with a psychosocial care provider for alcohol rehabilitation.

Smoking cessation. Cigarette smoking is linked to a higher risk of hepatocellular carcinoma in patients with chronic liver disease, including chronic HBV infection.7 Therefore, smokers should be counseled to quit.

Surveillance for hepatocellular carcinoma. Hepatocellular carcinoma can occur in patients with chronic hepatitis B, in most cases on top of cirrhosis, although important exceptions exist. The American Association for the Study of Liver Diseases recommends surveillance for hepatocellular carcinoma in all HBV carriers with cirrhosis and in the following groups regardless of whether they have cirrhosis8:

  • Asian men age 40 and older
  • Asian women age 50 and older
  • African patients age 20 and older
  • Patients with a family history of hepatocellular carcinoma
  • Possibly, those with high HBV DNA levels and ongoing inflammatory activity.

In the United States, liver ultrasonography and alpha fetoprotein measurement every 6 to 12 months is a reasonable strategy.

If there is evidence of cirrhosis, esophagogastroduodenoscopy is recommended to screen for esophageal and gastric varices.

Laboratory, radiologic, and histologic findings of prognostic value in HBV-infected patients are outlined in Table 4.

 

 

SCREEN BEFORE CHEMOTHERAPY OR IMMUNOSUPPRESSIVE THERAPY

When patients who are positive for HBV surface antigen undergo immunosuppressive therapy or cancer chemotherapy, from 20% to 50% develop reactivated HBV infection with high HBV viral loads. Even patients who have resolved hepatitis B (ie, negative for HBV surface antigen and positive for surface antibody) may experience hepatitis B reactivation, with serious consequences. Hepatic decompensation and death have been reported during and after chemotherapy, especially in patients with cirrhosis.9 Therefore, patients at risk of HBV infection should be screened for it before starting these therapies.4 Furthermore, perhaps all patients about to undergo anticancer therapies that include anti-B-cell or anti-T-cell therapies or hematopoietic stem cell transplantation should be screened.9

Recent data indicate that many oncologists have not been screening for HBV.10 Hence, more effort is needed to make this important testing routine in this setting.

The initial tests in these patients should be liver chemistry tests, HBV surface antigen, HBV surface antibody, and HBV core antibody. In those who test positive for surface antigen, one should test for e antigen, e antibody, and HBV DNA.

Patients with indications for anti-HBV therapy (Table 1) should receive antiviral therapy. Otherwise, those positive for surface antigen should start taking anti-HBV medication at the start of chemotherapy or immunosuppressive therapy and should continue taking it until 6 months after the chemotherapy or immunosuppressive therapy is finished.4 Some experts also recommend starting anti-HBV therapy 7 days before the chemotherapy or immunosuppressive therapy and continuing it for 1 year afterward.10 Those with HBV DNA levels higher than 2 × 103 IU/mL should continue HBV therapy until they reach the same treatment end points as for immunocompetent patients as outlined above.4

Because we have little information on patients who are negative for surface antigen and who have antibodies against surface antigen and core antigen, we cannot make an unequivocal recommendation for anti-HBV therapy in this group.11 Rather, these patients should be monitored during immunosuppressive treatment, preferably with liver chemistry tests and HBV DNA titers, and antiviral drugs should be given as a deferred therapy upon evidence of HBV reactivation.9 Few cases of fatal hepatic failure in patients with this serologic pattern receiving rituximab (Rituxan) have been reported.12–14

With their small risk of drug resistance and rapid onset of action, entecavir or tenofovir may be the preferred anti-HBV therapy in patients undergoing immunosuppression or chemotherapy, especially in those requiring prolonged immunosuppressive therapy (longer than 12 months). In those requiring shorter courses, lamivudine or telbivudine is a possible alternative.4

OUTCOMES OF LIVER TRANSPLANTATION HAVE IMPROVED IN HBV PATIENTS

The early results of liver transplantation for HBV were discouraging because many patients developed rapidly progressive recurrent disease (fibrosing cholestatic hepatitis) and died within 12 to 18 months after the operation.15 However, patients with HBV are now treated perioperatively with lamivudine or adefovir combined with prolonged administration of hepatitis B immune globulin, and their survival now exceeds that of patients who receive transplants for many other conditions.16

Like patients with cirrhosis due to other causes, those with HBV-related cirrhosis who have any of the following should be referred for liver transplantation evaluation16:

  • A Model for End-Stage Liver Disease (MELD) score of 10 or higher (calculated from the serum creatinine level, total bilirubin level, and international normalized ratio of the prothrombin time; see www.unos.org/resources/MeldPeldCalculator.asp?index=98).
  • A Child-Turcotte-Pugh score of 7 or higher (Table 5).
  • A major complication of cirrhosis such as ascites, variceal bleeding, hepatocellular carcinoma, or hepatic encephalopathy.

PREVENTING VERTICAL TRANSMISSION

The major problem in young women with chronic HBV infection is the risk of vertical (mother-to-infant) transmission at delivery. The risk varies, depending on the viral load and e antigen status of the mother at the time of delivery; if she is positive for e antigen, the risk of HBV infection in the newborn is 70% to 90% by the age of 6 months if the newborn does not receive postexposure immunoprophylaxis; if the mother is positive for surface antigen but negative for e antigen, the risk of chronic infection is less than 10%, even without postexposure immunoprophylaxis.17

All women should be tested for HBV surface antigen early in pregnancy each time they become pregnant. If a patient tests negative early in pregnancy but continues behaviors that put her at risk of HBV infection (eg, having multiple sexual partners, having had a sex partner positive for surface antigen, using injection drugs, or contracting any sexually transmitted disease), she should be retested at the time of admission to the hospital for delivery.17 This also includes women who were not screened prenatally and those with clinical hepatitis.

Vaccine and immune globulin for the infant

If the mother is positive for HBV surface antigen, the infant should receive single-antigen HBV vaccine and hepatitis B immune globulin within 12 hours of birth, given at different injection sites.17 The second dose of vaccine should be given at age 1 to 2 months and the third at age 6 months (but not before age 24 weeks). The response to vaccination should be ascertained by testing for surface antigen and surface antibody after completion of the vaccine series, at age 9 to 18 months.

Maternal HBV infection does not contraindicate breastfeeding, as studies suggest that breastfeeding by a mother positive for surface antigen does not increase the infant’s risk of acquiring HBV infection.18

Which HBV therapy for a pregnant woman?

Some evidence supports antiviral therapy with nucleoside/nucleotide analogues in pregnant women who have viral loads of 106 IU/mL or higher. Lamivudine is safe in pregnancy and, together with immunization of the infant, reduces HBV transmission. Interferon-based therapy is contraindicated in pregnant women (and in women who may want to become pregnant) because of interferon’s antiproliferative effects. Nucleoside/nucleotide analogues classified as category B (eg, lamivudine, telbivudine, and tenofovir) could be used when the benefit of treating the pregnant mother outweighs the risk to the mother or fetus,2 although the possible effects of tenofovir on bone density argue against its use during pregnancy or breastfeeding.19

 

 

VACCINATION HAS REDUCED THE INCIDENCE OF ACUTE HEPATITIS B

HBV vaccination, a major achievement in HBV management, has played a big role in reducing the incidence of acute HBV infection, especially in children and adolescents.20

The currently available vaccines in the United States contain HBV surface antigen derived through recombinant DNA technology from yeast.21 Two single-antigen vaccines are available in the United States, under the brand names Recombivax HB and Engerix B. Of the three licensed combination vaccines, one (Twinrix) is used in adults, and two (Comvax and Pediarix) are used in infants and young children. Twinrix contains recombinant HBV surface antigens and inactivated hepatitis A virus and it is recommended for people age 18 years and older and at risk of both HBV and hepatitis A infections.20

Vaccinate all infants

All infants should be vaccinated against HBV as part of the recommended childhood immunization schedule. The vaccine is given on a three-dose schedule at birth and again at 1 month and 6 months of age.16 All children and adolescents under age 19 who have not previously received HBV vaccine should be vaccinated at any age with an appropriate dose and schedule.16

Vaccinate adults at risk—or who ask for it

Hepatitis B vaccination is recommended for all unvaccinated adults at risk of HBV infection and for all adults who ask for it (Table 6).20

Table 7 summarizes the adult dosing schedule for HBV vaccines.20 The vaccines should be given intramuscularly in the deltoid with a 1- to 2-inch needle, depending on the patient’s sex and weight.20 If doses are missed, the series should be resumed as soon as possible; there is no need to restart the series if the time between doses is longer than recommended.

Vaccination is less effective in older people

The three-dose vaccine series given intramuscularly initially, then again at 1 month and 6 months, produces a protective antibody response in approximately 30% to 55% of healthy adults under age 40 after the first dose, 75% after the second dose, and more than 90% after the third dose.21,22 After age 40, however, the proportion of persons who have a protective antibody response after three doses declines to less than 90%, and by age 60, protective levels of antibody develop in only 75%.23

Other factors that lower the response to vaccination are smoking, obesity, genetic factors, and immune suppression.20

Postvaccination serologic testing for immunity is not necessary after routine vaccination of adults, but it is recommended for patients whose subsequent clinical management depends on knowledge of their immune status, such as health care workers who have contact with patients or blood and are at ongoing risk of injuries with sharp instruments or needlesticks; chronic hemodialysis patients and people infected with HIV or otherwise immunocompromised; and sex partners or needle-sharing partners of people positive for HBV surface antigen.20 A protective concentration of HBV surface antibody measured 1 to 2 months after completion of the vaccine series is defined as 10 mIU/mL. Further periodic testing to document persistence of protective levels of surface antibody is not indicated.

If the first series does not ‘take’

Patients who do not respond to the primary vaccine series should complete a second three-dose series, with doses at 0, 1, and 6 months. Serologic testing is done 1 to 2 months after finishing the second series.

Patients who do not have protective levels of HBV surface antibody after revaccination by the appropriate schedule in the deltoid muscle (< 5% of those receiving six doses of hepatitis B vaccine) either are primary nonresponders or are infected with HBV.20 Therefore, they should be tested for HBV surface antigen. If this test is negative, then they should be considered susceptible to HBV infection and should be counseled accordingly.

Contraindications and precautions

HBV vaccination is contraindicated in people with a history of hypersensitivity to baker’s yeast or to a previous dose of HBV vaccine.20 Patients with moderate or severe acute illness at the time the shot is scheduled should wait until they recover before getting HBV vaccine. Pregnancy is not a contraindication.20

References
  1. Elgouhari HM, Abu-Rajab Tamimi T, Carey WD. Hepatitis B virus infection: understanding its epidemiology, course, and diagnosis. Cleve Clin J Med 2008; 75:881889.
  2. Stravitz RT, Kramer AH, Davern T, et al. Intensive care of patients with acute liver failure: recommendations of the U.S. Acute Liver Failure Study Group. Crit Care Med 2007; 35:24982508.
  3. Hoofnagle JH, Doo E, Liang TJ, Fleischer R, Lok AS. Management of hepatitis B: summary of a clinical research workshop. Hepatology 2007; 45:10561075.
  4. Lok AS, McMahon BJ. Chronic hepatitis B. Hepatology 2007; 45:507539.
  5. Keeffe EB, Dieterich DT, Han SH, et al. A treatment algorithm for the management of chronic hepatitis B virus infection in the United States. Clin Gastroenterol Hepatol 2004; 2:87106.
  6. Jacobs RJ, Meyerhoff AS, Saab S. Immunization needs of chronic liver disease patients seen in primary care versus specialist settings. Dig Dis Sci 2005; 50:15251531.
  7. Wang LY, You SL, Lu SN, et al. Risk of hepatocellular carcinoma and habits of alcohol drinking, betel quid chewing and cigarette smoking: a cohort of 2416 HBsAg–seropositive and 9421 HBsAg–seronegative male residents in Taiwan. Cancer Causes Control 2003; 14:241250.
  8. Bruix J, Sherman M; Practice Guidelines Committee, American Association for the Study of Liver Diseases. Management of hepatocellular carcinoma. Hepatology 2005; 42:12081236.
  9. Yeo W, Johnson PJ. Diagnosis, prevention and management of hepatitis B virus reactivation during anticancer therapy. Hepatology 2006; 43:209220.
  10. Tran T, Oh M, Poordad F, Martin P. Screening for hepatitis B in chemotherapy patients: survey of current oncology practices [abstract]. Hepatology 2007; 46:978A.
  11. Kohrt HE, Ouyang DL, Keeffe EB. Antiviral prophylaxis for chemotherapy–induced reactivation of chronic hepatitis B virus infection. Clin Liver Dis 2007; 11:965991.
  12. Westhoff TH, Jochimsen F, Schmittel A, et al. Fatal hepatitis B virus reactivation by an escape mutant following rituximab therapy. Blood 2003; 102:1930.
  13. Sarrecchia C, Cappelli A, Aiello P. HBV reactivation with fatal fulminating hepatitis during rituximab treatment in a subject negative for HBsAg and positive for HBsAb and HBcAb. J Infect Chemother 2005; 11:189191.
  14. Law JK, Ho JK, Hoskins PJ, Erb SR, Steinbrecher UP, Yoshida FM. Fatal reactivation of hepatitis B post-chemotherapy for lymphoma in a hepatitis B surface antigen-negative, hepatitis B core antibody-positive patient: potential implications for future prophylaxis recommendations. Leuk Lymphoma 2005; 46:10851089.
  15. Todo S, Demetris AJ, Van Thiel D, Teperman L, Fung JJ, Starzl TE. Orthotopic liver transplantation for patients with hepatitis B virus-related liver disease. Hepatology 1991; 13:619626.
  16. Murray KF, Carithers RLAASLD. AASLD practice guidelines: Evaluation of the patient for liver transplantation. Hepatology 2005; 41:14071432.
  17. Mast EE, Margolis HS, Fiore AE, et al. A comprehensive immunization strategy to eliminate transmission of hepatitis B virus infection in the United States: recommendations of the Advisory Committee on Immunization Practices (ACIP) part 1: immunization of infants, children, and adolescents. MMWR Recomm Rep 2005; 54:131.
  18. Beasley RP, Stevens CE, Shiao IS, Meng HC. Evidence against breast–feeding as a mechanism for vertical transmission of hepatitis B. Lancet 1975; 2:740741.
  19. Parsonage MJ, Wilkins EG, Snowden N, Issa BG, Savage MW. The development of hypophosphataemic osteomalacia with myopathy in two patients with HIV infection receiving tenofovir therapy. HIV Med 2005; 6:341346.
  20. Mast EE, Weinbaum CM, Fiore AE, et al. A comprehensive immunization strategy to eliminate transmission of hepatitis B virus infection in the United States: recommendations of the Advisory Committee on Immunization Practices (ACIP) Part II: immunization of adults. MMWR Recomm Rep 2006; 55:133.
  21. Andre FE. Summary of safety and efficacy data on a yeast–derived hepatitis B vaccine. Am J Med 1989; 87:14S20S.
  22. Zajac BA, West DJ, McAleer WJ, Scolnick EM. Overview of clinical studies with hepatitis B vaccine made by recombinant DNA. J Infect 1986; 13( suppl A):3945.
  23. Averhoff F, Mahoney F, Coleman P, Schatz G, Hurwitz E, Margolis H. Immunogenicity of hepatitis B vaccines: implications for persons at occupational risk for hepatitis B virus infection. Am J Prev Med 1998; 15:18.
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Tarek I. Abu-Rajab Tamimi, MD
Department of Gastroenterology and Hepatology, Cleveland Clinic

William Carey, MD
Department of Gastroenterology and Hepatology, Cleveland Clinic

Address: William D. Carey, MD, Division of Gastroenterolgy and Hepatology, A30, Cleveland Clinic, 9500 Euclid Avenue, Cleveland, OH 44195; e-mail [email protected]

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Tarek I. Abu-Rajab Tamimi, MD
Department of Gastroenterology and Hepatology, Cleveland Clinic

William Carey, MD
Department of Gastroenterology and Hepatology, Cleveland Clinic

Address: William D. Carey, MD, Division of Gastroenterolgy and Hepatology, A30, Cleveland Clinic, 9500 Euclid Avenue, Cleveland, OH 44195; e-mail [email protected]

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Tarek I. Abu-Rajab Tamimi, MD
Department of Gastroenterology and Hepatology, Cleveland Clinic

William Carey, MD
Department of Gastroenterology and Hepatology, Cleveland Clinic

Address: William D. Carey, MD, Division of Gastroenterolgy and Hepatology, A30, Cleveland Clinic, 9500 Euclid Avenue, Cleveland, OH 44195; e-mail [email protected]

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Related Articles

Hepatitis b virus (HBV) infection is sometimes challenging to manage because the disease has several stages and many clinical scenarios. HBV-infected patients are a very heterogeneous group, and we cannot apply a single management approach to all.

An understanding of the natural history of HBV infection and its diagnosis, which we reviewed in last month’s issue of this Journal1, is critical to understanding how to manage HBV infection.

In this article, we will review the principles of HBV management in adults, including those on immunosuppressant therapy and pregnant women, and guidelines for HBV vaccination.

WORKUP FOR HBV INFECTION

Once the diagnosis of HBV infection is made,1 a full management strategy should be formulated, as outlined below.

History

When and how did the patient acquire HBV? This information is important to know when making treatment decisions. For example, most acute, adult-onset cases (eg, acquired recently via sexual contact or parenteral drug abuse) resolve spontaneously within a few months, whereas most chronic cases (defined as being positive for HBV surface antigen for more than 6 months) were acquired at birth or in early childhood. Therefore, we should try to determine if the patient’s mother, siblings, household contacts, and sexual partners are positive for HBV surface antigen or have risk factors for HBV infection1; those without infection or immunity to HBV should be vaccinated.

People at risk of HBV infection include:

  • Parenteral drug users
  • People with multiple sexual partners
  • Household contacts and sexual partners of people positive for HBV surface antigen
  • Infants born to HBV-infected mothers
  • Patients and staff in custodial institutions for the developmentally disabled
  • Recipients of certain plasma-derived products (including patients with congenital coagulation defects)
  • Hemodialysis patients
  • Health and public-safety workers who have contact with blood
  • People born in areas where HBV is endemic, and their children.1

Does the patient have risk factors for other infections? Especially look for risk factors for human immunodeficiency virus (HIV) infection (eg, intravenous drug users and men having sex with men) and hepatitis D virus (intravenous drug users and patients from countries where hepatitis D virus infection is common, particularly Eastern Europe, Mediterranean countries, and the Amazon basin).

Does the patient have other modifiable risk factors for progressive liver disease, particularly alcohol abuse and obesity?

Does the patient have symptoms or signs of cirrhosis or hepatocellular carcinoma? Symptoms and signs that involve multiple systems could be extrahepatic manifestations of HBV infection, such as polyarteritis nodosa, which causes abdominal pain, arthralgia, hypertension, and asymmetric polyneuropathy.

Baseline laboratory evaluation

At baseline we should obtain a complete blood count, blood urea nitrogen level, serum creatinine level, liver profile, prothrombin time, urinalysis, and HBV serologic markers. In addition, HBV DNA can be detected in the serum at levels as low as 60 IU/mL, and it should be measured in the initial evaluation to establish a baseline before starting antiviral therapy in patients with chronic HBV infection and subsequently to monitor the response.

All patients with chronic HBV infection should also be tested for serologic markers of hepatitis A and hepatitis C; patients at risk of HIV and hepatitis D should also be tested for these diseases.

Not all patients need liver biopsy

Liver biopsy is the most accurate tool for staging the degree of HBV-related hepatic fibrosis in patients who have no obvious clinical manifestations of cirrhosis.

Not all patients with HBV infection need a biopsy, however. In patients with acute HBV infection, liver biopsy has no benefit except if concomitant pathology (eg, iron overload, nonalcoholic steatohepatitis, or alcoholic steatohepatitis) is suspected. In patients with chronic hepatitis B, liver biopsy is helpful when the viral load alone does not provide sufficient guidance for treatment, eg, when the viral load is less than 2 × 104 IU/mL in a patient positive for hepatitis e antigen or less than 2 × 103 IU/mL in a patient negative for hepatitis e antigen. (The presence of e antigen is a marker of HBV replication and infectivity.1) Biopsy should also be considered in those who have been infected a long time (eg, more than 10 years), because they may have occult cirrhosis, and if they do they may need to undergo antiviral treatment, endoscopy to look for varices, and surveillance for liver cancer.

In some situations it is easy to decide whether antiviral therapy is indicated without resorting to liver biopsy.

We would treat:

  • A patient positive for HBV e antigen for more than 6 months, whose HBV DNA level is higher than 2 × 104 IU/mL and whose alanine aminotransferase (ALT) level is high
  • A patient with HBV for more than 6 months who is negative for e antigen and who has an HBV DNA level higher than 2 × 103 IU/mL and elevated ALT
  • A patient with compensated HBV cirrhosis and an HBV DNA level higher than 2 × 103 IU/mL
  • A patient with HBV cirrhosis with decompensation and any detectable HBV DNA.

We would not treat:

  • An HBV carrier with a normal ALT level and an HBV DNA level that is lower than 2 × 104 IU/mL or undetectable.

If a patient does not fit into one of these categories but has HBV DNA, a liver biopsy showing significant necroinflammation or fibrosis would be an indication for treatment.

 

 

ANTIVIRAL THERAPY

Below, we summarize the main principles of anti-HBV therapy, emphasizing whether to treat and with which agent. Treatment of HBV infection in patients who are also infected with HIV or hepatitis C virus and in those with resistant or refractory hepatitis B is not within the scope of this article.

Acute infection rarely needs treatment

Acute, adult-acquired HBV infection is self-limited in most cases,1 and antiviral therapy is not routinely indicated.

In the rare cases of acute liver failure related to acute HBV infection, use of a nucleoside or nucleotide analogue reverse transcriptase inhibitor (nucleoside/nucleotide analogues) has been recommended, although no properly designed studies have been done.2,3 This recommendation is based on anecdotal experience, the relative safety of the antiviral agents, the serious nature of acute liver failure, and the possible need for emergency liver transplantation that requires prophylaxis against recurrence.

The nucleoside/nucleotide analogues that have been recommended in acute liver failure are lamivudine (Epivir), telbivudine (Tyzeka), and entecavir (Baraclude)—but not adefovir (Hepsera), which has a slow action and potential nephrotoxicity. Interferon drugs are contraindicated because they frequently cause side effects and can worsen hepatitis.4

Patients with acute liver failure should be referred promptly to a liver transplant center, and other management measures should also be started in a timely fashion.

In chronic HBV infection, treatment decisions are individualized

In chronic hepatitis B (ie, lasting > 6 months), treatment decisions should be based on the patient’s clinical situation and test results. The route and duration of infection (if known), history of previous hepatitis flares, ALT levels, current and previous HBV serologic test results and DNA levels, findings on liver biopsy (if previously done), and clinically suspected cirrhosis are all important to consider when deciding whether antiviral therapy is needed.

Because the HBV DNA level has a major impact on the risk of cirrhosis and hepatocellular carcinoma, it is increasingly the main variable used for treatment decisions. These levels, however, differ according to the clinical stage of chronic HBV infection.4,5 Table 1 summarizes the common indications for anti-viral therapy in chronic HBV infection.

For many patients with chronic HBV infection, observation without antiviral therapy is warranted, eg:

  • Young patients (< 30 years old) who acquired HBV at birth and who have persistently normal ALT levels with no evidence of advanced liver disease, regardless of their HBV DNA level (immune tolerance phase)
  • Chronic inactive carriers who have no e antigen, persistently normal ALT levels, and very low or undetectable levels of HBV DNA without evidence of significant liver injury.

These patients can be managed by internists by close monitoring for hepatitis flares with serial ALT measurements along with other general management measures.

Antiviral agents for chronic HBV infection

An ideal agent for treating hepatitis B does not exist. Trade-offs are the essence of agent selection.

Interferons, the first drugs shown to be effective against HBV, can in some respects be considered the best available initial choice, especially in patients positive for hepatitis e antigen. Interferons have numerous side effects but, unlike all the other options, they have a well-defined duration of treatment (4–6 months in patients positive for e antigen). The principal goal of this therapy is disappearance of e antigen.

Interferon-based therapy is not recommended in patients with cirrhosis, however, because of the risk of hepatic decompensation associated with interferon-related flares of hepatitis.4

Nucleoside/nucleotide analogues are easy to use and therefore are usually the first-line therapy. Problems with these agents are that the optimal treatment duration is not known, and that drug resistance can emerge (Table 2, Table 3).

Of the analogues now available, we recommend tenofovir (Viread) or entecavir. These agents are less likely to result in emergence of resistant strains than the prototypical agent, lamivudine. Three other agents, clevudine, adefovir, and tenofovir with emtricitabine (Truvada), are also available or in late stages of clinical trials.

Although single-agent antiviral therapy may someday be replaced by a multidrug regimen, the data so far are not sufficiently robust to recommend multidrug regimens except possibly in cases of established drug resistance.

Adjunctive management

Vaccinations. All patients with chronic hepatitis B should be vaccinated against hepatitis A if serologic testing indicates they have no immunity to it. Influenza and pneumococcal vaccines are recommended for all patients with chronic liver disease.6

Alcohol rehabilitation. Patients who abuse alcohol should be counseled, and many need consultation with a psychosocial care provider for alcohol rehabilitation.

Smoking cessation. Cigarette smoking is linked to a higher risk of hepatocellular carcinoma in patients with chronic liver disease, including chronic HBV infection.7 Therefore, smokers should be counseled to quit.

Surveillance for hepatocellular carcinoma. Hepatocellular carcinoma can occur in patients with chronic hepatitis B, in most cases on top of cirrhosis, although important exceptions exist. The American Association for the Study of Liver Diseases recommends surveillance for hepatocellular carcinoma in all HBV carriers with cirrhosis and in the following groups regardless of whether they have cirrhosis8:

  • Asian men age 40 and older
  • Asian women age 50 and older
  • African patients age 20 and older
  • Patients with a family history of hepatocellular carcinoma
  • Possibly, those with high HBV DNA levels and ongoing inflammatory activity.

In the United States, liver ultrasonography and alpha fetoprotein measurement every 6 to 12 months is a reasonable strategy.

If there is evidence of cirrhosis, esophagogastroduodenoscopy is recommended to screen for esophageal and gastric varices.

Laboratory, radiologic, and histologic findings of prognostic value in HBV-infected patients are outlined in Table 4.

 

 

SCREEN BEFORE CHEMOTHERAPY OR IMMUNOSUPPRESSIVE THERAPY

When patients who are positive for HBV surface antigen undergo immunosuppressive therapy or cancer chemotherapy, from 20% to 50% develop reactivated HBV infection with high HBV viral loads. Even patients who have resolved hepatitis B (ie, negative for HBV surface antigen and positive for surface antibody) may experience hepatitis B reactivation, with serious consequences. Hepatic decompensation and death have been reported during and after chemotherapy, especially in patients with cirrhosis.9 Therefore, patients at risk of HBV infection should be screened for it before starting these therapies.4 Furthermore, perhaps all patients about to undergo anticancer therapies that include anti-B-cell or anti-T-cell therapies or hematopoietic stem cell transplantation should be screened.9

Recent data indicate that many oncologists have not been screening for HBV.10 Hence, more effort is needed to make this important testing routine in this setting.

The initial tests in these patients should be liver chemistry tests, HBV surface antigen, HBV surface antibody, and HBV core antibody. In those who test positive for surface antigen, one should test for e antigen, e antibody, and HBV DNA.

Patients with indications for anti-HBV therapy (Table 1) should receive antiviral therapy. Otherwise, those positive for surface antigen should start taking anti-HBV medication at the start of chemotherapy or immunosuppressive therapy and should continue taking it until 6 months after the chemotherapy or immunosuppressive therapy is finished.4 Some experts also recommend starting anti-HBV therapy 7 days before the chemotherapy or immunosuppressive therapy and continuing it for 1 year afterward.10 Those with HBV DNA levels higher than 2 × 103 IU/mL should continue HBV therapy until they reach the same treatment end points as for immunocompetent patients as outlined above.4

Because we have little information on patients who are negative for surface antigen and who have antibodies against surface antigen and core antigen, we cannot make an unequivocal recommendation for anti-HBV therapy in this group.11 Rather, these patients should be monitored during immunosuppressive treatment, preferably with liver chemistry tests and HBV DNA titers, and antiviral drugs should be given as a deferred therapy upon evidence of HBV reactivation.9 Few cases of fatal hepatic failure in patients with this serologic pattern receiving rituximab (Rituxan) have been reported.12–14

With their small risk of drug resistance and rapid onset of action, entecavir or tenofovir may be the preferred anti-HBV therapy in patients undergoing immunosuppression or chemotherapy, especially in those requiring prolonged immunosuppressive therapy (longer than 12 months). In those requiring shorter courses, lamivudine or telbivudine is a possible alternative.4

OUTCOMES OF LIVER TRANSPLANTATION HAVE IMPROVED IN HBV PATIENTS

The early results of liver transplantation for HBV were discouraging because many patients developed rapidly progressive recurrent disease (fibrosing cholestatic hepatitis) and died within 12 to 18 months after the operation.15 However, patients with HBV are now treated perioperatively with lamivudine or adefovir combined with prolonged administration of hepatitis B immune globulin, and their survival now exceeds that of patients who receive transplants for many other conditions.16

Like patients with cirrhosis due to other causes, those with HBV-related cirrhosis who have any of the following should be referred for liver transplantation evaluation16:

  • A Model for End-Stage Liver Disease (MELD) score of 10 or higher (calculated from the serum creatinine level, total bilirubin level, and international normalized ratio of the prothrombin time; see www.unos.org/resources/MeldPeldCalculator.asp?index=98).
  • A Child-Turcotte-Pugh score of 7 or higher (Table 5).
  • A major complication of cirrhosis such as ascites, variceal bleeding, hepatocellular carcinoma, or hepatic encephalopathy.

PREVENTING VERTICAL TRANSMISSION

The major problem in young women with chronic HBV infection is the risk of vertical (mother-to-infant) transmission at delivery. The risk varies, depending on the viral load and e antigen status of the mother at the time of delivery; if she is positive for e antigen, the risk of HBV infection in the newborn is 70% to 90% by the age of 6 months if the newborn does not receive postexposure immunoprophylaxis; if the mother is positive for surface antigen but negative for e antigen, the risk of chronic infection is less than 10%, even without postexposure immunoprophylaxis.17

All women should be tested for HBV surface antigen early in pregnancy each time they become pregnant. If a patient tests negative early in pregnancy but continues behaviors that put her at risk of HBV infection (eg, having multiple sexual partners, having had a sex partner positive for surface antigen, using injection drugs, or contracting any sexually transmitted disease), she should be retested at the time of admission to the hospital for delivery.17 This also includes women who were not screened prenatally and those with clinical hepatitis.

Vaccine and immune globulin for the infant

If the mother is positive for HBV surface antigen, the infant should receive single-antigen HBV vaccine and hepatitis B immune globulin within 12 hours of birth, given at different injection sites.17 The second dose of vaccine should be given at age 1 to 2 months and the third at age 6 months (but not before age 24 weeks). The response to vaccination should be ascertained by testing for surface antigen and surface antibody after completion of the vaccine series, at age 9 to 18 months.

Maternal HBV infection does not contraindicate breastfeeding, as studies suggest that breastfeeding by a mother positive for surface antigen does not increase the infant’s risk of acquiring HBV infection.18

Which HBV therapy for a pregnant woman?

Some evidence supports antiviral therapy with nucleoside/nucleotide analogues in pregnant women who have viral loads of 106 IU/mL or higher. Lamivudine is safe in pregnancy and, together with immunization of the infant, reduces HBV transmission. Interferon-based therapy is contraindicated in pregnant women (and in women who may want to become pregnant) because of interferon’s antiproliferative effects. Nucleoside/nucleotide analogues classified as category B (eg, lamivudine, telbivudine, and tenofovir) could be used when the benefit of treating the pregnant mother outweighs the risk to the mother or fetus,2 although the possible effects of tenofovir on bone density argue against its use during pregnancy or breastfeeding.19

 

 

VACCINATION HAS REDUCED THE INCIDENCE OF ACUTE HEPATITIS B

HBV vaccination, a major achievement in HBV management, has played a big role in reducing the incidence of acute HBV infection, especially in children and adolescents.20

The currently available vaccines in the United States contain HBV surface antigen derived through recombinant DNA technology from yeast.21 Two single-antigen vaccines are available in the United States, under the brand names Recombivax HB and Engerix B. Of the three licensed combination vaccines, one (Twinrix) is used in adults, and two (Comvax and Pediarix) are used in infants and young children. Twinrix contains recombinant HBV surface antigens and inactivated hepatitis A virus and it is recommended for people age 18 years and older and at risk of both HBV and hepatitis A infections.20

Vaccinate all infants

All infants should be vaccinated against HBV as part of the recommended childhood immunization schedule. The vaccine is given on a three-dose schedule at birth and again at 1 month and 6 months of age.16 All children and adolescents under age 19 who have not previously received HBV vaccine should be vaccinated at any age with an appropriate dose and schedule.16

Vaccinate adults at risk—or who ask for it

Hepatitis B vaccination is recommended for all unvaccinated adults at risk of HBV infection and for all adults who ask for it (Table 6).20

Table 7 summarizes the adult dosing schedule for HBV vaccines.20 The vaccines should be given intramuscularly in the deltoid with a 1- to 2-inch needle, depending on the patient’s sex and weight.20 If doses are missed, the series should be resumed as soon as possible; there is no need to restart the series if the time between doses is longer than recommended.

Vaccination is less effective in older people

The three-dose vaccine series given intramuscularly initially, then again at 1 month and 6 months, produces a protective antibody response in approximately 30% to 55% of healthy adults under age 40 after the first dose, 75% after the second dose, and more than 90% after the third dose.21,22 After age 40, however, the proportion of persons who have a protective antibody response after three doses declines to less than 90%, and by age 60, protective levels of antibody develop in only 75%.23

Other factors that lower the response to vaccination are smoking, obesity, genetic factors, and immune suppression.20

Postvaccination serologic testing for immunity is not necessary after routine vaccination of adults, but it is recommended for patients whose subsequent clinical management depends on knowledge of their immune status, such as health care workers who have contact with patients or blood and are at ongoing risk of injuries with sharp instruments or needlesticks; chronic hemodialysis patients and people infected with HIV or otherwise immunocompromised; and sex partners or needle-sharing partners of people positive for HBV surface antigen.20 A protective concentration of HBV surface antibody measured 1 to 2 months after completion of the vaccine series is defined as 10 mIU/mL. Further periodic testing to document persistence of protective levels of surface antibody is not indicated.

If the first series does not ‘take’

Patients who do not respond to the primary vaccine series should complete a second three-dose series, with doses at 0, 1, and 6 months. Serologic testing is done 1 to 2 months after finishing the second series.

Patients who do not have protective levels of HBV surface antibody after revaccination by the appropriate schedule in the deltoid muscle (< 5% of those receiving six doses of hepatitis B vaccine) either are primary nonresponders or are infected with HBV.20 Therefore, they should be tested for HBV surface antigen. If this test is negative, then they should be considered susceptible to HBV infection and should be counseled accordingly.

Contraindications and precautions

HBV vaccination is contraindicated in people with a history of hypersensitivity to baker’s yeast or to a previous dose of HBV vaccine.20 Patients with moderate or severe acute illness at the time the shot is scheduled should wait until they recover before getting HBV vaccine. Pregnancy is not a contraindication.20

Hepatitis b virus (HBV) infection is sometimes challenging to manage because the disease has several stages and many clinical scenarios. HBV-infected patients are a very heterogeneous group, and we cannot apply a single management approach to all.

An understanding of the natural history of HBV infection and its diagnosis, which we reviewed in last month’s issue of this Journal1, is critical to understanding how to manage HBV infection.

In this article, we will review the principles of HBV management in adults, including those on immunosuppressant therapy and pregnant women, and guidelines for HBV vaccination.

WORKUP FOR HBV INFECTION

Once the diagnosis of HBV infection is made,1 a full management strategy should be formulated, as outlined below.

History

When and how did the patient acquire HBV? This information is important to know when making treatment decisions. For example, most acute, adult-onset cases (eg, acquired recently via sexual contact or parenteral drug abuse) resolve spontaneously within a few months, whereas most chronic cases (defined as being positive for HBV surface antigen for more than 6 months) were acquired at birth or in early childhood. Therefore, we should try to determine if the patient’s mother, siblings, household contacts, and sexual partners are positive for HBV surface antigen or have risk factors for HBV infection1; those without infection or immunity to HBV should be vaccinated.

People at risk of HBV infection include:

  • Parenteral drug users
  • People with multiple sexual partners
  • Household contacts and sexual partners of people positive for HBV surface antigen
  • Infants born to HBV-infected mothers
  • Patients and staff in custodial institutions for the developmentally disabled
  • Recipients of certain plasma-derived products (including patients with congenital coagulation defects)
  • Hemodialysis patients
  • Health and public-safety workers who have contact with blood
  • People born in areas where HBV is endemic, and their children.1

Does the patient have risk factors for other infections? Especially look for risk factors for human immunodeficiency virus (HIV) infection (eg, intravenous drug users and men having sex with men) and hepatitis D virus (intravenous drug users and patients from countries where hepatitis D virus infection is common, particularly Eastern Europe, Mediterranean countries, and the Amazon basin).

Does the patient have other modifiable risk factors for progressive liver disease, particularly alcohol abuse and obesity?

Does the patient have symptoms or signs of cirrhosis or hepatocellular carcinoma? Symptoms and signs that involve multiple systems could be extrahepatic manifestations of HBV infection, such as polyarteritis nodosa, which causes abdominal pain, arthralgia, hypertension, and asymmetric polyneuropathy.

Baseline laboratory evaluation

At baseline we should obtain a complete blood count, blood urea nitrogen level, serum creatinine level, liver profile, prothrombin time, urinalysis, and HBV serologic markers. In addition, HBV DNA can be detected in the serum at levels as low as 60 IU/mL, and it should be measured in the initial evaluation to establish a baseline before starting antiviral therapy in patients with chronic HBV infection and subsequently to monitor the response.

All patients with chronic HBV infection should also be tested for serologic markers of hepatitis A and hepatitis C; patients at risk of HIV and hepatitis D should also be tested for these diseases.

Not all patients need liver biopsy

Liver biopsy is the most accurate tool for staging the degree of HBV-related hepatic fibrosis in patients who have no obvious clinical manifestations of cirrhosis.

Not all patients with HBV infection need a biopsy, however. In patients with acute HBV infection, liver biopsy has no benefit except if concomitant pathology (eg, iron overload, nonalcoholic steatohepatitis, or alcoholic steatohepatitis) is suspected. In patients with chronic hepatitis B, liver biopsy is helpful when the viral load alone does not provide sufficient guidance for treatment, eg, when the viral load is less than 2 × 104 IU/mL in a patient positive for hepatitis e antigen or less than 2 × 103 IU/mL in a patient negative for hepatitis e antigen. (The presence of e antigen is a marker of HBV replication and infectivity.1) Biopsy should also be considered in those who have been infected a long time (eg, more than 10 years), because they may have occult cirrhosis, and if they do they may need to undergo antiviral treatment, endoscopy to look for varices, and surveillance for liver cancer.

In some situations it is easy to decide whether antiviral therapy is indicated without resorting to liver biopsy.

We would treat:

  • A patient positive for HBV e antigen for more than 6 months, whose HBV DNA level is higher than 2 × 104 IU/mL and whose alanine aminotransferase (ALT) level is high
  • A patient with HBV for more than 6 months who is negative for e antigen and who has an HBV DNA level higher than 2 × 103 IU/mL and elevated ALT
  • A patient with compensated HBV cirrhosis and an HBV DNA level higher than 2 × 103 IU/mL
  • A patient with HBV cirrhosis with decompensation and any detectable HBV DNA.

We would not treat:

  • An HBV carrier with a normal ALT level and an HBV DNA level that is lower than 2 × 104 IU/mL or undetectable.

If a patient does not fit into one of these categories but has HBV DNA, a liver biopsy showing significant necroinflammation or fibrosis would be an indication for treatment.

 

 

ANTIVIRAL THERAPY

Below, we summarize the main principles of anti-HBV therapy, emphasizing whether to treat and with which agent. Treatment of HBV infection in patients who are also infected with HIV or hepatitis C virus and in those with resistant or refractory hepatitis B is not within the scope of this article.

Acute infection rarely needs treatment

Acute, adult-acquired HBV infection is self-limited in most cases,1 and antiviral therapy is not routinely indicated.

In the rare cases of acute liver failure related to acute HBV infection, use of a nucleoside or nucleotide analogue reverse transcriptase inhibitor (nucleoside/nucleotide analogues) has been recommended, although no properly designed studies have been done.2,3 This recommendation is based on anecdotal experience, the relative safety of the antiviral agents, the serious nature of acute liver failure, and the possible need for emergency liver transplantation that requires prophylaxis against recurrence.

The nucleoside/nucleotide analogues that have been recommended in acute liver failure are lamivudine (Epivir), telbivudine (Tyzeka), and entecavir (Baraclude)—but not adefovir (Hepsera), which has a slow action and potential nephrotoxicity. Interferon drugs are contraindicated because they frequently cause side effects and can worsen hepatitis.4

Patients with acute liver failure should be referred promptly to a liver transplant center, and other management measures should also be started in a timely fashion.

In chronic HBV infection, treatment decisions are individualized

In chronic hepatitis B (ie, lasting > 6 months), treatment decisions should be based on the patient’s clinical situation and test results. The route and duration of infection (if known), history of previous hepatitis flares, ALT levels, current and previous HBV serologic test results and DNA levels, findings on liver biopsy (if previously done), and clinically suspected cirrhosis are all important to consider when deciding whether antiviral therapy is needed.

Because the HBV DNA level has a major impact on the risk of cirrhosis and hepatocellular carcinoma, it is increasingly the main variable used for treatment decisions. These levels, however, differ according to the clinical stage of chronic HBV infection.4,5 Table 1 summarizes the common indications for anti-viral therapy in chronic HBV infection.

For many patients with chronic HBV infection, observation without antiviral therapy is warranted, eg:

  • Young patients (< 30 years old) who acquired HBV at birth and who have persistently normal ALT levels with no evidence of advanced liver disease, regardless of their HBV DNA level (immune tolerance phase)
  • Chronic inactive carriers who have no e antigen, persistently normal ALT levels, and very low or undetectable levels of HBV DNA without evidence of significant liver injury.

These patients can be managed by internists by close monitoring for hepatitis flares with serial ALT measurements along with other general management measures.

Antiviral agents for chronic HBV infection

An ideal agent for treating hepatitis B does not exist. Trade-offs are the essence of agent selection.

Interferons, the first drugs shown to be effective against HBV, can in some respects be considered the best available initial choice, especially in patients positive for hepatitis e antigen. Interferons have numerous side effects but, unlike all the other options, they have a well-defined duration of treatment (4–6 months in patients positive for e antigen). The principal goal of this therapy is disappearance of e antigen.

Interferon-based therapy is not recommended in patients with cirrhosis, however, because of the risk of hepatic decompensation associated with interferon-related flares of hepatitis.4

Nucleoside/nucleotide analogues are easy to use and therefore are usually the first-line therapy. Problems with these agents are that the optimal treatment duration is not known, and that drug resistance can emerge (Table 2, Table 3).

Of the analogues now available, we recommend tenofovir (Viread) or entecavir. These agents are less likely to result in emergence of resistant strains than the prototypical agent, lamivudine. Three other agents, clevudine, adefovir, and tenofovir with emtricitabine (Truvada), are also available or in late stages of clinical trials.

Although single-agent antiviral therapy may someday be replaced by a multidrug regimen, the data so far are not sufficiently robust to recommend multidrug regimens except possibly in cases of established drug resistance.

Adjunctive management

Vaccinations. All patients with chronic hepatitis B should be vaccinated against hepatitis A if serologic testing indicates they have no immunity to it. Influenza and pneumococcal vaccines are recommended for all patients with chronic liver disease.6

Alcohol rehabilitation. Patients who abuse alcohol should be counseled, and many need consultation with a psychosocial care provider for alcohol rehabilitation.

Smoking cessation. Cigarette smoking is linked to a higher risk of hepatocellular carcinoma in patients with chronic liver disease, including chronic HBV infection.7 Therefore, smokers should be counseled to quit.

Surveillance for hepatocellular carcinoma. Hepatocellular carcinoma can occur in patients with chronic hepatitis B, in most cases on top of cirrhosis, although important exceptions exist. The American Association for the Study of Liver Diseases recommends surveillance for hepatocellular carcinoma in all HBV carriers with cirrhosis and in the following groups regardless of whether they have cirrhosis8:

  • Asian men age 40 and older
  • Asian women age 50 and older
  • African patients age 20 and older
  • Patients with a family history of hepatocellular carcinoma
  • Possibly, those with high HBV DNA levels and ongoing inflammatory activity.

In the United States, liver ultrasonography and alpha fetoprotein measurement every 6 to 12 months is a reasonable strategy.

If there is evidence of cirrhosis, esophagogastroduodenoscopy is recommended to screen for esophageal and gastric varices.

Laboratory, radiologic, and histologic findings of prognostic value in HBV-infected patients are outlined in Table 4.

 

 

SCREEN BEFORE CHEMOTHERAPY OR IMMUNOSUPPRESSIVE THERAPY

When patients who are positive for HBV surface antigen undergo immunosuppressive therapy or cancer chemotherapy, from 20% to 50% develop reactivated HBV infection with high HBV viral loads. Even patients who have resolved hepatitis B (ie, negative for HBV surface antigen and positive for surface antibody) may experience hepatitis B reactivation, with serious consequences. Hepatic decompensation and death have been reported during and after chemotherapy, especially in patients with cirrhosis.9 Therefore, patients at risk of HBV infection should be screened for it before starting these therapies.4 Furthermore, perhaps all patients about to undergo anticancer therapies that include anti-B-cell or anti-T-cell therapies or hematopoietic stem cell transplantation should be screened.9

Recent data indicate that many oncologists have not been screening for HBV.10 Hence, more effort is needed to make this important testing routine in this setting.

The initial tests in these patients should be liver chemistry tests, HBV surface antigen, HBV surface antibody, and HBV core antibody. In those who test positive for surface antigen, one should test for e antigen, e antibody, and HBV DNA.

Patients with indications for anti-HBV therapy (Table 1) should receive antiviral therapy. Otherwise, those positive for surface antigen should start taking anti-HBV medication at the start of chemotherapy or immunosuppressive therapy and should continue taking it until 6 months after the chemotherapy or immunosuppressive therapy is finished.4 Some experts also recommend starting anti-HBV therapy 7 days before the chemotherapy or immunosuppressive therapy and continuing it for 1 year afterward.10 Those with HBV DNA levels higher than 2 × 103 IU/mL should continue HBV therapy until they reach the same treatment end points as for immunocompetent patients as outlined above.4

Because we have little information on patients who are negative for surface antigen and who have antibodies against surface antigen and core antigen, we cannot make an unequivocal recommendation for anti-HBV therapy in this group.11 Rather, these patients should be monitored during immunosuppressive treatment, preferably with liver chemistry tests and HBV DNA titers, and antiviral drugs should be given as a deferred therapy upon evidence of HBV reactivation.9 Few cases of fatal hepatic failure in patients with this serologic pattern receiving rituximab (Rituxan) have been reported.12–14

With their small risk of drug resistance and rapid onset of action, entecavir or tenofovir may be the preferred anti-HBV therapy in patients undergoing immunosuppression or chemotherapy, especially in those requiring prolonged immunosuppressive therapy (longer than 12 months). In those requiring shorter courses, lamivudine or telbivudine is a possible alternative.4

OUTCOMES OF LIVER TRANSPLANTATION HAVE IMPROVED IN HBV PATIENTS

The early results of liver transplantation for HBV were discouraging because many patients developed rapidly progressive recurrent disease (fibrosing cholestatic hepatitis) and died within 12 to 18 months after the operation.15 However, patients with HBV are now treated perioperatively with lamivudine or adefovir combined with prolonged administration of hepatitis B immune globulin, and their survival now exceeds that of patients who receive transplants for many other conditions.16

Like patients with cirrhosis due to other causes, those with HBV-related cirrhosis who have any of the following should be referred for liver transplantation evaluation16:

  • A Model for End-Stage Liver Disease (MELD) score of 10 or higher (calculated from the serum creatinine level, total bilirubin level, and international normalized ratio of the prothrombin time; see www.unos.org/resources/MeldPeldCalculator.asp?index=98).
  • A Child-Turcotte-Pugh score of 7 or higher (Table 5).
  • A major complication of cirrhosis such as ascites, variceal bleeding, hepatocellular carcinoma, or hepatic encephalopathy.

PREVENTING VERTICAL TRANSMISSION

The major problem in young women with chronic HBV infection is the risk of vertical (mother-to-infant) transmission at delivery. The risk varies, depending on the viral load and e antigen status of the mother at the time of delivery; if she is positive for e antigen, the risk of HBV infection in the newborn is 70% to 90% by the age of 6 months if the newborn does not receive postexposure immunoprophylaxis; if the mother is positive for surface antigen but negative for e antigen, the risk of chronic infection is less than 10%, even without postexposure immunoprophylaxis.17

All women should be tested for HBV surface antigen early in pregnancy each time they become pregnant. If a patient tests negative early in pregnancy but continues behaviors that put her at risk of HBV infection (eg, having multiple sexual partners, having had a sex partner positive for surface antigen, using injection drugs, or contracting any sexually transmitted disease), she should be retested at the time of admission to the hospital for delivery.17 This also includes women who were not screened prenatally and those with clinical hepatitis.

Vaccine and immune globulin for the infant

If the mother is positive for HBV surface antigen, the infant should receive single-antigen HBV vaccine and hepatitis B immune globulin within 12 hours of birth, given at different injection sites.17 The second dose of vaccine should be given at age 1 to 2 months and the third at age 6 months (but not before age 24 weeks). The response to vaccination should be ascertained by testing for surface antigen and surface antibody after completion of the vaccine series, at age 9 to 18 months.

Maternal HBV infection does not contraindicate breastfeeding, as studies suggest that breastfeeding by a mother positive for surface antigen does not increase the infant’s risk of acquiring HBV infection.18

Which HBV therapy for a pregnant woman?

Some evidence supports antiviral therapy with nucleoside/nucleotide analogues in pregnant women who have viral loads of 106 IU/mL or higher. Lamivudine is safe in pregnancy and, together with immunization of the infant, reduces HBV transmission. Interferon-based therapy is contraindicated in pregnant women (and in women who may want to become pregnant) because of interferon’s antiproliferative effects. Nucleoside/nucleotide analogues classified as category B (eg, lamivudine, telbivudine, and tenofovir) could be used when the benefit of treating the pregnant mother outweighs the risk to the mother or fetus,2 although the possible effects of tenofovir on bone density argue against its use during pregnancy or breastfeeding.19

 

 

VACCINATION HAS REDUCED THE INCIDENCE OF ACUTE HEPATITIS B

HBV vaccination, a major achievement in HBV management, has played a big role in reducing the incidence of acute HBV infection, especially in children and adolescents.20

The currently available vaccines in the United States contain HBV surface antigen derived through recombinant DNA technology from yeast.21 Two single-antigen vaccines are available in the United States, under the brand names Recombivax HB and Engerix B. Of the three licensed combination vaccines, one (Twinrix) is used in adults, and two (Comvax and Pediarix) are used in infants and young children. Twinrix contains recombinant HBV surface antigens and inactivated hepatitis A virus and it is recommended for people age 18 years and older and at risk of both HBV and hepatitis A infections.20

Vaccinate all infants

All infants should be vaccinated against HBV as part of the recommended childhood immunization schedule. The vaccine is given on a three-dose schedule at birth and again at 1 month and 6 months of age.16 All children and adolescents under age 19 who have not previously received HBV vaccine should be vaccinated at any age with an appropriate dose and schedule.16

Vaccinate adults at risk—or who ask for it

Hepatitis B vaccination is recommended for all unvaccinated adults at risk of HBV infection and for all adults who ask for it (Table 6).20

Table 7 summarizes the adult dosing schedule for HBV vaccines.20 The vaccines should be given intramuscularly in the deltoid with a 1- to 2-inch needle, depending on the patient’s sex and weight.20 If doses are missed, the series should be resumed as soon as possible; there is no need to restart the series if the time between doses is longer than recommended.

Vaccination is less effective in older people

The three-dose vaccine series given intramuscularly initially, then again at 1 month and 6 months, produces a protective antibody response in approximately 30% to 55% of healthy adults under age 40 after the first dose, 75% after the second dose, and more than 90% after the third dose.21,22 After age 40, however, the proportion of persons who have a protective antibody response after three doses declines to less than 90%, and by age 60, protective levels of antibody develop in only 75%.23

Other factors that lower the response to vaccination are smoking, obesity, genetic factors, and immune suppression.20

Postvaccination serologic testing for immunity is not necessary after routine vaccination of adults, but it is recommended for patients whose subsequent clinical management depends on knowledge of their immune status, such as health care workers who have contact with patients or blood and are at ongoing risk of injuries with sharp instruments or needlesticks; chronic hemodialysis patients and people infected with HIV or otherwise immunocompromised; and sex partners or needle-sharing partners of people positive for HBV surface antigen.20 A protective concentration of HBV surface antibody measured 1 to 2 months after completion of the vaccine series is defined as 10 mIU/mL. Further periodic testing to document persistence of protective levels of surface antibody is not indicated.

If the first series does not ‘take’

Patients who do not respond to the primary vaccine series should complete a second three-dose series, with doses at 0, 1, and 6 months. Serologic testing is done 1 to 2 months after finishing the second series.

Patients who do not have protective levels of HBV surface antibody after revaccination by the appropriate schedule in the deltoid muscle (< 5% of those receiving six doses of hepatitis B vaccine) either are primary nonresponders or are infected with HBV.20 Therefore, they should be tested for HBV surface antigen. If this test is negative, then they should be considered susceptible to HBV infection and should be counseled accordingly.

Contraindications and precautions

HBV vaccination is contraindicated in people with a history of hypersensitivity to baker’s yeast or to a previous dose of HBV vaccine.20 Patients with moderate or severe acute illness at the time the shot is scheduled should wait until they recover before getting HBV vaccine. Pregnancy is not a contraindication.20

References
  1. Elgouhari HM, Abu-Rajab Tamimi T, Carey WD. Hepatitis B virus infection: understanding its epidemiology, course, and diagnosis. Cleve Clin J Med 2008; 75:881889.
  2. Stravitz RT, Kramer AH, Davern T, et al. Intensive care of patients with acute liver failure: recommendations of the U.S. Acute Liver Failure Study Group. Crit Care Med 2007; 35:24982508.
  3. Hoofnagle JH, Doo E, Liang TJ, Fleischer R, Lok AS. Management of hepatitis B: summary of a clinical research workshop. Hepatology 2007; 45:10561075.
  4. Lok AS, McMahon BJ. Chronic hepatitis B. Hepatology 2007; 45:507539.
  5. Keeffe EB, Dieterich DT, Han SH, et al. A treatment algorithm for the management of chronic hepatitis B virus infection in the United States. Clin Gastroenterol Hepatol 2004; 2:87106.
  6. Jacobs RJ, Meyerhoff AS, Saab S. Immunization needs of chronic liver disease patients seen in primary care versus specialist settings. Dig Dis Sci 2005; 50:15251531.
  7. Wang LY, You SL, Lu SN, et al. Risk of hepatocellular carcinoma and habits of alcohol drinking, betel quid chewing and cigarette smoking: a cohort of 2416 HBsAg–seropositive and 9421 HBsAg–seronegative male residents in Taiwan. Cancer Causes Control 2003; 14:241250.
  8. Bruix J, Sherman M; Practice Guidelines Committee, American Association for the Study of Liver Diseases. Management of hepatocellular carcinoma. Hepatology 2005; 42:12081236.
  9. Yeo W, Johnson PJ. Diagnosis, prevention and management of hepatitis B virus reactivation during anticancer therapy. Hepatology 2006; 43:209220.
  10. Tran T, Oh M, Poordad F, Martin P. Screening for hepatitis B in chemotherapy patients: survey of current oncology practices [abstract]. Hepatology 2007; 46:978A.
  11. Kohrt HE, Ouyang DL, Keeffe EB. Antiviral prophylaxis for chemotherapy–induced reactivation of chronic hepatitis B virus infection. Clin Liver Dis 2007; 11:965991.
  12. Westhoff TH, Jochimsen F, Schmittel A, et al. Fatal hepatitis B virus reactivation by an escape mutant following rituximab therapy. Blood 2003; 102:1930.
  13. Sarrecchia C, Cappelli A, Aiello P. HBV reactivation with fatal fulminating hepatitis during rituximab treatment in a subject negative for HBsAg and positive for HBsAb and HBcAb. J Infect Chemother 2005; 11:189191.
  14. Law JK, Ho JK, Hoskins PJ, Erb SR, Steinbrecher UP, Yoshida FM. Fatal reactivation of hepatitis B post-chemotherapy for lymphoma in a hepatitis B surface antigen-negative, hepatitis B core antibody-positive patient: potential implications for future prophylaxis recommendations. Leuk Lymphoma 2005; 46:10851089.
  15. Todo S, Demetris AJ, Van Thiel D, Teperman L, Fung JJ, Starzl TE. Orthotopic liver transplantation for patients with hepatitis B virus-related liver disease. Hepatology 1991; 13:619626.
  16. Murray KF, Carithers RLAASLD. AASLD practice guidelines: Evaluation of the patient for liver transplantation. Hepatology 2005; 41:14071432.
  17. Mast EE, Margolis HS, Fiore AE, et al. A comprehensive immunization strategy to eliminate transmission of hepatitis B virus infection in the United States: recommendations of the Advisory Committee on Immunization Practices (ACIP) part 1: immunization of infants, children, and adolescents. MMWR Recomm Rep 2005; 54:131.
  18. Beasley RP, Stevens CE, Shiao IS, Meng HC. Evidence against breast–feeding as a mechanism for vertical transmission of hepatitis B. Lancet 1975; 2:740741.
  19. Parsonage MJ, Wilkins EG, Snowden N, Issa BG, Savage MW. The development of hypophosphataemic osteomalacia with myopathy in two patients with HIV infection receiving tenofovir therapy. HIV Med 2005; 6:341346.
  20. Mast EE, Weinbaum CM, Fiore AE, et al. A comprehensive immunization strategy to eliminate transmission of hepatitis B virus infection in the United States: recommendations of the Advisory Committee on Immunization Practices (ACIP) Part II: immunization of adults. MMWR Recomm Rep 2006; 55:133.
  21. Andre FE. Summary of safety and efficacy data on a yeast–derived hepatitis B vaccine. Am J Med 1989; 87:14S20S.
  22. Zajac BA, West DJ, McAleer WJ, Scolnick EM. Overview of clinical studies with hepatitis B vaccine made by recombinant DNA. J Infect 1986; 13( suppl A):3945.
  23. Averhoff F, Mahoney F, Coleman P, Schatz G, Hurwitz E, Margolis H. Immunogenicity of hepatitis B vaccines: implications for persons at occupational risk for hepatitis B virus infection. Am J Prev Med 1998; 15:18.
References
  1. Elgouhari HM, Abu-Rajab Tamimi T, Carey WD. Hepatitis B virus infection: understanding its epidemiology, course, and diagnosis. Cleve Clin J Med 2008; 75:881889.
  2. Stravitz RT, Kramer AH, Davern T, et al. Intensive care of patients with acute liver failure: recommendations of the U.S. Acute Liver Failure Study Group. Crit Care Med 2007; 35:24982508.
  3. Hoofnagle JH, Doo E, Liang TJ, Fleischer R, Lok AS. Management of hepatitis B: summary of a clinical research workshop. Hepatology 2007; 45:10561075.
  4. Lok AS, McMahon BJ. Chronic hepatitis B. Hepatology 2007; 45:507539.
  5. Keeffe EB, Dieterich DT, Han SH, et al. A treatment algorithm for the management of chronic hepatitis B virus infection in the United States. Clin Gastroenterol Hepatol 2004; 2:87106.
  6. Jacobs RJ, Meyerhoff AS, Saab S. Immunization needs of chronic liver disease patients seen in primary care versus specialist settings. Dig Dis Sci 2005; 50:15251531.
  7. Wang LY, You SL, Lu SN, et al. Risk of hepatocellular carcinoma and habits of alcohol drinking, betel quid chewing and cigarette smoking: a cohort of 2416 HBsAg–seropositive and 9421 HBsAg–seronegative male residents in Taiwan. Cancer Causes Control 2003; 14:241250.
  8. Bruix J, Sherman M; Practice Guidelines Committee, American Association for the Study of Liver Diseases. Management of hepatocellular carcinoma. Hepatology 2005; 42:12081236.
  9. Yeo W, Johnson PJ. Diagnosis, prevention and management of hepatitis B virus reactivation during anticancer therapy. Hepatology 2006; 43:209220.
  10. Tran T, Oh M, Poordad F, Martin P. Screening for hepatitis B in chemotherapy patients: survey of current oncology practices [abstract]. Hepatology 2007; 46:978A.
  11. Kohrt HE, Ouyang DL, Keeffe EB. Antiviral prophylaxis for chemotherapy–induced reactivation of chronic hepatitis B virus infection. Clin Liver Dis 2007; 11:965991.
  12. Westhoff TH, Jochimsen F, Schmittel A, et al. Fatal hepatitis B virus reactivation by an escape mutant following rituximab therapy. Blood 2003; 102:1930.
  13. Sarrecchia C, Cappelli A, Aiello P. HBV reactivation with fatal fulminating hepatitis during rituximab treatment in a subject negative for HBsAg and positive for HBsAb and HBcAb. J Infect Chemother 2005; 11:189191.
  14. Law JK, Ho JK, Hoskins PJ, Erb SR, Steinbrecher UP, Yoshida FM. Fatal reactivation of hepatitis B post-chemotherapy for lymphoma in a hepatitis B surface antigen-negative, hepatitis B core antibody-positive patient: potential implications for future prophylaxis recommendations. Leuk Lymphoma 2005; 46:10851089.
  15. Todo S, Demetris AJ, Van Thiel D, Teperman L, Fung JJ, Starzl TE. Orthotopic liver transplantation for patients with hepatitis B virus-related liver disease. Hepatology 1991; 13:619626.
  16. Murray KF, Carithers RLAASLD. AASLD practice guidelines: Evaluation of the patient for liver transplantation. Hepatology 2005; 41:14071432.
  17. Mast EE, Margolis HS, Fiore AE, et al. A comprehensive immunization strategy to eliminate transmission of hepatitis B virus infection in the United States: recommendations of the Advisory Committee on Immunization Practices (ACIP) part 1: immunization of infants, children, and adolescents. MMWR Recomm Rep 2005; 54:131.
  18. Beasley RP, Stevens CE, Shiao IS, Meng HC. Evidence against breast–feeding as a mechanism for vertical transmission of hepatitis B. Lancet 1975; 2:740741.
  19. Parsonage MJ, Wilkins EG, Snowden N, Issa BG, Savage MW. The development of hypophosphataemic osteomalacia with myopathy in two patients with HIV infection receiving tenofovir therapy. HIV Med 2005; 6:341346.
  20. Mast EE, Weinbaum CM, Fiore AE, et al. A comprehensive immunization strategy to eliminate transmission of hepatitis B virus infection in the United States: recommendations of the Advisory Committee on Immunization Practices (ACIP) Part II: immunization of adults. MMWR Recomm Rep 2006; 55:133.
  21. Andre FE. Summary of safety and efficacy data on a yeast–derived hepatitis B vaccine. Am J Med 1989; 87:14S20S.
  22. Zajac BA, West DJ, McAleer WJ, Scolnick EM. Overview of clinical studies with hepatitis B vaccine made by recombinant DNA. J Infect 1986; 13( suppl A):3945.
  23. Averhoff F, Mahoney F, Coleman P, Schatz G, Hurwitz E, Margolis H. Immunogenicity of hepatitis B vaccines: implications for persons at occupational risk for hepatitis B virus infection. Am J Prev Med 1998; 15:18.
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KEY POINTS

  • Patients with HBV infection should be screened for hepatocellular carcinoma, especially if they have cirrhosis.
  • Nucleoside and nucleotide analogue reverse transcriptase inhibitors are easy to use and therefore are usually the first-line therapy. Problems with these agents are that the optimal treatment duration is not known, and that drug resistance can emerge.
  • Patients with advanced liver disease or hepatocellular carcinoma should be referred promptly for possible liver transplantation.
  • Candidates for immunosuppressant therapy or cytotoxic chemotherapy should be screened for HBV, as this therapy can cause a potentially fatal flare of HBV.
  • People at risk should be vaccinated; many have not been.
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A persistently swollen lip

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A persistently swollen lip

A 44-year-old man is referred for evaluation of asymptomatic swelling of the lower lip that has persisted for 10 months. He has been treated unsuccessfully with oral antihistamines for suspected chronic angioedema. He has no other symptoms and appears to be well otherwise. He has no history of applied irritants or local trauma, and his medical history is unremarkable.

Figure 1.
Physical examination shows a swollen and indurated lower lip (Figure 1). The tongue and gums are normal, and the ophthalmologic evaluation reveals no abnormalities. No facial paralysis is observed.

Results of the laboratory evaluation, including serum angiotensin-converting enzyme level, are normal. Patch tests to detect contact sensitivity to food additives are negative. Biopsy of the affected lip reveals dense infiltrate of the submucosal connective tissue with focal nonnecrotizing granulomas. Imaging and endoscopic studies show no evidence of sarcoidosis or Crohn disease.

Q: Given what we know so far, which of the following is the most likely diagnosis of the persistent lip swelling?

  • Melkersson-Rosenthal syndrome
  • Amyloidosis
  • Quincke edema
  • Cheilitis granulomatosa
  • Cutaneous tuberculosis

A: From what we know so far, the correct answer is cheilitis granulomatosa. While this rare condition may be a feature of Melkersson-Rosenthal syndrome and amyloidosis, at this point in the evaluation these have not been confirmed. Quincke edema (ie, angioedema) is unlikely, given the ineffectiveness of previous treatment with oral antihistamines. Cutaneous tuberculosis usually presents as “lupus vulgaris,” which is characterized by solitary, small, sharply marginated, red-brown papules of gelatinous consistency (“apple-jelly nodules”), mainly on the head and neck.

Cheilitis granulomatosa is a rare inflammatory disorder1 that primarily affects young adults. Its key feature is recurrent or persistent painless swelling of one or both lips. It may occur without other signs of disease, but it is also a manifestation of Melkersson-Rosenthal syndrome and it may be a presenting symptom of Crohn disease or, rarely, sarcoidosis.2 The term “orofacial granulomatosis” was introduced to encompass the broad spectrum of nonnecrotizing granulomatous inflammation in the orofacial region, including cheilitis granulomatosa, the complete Melkersson-Rosenthal syndrome, sarcoidosis, Crohn disease, and infectious disorders such as tuberculosis.1

The cause of cheilitis granulomatosa is unknown. Specific T-cell clonality has been identified in several patients with orofacial granulomatosis, suggesting a delayed hypersensitivity response. Moreover, the HLA haplotypes HLA-A2 and HLA-A11 have been found in 25% of patients with orofacial granulomatosis, suggesting a viral etiology. A genetic predisposition may exist in Melkersson- Rosenthal syndrome: siblings have been affected, and otherwise unaffected relatives may have a fissured tongue (lingua plicata).

Melkersson-Rosenthal syndrome, a rare condition, is characterized by a classic triad of recurrent swelling of the lips or face (or both), fissured tongue, and relapsing peripheral facial nerve paralysis. It is an unusual cause of facial swelling that can be confused with angioedema.3 This syndrome can be ruled out in this patient because he has only one of the three classic signs. Contact antigens are sometimes implicated.

DIFFERENTIAL DIAGNOSIS OF CHEILITIS GRANULOMATOSA

The differential diagnosis of cheilitis granulomatosa is extensive and includes amyloidosis, cheilitis glandularis, sarcoidosis, Crohn disease, actinic cheilitis, neoplasms, and infections, such as tuberculosis, syphilis, and leprosy.1

As many as 11% of patients with Crohn disease may develop mucocutaneous lesions. Oral lesions of Crohn disease include apthae, cobblestoning of the buccal mucosa, swelling of one or both lips (soft or rubbery), vertical clefts of the lips, or hypertrophic gingivitis. Only 5% of patients with Crohn disease ever develop cheilitis granulomatosa, though most cases occur in children.

Ultimately, the diagnosis of cheilitis granulomatosa is made by correlating the patient’s history and clinical features, usually supported by histopathologic findings of nonnecrotic granulomas extending into the deep dermis, composed of histiocytes and giant cells and associated with a lymphomonocytic infiltrate.

TREATMENT

Treatment of cheilitis granulomatosa is difficult because the cause is unknown and the rate of recurrence is high. Response to treatment is often late and unpredictable. Corticosteroids, clofazimine (Lamprene), and surgical intervention such as cheiloplasty have been described as treatment options. Other treatment options include thalidomide (Thalomid), sulfasalazine (Sulfazine), erythromycin, azathioprine (Imuran), and cyclosporine (Sandimmune). Infliximab (Remicade) has been recently reported as a new alternative treatment, in particular for Melkersson-Rosenthal syndrome.4

In our patient, twice-monthly injections of 1 mL of triamcinolone acetonide 10 mg/mL into the affected lip brought acceptable improvement at 3 months. The patient is on maintenance treatment with twice-monthly triamcinolone injections and has had no relapses after 2 years.

References
  1. van der Waal RI, Schulten EA, van de Scheur MR, Wauters IM, Starink TM, van der Waal I. Cheilitis granulomatosa. J Eur Acad Dermatol Venereol 2001; 15:519523.
  2. van der Waal RI, Schulten EA, van der Meij EH, van de Scheur MR, Starink TM, van der Waal I. Cheilitis granulomatosa: overview of 13 patients with long-term follow-up—results of management. Int J Dermatol 2002; 41:225229.
  3. Kakimoto C, Sparks C, White AA. Melkersson-Rosenthal syndrome: a form of pseudoangioedema. Ann Allergy Asthma Immunol 2007; 99:185189.
  4. Ratzinger G, Sepp N, Vogetseder W, Tilg H. Cheilitis granulomatosa and Melkersson-Rosenthal syndrome: evaluation of gastrointestinal involvement and therapeutic regimens in a series of 14 patients. J Eur Acad Dermatol Venereol 2007; 21:10651070.
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Sergio Vañó-Galván, MD
Department of Dermatology, Ramón y Cajal Hospital, University of Alcalá, Madrid, Spain

Paula Moreno-Martin, MD
Department of Ophthalmology, La Princesa University Hospital, Madrid, Spain

José-María Arrazola, MD
Department of Dermatology, Ramón y Cajal Hospital, University of Alcalá, Madrid, Spain

Pedro Jaén, PhD
Department of Dermatology, Ramón y Cajal Hospital, University of Alcalá, Madrid, Spain

Address: Sergio Vañó-Galván, MD, Department of Dermatology, Ramón y Cajal Hospital, University of Alcalá, Carretera de Colmenar Viejo, km 9.100, 28034 Madrid, Spain; e-mail [email protected]

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Department of Dermatology, Ramón y Cajal Hospital, University of Alcalá, Madrid, Spain

Paula Moreno-Martin, MD
Department of Ophthalmology, La Princesa University Hospital, Madrid, Spain

José-María Arrazola, MD
Department of Dermatology, Ramón y Cajal Hospital, University of Alcalá, Madrid, Spain

Pedro Jaén, PhD
Department of Dermatology, Ramón y Cajal Hospital, University of Alcalá, Madrid, Spain

Address: Sergio Vañó-Galván, MD, Department of Dermatology, Ramón y Cajal Hospital, University of Alcalá, Carretera de Colmenar Viejo, km 9.100, 28034 Madrid, Spain; e-mail [email protected]

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Sergio Vañó-Galván, MD
Department of Dermatology, Ramón y Cajal Hospital, University of Alcalá, Madrid, Spain

Paula Moreno-Martin, MD
Department of Ophthalmology, La Princesa University Hospital, Madrid, Spain

José-María Arrazola, MD
Department of Dermatology, Ramón y Cajal Hospital, University of Alcalá, Madrid, Spain

Pedro Jaén, PhD
Department of Dermatology, Ramón y Cajal Hospital, University of Alcalá, Madrid, Spain

Address: Sergio Vañó-Galván, MD, Department of Dermatology, Ramón y Cajal Hospital, University of Alcalá, Carretera de Colmenar Viejo, km 9.100, 28034 Madrid, Spain; e-mail [email protected]

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A 44-year-old man is referred for evaluation of asymptomatic swelling of the lower lip that has persisted for 10 months. He has been treated unsuccessfully with oral antihistamines for suspected chronic angioedema. He has no other symptoms and appears to be well otherwise. He has no history of applied irritants or local trauma, and his medical history is unremarkable.

Figure 1.
Physical examination shows a swollen and indurated lower lip (Figure 1). The tongue and gums are normal, and the ophthalmologic evaluation reveals no abnormalities. No facial paralysis is observed.

Results of the laboratory evaluation, including serum angiotensin-converting enzyme level, are normal. Patch tests to detect contact sensitivity to food additives are negative. Biopsy of the affected lip reveals dense infiltrate of the submucosal connective tissue with focal nonnecrotizing granulomas. Imaging and endoscopic studies show no evidence of sarcoidosis or Crohn disease.

Q: Given what we know so far, which of the following is the most likely diagnosis of the persistent lip swelling?

  • Melkersson-Rosenthal syndrome
  • Amyloidosis
  • Quincke edema
  • Cheilitis granulomatosa
  • Cutaneous tuberculosis

A: From what we know so far, the correct answer is cheilitis granulomatosa. While this rare condition may be a feature of Melkersson-Rosenthal syndrome and amyloidosis, at this point in the evaluation these have not been confirmed. Quincke edema (ie, angioedema) is unlikely, given the ineffectiveness of previous treatment with oral antihistamines. Cutaneous tuberculosis usually presents as “lupus vulgaris,” which is characterized by solitary, small, sharply marginated, red-brown papules of gelatinous consistency (“apple-jelly nodules”), mainly on the head and neck.

Cheilitis granulomatosa is a rare inflammatory disorder1 that primarily affects young adults. Its key feature is recurrent or persistent painless swelling of one or both lips. It may occur without other signs of disease, but it is also a manifestation of Melkersson-Rosenthal syndrome and it may be a presenting symptom of Crohn disease or, rarely, sarcoidosis.2 The term “orofacial granulomatosis” was introduced to encompass the broad spectrum of nonnecrotizing granulomatous inflammation in the orofacial region, including cheilitis granulomatosa, the complete Melkersson-Rosenthal syndrome, sarcoidosis, Crohn disease, and infectious disorders such as tuberculosis.1

The cause of cheilitis granulomatosa is unknown. Specific T-cell clonality has been identified in several patients with orofacial granulomatosis, suggesting a delayed hypersensitivity response. Moreover, the HLA haplotypes HLA-A2 and HLA-A11 have been found in 25% of patients with orofacial granulomatosis, suggesting a viral etiology. A genetic predisposition may exist in Melkersson- Rosenthal syndrome: siblings have been affected, and otherwise unaffected relatives may have a fissured tongue (lingua plicata).

Melkersson-Rosenthal syndrome, a rare condition, is characterized by a classic triad of recurrent swelling of the lips or face (or both), fissured tongue, and relapsing peripheral facial nerve paralysis. It is an unusual cause of facial swelling that can be confused with angioedema.3 This syndrome can be ruled out in this patient because he has only one of the three classic signs. Contact antigens are sometimes implicated.

DIFFERENTIAL DIAGNOSIS OF CHEILITIS GRANULOMATOSA

The differential diagnosis of cheilitis granulomatosa is extensive and includes amyloidosis, cheilitis glandularis, sarcoidosis, Crohn disease, actinic cheilitis, neoplasms, and infections, such as tuberculosis, syphilis, and leprosy.1

As many as 11% of patients with Crohn disease may develop mucocutaneous lesions. Oral lesions of Crohn disease include apthae, cobblestoning of the buccal mucosa, swelling of one or both lips (soft or rubbery), vertical clefts of the lips, or hypertrophic gingivitis. Only 5% of patients with Crohn disease ever develop cheilitis granulomatosa, though most cases occur in children.

Ultimately, the diagnosis of cheilitis granulomatosa is made by correlating the patient’s history and clinical features, usually supported by histopathologic findings of nonnecrotic granulomas extending into the deep dermis, composed of histiocytes and giant cells and associated with a lymphomonocytic infiltrate.

TREATMENT

Treatment of cheilitis granulomatosa is difficult because the cause is unknown and the rate of recurrence is high. Response to treatment is often late and unpredictable. Corticosteroids, clofazimine (Lamprene), and surgical intervention such as cheiloplasty have been described as treatment options. Other treatment options include thalidomide (Thalomid), sulfasalazine (Sulfazine), erythromycin, azathioprine (Imuran), and cyclosporine (Sandimmune). Infliximab (Remicade) has been recently reported as a new alternative treatment, in particular for Melkersson-Rosenthal syndrome.4

In our patient, twice-monthly injections of 1 mL of triamcinolone acetonide 10 mg/mL into the affected lip brought acceptable improvement at 3 months. The patient is on maintenance treatment with twice-monthly triamcinolone injections and has had no relapses after 2 years.

A 44-year-old man is referred for evaluation of asymptomatic swelling of the lower lip that has persisted for 10 months. He has been treated unsuccessfully with oral antihistamines for suspected chronic angioedema. He has no other symptoms and appears to be well otherwise. He has no history of applied irritants or local trauma, and his medical history is unremarkable.

Figure 1.
Physical examination shows a swollen and indurated lower lip (Figure 1). The tongue and gums are normal, and the ophthalmologic evaluation reveals no abnormalities. No facial paralysis is observed.

Results of the laboratory evaluation, including serum angiotensin-converting enzyme level, are normal. Patch tests to detect contact sensitivity to food additives are negative. Biopsy of the affected lip reveals dense infiltrate of the submucosal connective tissue with focal nonnecrotizing granulomas. Imaging and endoscopic studies show no evidence of sarcoidosis or Crohn disease.

Q: Given what we know so far, which of the following is the most likely diagnosis of the persistent lip swelling?

  • Melkersson-Rosenthal syndrome
  • Amyloidosis
  • Quincke edema
  • Cheilitis granulomatosa
  • Cutaneous tuberculosis

A: From what we know so far, the correct answer is cheilitis granulomatosa. While this rare condition may be a feature of Melkersson-Rosenthal syndrome and amyloidosis, at this point in the evaluation these have not been confirmed. Quincke edema (ie, angioedema) is unlikely, given the ineffectiveness of previous treatment with oral antihistamines. Cutaneous tuberculosis usually presents as “lupus vulgaris,” which is characterized by solitary, small, sharply marginated, red-brown papules of gelatinous consistency (“apple-jelly nodules”), mainly on the head and neck.

Cheilitis granulomatosa is a rare inflammatory disorder1 that primarily affects young adults. Its key feature is recurrent or persistent painless swelling of one or both lips. It may occur without other signs of disease, but it is also a manifestation of Melkersson-Rosenthal syndrome and it may be a presenting symptom of Crohn disease or, rarely, sarcoidosis.2 The term “orofacial granulomatosis” was introduced to encompass the broad spectrum of nonnecrotizing granulomatous inflammation in the orofacial region, including cheilitis granulomatosa, the complete Melkersson-Rosenthal syndrome, sarcoidosis, Crohn disease, and infectious disorders such as tuberculosis.1

The cause of cheilitis granulomatosa is unknown. Specific T-cell clonality has been identified in several patients with orofacial granulomatosis, suggesting a delayed hypersensitivity response. Moreover, the HLA haplotypes HLA-A2 and HLA-A11 have been found in 25% of patients with orofacial granulomatosis, suggesting a viral etiology. A genetic predisposition may exist in Melkersson- Rosenthal syndrome: siblings have been affected, and otherwise unaffected relatives may have a fissured tongue (lingua plicata).

Melkersson-Rosenthal syndrome, a rare condition, is characterized by a classic triad of recurrent swelling of the lips or face (or both), fissured tongue, and relapsing peripheral facial nerve paralysis. It is an unusual cause of facial swelling that can be confused with angioedema.3 This syndrome can be ruled out in this patient because he has only one of the three classic signs. Contact antigens are sometimes implicated.

DIFFERENTIAL DIAGNOSIS OF CHEILITIS GRANULOMATOSA

The differential diagnosis of cheilitis granulomatosa is extensive and includes amyloidosis, cheilitis glandularis, sarcoidosis, Crohn disease, actinic cheilitis, neoplasms, and infections, such as tuberculosis, syphilis, and leprosy.1

As many as 11% of patients with Crohn disease may develop mucocutaneous lesions. Oral lesions of Crohn disease include apthae, cobblestoning of the buccal mucosa, swelling of one or both lips (soft or rubbery), vertical clefts of the lips, or hypertrophic gingivitis. Only 5% of patients with Crohn disease ever develop cheilitis granulomatosa, though most cases occur in children.

Ultimately, the diagnosis of cheilitis granulomatosa is made by correlating the patient’s history and clinical features, usually supported by histopathologic findings of nonnecrotic granulomas extending into the deep dermis, composed of histiocytes and giant cells and associated with a lymphomonocytic infiltrate.

TREATMENT

Treatment of cheilitis granulomatosa is difficult because the cause is unknown and the rate of recurrence is high. Response to treatment is often late and unpredictable. Corticosteroids, clofazimine (Lamprene), and surgical intervention such as cheiloplasty have been described as treatment options. Other treatment options include thalidomide (Thalomid), sulfasalazine (Sulfazine), erythromycin, azathioprine (Imuran), and cyclosporine (Sandimmune). Infliximab (Remicade) has been recently reported as a new alternative treatment, in particular for Melkersson-Rosenthal syndrome.4

In our patient, twice-monthly injections of 1 mL of triamcinolone acetonide 10 mg/mL into the affected lip brought acceptable improvement at 3 months. The patient is on maintenance treatment with twice-monthly triamcinolone injections and has had no relapses after 2 years.

References
  1. van der Waal RI, Schulten EA, van de Scheur MR, Wauters IM, Starink TM, van der Waal I. Cheilitis granulomatosa. J Eur Acad Dermatol Venereol 2001; 15:519523.
  2. van der Waal RI, Schulten EA, van der Meij EH, van de Scheur MR, Starink TM, van der Waal I. Cheilitis granulomatosa: overview of 13 patients with long-term follow-up—results of management. Int J Dermatol 2002; 41:225229.
  3. Kakimoto C, Sparks C, White AA. Melkersson-Rosenthal syndrome: a form of pseudoangioedema. Ann Allergy Asthma Immunol 2007; 99:185189.
  4. Ratzinger G, Sepp N, Vogetseder W, Tilg H. Cheilitis granulomatosa and Melkersson-Rosenthal syndrome: evaluation of gastrointestinal involvement and therapeutic regimens in a series of 14 patients. J Eur Acad Dermatol Venereol 2007; 21:10651070.
References
  1. van der Waal RI, Schulten EA, van de Scheur MR, Wauters IM, Starink TM, van der Waal I. Cheilitis granulomatosa. J Eur Acad Dermatol Venereol 2001; 15:519523.
  2. van der Waal RI, Schulten EA, van der Meij EH, van de Scheur MR, Starink TM, van der Waal I. Cheilitis granulomatosa: overview of 13 patients with long-term follow-up—results of management. Int J Dermatol 2002; 41:225229.
  3. Kakimoto C, Sparks C, White AA. Melkersson-Rosenthal syndrome: a form of pseudoangioedema. Ann Allergy Asthma Immunol 2007; 99:185189.
  4. Ratzinger G, Sepp N, Vogetseder W, Tilg H. Cheilitis granulomatosa and Melkersson-Rosenthal syndrome: evaluation of gastrointestinal involvement and therapeutic regimens in a series of 14 patients. J Eur Acad Dermatol Venereol 2007; 21:10651070.
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Surprises and reaffirmations in 2008 clinical trials

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Surprises and reaffirmations in 2008 clinical trials

Several clinical trials published last year may ultimately shape the way we practice medicine. Some of the findings were surprises that prompted us to rethink some of the basic tenets of our clinical practice, but others reaffirmed our practice patterns.

The ACCORD trial (Action to Control Cardiovascular Risk in Diabetes) investigated very aggressive glucose control in type 2 diabetes. To our surprise, it did not extend the findings of earlier landmark trials that had showed marked microvascular benefits with modestly aggressive glucose control. Instead, as discussed by Dr. Byron Hoogwerf in our October 2008 issue, the ACCORD trial found that more patients died who underwent the extremely aggressive glucose-control strategy.

Like the ACCORD trial, the JUPITER trial (Justification for the Use of Statins in Prevention: An Intervention Trial Evaluating Rosuvastatin) examined how far you can pharmacologically lower a causative factor—in this case, low-density lipoprotein cholesterol (LDL-C)—without causing adverse effects. In this month’s issue, Drs. Shishehbor and Hazen discuss the results of the JUPITER trial, in which “healthy” patients with LCL-C levels lower than 130 mg/dL and elevated high-sensitivity C-reactive protein (hs-CRP) levels were aggressively treated with rosuvastatin (Crestor). The median LDL-C level fell from 108 to 55 mg/dL, and the trial was stopped early when the number of predefined cardiovascular events was found to be 44% lower in the treated group than in the placebo group.

The efficacy result is not that surprising—there is probably no specific LDL-C number that should trigger a decision to treat. Furthermore, in JUPITER, unlike in ACCORD, there was no downside to the aggressive treatment that outweighed the benefits. The acute-phase reactant hs-CRP (or the company it kept, ie, metabolic syndrome) was a useful marker in identifying patients at risk of cardiovascular events, thus permitting the earlier-than-expected outcome differences. But the study does not resolve the question of whether hs-CRP is pathogenic in its own right.

So, as we begin 2009, we know that too much glucose is bad, but trying too hard to lower it in type 2 diabetes may be worse. We start the new year with a reaffirmation of the LDL-C hypothesis: LDL-C promotes cardiovascular morbidity, and starts to do so even when the person is apparently healthy. I am still not convinced that hs-CRP is an active player in the pathogenesis of atherogenesis, but that is a study for another year.

On behalf of the editorial staff of the Journal, I wish you all a happy, healthy, and most of all more peaceful 2009.

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Several clinical trials published last year may ultimately shape the way we practice medicine. Some of the findings were surprises that prompted us to rethink some of the basic tenets of our clinical practice, but others reaffirmed our practice patterns.

The ACCORD trial (Action to Control Cardiovascular Risk in Diabetes) investigated very aggressive glucose control in type 2 diabetes. To our surprise, it did not extend the findings of earlier landmark trials that had showed marked microvascular benefits with modestly aggressive glucose control. Instead, as discussed by Dr. Byron Hoogwerf in our October 2008 issue, the ACCORD trial found that more patients died who underwent the extremely aggressive glucose-control strategy.

Like the ACCORD trial, the JUPITER trial (Justification for the Use of Statins in Prevention: An Intervention Trial Evaluating Rosuvastatin) examined how far you can pharmacologically lower a causative factor—in this case, low-density lipoprotein cholesterol (LDL-C)—without causing adverse effects. In this month’s issue, Drs. Shishehbor and Hazen discuss the results of the JUPITER trial, in which “healthy” patients with LCL-C levels lower than 130 mg/dL and elevated high-sensitivity C-reactive protein (hs-CRP) levels were aggressively treated with rosuvastatin (Crestor). The median LDL-C level fell from 108 to 55 mg/dL, and the trial was stopped early when the number of predefined cardiovascular events was found to be 44% lower in the treated group than in the placebo group.

The efficacy result is not that surprising—there is probably no specific LDL-C number that should trigger a decision to treat. Furthermore, in JUPITER, unlike in ACCORD, there was no downside to the aggressive treatment that outweighed the benefits. The acute-phase reactant hs-CRP (or the company it kept, ie, metabolic syndrome) was a useful marker in identifying patients at risk of cardiovascular events, thus permitting the earlier-than-expected outcome differences. But the study does not resolve the question of whether hs-CRP is pathogenic in its own right.

So, as we begin 2009, we know that too much glucose is bad, but trying too hard to lower it in type 2 diabetes may be worse. We start the new year with a reaffirmation of the LDL-C hypothesis: LDL-C promotes cardiovascular morbidity, and starts to do so even when the person is apparently healthy. I am still not convinced that hs-CRP is an active player in the pathogenesis of atherogenesis, but that is a study for another year.

On behalf of the editorial staff of the Journal, I wish you all a happy, healthy, and most of all more peaceful 2009.

Several clinical trials published last year may ultimately shape the way we practice medicine. Some of the findings were surprises that prompted us to rethink some of the basic tenets of our clinical practice, but others reaffirmed our practice patterns.

The ACCORD trial (Action to Control Cardiovascular Risk in Diabetes) investigated very aggressive glucose control in type 2 diabetes. To our surprise, it did not extend the findings of earlier landmark trials that had showed marked microvascular benefits with modestly aggressive glucose control. Instead, as discussed by Dr. Byron Hoogwerf in our October 2008 issue, the ACCORD trial found that more patients died who underwent the extremely aggressive glucose-control strategy.

Like the ACCORD trial, the JUPITER trial (Justification for the Use of Statins in Prevention: An Intervention Trial Evaluating Rosuvastatin) examined how far you can pharmacologically lower a causative factor—in this case, low-density lipoprotein cholesterol (LDL-C)—without causing adverse effects. In this month’s issue, Drs. Shishehbor and Hazen discuss the results of the JUPITER trial, in which “healthy” patients with LCL-C levels lower than 130 mg/dL and elevated high-sensitivity C-reactive protein (hs-CRP) levels were aggressively treated with rosuvastatin (Crestor). The median LDL-C level fell from 108 to 55 mg/dL, and the trial was stopped early when the number of predefined cardiovascular events was found to be 44% lower in the treated group than in the placebo group.

The efficacy result is not that surprising—there is probably no specific LDL-C number that should trigger a decision to treat. Furthermore, in JUPITER, unlike in ACCORD, there was no downside to the aggressive treatment that outweighed the benefits. The acute-phase reactant hs-CRP (or the company it kept, ie, metabolic syndrome) was a useful marker in identifying patients at risk of cardiovascular events, thus permitting the earlier-than-expected outcome differences. But the study does not resolve the question of whether hs-CRP is pathogenic in its own right.

So, as we begin 2009, we know that too much glucose is bad, but trying too hard to lower it in type 2 diabetes may be worse. We start the new year with a reaffirmation of the LDL-C hypothesis: LDL-C promotes cardiovascular morbidity, and starts to do so even when the person is apparently healthy. I am still not convinced that hs-CRP is an active player in the pathogenesis of atherogenesis, but that is a study for another year.

On behalf of the editorial staff of the Journal, I wish you all a happy, healthy, and most of all more peaceful 2009.

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Cleveland Clinic Journal of Medicine - 76(1)
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Cleveland Clinic Journal of Medicine - 76(1)
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Surprises and reaffirmations in 2008 clinical trials
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