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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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A medical center is not a hospital: More letters

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We must work together to save health care in our country

To the Editor: Dr. Lansdale’s comments sadly illustrate all that is wrong with our health care system.1 Desperately ill patients are hospitalized for as few days as possible in order to receive substandard care from agency nurses. Physicians have become assembly-line workers who must order large batteries of tests and procedures because they don’t have the time to sit down, talk to, or examine their patients. This is the type of care that medical students, interns, and residents are learning to practice. Sadly, this is the type of care that patients now expect: an MRI provides better reassurance than a physician’s competent assessment. Business, not physicians, dictates how medicine is practiced.

Internists who care about quality, like Dr. Lansdale, are leaving the profession in droves. But rather than passively leave, they should become leaders in an effort to reclaim health care. If internists worked together, they might be able to enact major changes rather than passively watch as the ship sinks under them. There have been calls to do something.2

Some physicians are taking matters into their own hands by opting out of the system altogether; they no longer accept any type of insurance. While extreme, if done en masse this option could send a powerful message to policy makers and insurers that physicians will be pawns no longer. If physicians do decide to do this, they should make every effort to keep fees, tests, and procedures to a minimum in order to reduce costs.

The United States stands head and shoulders above all other industrialized countries in per-capita spending on health care.3 This level of spending is not sustainable, especially in a nation beset by worsening financial conditions. 4 The United States desperately needs its physicians to be leaders in addressing our health care woes. We must work together to save health care in our country: quitting should not be an option.

References

 

1. Lansdale TF. A medical center is not a hospital. Cleve Clin J Med 2008; 75:618–622.

2. Larson EB. Society of General Internal Medicine (SGIM) Task Force on the Domain of General Internal Medicine. Ann Intern Med 2004; 140:639–643.

3. Reinhardt UE, Hussey PS, Anderson GF. U.S. health care spending in an international context. Health Aff (Millwood) 2004; 23:10–25.

4. Krugman P. Financial Russian Roulette. NY Times. Sept. 15, 2008. http://www.nytimes.com/2008/09/15/opinion/15krugman.html?ref=opinion.

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We must work together to save health care in our country

To the Editor: Dr. Lansdale’s comments sadly illustrate all that is wrong with our health care system.1 Desperately ill patients are hospitalized for as few days as possible in order to receive substandard care from agency nurses. Physicians have become assembly-line workers who must order large batteries of tests and procedures because they don’t have the time to sit down, talk to, or examine their patients. This is the type of care that medical students, interns, and residents are learning to practice. Sadly, this is the type of care that patients now expect: an MRI provides better reassurance than a physician’s competent assessment. Business, not physicians, dictates how medicine is practiced.

Internists who care about quality, like Dr. Lansdale, are leaving the profession in droves. But rather than passively leave, they should become leaders in an effort to reclaim health care. If internists worked together, they might be able to enact major changes rather than passively watch as the ship sinks under them. There have been calls to do something.2

Some physicians are taking matters into their own hands by opting out of the system altogether; they no longer accept any type of insurance. While extreme, if done en masse this option could send a powerful message to policy makers and insurers that physicians will be pawns no longer. If physicians do decide to do this, they should make every effort to keep fees, tests, and procedures to a minimum in order to reduce costs.

The United States stands head and shoulders above all other industrialized countries in per-capita spending on health care.3 This level of spending is not sustainable, especially in a nation beset by worsening financial conditions. 4 The United States desperately needs its physicians to be leaders in addressing our health care woes. We must work together to save health care in our country: quitting should not be an option.

We must work together to save health care in our country

To the Editor: Dr. Lansdale’s comments sadly illustrate all that is wrong with our health care system.1 Desperately ill patients are hospitalized for as few days as possible in order to receive substandard care from agency nurses. Physicians have become assembly-line workers who must order large batteries of tests and procedures because they don’t have the time to sit down, talk to, or examine their patients. This is the type of care that medical students, interns, and residents are learning to practice. Sadly, this is the type of care that patients now expect: an MRI provides better reassurance than a physician’s competent assessment. Business, not physicians, dictates how medicine is practiced.

Internists who care about quality, like Dr. Lansdale, are leaving the profession in droves. But rather than passively leave, they should become leaders in an effort to reclaim health care. If internists worked together, they might be able to enact major changes rather than passively watch as the ship sinks under them. There have been calls to do something.2

Some physicians are taking matters into their own hands by opting out of the system altogether; they no longer accept any type of insurance. While extreme, if done en masse this option could send a powerful message to policy makers and insurers that physicians will be pawns no longer. If physicians do decide to do this, they should make every effort to keep fees, tests, and procedures to a minimum in order to reduce costs.

The United States stands head and shoulders above all other industrialized countries in per-capita spending on health care.3 This level of spending is not sustainable, especially in a nation beset by worsening financial conditions. 4 The United States desperately needs its physicians to be leaders in addressing our health care woes. We must work together to save health care in our country: quitting should not be an option.

References

 

1. Lansdale TF. A medical center is not a hospital. Cleve Clin J Med 2008; 75:618–622.

2. Larson EB. Society of General Internal Medicine (SGIM) Task Force on the Domain of General Internal Medicine. Ann Intern Med 2004; 140:639–643.

3. Reinhardt UE, Hussey PS, Anderson GF. U.S. health care spending in an international context. Health Aff (Millwood) 2004; 23:10–25.

4. Krugman P. Financial Russian Roulette. NY Times. Sept. 15, 2008. http://www.nytimes.com/2008/09/15/opinion/15krugman.html?ref=opinion.

References

 

1. Lansdale TF. A medical center is not a hospital. Cleve Clin J Med 2008; 75:618–622.

2. Larson EB. Society of General Internal Medicine (SGIM) Task Force on the Domain of General Internal Medicine. Ann Intern Med 2004; 140:639–643.

3. Reinhardt UE, Hussey PS, Anderson GF. U.S. health care spending in an international context. Health Aff (Millwood) 2004; 23:10–25.

4. Krugman P. Financial Russian Roulette. NY Times. Sept. 15, 2008. http://www.nytimes.com/2008/09/15/opinion/15krugman.html?ref=opinion.

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A medical center is not a hospital: More letters

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General internal medicine is extinct

To the Editor: General internal medicine has become extinct. Its practitioners have been pushed out of their leadership roles, have been pushed from clinical practice due to red tape and impediments of frustration, and have been marginalized by specialties and subspecialties, our so-called brethren. Only through revolutionary metamorphosis such as clinical homes or other unique systems by which primary care is delivered at high-quality levels such as MDVIP can general internal medicine survive.

Hospitalists are not general internists. Family practitioners are not general internists. Nurse practitioners are not general internists. And certainly none of the subspecialists are general internists. We must forge a new identity and role in the health care system because our previous identity has been destroyed.

Without our unique ability to temper high tech with clinical judgment, our system fails on quality and cost.

The article by Dr. Lansdale was more eloquent than I could express, but I believe the words written above are more accurate and to the point.

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Naples, FL

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General internal medicine is extinct

To the Editor: General internal medicine has become extinct. Its practitioners have been pushed out of their leadership roles, have been pushed from clinical practice due to red tape and impediments of frustration, and have been marginalized by specialties and subspecialties, our so-called brethren. Only through revolutionary metamorphosis such as clinical homes or other unique systems by which primary care is delivered at high-quality levels such as MDVIP can general internal medicine survive.

Hospitalists are not general internists. Family practitioners are not general internists. Nurse practitioners are not general internists. And certainly none of the subspecialists are general internists. We must forge a new identity and role in the health care system because our previous identity has been destroyed.

Without our unique ability to temper high tech with clinical judgment, our system fails on quality and cost.

The article by Dr. Lansdale was more eloquent than I could express, but I believe the words written above are more accurate and to the point.

General internal medicine is extinct

To the Editor: General internal medicine has become extinct. Its practitioners have been pushed out of their leadership roles, have been pushed from clinical practice due to red tape and impediments of frustration, and have been marginalized by specialties and subspecialties, our so-called brethren. Only through revolutionary metamorphosis such as clinical homes or other unique systems by which primary care is delivered at high-quality levels such as MDVIP can general internal medicine survive.

Hospitalists are not general internists. Family practitioners are not general internists. Nurse practitioners are not general internists. And certainly none of the subspecialists are general internists. We must forge a new identity and role in the health care system because our previous identity has been destroyed.

Without our unique ability to temper high tech with clinical judgment, our system fails on quality and cost.

The article by Dr. Lansdale was more eloquent than I could express, but I believe the words written above are more accurate and to the point.

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The name of the devil

To the Editor: Dr. Lansdale’s commentary1 reveals the price we pay when we focus on one important goal to the exclusion of others. He illustrates that reductions in health care cost were paid for with reduced health care quality, and a loss of camaraderie and job satisfaction. Missing from his commentary, however, is any acknowledgment that reducing the cost of health care is an important and worthy goal—and his wistfulness for the old days suggests his willingness to trade increased cost for better quality and job satisfaction.

Unfortunately, the biggest problem in this conflict is not that Dr. Lansdale and his former administrators disagree on whether cost is more important than quality and job satisfaction, but that both mistakenly agree that each must be traded off for the others. This hidden agreement is the chief mischief in health care today.

For example, much of the effort to improve health care quality has been oblivious to costs and employee satisfaction. Efforts to reduce errors have led to additional process steps, new checkers and coordinators, and expensive IT systems. These have increased costs, while frequently reducing job satisfaction and in some cases even failing to improve quality. Computerized order entry systems have been shown, for example, to disrupt physician-nurse communication patterns that were one of the major ways the old system prevented errors, and were a source of job satisfaction to both parties.2 In some cases, patient mortality rates increased after they were implemented.3 Another new system plans to police handwashing by putting video cameras in patient rooms.4 Costly, yes, and the consequences for clinical-staff jobsatisfaction are predictable.

The core problem is focusing on one-dimensional outcomes, instead of insisting that cost, quality, and job satisfaction are all vital, and that we will not truly achieve any of them until we achieve all three. Poor quality is wasteful, and waste costs money. Employees are most satisfied where they are productively employed providing high-quality services, and productive employees cost less in the long run than unproductive ones.

How can we have high-quality, low-cost, high-satisfaction health care? By fundamentally redesigning the way care is delivered, radically simplifying care processes to focus on the limited number of elements that produce health outcomes for the patient. Toyota has demonstrated that it is possible for a manufacturer to be high-quality, low-cost, and high-satisfaction by using an analogous approach, and the many manufacturers that have followed its example testify that Toyota was no fluke.5 Early efforts are underway to apply so-called lean approaches in health care settings, but most are pruning the branches of waste instead of pulling it out by the roots, for example, redesigning labs and supply closets far from the patient’s side.6,7

A former boss was fond of quoting economist Kenneth Boulding: “The name of the devil is suboptimization!” Let’s begin by agreeing that cost, quality, and job satisfaction are all important, and commit to working to achieve all three together.

References
  1. Lansdale T. A medical center is not a hospital. Cleve Clin J Med 2008; 75:618–622.
  2. Harrison M, Koppel R, Bar-Lev S. Unintended consequences of information technologies in health care—an interactive sociotechnical analysis. J Am Med Inform Assoc 2007; 14:542–549.
  3. Han Y, Carcillo J, Venkataraman S, et al. Unexpected increased mortality after implementation of a commercially sold computerized physician order entry system. Pediatrics 2005; 116:1506–1512.
  4. Landro L. Health blog. Hospitals to dirty-handed workers: we’ll be watching you. 9/23/08. http://blogs.wsj.com/health/2008/09/23/hospitals-to-dirty-handed-workerswell-be-watching-you. Accessed 9/29/08.
  5. Womack J, Jones D. Lean Thinking. New York: Simon and Schuster, 1996.
  6. Zidel T. A lean toolbox—using lean principles and techniques in healthcare. Journal for Healthcare Quality Web Exclusive 2006; 28(1):W1-7–W1-15.
  7. Zidel T, SanLuis R. Lean tools: principles to improve lab performance. Advance for Administrators of the Laboratory 2007; 17(2):62.
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The name of the devil

To the Editor: Dr. Lansdale’s commentary1 reveals the price we pay when we focus on one important goal to the exclusion of others. He illustrates that reductions in health care cost were paid for with reduced health care quality, and a loss of camaraderie and job satisfaction. Missing from his commentary, however, is any acknowledgment that reducing the cost of health care is an important and worthy goal—and his wistfulness for the old days suggests his willingness to trade increased cost for better quality and job satisfaction.

Unfortunately, the biggest problem in this conflict is not that Dr. Lansdale and his former administrators disagree on whether cost is more important than quality and job satisfaction, but that both mistakenly agree that each must be traded off for the others. This hidden agreement is the chief mischief in health care today.

For example, much of the effort to improve health care quality has been oblivious to costs and employee satisfaction. Efforts to reduce errors have led to additional process steps, new checkers and coordinators, and expensive IT systems. These have increased costs, while frequently reducing job satisfaction and in some cases even failing to improve quality. Computerized order entry systems have been shown, for example, to disrupt physician-nurse communication patterns that were one of the major ways the old system prevented errors, and were a source of job satisfaction to both parties.2 In some cases, patient mortality rates increased after they were implemented.3 Another new system plans to police handwashing by putting video cameras in patient rooms.4 Costly, yes, and the consequences for clinical-staff jobsatisfaction are predictable.

The core problem is focusing on one-dimensional outcomes, instead of insisting that cost, quality, and job satisfaction are all vital, and that we will not truly achieve any of them until we achieve all three. Poor quality is wasteful, and waste costs money. Employees are most satisfied where they are productively employed providing high-quality services, and productive employees cost less in the long run than unproductive ones.

How can we have high-quality, low-cost, high-satisfaction health care? By fundamentally redesigning the way care is delivered, radically simplifying care processes to focus on the limited number of elements that produce health outcomes for the patient. Toyota has demonstrated that it is possible for a manufacturer to be high-quality, low-cost, and high-satisfaction by using an analogous approach, and the many manufacturers that have followed its example testify that Toyota was no fluke.5 Early efforts are underway to apply so-called lean approaches in health care settings, but most are pruning the branches of waste instead of pulling it out by the roots, for example, redesigning labs and supply closets far from the patient’s side.6,7

A former boss was fond of quoting economist Kenneth Boulding: “The name of the devil is suboptimization!” Let’s begin by agreeing that cost, quality, and job satisfaction are all important, and commit to working to achieve all three together.

The name of the devil

To the Editor: Dr. Lansdale’s commentary1 reveals the price we pay when we focus on one important goal to the exclusion of others. He illustrates that reductions in health care cost were paid for with reduced health care quality, and a loss of camaraderie and job satisfaction. Missing from his commentary, however, is any acknowledgment that reducing the cost of health care is an important and worthy goal—and his wistfulness for the old days suggests his willingness to trade increased cost for better quality and job satisfaction.

Unfortunately, the biggest problem in this conflict is not that Dr. Lansdale and his former administrators disagree on whether cost is more important than quality and job satisfaction, but that both mistakenly agree that each must be traded off for the others. This hidden agreement is the chief mischief in health care today.

For example, much of the effort to improve health care quality has been oblivious to costs and employee satisfaction. Efforts to reduce errors have led to additional process steps, new checkers and coordinators, and expensive IT systems. These have increased costs, while frequently reducing job satisfaction and in some cases even failing to improve quality. Computerized order entry systems have been shown, for example, to disrupt physician-nurse communication patterns that were one of the major ways the old system prevented errors, and were a source of job satisfaction to both parties.2 In some cases, patient mortality rates increased after they were implemented.3 Another new system plans to police handwashing by putting video cameras in patient rooms.4 Costly, yes, and the consequences for clinical-staff jobsatisfaction are predictable.

The core problem is focusing on one-dimensional outcomes, instead of insisting that cost, quality, and job satisfaction are all vital, and that we will not truly achieve any of them until we achieve all three. Poor quality is wasteful, and waste costs money. Employees are most satisfied where they are productively employed providing high-quality services, and productive employees cost less in the long run than unproductive ones.

How can we have high-quality, low-cost, high-satisfaction health care? By fundamentally redesigning the way care is delivered, radically simplifying care processes to focus on the limited number of elements that produce health outcomes for the patient. Toyota has demonstrated that it is possible for a manufacturer to be high-quality, low-cost, and high-satisfaction by using an analogous approach, and the many manufacturers that have followed its example testify that Toyota was no fluke.5 Early efforts are underway to apply so-called lean approaches in health care settings, but most are pruning the branches of waste instead of pulling it out by the roots, for example, redesigning labs and supply closets far from the patient’s side.6,7

A former boss was fond of quoting economist Kenneth Boulding: “The name of the devil is suboptimization!” Let’s begin by agreeing that cost, quality, and job satisfaction are all important, and commit to working to achieve all three together.

References
  1. Lansdale T. A medical center is not a hospital. Cleve Clin J Med 2008; 75:618–622.
  2. Harrison M, Koppel R, Bar-Lev S. Unintended consequences of information technologies in health care—an interactive sociotechnical analysis. J Am Med Inform Assoc 2007; 14:542–549.
  3. Han Y, Carcillo J, Venkataraman S, et al. Unexpected increased mortality after implementation of a commercially sold computerized physician order entry system. Pediatrics 2005; 116:1506–1512.
  4. Landro L. Health blog. Hospitals to dirty-handed workers: we’ll be watching you. 9/23/08. http://blogs.wsj.com/health/2008/09/23/hospitals-to-dirty-handed-workerswell-be-watching-you. Accessed 9/29/08.
  5. Womack J, Jones D. Lean Thinking. New York: Simon and Schuster, 1996.
  6. Zidel T. A lean toolbox—using lean principles and techniques in healthcare. Journal for Healthcare Quality Web Exclusive 2006; 28(1):W1-7–W1-15.
  7. Zidel T, SanLuis R. Lean tools: principles to improve lab performance. Advance for Administrators of the Laboratory 2007; 17(2):62.
References
  1. Lansdale T. A medical center is not a hospital. Cleve Clin J Med 2008; 75:618–622.
  2. Harrison M, Koppel R, Bar-Lev S. Unintended consequences of information technologies in health care—an interactive sociotechnical analysis. J Am Med Inform Assoc 2007; 14:542–549.
  3. Han Y, Carcillo J, Venkataraman S, et al. Unexpected increased mortality after implementation of a commercially sold computerized physician order entry system. Pediatrics 2005; 116:1506–1512.
  4. Landro L. Health blog. Hospitals to dirty-handed workers: we’ll be watching you. 9/23/08. http://blogs.wsj.com/health/2008/09/23/hospitals-to-dirty-handed-workerswell-be-watching-you. Accessed 9/29/08.
  5. Womack J, Jones D. Lean Thinking. New York: Simon and Schuster, 1996.
  6. Zidel T. A lean toolbox—using lean principles and techniques in healthcare. Journal for Healthcare Quality Web Exclusive 2006; 28(1):W1-7–W1-15.
  7. Zidel T, SanLuis R. Lean tools: principles to improve lab performance. Advance for Administrators of the Laboratory 2007; 17(2):62.
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Correction: A case of refractory diarrhea

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Two errors appeared in: Monti J, Isaacson JH, Lashner B. A case of refractory diarrhea. Cleve Clin J Med 2008; 75:677–680. On page 679, the proprietary name of lansoprazole was incorrectly given as Prilosec and the proprietary name of omeprazole was incorrectly given as Prevacid. The proprietary names were reversed. The correct listing should have been: Lansoprazole (Prevacid) and omeprazole (Prilosec).

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Two errors appeared in: Monti J, Isaacson JH, Lashner B. A case of refractory diarrhea. Cleve Clin J Med 2008; 75:677–680. On page 679, the proprietary name of lansoprazole was incorrectly given as Prilosec and the proprietary name of omeprazole was incorrectly given as Prevacid. The proprietary names were reversed. The correct listing should have been: Lansoprazole (Prevacid) and omeprazole (Prilosec).

Two errors appeared in: Monti J, Isaacson JH, Lashner B. A case of refractory diarrhea. Cleve Clin J Med 2008; 75:677–680. On page 679, the proprietary name of lansoprazole was incorrectly given as Prilosec and the proprietary name of omeprazole was incorrectly given as Prevacid. The proprietary names were reversed. The correct listing should have been: Lansoprazole (Prevacid) and omeprazole (Prilosec).

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Hepatitis B virus infection: Understanding its epidemiology, course, and diagnosis

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Our knowledge about hepatitis B and related diseases has dramatically increased since the discovery of the causative virus, HBV, in 1963. Despite effective vaccination, hepatitis B still constitutes a major public health problem.

In two parts, this comprehensive review will highlight a practical clinical approach to HBV infection. In this first part, we discuss the epidemiology, natural history, and diagnosis of HBV infection. In the second part, to be published in the next issue of this journal, we will review the general principles of its management, its management in patients on immunosuppressant therapy and in pregnant women, and HBV vaccination.

COMMON IN ASIA, LESS SO IN AMERICA

More than 2 billion people—one-third of the world’s population—alive today have been infected with HBV at some time in their life, and of these, about 350 million remain infected.1 Every year, 1 million people die of HBV-related cirrhosis or hepatocellular carcinoma, which means that HBV takes a life every 30 seconds.2

World Health Organization. Introduction of hepatitis B vaccine into childhood immunization services. Geneva: WHO; 2001. WHO/V AND B/01.31.
Figure 1. Global prevalence of hepatitis B virus (HBV) surface antigenemia.
HBV infection is highly prevalent in Asia, sub-Saharan Africa, and other parts of the developing world, but less so in the United States, except in Alaskan natives and immigrants from regions of high prevalence (Figure 1). By some estimates, 1.25 million carriers, defined as those positive for the HBV surface antigen for more than 6 months, live in the United States, and about half of them are Asian-American.3,4 Other estimates put the number as high as 2 million, taking into account the prevalence of HBV in immigrant populations.

The incidence of acute hepatitis B in the United States has declined from 8.5 per 100,000 population in 1990 to 2.1 per 100,000 population in 2004, with the greatest declines (94%) in children and adolescents, coincident with an increase in hepatitis B vaccination in these age groups.5 Despite these advances, HBV still causes a considerable number of cases of cirrhosis, cancer, and death—about 5,000 deaths each year in the United States.

HBV HAS FOUR GENES, EIGHT GENOTYPES

HBV is a DNA virus of the Hepadnaviridae family. Its genome is double-stranded with four genes, each one encoding a specific structural protein or proteins6,7:

  • S gene, for the viral envelope (surface antigen)
  • C gene, for both the nucleocapsid (core) antigen and the pre-core (e) antigen
  • X gene, for two regulatory proteins required for HBV replication
  • P gene, for DNA polymerase.

Several clinically important mutations in the HBV genome are known (Table 1).7–12

Eight genotypes of HBV (labeled A though H) have been identified.13,14 All eight have been found in the United States, but genotype A accounts for 35% of cases, genotype B for 22%, and genotype C for 31%.15

The clinical significance of HBV genotypes is not as clear as that of hepatitis C virus genotypes. Although recent data have suggested that different HBV genotypes may be associated with different rates of progression of liver disease and different rates of response to interferon therapy,13 these data were not enough to recommend routine testing for HBV genotypes in clinical practice.16

In HBV infection, the virus itself does not injure liver cells. Rather, the damage of hepatitis is immune-mediated and begins to appear as the host’s immune system attempts to clear the virus.

MARKERS OF HBV INFECTION

Figure 2.
HBV produces several antigens that can be detected in the blood and that disappear as the body produces antibodies against them. The patterns of these and other markers provide clues to the phase of infection (Figure 2).

HBV surface antigen and HBV DNA are often the first detectable markers of acute infection, appearing before the onset of symptoms or before elevation of alanine aminotransferase (ALT) occurs. By definition, an HBV infection is chronic if surface antigen persists longer than 6 months.

HBV e antigen, derived from pre-core protein, is considered a marker of HBV replication and infectivity. In chronic infection, e antigen can persist for years or decades.

HBV core antigen cannot be detected in the serum, but antibodies against it can, first immunoglobulin M (IgM) and later immunoglobulin G (IgG).

TRANSMISSION: VERTICAL OR HORIZONTAL

Because HBV replicates profusely and produces high titers in the blood (108 to 1,010 virions/ mL), any parenteral or mucosal exposure to infected blood poses a high risk of HBV acquisition. The risk of HBV transmission from a single needlestick is 1% to 6% if the blood is positive for HBV surface antigen but negative for HBV e antigen, and 22% to 40% if positive for both antigens.17–19 Saliva, nasopharyngeal fluid, breast milk, semen, urine, and cervical secretions can also harbor HBV.20

Worldwide, perinatal (vertical) transmission is the predominant mode of HBV transmission, whereas intravenous drug abuse and unprotected sexual intercourse are the main routes of infection in areas of low prevalence, such as the United States. In sub-Saharan Africa, Alaska, and Mediterranean countries, transmission of HBV usually occurs horizontally during childhood, presumably via contact with nonintact skin.21–24 Saliva has also been thought to be the route of HBV transmission in sporadic cases through human bites.25

People at risk of HBV infection include:

  • Parenteral drug users
  • People with multiple sexual partners
  • Household contacts and sexual partners of people who are 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.

These people—as well as all pregnant women, patients infected with hepatitis C virus or human immunodeficiency virus, and patients with chronically elevated ALT or aspartate aminotransferase (AST) levels—should be screened for HBV infection with serologic markers.

 

 

CLINICAL MANIFESTATIONS VARY

HBV infection, acute or chronic, has variable manifestations. During the acute stage, HBV infection can manifest as anicteric (subclinical) hepatitis, icteric hepatitis, or, rarely, acute fulminant hepatitis. Chronic HBV infection can be asymptomatic (the HBV surface antigen carrier state), or it can be manifested by symptoms and signs of cirrhosis or hepatocellular carcinoma or both. Extrahepatic manifestations, including serum sickness, polyarteritis nodosa, essential mixed cryoglobulinemia, membranous glomerulonephritis, and aplastic anemia, have been reported in patients with HBV infection.26

Acute hepatitis B

The incubation period of HBV ranges from 2 weeks to 4 months. Initially, patients complain of fatigue, malaise, anorexia, right upper quad-rant discomfort, or flu-like symptoms (coryza, photophobia, headache, and myalgia); then jaundice becomes apparent, usually within 10 days of the onset of symptoms. Low-grade fever, jaundice, and mildly tender hepatomegaly are the most common signs. Generalized lymphadenopathy is not a feature of acute HBV infection. If the patient also has hepatitis D virus infection or underlying liver disease (eg, alcoholic liver disease), then acute HBV infection may be more severe.

In the acute phase, ALT and AST levels rise, sometimes to values above 1,000 IU/L. In icteric hepatitis, bilirubin levels also rise, usually after the ALT level does. Although the peak ALT level reflects the hepatocellular injury, it has no prognostic value. With recovery, ALT levels normalize in 1 to 4 months.

Acute fulminant hepatitis B occurs in 0.1% to 0.5% of patients, and causes about 10% of cases of acute liver failure in the United States.27 Patients typically present with rapidly progressive acute hepatitis characterized by signs of liver failure, such as coagulopathy, encephalopathy, and cerebral edema.

In the so-called window phase, laboratory testing may not reveal HBV surface antigen because of early clearance but shows IgM antibody against the HBV core antigen. HBV DNA may be low or undetected.

Chronic hepatitis B

Chronic hepatitis B is usually diagnosed as a result of a workup for abnormal liver function tests or as a result of screening patients at risk for HBV infection. Many patients with chronic hepatitis B have no symptoms or have nonspecific symptoms such as fatigue or right upper quadrant discomfort.

Acute exacerbations due to HBV e antigen seroreversion (ie, in which e antigen reappears) occasionally occur in patients with chronic hepatitis B. Most of these exacerbations are asymptomatic, but occasionally an acute hepatitis-like clinical picture with detectable IgM antibody against the core antigen occurs, leading to misdiagnosis of acute HBV infection in patients not previously known to have chronic HBV infection.28

In late cases, signs of cirrhosis such as jaundice, ascites, splenomegaly, pedal edema, encephalopathy, or variceal bleeding can be present.

Hepatocellular carcinoma should be suspected in cirrhotic patients with new-onset right upper quadrant pain, rapidly developing ascites, a palpable liver mass, or hepatic encephalopathy. Other nonspecific features of hepatocellular carcinoma include watery diarrhea, hypoglycemia, and certain cutaneous manifestations such as acanthosis nigricans and the Leser-Trelat sign (multiple pruritic seborrheic keratoses of sudden onset).

In chronic hepatitis B, liver enzyme levels can be normal, even in patients with wellcompensated cirrhosis. ALT levels may range from normal to five times higher than normal. Thrombocytopenia, hypoalbuminemia, direct hyperbilirubinemia, and prolonged prothrombin time suggest cirrhosis.

Findings of chronic hepatitis B on liver biopsy range from minimal inflammation to cirrhosis. The most characteristic histologic feature of chronic HBV infection is the “ground-glass hepatocyte,” which is due to intracellular accumulation of HBV surface antigen. 29

FEW ADULTS (BUT MANY CHILDREN) REMAIN CHRONICALLY INFECTED

Figure 3. Natural history of HBV infection.
The natural history of HBV infection has become better defined, thanks to extensive epidemiologic studies and highly sensitive HBV DNA assays (Figure 3). It is crucial for clinicians to understand the natural history of HBV infection to appropriately decide which infected patients need antiviral therapy. This will be discussed in our second article.

HBV surface antigen can be detected in the blood approximately 2 to 4 weeks after inoculation. Simultaneously, HBV DNA, usually in very high levels, is also detectable in the blood. However, in the rare cases of acute fulminant hepatitis, HBV DNA levels can be low or undetectable at the time of presentation because the immune system mounts a robust response with extensive damage to HBVinfected hepatocytes.

The rate of spontaneous recovery from acute HBV infection varies, depending on the patient’s age at the time of HBV acquisition and the patient’s immune status. Fewer than 5% of immunocompetent adults infected with HBV remain chronically infected, defined as being positive for HBV surface antigen for more than 6 months. On the other hand, 80% to 90% of infected infants and about 20% to 50% of children 1 to 5 years old at the time of acute infection remain chronically infected.21

 

 

Four phases of chronic HBV infection

Four phases of chronic HBV infection have been outlined (Table 2),30 although all patients do not go through all phases. HBV surface antigen is detectable in all of them.

The immune tolerance phase, the initial phase of chronic HBV infection, is seen almost exclusively in those who acquired HBV infection vertically or during early childhood. Although patients have high HBV DNA levels, they do not have significant liver disease. This discrepancy is thought to be related to the immune tolerance to HBV; however, the exact mechanism of that tolerance is unclear.31

Only 15% of those with immune tolerance have spontaneous HBV e antigen seroconversion (ie, loss of e antigen and appearance of anti-e antibody) within 20 years after infection. 32

The immune clearance phase (HBV e antigen-positive chronic hepatitis) appears about 20 to 30 years after the onset of the immune tolerance phase in patients who acquire HBV early in life. It is also often seen in patients with infections acquired late in childhood or in adulthood.

This phase marks the start of an immunemediated process aimed at clearing the viral infection, but it also leads to concomitant hepatocellular injury. Spontaneous clearance of the e antigen increases in this phase to an annual rate of 10% to 20%.32,33 The strongest predictors of spontaneous e antigen seroconversion are old age, an elevated ALT level, and an acute exacerbation.26

Although ALT levels are elevated and there is evidence on liver biopsy of chronic active hepatitis, this phase is usually asymptomatic. Rarely, however, it presents with an acute flare of hepatitis, sometimes accompanied by IgM antibodies against the HBV core antigen (in low titer), leading to an incorrect diagnosis of acute HBV infection.

Depending on the duration of the chronic hepatitis and the frequency and severity of flares, about 12% to 20% of patients in the immune-clearance phase develop serious liver disease within 5 years.31

The inactive carrier phase following HBV e antigen seroconversion is characterized by undetectable or low HBV DNA levels (< 1,000 copies/mL), normal ALT levels, and minimal or no necroinflammation on liver biopsy. 30 Such patients should be followed with serial testing, as 4% to 20% of them spontaneously revert to being positive for e antigen at least once.16 On the other hand, only 0.5% to 2% of surface antigen carriers in western countries clear themselves of surface antigen yearly, but up to half of those who clear the surface antigen have low-level HBV viremia. 34

The reactivation phase (HBV e antigennegative chronic hepatitis) is seen in some HBV-infected patients, especially those from Asia and southern Europe, in whom the virus has a spontaneous pre-core or core mutation that makes infected cells unable to secrete the e antigen. Although these patients have no e antigen in their blood, they do have intermittent or persistent elevation of ALT, elevated HBV DNA, and histopathologic findings of chronic hepatitis. Compared with those in the immune clearance phase, patients in the reactivation phase tend to be older and to have lower HBV DNA levels but advanced hepatic damage.

Immunity to HBV infection is characterized by loss of HBV surface antigen, DNA, e antigen, and anti-core antigen IgM with development of anti-surface antigen antibody and anti-core antigen IgG (total anti-core antigen antibody). The presence of anti-surface antigen antibody and anti-core antigen IgG together differentiates natural immunity through resolved infection from that which is acquired through vaccination, which is denoted by isolated anti-surface antigen antibody.

Figure 2 illustrates the typical serologic course of HBV infection, and Table 3 summarizes how to interpret the various serologic patterns.

Cirrhosis, liver failure, cancer

Cirrhosis, hepatic decompensation, and hepatocellular carcinoma are the major long-term complications of HBV infection. In untreated patients, the annual rate of progression to cirrhosis has been estimated to be 2% to 6% in patients with HBV e antigen-positive chronic hepatitis and 8% to 9% in those with e antigen- negative chronic hepatitis.30

The likely explanation for these surprising cirrhosis rates is that e antigen-negative chronic hepatitis usually represents a late stage of the disease, and patients in this phase are usually older and have more advanced liver disease.

Subsequently, the annual rate of progression from compensated cirrhosis to hepatic decompensation has been estimated to be about 5%.35

Across all the stages described above, a high serum HBV DNA level has been shown to be a strong predictor of progression to cirrhosis in patients with chronic HBV infection. In a population-based prospective cohort study of 3,582 untreated HBV-infected patients in Taiwan, Iloeje et al36 found that, compared with patients with serum HBV DNA levels lower than 104 copies/mL, those with levels of 104 or higher had an adjusted relative risk of cirrhosis of 2.5. The relative risk rose to 5.9 with HBV DNA levels of 105 or higher, and 9.8 with levels of 106 copies/mL or higher. More studies in different patient populations are needed for confirmation.

HBV is a strong carcinogen, and the risk of hepatocellular carcinoma is 100 times higher in patients with HBV infection than in uninfected ones.31

The most important risk factor for hepatocellular carcinoma in HBV-infected patients is cirrhosis, but this cancer can also develop in noncirrhotic livers.37 The annual rate of hepatocelluar carcinoma has been estimated to be higher (2.5%–3%) in patients with cirrhosis than in noncirrhotic carriers (0.5%–1%).30,35–38 Risk factors for cirrhosis and hepatocellular carcinoma are summarized in Table 4.16,30

References
  1. World Health Organization. Hepatitis B. www.who.int/csr/disease/hepatitis/whocdscsrlyo20022/en. Accessed 11/10/2008.
  2. Center for Disease Control and Prevention. HBV a silent killer. www.cdc.gov/ncidod/diseases/hepatitis/b/hbv_silent_killer. Accessed 2/19/2007.
  3. McQuillan GM, Coleman PJ, Kruszon-Moran D, Moyer LA, Lambert SB, Margolis HS. Prevalence of hepatitis B virus infection in the United States: the National Health and Nutrition Examination Surveys, 1976 through 1994. Am J Public Health 1999; 89:1418.
  4. Armstrong GL, Mast EE, Wojczynski M, Margolis HS. Childhood hepatitis B virus infections in the United States before hepatitis B immunization. Pediatrics 2001; 108:11231128.
  5. 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 Dec 8; 55(RR-16):133.
  6. Gish RG, Gadano AC. Chronic hepatitis B: current epidemiology in the Americas and implications for management. J Viral Hepatol 2006; 13:787798.
  7. Wei Y, Tiollais PK. Molecular biology of hepatitis B virus. Clin Liver Dis 1999; 3:189219.
  8. Seeger C, Mason WS. Hepatitis B virus biology. Microbiol Mol Biol Rev 2000; 64:5168.
  9. Hunt CM, McGill JM, Allen MI, Condreay LD. Clinical relevance of hepatitis B viral mutations. Hepatology 2000; 3:10371044.
  10. Allen MI, Deslauriers M, Andrews CW, et al. Identification and characterization of mutations in hepatitis B virus resistant to lamivudine. Lamivudine Clinical Investigation Group. Hepatology 1998; 27:16701677.
  11. Hadziyannis SJ, Vassilopoulos D. Hepatitis B e antigen- negative chronic hepatitis B. Hepatology 2001; 34:617624.
  12. Wai CT, Fontana RJ. Clinical significance of hepatitis B virus genotypes, variants, and mutants. Clin Liver Dis 2004; 8:321352.
  13. Fung SK, Lok AS. Hepatitis B virus genotypes: do they play a role in the outcome of HBV infection? Hepatology 2004; 40:790792.
  14. Norder H, Courouce AM, Coursaget P, et al. Genetic diversity of hepatitis B virus strains derived worldwide: genotypes, subgenotypes, and HBsAg subtypes. Intervirology 2004; 47:289309.
  15. Chu CJ, Keeffe EB, Han SH, et al. Hepatitis B virus genotypes in the United States: results of a nationwide study. Gastroenterology 2003; 125:444451.
  16. Lok AS, McMahon BJ. Chronic hepatitis B. Hepatology 2007; 45:507539.
  17. Mast EE, Alter MJ. Prevention of hepatitis B virus infection among health-care workers. In:Ellis RE, editor. Hepatitis B Vaccines in Clinical Practice. New York: Marcel Dekker, 1993:295307.
  18. Werner BG, Grady GF. Accidental hepatitis-B-surface-antigen-positive inoculations: use of e antigen to estimate infectivity. Ann Intern Med 1982; 97:367369.
  19. Gerberding JL. Management of occupational exposures to blood-borne viruses. N Engl J Med 1995; 332:444451.
  20. Kidd-Ljunggren K, Holmberg A, Blackberg J, Lindqvist B. High levels of hepatitis B virus DNA in body fluids from chronic carriers. J Hosp Infect 2006; 64:352357.
  21. McMahon BJ, Alward WL, Hall DB, et al. Acute hepatitis B virus infection: relation of age to the clinical expression of disease and subsequent development of the carrier state. J Infect Dis 1985; 151:599603.
  22. Dusheiko GM, Brink BA, Conradie JD, Marimuthu T, Sher R. Regional prevalence of hepatitis B, delta, and human immunodeficiency virus infection in southern Africa: a large population survey. Am J Epidemiol 1989; 129:13845.
  23. Bortolotti F, Guido M, Bartolacci S, et al. Chronic hepatitis B in children after e antigen seroclearance: final report of a 29-year longitudinal study. Hepatology 2006; 43:556562.
  24. Moreno MR, Otero M, Millan A, et al. Clinical and histological outcome after hepatitis B e antigen to antibody seroconversion in children with chronic hepatitis B. Hepatology 1999:572575.
  25. Hui AY, Hung LC, Tse PC, Leung WK, Chan PK, Chan HL. Transmission of hepatitis B by human bite--confirmation by detection of virus in saliva and full genome sequencing. J Clin Virol 2005; 33:254256.
  26. Cacoub P, Saadoun D, Bourlière M, et al. Hepatitis B virus genotypes and extrahepatic manifestations. J Hepatol 2005; 43:764770.
  27. Schiodt FV, Atillasoy E, Shakil AO, et al. Etiology and outcome for 295 patients with acute liver failure in the United States. Liver Transplant Surg 1999; 5:2934.
  28. Chu CM, Liaw YF, Pao CC, Huang MJ. The etiology of acute hepatitis superimposed upon previously unrecognized asymptomatic HBsAg carriers. Hepatology 1989; 9:452456.
  29. Gerber MA, Hadziyannis S, Vissoulis C, et al. Electron microscopy and immunoelectronmicroscopy of cytoplasmic hepatitis B antigen in hepatocytes. Am J Pathol 1974; 75:489502.
  30. Yim HJ, Lok AS. Natural history of chronic hepatitis B virus infection: what we knew in 1981 and what we know in 2005. Hepatology 2006; 43:S173S181.
  31. Pungpapong S, Kim WR, Poterucha JJ. Natural history of hepatitis B virus infection: an update for clinicians. Mayo Clin Proc 2007; 82:967975.
  32. Lok AS, Lai CL, Wu PC, Leung EK, Lam TS. Spontaneous hepatitis B e antigen to antibody seroconversion and reversion in Chinese patients with chronic hepatitis B virus infection. Gastroenterology 1987; 92:18391843.
  33. McMahon BJ, Holck P, Bulkow L, Snowball M. Serologic and clinical outcomes in 1536 Alaska Natives chronically infected with hepatitis B virus. Ann Intern Med 2001; 135:759768.
  34. McMahon BJ. Epidemiology and natural history of hepatitis B. Semin Liver Dis 2005; 25( suppl 1):38.
  35. Benvegnu L, Gios M, Boccato S, Alberti A. Natural history of compensated viral cirrhosis: a prospective study on the incidence and hierarchy of major complications. Gut 2004; 53:744749.
  36. Iloeje UH, Yang HI, Su J, Jen CL, You SL, Chen CJ. Risk evaluation of viral load elevation and associated liver disease/cancer in HBV. The REVEAL-HBV Study Group. Predicting cirrhosis risk based on the level of circulating hepatitis B viral load. Gastroenterology 2006; 130:678686.
  37. Bosch FX, Ribes J, Cleries R, Diaz M. Epidemiology of hepatocellular carcinoma. Clin Liver Dis 2005; 9:191211.
  38. Fattovich G. Natural history of hepatitis B. J Hepatol 2003; 39:S50S58.
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Hesham M. Elgouhari, MD
Assistant Professor of Medicine, University of South Dakota School of Medicine; Avera Center for Liver Disease/Transplant Institute, Sioux Falls, SD

Tarek I. Abu-Rajab Tamimi, MD
Department of Gastroenterology and Hepatology, Cleveland Clinic

William D. Carey, MD
Department of Gastroenterology and Hepatology, Cleveland Clinic

Address: William D. Carey, MD, Department of Gastroenterology and Hepatology, A30, Cleveland Clinic, 9500 Euclid Avenue, Cleveland, OH 44195; [email protected]

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Assistant Professor of Medicine, University of South Dakota School of Medicine; Avera Center for Liver Disease/Transplant Institute, Sioux Falls, SD

Tarek I. Abu-Rajab Tamimi, MD
Department of Gastroenterology and Hepatology, Cleveland Clinic

William D. Carey, MD
Department of Gastroenterology and Hepatology, Cleveland Clinic

Address: William D. Carey, MD, Department of Gastroenterology and Hepatology, A30, Cleveland Clinic, 9500 Euclid Avenue, Cleveland, OH 44195; [email protected]

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Hesham M. Elgouhari, MD
Assistant Professor of Medicine, University of South Dakota School of Medicine; Avera Center for Liver Disease/Transplant Institute, Sioux Falls, SD

Tarek I. Abu-Rajab Tamimi, MD
Department of Gastroenterology and Hepatology, Cleveland Clinic

William D. Carey, MD
Department of Gastroenterology and Hepatology, Cleveland Clinic

Address: William D. Carey, MD, Department of Gastroenterology and Hepatology, A30, Cleveland Clinic, 9500 Euclid Avenue, Cleveland, OH 44195; [email protected]

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Our knowledge about hepatitis B and related diseases has dramatically increased since the discovery of the causative virus, HBV, in 1963. Despite effective vaccination, hepatitis B still constitutes a major public health problem.

In two parts, this comprehensive review will highlight a practical clinical approach to HBV infection. In this first part, we discuss the epidemiology, natural history, and diagnosis of HBV infection. In the second part, to be published in the next issue of this journal, we will review the general principles of its management, its management in patients on immunosuppressant therapy and in pregnant women, and HBV vaccination.

COMMON IN ASIA, LESS SO IN AMERICA

More than 2 billion people—one-third of the world’s population—alive today have been infected with HBV at some time in their life, and of these, about 350 million remain infected.1 Every year, 1 million people die of HBV-related cirrhosis or hepatocellular carcinoma, which means that HBV takes a life every 30 seconds.2

World Health Organization. Introduction of hepatitis B vaccine into childhood immunization services. Geneva: WHO; 2001. WHO/V AND B/01.31.
Figure 1. Global prevalence of hepatitis B virus (HBV) surface antigenemia.
HBV infection is highly prevalent in Asia, sub-Saharan Africa, and other parts of the developing world, but less so in the United States, except in Alaskan natives and immigrants from regions of high prevalence (Figure 1). By some estimates, 1.25 million carriers, defined as those positive for the HBV surface antigen for more than 6 months, live in the United States, and about half of them are Asian-American.3,4 Other estimates put the number as high as 2 million, taking into account the prevalence of HBV in immigrant populations.

The incidence of acute hepatitis B in the United States has declined from 8.5 per 100,000 population in 1990 to 2.1 per 100,000 population in 2004, with the greatest declines (94%) in children and adolescents, coincident with an increase in hepatitis B vaccination in these age groups.5 Despite these advances, HBV still causes a considerable number of cases of cirrhosis, cancer, and death—about 5,000 deaths each year in the United States.

HBV HAS FOUR GENES, EIGHT GENOTYPES

HBV is a DNA virus of the Hepadnaviridae family. Its genome is double-stranded with four genes, each one encoding a specific structural protein or proteins6,7:

  • S gene, for the viral envelope (surface antigen)
  • C gene, for both the nucleocapsid (core) antigen and the pre-core (e) antigen
  • X gene, for two regulatory proteins required for HBV replication
  • P gene, for DNA polymerase.

Several clinically important mutations in the HBV genome are known (Table 1).7–12

Eight genotypes of HBV (labeled A though H) have been identified.13,14 All eight have been found in the United States, but genotype A accounts for 35% of cases, genotype B for 22%, and genotype C for 31%.15

The clinical significance of HBV genotypes is not as clear as that of hepatitis C virus genotypes. Although recent data have suggested that different HBV genotypes may be associated with different rates of progression of liver disease and different rates of response to interferon therapy,13 these data were not enough to recommend routine testing for HBV genotypes in clinical practice.16

In HBV infection, the virus itself does not injure liver cells. Rather, the damage of hepatitis is immune-mediated and begins to appear as the host’s immune system attempts to clear the virus.

MARKERS OF HBV INFECTION

Figure 2.
HBV produces several antigens that can be detected in the blood and that disappear as the body produces antibodies against them. The patterns of these and other markers provide clues to the phase of infection (Figure 2).

HBV surface antigen and HBV DNA are often the first detectable markers of acute infection, appearing before the onset of symptoms or before elevation of alanine aminotransferase (ALT) occurs. By definition, an HBV infection is chronic if surface antigen persists longer than 6 months.

HBV e antigen, derived from pre-core protein, is considered a marker of HBV replication and infectivity. In chronic infection, e antigen can persist for years or decades.

HBV core antigen cannot be detected in the serum, but antibodies against it can, first immunoglobulin M (IgM) and later immunoglobulin G (IgG).

TRANSMISSION: VERTICAL OR HORIZONTAL

Because HBV replicates profusely and produces high titers in the blood (108 to 1,010 virions/ mL), any parenteral or mucosal exposure to infected blood poses a high risk of HBV acquisition. The risk of HBV transmission from a single needlestick is 1% to 6% if the blood is positive for HBV surface antigen but negative for HBV e antigen, and 22% to 40% if positive for both antigens.17–19 Saliva, nasopharyngeal fluid, breast milk, semen, urine, and cervical secretions can also harbor HBV.20

Worldwide, perinatal (vertical) transmission is the predominant mode of HBV transmission, whereas intravenous drug abuse and unprotected sexual intercourse are the main routes of infection in areas of low prevalence, such as the United States. In sub-Saharan Africa, Alaska, and Mediterranean countries, transmission of HBV usually occurs horizontally during childhood, presumably via contact with nonintact skin.21–24 Saliva has also been thought to be the route of HBV transmission in sporadic cases through human bites.25

People at risk of HBV infection include:

  • Parenteral drug users
  • People with multiple sexual partners
  • Household contacts and sexual partners of people who are 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.

These people—as well as all pregnant women, patients infected with hepatitis C virus or human immunodeficiency virus, and patients with chronically elevated ALT or aspartate aminotransferase (AST) levels—should be screened for HBV infection with serologic markers.

 

 

CLINICAL MANIFESTATIONS VARY

HBV infection, acute or chronic, has variable manifestations. During the acute stage, HBV infection can manifest as anicteric (subclinical) hepatitis, icteric hepatitis, or, rarely, acute fulminant hepatitis. Chronic HBV infection can be asymptomatic (the HBV surface antigen carrier state), or it can be manifested by symptoms and signs of cirrhosis or hepatocellular carcinoma or both. Extrahepatic manifestations, including serum sickness, polyarteritis nodosa, essential mixed cryoglobulinemia, membranous glomerulonephritis, and aplastic anemia, have been reported in patients with HBV infection.26

Acute hepatitis B

The incubation period of HBV ranges from 2 weeks to 4 months. Initially, patients complain of fatigue, malaise, anorexia, right upper quad-rant discomfort, or flu-like symptoms (coryza, photophobia, headache, and myalgia); then jaundice becomes apparent, usually within 10 days of the onset of symptoms. Low-grade fever, jaundice, and mildly tender hepatomegaly are the most common signs. Generalized lymphadenopathy is not a feature of acute HBV infection. If the patient also has hepatitis D virus infection or underlying liver disease (eg, alcoholic liver disease), then acute HBV infection may be more severe.

In the acute phase, ALT and AST levels rise, sometimes to values above 1,000 IU/L. In icteric hepatitis, bilirubin levels also rise, usually after the ALT level does. Although the peak ALT level reflects the hepatocellular injury, it has no prognostic value. With recovery, ALT levels normalize in 1 to 4 months.

Acute fulminant hepatitis B occurs in 0.1% to 0.5% of patients, and causes about 10% of cases of acute liver failure in the United States.27 Patients typically present with rapidly progressive acute hepatitis characterized by signs of liver failure, such as coagulopathy, encephalopathy, and cerebral edema.

In the so-called window phase, laboratory testing may not reveal HBV surface antigen because of early clearance but shows IgM antibody against the HBV core antigen. HBV DNA may be low or undetected.

Chronic hepatitis B

Chronic hepatitis B is usually diagnosed as a result of a workup for abnormal liver function tests or as a result of screening patients at risk for HBV infection. Many patients with chronic hepatitis B have no symptoms or have nonspecific symptoms such as fatigue or right upper quadrant discomfort.

Acute exacerbations due to HBV e antigen seroreversion (ie, in which e antigen reappears) occasionally occur in patients with chronic hepatitis B. Most of these exacerbations are asymptomatic, but occasionally an acute hepatitis-like clinical picture with detectable IgM antibody against the core antigen occurs, leading to misdiagnosis of acute HBV infection in patients not previously known to have chronic HBV infection.28

In late cases, signs of cirrhosis such as jaundice, ascites, splenomegaly, pedal edema, encephalopathy, or variceal bleeding can be present.

Hepatocellular carcinoma should be suspected in cirrhotic patients with new-onset right upper quadrant pain, rapidly developing ascites, a palpable liver mass, or hepatic encephalopathy. Other nonspecific features of hepatocellular carcinoma include watery diarrhea, hypoglycemia, and certain cutaneous manifestations such as acanthosis nigricans and the Leser-Trelat sign (multiple pruritic seborrheic keratoses of sudden onset).

In chronic hepatitis B, liver enzyme levels can be normal, even in patients with wellcompensated cirrhosis. ALT levels may range from normal to five times higher than normal. Thrombocytopenia, hypoalbuminemia, direct hyperbilirubinemia, and prolonged prothrombin time suggest cirrhosis.

Findings of chronic hepatitis B on liver biopsy range from minimal inflammation to cirrhosis. The most characteristic histologic feature of chronic HBV infection is the “ground-glass hepatocyte,” which is due to intracellular accumulation of HBV surface antigen. 29

FEW ADULTS (BUT MANY CHILDREN) REMAIN CHRONICALLY INFECTED

Figure 3. Natural history of HBV infection.
The natural history of HBV infection has become better defined, thanks to extensive epidemiologic studies and highly sensitive HBV DNA assays (Figure 3). It is crucial for clinicians to understand the natural history of HBV infection to appropriately decide which infected patients need antiviral therapy. This will be discussed in our second article.

HBV surface antigen can be detected in the blood approximately 2 to 4 weeks after inoculation. Simultaneously, HBV DNA, usually in very high levels, is also detectable in the blood. However, in the rare cases of acute fulminant hepatitis, HBV DNA levels can be low or undetectable at the time of presentation because the immune system mounts a robust response with extensive damage to HBVinfected hepatocytes.

The rate of spontaneous recovery from acute HBV infection varies, depending on the patient’s age at the time of HBV acquisition and the patient’s immune status. Fewer than 5% of immunocompetent adults infected with HBV remain chronically infected, defined as being positive for HBV surface antigen for more than 6 months. On the other hand, 80% to 90% of infected infants and about 20% to 50% of children 1 to 5 years old at the time of acute infection remain chronically infected.21

 

 

Four phases of chronic HBV infection

Four phases of chronic HBV infection have been outlined (Table 2),30 although all patients do not go through all phases. HBV surface antigen is detectable in all of them.

The immune tolerance phase, the initial phase of chronic HBV infection, is seen almost exclusively in those who acquired HBV infection vertically or during early childhood. Although patients have high HBV DNA levels, they do not have significant liver disease. This discrepancy is thought to be related to the immune tolerance to HBV; however, the exact mechanism of that tolerance is unclear.31

Only 15% of those with immune tolerance have spontaneous HBV e antigen seroconversion (ie, loss of e antigen and appearance of anti-e antibody) within 20 years after infection. 32

The immune clearance phase (HBV e antigen-positive chronic hepatitis) appears about 20 to 30 years after the onset of the immune tolerance phase in patients who acquire HBV early in life. It is also often seen in patients with infections acquired late in childhood or in adulthood.

This phase marks the start of an immunemediated process aimed at clearing the viral infection, but it also leads to concomitant hepatocellular injury. Spontaneous clearance of the e antigen increases in this phase to an annual rate of 10% to 20%.32,33 The strongest predictors of spontaneous e antigen seroconversion are old age, an elevated ALT level, and an acute exacerbation.26

Although ALT levels are elevated and there is evidence on liver biopsy of chronic active hepatitis, this phase is usually asymptomatic. Rarely, however, it presents with an acute flare of hepatitis, sometimes accompanied by IgM antibodies against the HBV core antigen (in low titer), leading to an incorrect diagnosis of acute HBV infection.

Depending on the duration of the chronic hepatitis and the frequency and severity of flares, about 12% to 20% of patients in the immune-clearance phase develop serious liver disease within 5 years.31

The inactive carrier phase following HBV e antigen seroconversion is characterized by undetectable or low HBV DNA levels (< 1,000 copies/mL), normal ALT levels, and minimal or no necroinflammation on liver biopsy. 30 Such patients should be followed with serial testing, as 4% to 20% of them spontaneously revert to being positive for e antigen at least once.16 On the other hand, only 0.5% to 2% of surface antigen carriers in western countries clear themselves of surface antigen yearly, but up to half of those who clear the surface antigen have low-level HBV viremia. 34

The reactivation phase (HBV e antigennegative chronic hepatitis) is seen in some HBV-infected patients, especially those from Asia and southern Europe, in whom the virus has a spontaneous pre-core or core mutation that makes infected cells unable to secrete the e antigen. Although these patients have no e antigen in their blood, they do have intermittent or persistent elevation of ALT, elevated HBV DNA, and histopathologic findings of chronic hepatitis. Compared with those in the immune clearance phase, patients in the reactivation phase tend to be older and to have lower HBV DNA levels but advanced hepatic damage.

Immunity to HBV infection is characterized by loss of HBV surface antigen, DNA, e antigen, and anti-core antigen IgM with development of anti-surface antigen antibody and anti-core antigen IgG (total anti-core antigen antibody). The presence of anti-surface antigen antibody and anti-core antigen IgG together differentiates natural immunity through resolved infection from that which is acquired through vaccination, which is denoted by isolated anti-surface antigen antibody.

Figure 2 illustrates the typical serologic course of HBV infection, and Table 3 summarizes how to interpret the various serologic patterns.

Cirrhosis, liver failure, cancer

Cirrhosis, hepatic decompensation, and hepatocellular carcinoma are the major long-term complications of HBV infection. In untreated patients, the annual rate of progression to cirrhosis has been estimated to be 2% to 6% in patients with HBV e antigen-positive chronic hepatitis and 8% to 9% in those with e antigen- negative chronic hepatitis.30

The likely explanation for these surprising cirrhosis rates is that e antigen-negative chronic hepatitis usually represents a late stage of the disease, and patients in this phase are usually older and have more advanced liver disease.

Subsequently, the annual rate of progression from compensated cirrhosis to hepatic decompensation has been estimated to be about 5%.35

Across all the stages described above, a high serum HBV DNA level has been shown to be a strong predictor of progression to cirrhosis in patients with chronic HBV infection. In a population-based prospective cohort study of 3,582 untreated HBV-infected patients in Taiwan, Iloeje et al36 found that, compared with patients with serum HBV DNA levels lower than 104 copies/mL, those with levels of 104 or higher had an adjusted relative risk of cirrhosis of 2.5. The relative risk rose to 5.9 with HBV DNA levels of 105 or higher, and 9.8 with levels of 106 copies/mL or higher. More studies in different patient populations are needed for confirmation.

HBV is a strong carcinogen, and the risk of hepatocellular carcinoma is 100 times higher in patients with HBV infection than in uninfected ones.31

The most important risk factor for hepatocellular carcinoma in HBV-infected patients is cirrhosis, but this cancer can also develop in noncirrhotic livers.37 The annual rate of hepatocelluar carcinoma has been estimated to be higher (2.5%–3%) in patients with cirrhosis than in noncirrhotic carriers (0.5%–1%).30,35–38 Risk factors for cirrhosis and hepatocellular carcinoma are summarized in Table 4.16,30

Our knowledge about hepatitis B and related diseases has dramatically increased since the discovery of the causative virus, HBV, in 1963. Despite effective vaccination, hepatitis B still constitutes a major public health problem.

In two parts, this comprehensive review will highlight a practical clinical approach to HBV infection. In this first part, we discuss the epidemiology, natural history, and diagnosis of HBV infection. In the second part, to be published in the next issue of this journal, we will review the general principles of its management, its management in patients on immunosuppressant therapy and in pregnant women, and HBV vaccination.

COMMON IN ASIA, LESS SO IN AMERICA

More than 2 billion people—one-third of the world’s population—alive today have been infected with HBV at some time in their life, and of these, about 350 million remain infected.1 Every year, 1 million people die of HBV-related cirrhosis or hepatocellular carcinoma, which means that HBV takes a life every 30 seconds.2

World Health Organization. Introduction of hepatitis B vaccine into childhood immunization services. Geneva: WHO; 2001. WHO/V AND B/01.31.
Figure 1. Global prevalence of hepatitis B virus (HBV) surface antigenemia.
HBV infection is highly prevalent in Asia, sub-Saharan Africa, and other parts of the developing world, but less so in the United States, except in Alaskan natives and immigrants from regions of high prevalence (Figure 1). By some estimates, 1.25 million carriers, defined as those positive for the HBV surface antigen for more than 6 months, live in the United States, and about half of them are Asian-American.3,4 Other estimates put the number as high as 2 million, taking into account the prevalence of HBV in immigrant populations.

The incidence of acute hepatitis B in the United States has declined from 8.5 per 100,000 population in 1990 to 2.1 per 100,000 population in 2004, with the greatest declines (94%) in children and adolescents, coincident with an increase in hepatitis B vaccination in these age groups.5 Despite these advances, HBV still causes a considerable number of cases of cirrhosis, cancer, and death—about 5,000 deaths each year in the United States.

HBV HAS FOUR GENES, EIGHT GENOTYPES

HBV is a DNA virus of the Hepadnaviridae family. Its genome is double-stranded with four genes, each one encoding a specific structural protein or proteins6,7:

  • S gene, for the viral envelope (surface antigen)
  • C gene, for both the nucleocapsid (core) antigen and the pre-core (e) antigen
  • X gene, for two regulatory proteins required for HBV replication
  • P gene, for DNA polymerase.

Several clinically important mutations in the HBV genome are known (Table 1).7–12

Eight genotypes of HBV (labeled A though H) have been identified.13,14 All eight have been found in the United States, but genotype A accounts for 35% of cases, genotype B for 22%, and genotype C for 31%.15

The clinical significance of HBV genotypes is not as clear as that of hepatitis C virus genotypes. Although recent data have suggested that different HBV genotypes may be associated with different rates of progression of liver disease and different rates of response to interferon therapy,13 these data were not enough to recommend routine testing for HBV genotypes in clinical practice.16

In HBV infection, the virus itself does not injure liver cells. Rather, the damage of hepatitis is immune-mediated and begins to appear as the host’s immune system attempts to clear the virus.

MARKERS OF HBV INFECTION

Figure 2.
HBV produces several antigens that can be detected in the blood and that disappear as the body produces antibodies against them. The patterns of these and other markers provide clues to the phase of infection (Figure 2).

HBV surface antigen and HBV DNA are often the first detectable markers of acute infection, appearing before the onset of symptoms or before elevation of alanine aminotransferase (ALT) occurs. By definition, an HBV infection is chronic if surface antigen persists longer than 6 months.

HBV e antigen, derived from pre-core protein, is considered a marker of HBV replication and infectivity. In chronic infection, e antigen can persist for years or decades.

HBV core antigen cannot be detected in the serum, but antibodies against it can, first immunoglobulin M (IgM) and later immunoglobulin G (IgG).

TRANSMISSION: VERTICAL OR HORIZONTAL

Because HBV replicates profusely and produces high titers in the blood (108 to 1,010 virions/ mL), any parenteral or mucosal exposure to infected blood poses a high risk of HBV acquisition. The risk of HBV transmission from a single needlestick is 1% to 6% if the blood is positive for HBV surface antigen but negative for HBV e antigen, and 22% to 40% if positive for both antigens.17–19 Saliva, nasopharyngeal fluid, breast milk, semen, urine, and cervical secretions can also harbor HBV.20

Worldwide, perinatal (vertical) transmission is the predominant mode of HBV transmission, whereas intravenous drug abuse and unprotected sexual intercourse are the main routes of infection in areas of low prevalence, such as the United States. In sub-Saharan Africa, Alaska, and Mediterranean countries, transmission of HBV usually occurs horizontally during childhood, presumably via contact with nonintact skin.21–24 Saliva has also been thought to be the route of HBV transmission in sporadic cases through human bites.25

People at risk of HBV infection include:

  • Parenteral drug users
  • People with multiple sexual partners
  • Household contacts and sexual partners of people who are 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.

These people—as well as all pregnant women, patients infected with hepatitis C virus or human immunodeficiency virus, and patients with chronically elevated ALT or aspartate aminotransferase (AST) levels—should be screened for HBV infection with serologic markers.

 

 

CLINICAL MANIFESTATIONS VARY

HBV infection, acute or chronic, has variable manifestations. During the acute stage, HBV infection can manifest as anicteric (subclinical) hepatitis, icteric hepatitis, or, rarely, acute fulminant hepatitis. Chronic HBV infection can be asymptomatic (the HBV surface antigen carrier state), or it can be manifested by symptoms and signs of cirrhosis or hepatocellular carcinoma or both. Extrahepatic manifestations, including serum sickness, polyarteritis nodosa, essential mixed cryoglobulinemia, membranous glomerulonephritis, and aplastic anemia, have been reported in patients with HBV infection.26

Acute hepatitis B

The incubation period of HBV ranges from 2 weeks to 4 months. Initially, patients complain of fatigue, malaise, anorexia, right upper quad-rant discomfort, or flu-like symptoms (coryza, photophobia, headache, and myalgia); then jaundice becomes apparent, usually within 10 days of the onset of symptoms. Low-grade fever, jaundice, and mildly tender hepatomegaly are the most common signs. Generalized lymphadenopathy is not a feature of acute HBV infection. If the patient also has hepatitis D virus infection or underlying liver disease (eg, alcoholic liver disease), then acute HBV infection may be more severe.

In the acute phase, ALT and AST levels rise, sometimes to values above 1,000 IU/L. In icteric hepatitis, bilirubin levels also rise, usually after the ALT level does. Although the peak ALT level reflects the hepatocellular injury, it has no prognostic value. With recovery, ALT levels normalize in 1 to 4 months.

Acute fulminant hepatitis B occurs in 0.1% to 0.5% of patients, and causes about 10% of cases of acute liver failure in the United States.27 Patients typically present with rapidly progressive acute hepatitis characterized by signs of liver failure, such as coagulopathy, encephalopathy, and cerebral edema.

In the so-called window phase, laboratory testing may not reveal HBV surface antigen because of early clearance but shows IgM antibody against the HBV core antigen. HBV DNA may be low or undetected.

Chronic hepatitis B

Chronic hepatitis B is usually diagnosed as a result of a workup for abnormal liver function tests or as a result of screening patients at risk for HBV infection. Many patients with chronic hepatitis B have no symptoms or have nonspecific symptoms such as fatigue or right upper quadrant discomfort.

Acute exacerbations due to HBV e antigen seroreversion (ie, in which e antigen reappears) occasionally occur in patients with chronic hepatitis B. Most of these exacerbations are asymptomatic, but occasionally an acute hepatitis-like clinical picture with detectable IgM antibody against the core antigen occurs, leading to misdiagnosis of acute HBV infection in patients not previously known to have chronic HBV infection.28

In late cases, signs of cirrhosis such as jaundice, ascites, splenomegaly, pedal edema, encephalopathy, or variceal bleeding can be present.

Hepatocellular carcinoma should be suspected in cirrhotic patients with new-onset right upper quadrant pain, rapidly developing ascites, a palpable liver mass, or hepatic encephalopathy. Other nonspecific features of hepatocellular carcinoma include watery diarrhea, hypoglycemia, and certain cutaneous manifestations such as acanthosis nigricans and the Leser-Trelat sign (multiple pruritic seborrheic keratoses of sudden onset).

In chronic hepatitis B, liver enzyme levels can be normal, even in patients with wellcompensated cirrhosis. ALT levels may range from normal to five times higher than normal. Thrombocytopenia, hypoalbuminemia, direct hyperbilirubinemia, and prolonged prothrombin time suggest cirrhosis.

Findings of chronic hepatitis B on liver biopsy range from minimal inflammation to cirrhosis. The most characteristic histologic feature of chronic HBV infection is the “ground-glass hepatocyte,” which is due to intracellular accumulation of HBV surface antigen. 29

FEW ADULTS (BUT MANY CHILDREN) REMAIN CHRONICALLY INFECTED

Figure 3. Natural history of HBV infection.
The natural history of HBV infection has become better defined, thanks to extensive epidemiologic studies and highly sensitive HBV DNA assays (Figure 3). It is crucial for clinicians to understand the natural history of HBV infection to appropriately decide which infected patients need antiviral therapy. This will be discussed in our second article.

HBV surface antigen can be detected in the blood approximately 2 to 4 weeks after inoculation. Simultaneously, HBV DNA, usually in very high levels, is also detectable in the blood. However, in the rare cases of acute fulminant hepatitis, HBV DNA levels can be low or undetectable at the time of presentation because the immune system mounts a robust response with extensive damage to HBVinfected hepatocytes.

The rate of spontaneous recovery from acute HBV infection varies, depending on the patient’s age at the time of HBV acquisition and the patient’s immune status. Fewer than 5% of immunocompetent adults infected with HBV remain chronically infected, defined as being positive for HBV surface antigen for more than 6 months. On the other hand, 80% to 90% of infected infants and about 20% to 50% of children 1 to 5 years old at the time of acute infection remain chronically infected.21

 

 

Four phases of chronic HBV infection

Four phases of chronic HBV infection have been outlined (Table 2),30 although all patients do not go through all phases. HBV surface antigen is detectable in all of them.

The immune tolerance phase, the initial phase of chronic HBV infection, is seen almost exclusively in those who acquired HBV infection vertically or during early childhood. Although patients have high HBV DNA levels, they do not have significant liver disease. This discrepancy is thought to be related to the immune tolerance to HBV; however, the exact mechanism of that tolerance is unclear.31

Only 15% of those with immune tolerance have spontaneous HBV e antigen seroconversion (ie, loss of e antigen and appearance of anti-e antibody) within 20 years after infection. 32

The immune clearance phase (HBV e antigen-positive chronic hepatitis) appears about 20 to 30 years after the onset of the immune tolerance phase in patients who acquire HBV early in life. It is also often seen in patients with infections acquired late in childhood or in adulthood.

This phase marks the start of an immunemediated process aimed at clearing the viral infection, but it also leads to concomitant hepatocellular injury. Spontaneous clearance of the e antigen increases in this phase to an annual rate of 10% to 20%.32,33 The strongest predictors of spontaneous e antigen seroconversion are old age, an elevated ALT level, and an acute exacerbation.26

Although ALT levels are elevated and there is evidence on liver biopsy of chronic active hepatitis, this phase is usually asymptomatic. Rarely, however, it presents with an acute flare of hepatitis, sometimes accompanied by IgM antibodies against the HBV core antigen (in low titer), leading to an incorrect diagnosis of acute HBV infection.

Depending on the duration of the chronic hepatitis and the frequency and severity of flares, about 12% to 20% of patients in the immune-clearance phase develop serious liver disease within 5 years.31

The inactive carrier phase following HBV e antigen seroconversion is characterized by undetectable or low HBV DNA levels (< 1,000 copies/mL), normal ALT levels, and minimal or no necroinflammation on liver biopsy. 30 Such patients should be followed with serial testing, as 4% to 20% of them spontaneously revert to being positive for e antigen at least once.16 On the other hand, only 0.5% to 2% of surface antigen carriers in western countries clear themselves of surface antigen yearly, but up to half of those who clear the surface antigen have low-level HBV viremia. 34

The reactivation phase (HBV e antigennegative chronic hepatitis) is seen in some HBV-infected patients, especially those from Asia and southern Europe, in whom the virus has a spontaneous pre-core or core mutation that makes infected cells unable to secrete the e antigen. Although these patients have no e antigen in their blood, they do have intermittent or persistent elevation of ALT, elevated HBV DNA, and histopathologic findings of chronic hepatitis. Compared with those in the immune clearance phase, patients in the reactivation phase tend to be older and to have lower HBV DNA levels but advanced hepatic damage.

Immunity to HBV infection is characterized by loss of HBV surface antigen, DNA, e antigen, and anti-core antigen IgM with development of anti-surface antigen antibody and anti-core antigen IgG (total anti-core antigen antibody). The presence of anti-surface antigen antibody and anti-core antigen IgG together differentiates natural immunity through resolved infection from that which is acquired through vaccination, which is denoted by isolated anti-surface antigen antibody.

Figure 2 illustrates the typical serologic course of HBV infection, and Table 3 summarizes how to interpret the various serologic patterns.

Cirrhosis, liver failure, cancer

Cirrhosis, hepatic decompensation, and hepatocellular carcinoma are the major long-term complications of HBV infection. In untreated patients, the annual rate of progression to cirrhosis has been estimated to be 2% to 6% in patients with HBV e antigen-positive chronic hepatitis and 8% to 9% in those with e antigen- negative chronic hepatitis.30

The likely explanation for these surprising cirrhosis rates is that e antigen-negative chronic hepatitis usually represents a late stage of the disease, and patients in this phase are usually older and have more advanced liver disease.

Subsequently, the annual rate of progression from compensated cirrhosis to hepatic decompensation has been estimated to be about 5%.35

Across all the stages described above, a high serum HBV DNA level has been shown to be a strong predictor of progression to cirrhosis in patients with chronic HBV infection. In a population-based prospective cohort study of 3,582 untreated HBV-infected patients in Taiwan, Iloeje et al36 found that, compared with patients with serum HBV DNA levels lower than 104 copies/mL, those with levels of 104 or higher had an adjusted relative risk of cirrhosis of 2.5. The relative risk rose to 5.9 with HBV DNA levels of 105 or higher, and 9.8 with levels of 106 copies/mL or higher. More studies in different patient populations are needed for confirmation.

HBV is a strong carcinogen, and the risk of hepatocellular carcinoma is 100 times higher in patients with HBV infection than in uninfected ones.31

The most important risk factor for hepatocellular carcinoma in HBV-infected patients is cirrhosis, but this cancer can also develop in noncirrhotic livers.37 The annual rate of hepatocelluar carcinoma has been estimated to be higher (2.5%–3%) in patients with cirrhosis than in noncirrhotic carriers (0.5%–1%).30,35–38 Risk factors for cirrhosis and hepatocellular carcinoma are summarized in Table 4.16,30

References
  1. World Health Organization. Hepatitis B. www.who.int/csr/disease/hepatitis/whocdscsrlyo20022/en. Accessed 11/10/2008.
  2. Center for Disease Control and Prevention. HBV a silent killer. www.cdc.gov/ncidod/diseases/hepatitis/b/hbv_silent_killer. Accessed 2/19/2007.
  3. McQuillan GM, Coleman PJ, Kruszon-Moran D, Moyer LA, Lambert SB, Margolis HS. Prevalence of hepatitis B virus infection in the United States: the National Health and Nutrition Examination Surveys, 1976 through 1994. Am J Public Health 1999; 89:1418.
  4. Armstrong GL, Mast EE, Wojczynski M, Margolis HS. Childhood hepatitis B virus infections in the United States before hepatitis B immunization. Pediatrics 2001; 108:11231128.
  5. 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 Dec 8; 55(RR-16):133.
  6. Gish RG, Gadano AC. Chronic hepatitis B: current epidemiology in the Americas and implications for management. J Viral Hepatol 2006; 13:787798.
  7. Wei Y, Tiollais PK. Molecular biology of hepatitis B virus. Clin Liver Dis 1999; 3:189219.
  8. Seeger C, Mason WS. Hepatitis B virus biology. Microbiol Mol Biol Rev 2000; 64:5168.
  9. Hunt CM, McGill JM, Allen MI, Condreay LD. Clinical relevance of hepatitis B viral mutations. Hepatology 2000; 3:10371044.
  10. Allen MI, Deslauriers M, Andrews CW, et al. Identification and characterization of mutations in hepatitis B virus resistant to lamivudine. Lamivudine Clinical Investigation Group. Hepatology 1998; 27:16701677.
  11. Hadziyannis SJ, Vassilopoulos D. Hepatitis B e antigen- negative chronic hepatitis B. Hepatology 2001; 34:617624.
  12. Wai CT, Fontana RJ. Clinical significance of hepatitis B virus genotypes, variants, and mutants. Clin Liver Dis 2004; 8:321352.
  13. Fung SK, Lok AS. Hepatitis B virus genotypes: do they play a role in the outcome of HBV infection? Hepatology 2004; 40:790792.
  14. Norder H, Courouce AM, Coursaget P, et al. Genetic diversity of hepatitis B virus strains derived worldwide: genotypes, subgenotypes, and HBsAg subtypes. Intervirology 2004; 47:289309.
  15. Chu CJ, Keeffe EB, Han SH, et al. Hepatitis B virus genotypes in the United States: results of a nationwide study. Gastroenterology 2003; 125:444451.
  16. Lok AS, McMahon BJ. Chronic hepatitis B. Hepatology 2007; 45:507539.
  17. Mast EE, Alter MJ. Prevention of hepatitis B virus infection among health-care workers. In:Ellis RE, editor. Hepatitis B Vaccines in Clinical Practice. New York: Marcel Dekker, 1993:295307.
  18. Werner BG, Grady GF. Accidental hepatitis-B-surface-antigen-positive inoculations: use of e antigen to estimate infectivity. Ann Intern Med 1982; 97:367369.
  19. Gerberding JL. Management of occupational exposures to blood-borne viruses. N Engl J Med 1995; 332:444451.
  20. Kidd-Ljunggren K, Holmberg A, Blackberg J, Lindqvist B. High levels of hepatitis B virus DNA in body fluids from chronic carriers. J Hosp Infect 2006; 64:352357.
  21. McMahon BJ, Alward WL, Hall DB, et al. Acute hepatitis B virus infection: relation of age to the clinical expression of disease and subsequent development of the carrier state. J Infect Dis 1985; 151:599603.
  22. Dusheiko GM, Brink BA, Conradie JD, Marimuthu T, Sher R. Regional prevalence of hepatitis B, delta, and human immunodeficiency virus infection in southern Africa: a large population survey. Am J Epidemiol 1989; 129:13845.
  23. Bortolotti F, Guido M, Bartolacci S, et al. Chronic hepatitis B in children after e antigen seroclearance: final report of a 29-year longitudinal study. Hepatology 2006; 43:556562.
  24. Moreno MR, Otero M, Millan A, et al. Clinical and histological outcome after hepatitis B e antigen to antibody seroconversion in children with chronic hepatitis B. Hepatology 1999:572575.
  25. Hui AY, Hung LC, Tse PC, Leung WK, Chan PK, Chan HL. Transmission of hepatitis B by human bite--confirmation by detection of virus in saliva and full genome sequencing. J Clin Virol 2005; 33:254256.
  26. Cacoub P, Saadoun D, Bourlière M, et al. Hepatitis B virus genotypes and extrahepatic manifestations. J Hepatol 2005; 43:764770.
  27. Schiodt FV, Atillasoy E, Shakil AO, et al. Etiology and outcome for 295 patients with acute liver failure in the United States. Liver Transplant Surg 1999; 5:2934.
  28. Chu CM, Liaw YF, Pao CC, Huang MJ. The etiology of acute hepatitis superimposed upon previously unrecognized asymptomatic HBsAg carriers. Hepatology 1989; 9:452456.
  29. Gerber MA, Hadziyannis S, Vissoulis C, et al. Electron microscopy and immunoelectronmicroscopy of cytoplasmic hepatitis B antigen in hepatocytes. Am J Pathol 1974; 75:489502.
  30. Yim HJ, Lok AS. Natural history of chronic hepatitis B virus infection: what we knew in 1981 and what we know in 2005. Hepatology 2006; 43:S173S181.
  31. Pungpapong S, Kim WR, Poterucha JJ. Natural history of hepatitis B virus infection: an update for clinicians. Mayo Clin Proc 2007; 82:967975.
  32. Lok AS, Lai CL, Wu PC, Leung EK, Lam TS. Spontaneous hepatitis B e antigen to antibody seroconversion and reversion in Chinese patients with chronic hepatitis B virus infection. Gastroenterology 1987; 92:18391843.
  33. McMahon BJ, Holck P, Bulkow L, Snowball M. Serologic and clinical outcomes in 1536 Alaska Natives chronically infected with hepatitis B virus. Ann Intern Med 2001; 135:759768.
  34. McMahon BJ. Epidemiology and natural history of hepatitis B. Semin Liver Dis 2005; 25( suppl 1):38.
  35. Benvegnu L, Gios M, Boccato S, Alberti A. Natural history of compensated viral cirrhosis: a prospective study on the incidence and hierarchy of major complications. Gut 2004; 53:744749.
  36. Iloeje UH, Yang HI, Su J, Jen CL, You SL, Chen CJ. Risk evaluation of viral load elevation and associated liver disease/cancer in HBV. The REVEAL-HBV Study Group. Predicting cirrhosis risk based on the level of circulating hepatitis B viral load. Gastroenterology 2006; 130:678686.
  37. Bosch FX, Ribes J, Cleries R, Diaz M. Epidemiology of hepatocellular carcinoma. Clin Liver Dis 2005; 9:191211.
  38. Fattovich G. Natural history of hepatitis B. J Hepatol 2003; 39:S50S58.
References
  1. World Health Organization. Hepatitis B. www.who.int/csr/disease/hepatitis/whocdscsrlyo20022/en. Accessed 11/10/2008.
  2. Center for Disease Control and Prevention. HBV a silent killer. www.cdc.gov/ncidod/diseases/hepatitis/b/hbv_silent_killer. Accessed 2/19/2007.
  3. McQuillan GM, Coleman PJ, Kruszon-Moran D, Moyer LA, Lambert SB, Margolis HS. Prevalence of hepatitis B virus infection in the United States: the National Health and Nutrition Examination Surveys, 1976 through 1994. Am J Public Health 1999; 89:1418.
  4. Armstrong GL, Mast EE, Wojczynski M, Margolis HS. Childhood hepatitis B virus infections in the United States before hepatitis B immunization. Pediatrics 2001; 108:11231128.
  5. 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 Dec 8; 55(RR-16):133.
  6. Gish RG, Gadano AC. Chronic hepatitis B: current epidemiology in the Americas and implications for management. J Viral Hepatol 2006; 13:787798.
  7. Wei Y, Tiollais PK. Molecular biology of hepatitis B virus. Clin Liver Dis 1999; 3:189219.
  8. Seeger C, Mason WS. Hepatitis B virus biology. Microbiol Mol Biol Rev 2000; 64:5168.
  9. Hunt CM, McGill JM, Allen MI, Condreay LD. Clinical relevance of hepatitis B viral mutations. Hepatology 2000; 3:10371044.
  10. Allen MI, Deslauriers M, Andrews CW, et al. Identification and characterization of mutations in hepatitis B virus resistant to lamivudine. Lamivudine Clinical Investigation Group. Hepatology 1998; 27:16701677.
  11. Hadziyannis SJ, Vassilopoulos D. Hepatitis B e antigen- negative chronic hepatitis B. Hepatology 2001; 34:617624.
  12. Wai CT, Fontana RJ. Clinical significance of hepatitis B virus genotypes, variants, and mutants. Clin Liver Dis 2004; 8:321352.
  13. Fung SK, Lok AS. Hepatitis B virus genotypes: do they play a role in the outcome of HBV infection? Hepatology 2004; 40:790792.
  14. Norder H, Courouce AM, Coursaget P, et al. Genetic diversity of hepatitis B virus strains derived worldwide: genotypes, subgenotypes, and HBsAg subtypes. Intervirology 2004; 47:289309.
  15. Chu CJ, Keeffe EB, Han SH, et al. Hepatitis B virus genotypes in the United States: results of a nationwide study. Gastroenterology 2003; 125:444451.
  16. Lok AS, McMahon BJ. Chronic hepatitis B. Hepatology 2007; 45:507539.
  17. Mast EE, Alter MJ. Prevention of hepatitis B virus infection among health-care workers. In:Ellis RE, editor. Hepatitis B Vaccines in Clinical Practice. New York: Marcel Dekker, 1993:295307.
  18. Werner BG, Grady GF. Accidental hepatitis-B-surface-antigen-positive inoculations: use of e antigen to estimate infectivity. Ann Intern Med 1982; 97:367369.
  19. Gerberding JL. Management of occupational exposures to blood-borne viruses. N Engl J Med 1995; 332:444451.
  20. Kidd-Ljunggren K, Holmberg A, Blackberg J, Lindqvist B. High levels of hepatitis B virus DNA in body fluids from chronic carriers. J Hosp Infect 2006; 64:352357.
  21. McMahon BJ, Alward WL, Hall DB, et al. Acute hepatitis B virus infection: relation of age to the clinical expression of disease and subsequent development of the carrier state. J Infect Dis 1985; 151:599603.
  22. Dusheiko GM, Brink BA, Conradie JD, Marimuthu T, Sher R. Regional prevalence of hepatitis B, delta, and human immunodeficiency virus infection in southern Africa: a large population survey. Am J Epidemiol 1989; 129:13845.
  23. Bortolotti F, Guido M, Bartolacci S, et al. Chronic hepatitis B in children after e antigen seroclearance: final report of a 29-year longitudinal study. Hepatology 2006; 43:556562.
  24. Moreno MR, Otero M, Millan A, et al. Clinical and histological outcome after hepatitis B e antigen to antibody seroconversion in children with chronic hepatitis B. Hepatology 1999:572575.
  25. Hui AY, Hung LC, Tse PC, Leung WK, Chan PK, Chan HL. Transmission of hepatitis B by human bite--confirmation by detection of virus in saliva and full genome sequencing. J Clin Virol 2005; 33:254256.
  26. Cacoub P, Saadoun D, Bourlière M, et al. Hepatitis B virus genotypes and extrahepatic manifestations. J Hepatol 2005; 43:764770.
  27. Schiodt FV, Atillasoy E, Shakil AO, et al. Etiology and outcome for 295 patients with acute liver failure in the United States. Liver Transplant Surg 1999; 5:2934.
  28. Chu CM, Liaw YF, Pao CC, Huang MJ. The etiology of acute hepatitis superimposed upon previously unrecognized asymptomatic HBsAg carriers. Hepatology 1989; 9:452456.
  29. Gerber MA, Hadziyannis S, Vissoulis C, et al. Electron microscopy and immunoelectronmicroscopy of cytoplasmic hepatitis B antigen in hepatocytes. Am J Pathol 1974; 75:489502.
  30. Yim HJ, Lok AS. Natural history of chronic hepatitis B virus infection: what we knew in 1981 and what we know in 2005. Hepatology 2006; 43:S173S181.
  31. Pungpapong S, Kim WR, Poterucha JJ. Natural history of hepatitis B virus infection: an update for clinicians. Mayo Clin Proc 2007; 82:967975.
  32. Lok AS, Lai CL, Wu PC, Leung EK, Lam TS. Spontaneous hepatitis B e antigen to antibody seroconversion and reversion in Chinese patients with chronic hepatitis B virus infection. Gastroenterology 1987; 92:18391843.
  33. McMahon BJ, Holck P, Bulkow L, Snowball M. Serologic and clinical outcomes in 1536 Alaska Natives chronically infected with hepatitis B virus. Ann Intern Med 2001; 135:759768.
  34. McMahon BJ. Epidemiology and natural history of hepatitis B. Semin Liver Dis 2005; 25( suppl 1):38.
  35. Benvegnu L, Gios M, Boccato S, Alberti A. Natural history of compensated viral cirrhosis: a prospective study on the incidence and hierarchy of major complications. Gut 2004; 53:744749.
  36. Iloeje UH, Yang HI, Su J, Jen CL, You SL, Chen CJ. Risk evaluation of viral load elevation and associated liver disease/cancer in HBV. The REVEAL-HBV Study Group. Predicting cirrhosis risk based on the level of circulating hepatitis B viral load. Gastroenterology 2006; 130:678686.
  37. Bosch FX, Ribes J, Cleries R, Diaz M. Epidemiology of hepatocellular carcinoma. Clin Liver Dis 2005; 9:191211.
  38. Fattovich G. Natural history of hepatitis B. J Hepatol 2003; 39:S50S58.
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KEY POINTS

  • HBV infection is much more likely to persist and become chronic if it is acquired at birth or in early childhood rather than during adulthood.
  • Chronic HBV infection is defined as persistence of HBV surface antigen in the serum for more than 6 months.
  • Although many cases of chronic HBV infection resolve spontaneously, some progress to cirrhosis, hepatocellular carcinoma, and death.
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Bisphosphonates and osteonecrosis of the jaw: Innocent association or significant risk?

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Bisphosphonates and osteonecrosis of the jaw: Innocent association or significant risk?

Recent case reports have linked bisphosphonate drugs to osteonecrosis of the jaw, and these reports have been widely publicized. Many patients receiving these drugs are asking their dentists and doctors whether the drugs do more harm than good, and some have even stopped taking them against medical advice. Health care professionals may be unsure what to tell patients and may be fearful of litigation.

However, most of the cases reported were in cancer patients, who are at significantly higher risk of osteonecrosis of the jaw for several reasons, and who receive much higher doses of bisphosphonates than do patients with osteoporosis or Paget disease of bone.

Moreover, although case reports have clearly documented an association between these drugs and osteonecrosis of the jaw, there is a lack of robust scientific evidence to support a cause-and-effect relationship. In fact, wellcontrolled clinical studies have not shown an increased risk of this complication in patients with osteoporosis or Paget disease of bone who were exposed to these agents, nor have they elucidated definite pathogenic mechanisms by which it might occur.

For these reasons, we believe that patients with osteoporosis should be advised of:

  • Their risk of fracture
  • The significant risk of morbidity and death following such a fracture
  • The effectiveness and excellent safety of bisphosphonate therapy in preventing fractures
  • The evidence that such therapy for osteoporosis and Paget disease poses little or no risk of osteonecrosis of the jaw
  • The need for further research.

WHAT IS OSTEONECROSIS OF THE JAW?

Osteonecrosis—a general loss of bone tissue as a result of cell death1—can occur at any skeletal site, but it typically involves the long bones, ie, the femur, tibia, and humerus.

Osteonecrosis of the jaw is a rare disorder characterized by exposure and loss of bone in the maxillofacial complex. It can result in significant morbidity and can be resistant or refractory to conventional therapy.

This condition is not new, having been described in 19th century factory workers exposed to white phosphorus used in matchstick manufacturing. Known then as “phossy jaw,” it was associated with poor dentition and often resulted in severe disfigurement, disease, and death. Use of white phosphorus, and matches containing it, were subsequently banned in many countries.2

In the early 20th century, radiation therapy for cancers of the head and neck area came into vogue, but its side effects included damage to the skeleton, or osteoradionecrosis.3 In 1950, LaDow4 described a case of osteoradionecrosis of the jaw and reviewed the literature available at that time. He concluded that there were three main causes of osteonecrosis of the jaw, namely, radiation therapy, trauma, and infection.

Although many such cases have since been reported in association with radiation therapy, chemotherapy, or both, and involvement of other skeletal sites is well described,5–8 the actual incidence of osteoradionecrosis in the general population remains unclear because no large epidemiologic studies to elucidate accurate numbers have been published.

BISPHOSPHONATE-ASSOCIATED OSTEONECROSIS OF THE JAW

Bisphosphonate-associated osteonecrosis of the jaw is a relatively new condition, having been first reported in three case series9–11 published in 2003 and 2004. The patients had exposure of areas of alveolar bone, mostly after oral surgery, eg, mucogingival flap elevation procedures (such as tooth extraction), that did not respond or were refractory to conventional treatment. All had received a bisphosphonate drug.

After these articles were published, the number of reported cases rose dramatically, including a case presented by one of us.12 By the end of January 2008, more than 500 papers on this condition were listed in PubMed. More than 60% had been printed since 2003, and approximately 85% concerned the association between osteonecrosis of the jaw and bisphosphonate use (search terms: “osteonecrosis of the jaw” and “bisphosphonate”).13

Although some dentists and oral surgeons claim to have seen many patients with this disorder, physicians who specialize in osteoporosis and metabolic bone disease do not. The medical literature and popular press have suggested that bisphosphonates are the cause of this malady. However, such articles are more perspective than evidence, as they are not scientific studies but rather reports of cases or series, or reviews of these. High-impact journals have given such articles prominent positions, highlighting the issue further, rather than balancing what is known and what is not known.

Thus, medicine safety boards, physicians, dentists, and oral surgeons have become increasingly concerned about the possible risk of this disorder in their patients on long-term bisphosphonate therapy, prompting organizations to issue management guidelines for this disorder and regulatory bodies to mandate warning labels on all drugs in this class about the possible risk.14–18 Funding agencies have highlighted this as an area in need of further investigation.17

However, robust evidence of a causal relationship is lacking. Contributing to the problem, other disorders can have similar presentations.

As a result, the diagnosis requires a dental examination and dental imaging, which are often impossible or impractical in a medical setting. Well-designed studies have relied on blinded panels of dental specialists using clinical and imaging data to adjudicate cases as osteonecrosis of the jaw before including them in published reports; case reports, however, often do not.

 

 

HOW IS OSTEONECROSIS OF THE JAW DIAGNOSED AND MANAGED?

A working definition of osteonecrosis of the jaw has recently emerged, and it will likely continue to evolve as results of further investigation become available.

A confirmed case is defined as an area of exposed bone in the maxillofacial region that does not heal within 8 weeks after being identified by a health care provider, in a patient who is currently receiving or has been exposed to a bisphosphonate and who has not had radiation therapy to the craniofacial region.14,17 This 8-week duration is consistent with the time frame in which soft tissue would be expected to close and exposed bone would be expected to heal under normal conditions after oral surgery such as dental extraction or a flap elevation procedure.

The working definition is one of inclusion and exclusion because the clinical presentation of osteonecrosis of the jaw is very similar to that of other diseases (Table 1).14,17 It is important for health professionals to understand this, since patients who have established osteonecrosis of the jaw or who are deemed to be at risk of it can also present with these other common clinical conditions that should not be confused with it.

Patients may have no symptoms at the time of presentation. However, symptoms can include oral or jaw pain, difficulty chewing, evidence of infection, and dental loss. Bone loss is often apparent radiographically, and it may be focal or generalized. Other imaging studies such as cone beam computed tomography provide greater detail on the extent and nature of the lesions, and thus provide a better assessment.

Histologically, there is evidence of necrosis, cell death, and, usually, concomitant infection.9–12,17

Management can be difficult

Osteonecrosis of the jaw can be difficult to manage, and extensive guidelines have been published.14–17 Its treatment is complicated because resection of the necrotic area often only makes the necrotic area bigger. Unlike in osteoradionecrosis, surgical removal of the affected area often results in necrosis at the margins of resected bone. This creates a potential situation of “chasing” affected bone in procedure after procedure, which results in significant morbidity.

Staging guidelines provide a framework for treatment (Table 2).14,16 Some case studies suggest that mucoperiosteal flap elevation procedures such as bone grafting, the use of bone morphogenic proteins, and alveolar bone decortication can succeed, but no randomized, placebo-controlled trials have been conducted. 19 Treatment with analgesics, antibiotics, surgery, and hyperbarbic oxygen may also be beneficial. Most authors have concluded that prevention is the ideal approach.14–20

A preventive protocol for cancer patients

Most of the cases reported so far have been in cancer patients receiving long-term treatment with potent bisphosphonates in high intravenous doses (12 times the usual dose for osteoporosis) after a mucoperiosteal flap elevation dental procedure (many of which were performed on an emergency basis).9–12,14–20 Authors have thus concluded that a preventive protocol should be followed for all patients being considered for intensive bisphosphonate treatment, similar to that adopted for patients receiving head and neck radiation.

Specifically, all chronic dental and periodontal conditions should be identified and stabilized before starting intensive bisphosphonate therapy. Experts today believe that controlling all chronic dental problems before starting intensive intravenous bisphosphonate therapy may be the best method to avoid dental surgery after bisphosphonate therapy has begun, particularly since the washout period (time to elimination of the drug) for bisphosphonates in alveolar bone is unknown.14–20

Although authors seem to agree that such a preventive protocol is prudent for intensive intravenous therapy, it does not appear to be necessary for patients without cancer.14,17 Indeed, such an approach is impractical, given the huge numbers involved and the lack of evidence to support it.

WHAT ARE BISPHOSPHONATES, AND WHY THE CONCERN?

Bisphosphonates are analogues of pyrophosphates, inorganic compounds developed to remove calcium carbonate from water in industrial pipes and laundry machines. Pyrophosphate use in humans arose from their affinity for calcium phosphate, which proved beneficial in scintigraphic imaging studies and in preventing tartar build-up, resulting in their incorporation into toothpastes. Modifications of the pyrophosphate molecule led to the development of diphosphonate compounds (later known as bisphosphonates), which have gained widespread use in treating a variety of disorders of the skeleton and of calcium metabolism.

These drugs prevent bone resorption by selectively inhibiting osteoclastic activity through several mechanisms (depending on the compound), thus helping prevent bone loss, bone pain, and hypercalcemia in diseases of the skeleton.

 

 

Bisphosphonates are widely used

Today, oral and intravenous bisphosphonates are widely prescribed for several skeletal disorders, including metastatic disease, malignant hypercalcemia, Paget disease of bone, and prevention and treatment of osteoporosis.21–23

More than 10 million Americans and more than 200 million people worldwide may have osteoporosis, which results in more than 1 million fractures each year. The lifetime risk of fracture for a postmenopausal white woman today is approximately 40% (approximately 15% for a 50-year-old man), and her annual risk of fracture is greater than her combined risk of stroke, heart attack, and breast cancer.22 Several bisphosphonates have been shown to safely and significantly reduce the risk of fracture in patients with osteoporosis and to be effective therapies for Paget disease of bone.24–31

Bisphosphonates are the most widely prescribed drugs for osteoporosis,22,23,29 with almost 200 million prescriptions for oral bisphosphonates worldwide. As of 2004, exposure to alendronate (Fosamax) was estimated to be about 20 million patient-years.32 Noncompliance limits their effectiveness in practice, due in part to concerns about adverse effects.

Since bisphosphonates are so widely prescribed, concern has been raised that they may be causing a new epidemic of osteonecrosis of the jaw.9 However, most reported cases have been in cancer patients, who are known to be at increased risk of this condition and who receive doses of bisphosphonates up to 12 times higher than in patients with osteoporosis or Paget disease of bone.9–12,33–38

The optimal duration of bisphosphonate therapy for these diseases to obtain the maximum benefit and minimize cost and harm remains unclear. Although a recent report suggests a bisphosphonate “drug holiday” may be an option when treating postmenopausal osteoporosis, larger, more robust studies of longer duration are needed.39 Outcomes of osteonecrosis of the jaw related to drug holidays have not been investigated.

‘IF I TAKE THIS TO STOP BONE LOSS, WILL IT HURT MY JAWS?’

The recently described association between bisphosphonates and osteonecrosis of the jaw has received considerable attention. Guidelines have been drawn up, some based on the assumption that bisphosphonates cause the osteonecrosis, but not based on scientific research.14–18 More than 90% of reported cases have been in cancer patients, a group known to be at increased risk of osteonecrosis of the jaw and other skeletal sites, for reasons that include radiation therapy, chemotherapy, corticosteroid use, and increased risk of infections.4,6,9–12,33–38 Nevertheless, it has been assumed that these patients are the same as osteoporosis patients, and sometimes that causation is beyond dispute. This is problematic for two main reasons:

  • Since noncompliance and lack of adherence (due to lack of knowledge about the dangers posed by osteoporosis, cost of the drugs, difficulty with dosing regimens, and fear of adverse effects) limit the effectiveness of these therapies in clinical practice, such attention has already persuaded patients to discontinue or refuse therapy (J.J. Carey, personal experience and communications from colleagues); and
  • Patients with osteoporosis and osteoporotic fractures have increased rates of morbidity and mortality and significantly higher fracture risk, which can be prevented with these agents if they are willing to take them.

Association does not prove causation

However, association does not prove causation. A relationship between a drug and a disease may be due to chance alone or to confounding factors.40 To judge the exact nature of this relationship, several issues need to be considered when reviewing the available evidence.

Substantiating that an agent causes a disease requires careful consideration of several aspects of their relationship: temporality, strength, dose-response, reversibility, consistency, biologic plausibility, and specificity.41 Correct interpretation of the strength of the evidence should also incorporate an evaluation of the study design, size, and reporting mechanism. Accordingly, case reports and case series are considered to constitute the weakest evidence, while randomized controlled trials and meta-analyses are usually considered the strongest.

When a true cause-and-effect relationship does exist, the situation can be a simple one in which only a single agent is involved. However, the issue can be decidedly more complex when the cause is an effect-modifier, requiring the interaction of additional factors.

When a cause has been assumed, demonstration of the dose-response relationship is also important: whether the risk is related in a continuous fashion to dose and duration of therapy (all patients), is seen only with particular doses or regimens (such as frequent use of high doses of potent bisphosphonates), or exists only in people who have passed a certain threshold value (for example, it may only occur in those who have received 0.5 g of an intravenous or 10 g of an oral bisphosphonate). Bearing in mind these considerations, the nature of the relationship between an agent and a disease can be better understood.40–43

A cause-and-effect relationship has not been established

A cause-and-effect relationship between bisphosphonates and osteonecrosis of the jaw has not been clearly established.14,17 Although case series highlight a relationship between the two, large controlled trials evaluating the occurrence of osteonecrosis of the jaw as the primary outcome have not been conducted. To date, most cases have been reported as uncontrolled case series, generally considered the weakest form of evidence.43

 

 

Most cases have been in cancer patients

Most cases of osteonecrosis of the jaw were in patients with cancer (particularly breast cancer and multiple myeloma) receiving potent intravenous bisphosphonates in high doses, most of whom had other documented risk factors, including recent dental procedures such as tooth extraction.9–12,15–19,33–38

One of the most compelling studies supporting causation examined the prevalence of osteonecrosis of the jaw in a cohort of 303 myeloma patients from 1991 to 2003. Osteonecrosis of the jaw developed only in those taking bisphosphonates (28 of 254), and the risk appeared greatest in those treated with both zoledronic acid (Zometa) and thalidomide (Thalomid). The importance of additional chemotherapies, concomitant diseases, and baseline dental pathology was not described.35 Biases, including channeling bias (in which patients who appear at increased risk of this rare condition also appear to be most likely to receive this medication), referral bias, and survivor bias, were not addressed in this paper or in others claiming that the risk is related to the type of bisphosphonate used and the duration of its use.15,33–38

A review of all cases of osteonecrosis of the jaw over a 5-year period in one institution (N = 163) found that only 17 (10%) were associated with bisphosphonate use, and all 17 patients had other risk factors, such as concomitant therapy for malignancy and recent dental surgery.34 The authors’ concern that longer follow-up may have shown a higher incidence of this problem is supported by the temporal relationship seen in other reports in which cancer patients with osteonecrosis of the jaw appear to have had higher cumulative doses of intravenous bisphosphonates than those without.9–12,15,34,35,37,38 Unfortunately, only one study had a control group to highlight the incidence of osteonecrosis of the jaw in similar patients not treated with bisphosphonates.35 The incidence in cancer patients treated with intravenous bisphosphonates has been reported as between 0% and 11%, and the incidence is higher following dental procedures and with a greater duration of drug exposure.11,14,15,17,35,38,44

Interestingly, in a recent survey of oncologists prescribing bisphosphonate medications for metastatic indications, two-thirds said they believe their patients probably have undiagnosed chronic oral conditions that could increase the risk of osteonecrosis of the jaw following bisphosphonate therapy and dental surgery procedures. A similar number reported that their patients receive routine dental care (access to and cost of dental care and the difficulty in physician prescreening are cited as obstacles), but only about one-third actually refer their patients to dentists before starting bisphosphonate therapy.45

What recent studies in osteoporosis and Paget disease showed

Controlled scientific studies in osteoporosis and Paget disease of bone have not shown osteonecrosis of the jaw to emerge, even after years of treatment with bisphosphonate drugs.24–31,46–49 To date, more than 50,000 patients have been treated with oral bisphosphonates— more than 100,000 patient-years for each drug: alendronate, risedronate (Actonel), and ibandronate (Boniva)—in clinical trials, and there has not been a single case of bisphosphonate-associated osteonecrosis in any of these studies.48

Recent publications have addressed the results of clinical trials comparing zoledronic acid (the drug most often associated with this condition in published case series) and risedronate in more than 300 patients with Paget disease of bone,31 and with placebo in postmenopausal women with osteoporosis and persons over 50 years of age suffering a hip fracture treated for up to 3 years following their fracture.29,30

In the largest trial, almost 4,000 osteoporotic women were treated with 5 mg of zoledronic acid annually for 3 years, and a similar number received placebo. Despite a rigorous search for any potential cases of bisphosphonate-associated osteonecrosis of the jaw—adjudicated by a blinded panel of ex on the basis of clinical and dental diagnostic imaging—only two possible cases were found: one in the placebo group and one in the treatment group (a case of osteomyelitis that preceded any treatment with zoledronic acid). Both patients recovered following a course of oral antibiotics and debridement. There was no increase in osteonecrosis at other skeletal sites.29,49

Observational studies have yielded conflicting results. An Australian postal survey of oral surgeons and dentists combined with drug adverse events data suggested the frequency of osteonecrosis of the jaw was 1:2,260 to 1:8,470 in patients on weekly alendronate treatment for osteoporosis, and 1:56 to 1:380 in patients with Paget disease. Following dental extractions, this rose to 1:296 to 1:1,130 and 1:7.4 to 1:48, respectively. Results in patients with malignancy were similar to those in other studies.44 The study raises issues similar to those in other studies: lack of an appropriate control group, reporting bias, and the possibility of multiple reportings of the same patients.

Unpublished information from pharmaceutical companies has suggested the incidence of unconfirmed cases of osteonecrosis of the jaw in persons taking alendronate is 0.7/100,000 person-years.14,17 One study using administrative claims data did not find evidence of increased bisphosphonate use in patients undergoing jaw surgery (used as a surrogate for osteonecrosis of the jaw),50 while another actually found that oral bisphosphonates had a protective effect against osteonecrosis of the jaw, inflammatory conditions of the jaw, and need for major jaw surgery.51

 

 

The risk, if any, is probably very small

This information suggests that if these drugs, used at the recommended dose, really do pose a risk, it is probably very small: less than 1 case in 100,000 patient-years if taking an oral bisphosphonate such as alendronate.14,17 This is significantly less than the risk of fracture in these patients (which may be higher than 1 in 10), the risk of death following such a fracture,22–30 or the risk of death from drowning, house fire, or motor vehicle accident.52

The cases of osteonecrosis of the jaw that we have personally seen—all in cancer patients treated with chemotherapy and highdose bisphosphonates—all showed histologic evidence of necrosis and concomitant infections, suggesting the actual diagnosis was osteomyelitis. Bone biopsies from affected but macroscopically normal mandibles at the time of surgical debridement for osteonecrosis of the jaw showed normal or increased osteoclastic activity, in contrast to what one would expect if there were oversuppression of bone turnover (unpublished data, J. Christian, J. Carey, Cleveland Clinic).

Recently, this family of drugs has shown some promise in limiting the progression of alveolar bone loss in periodontal disease (though they are not approved for this indication).53–55 Finally, published studies suggest bisphosphonate therapy may even be beneficial in animals and humans with osteonecrosis,56–58 and in conditions that mimic osteonecrosis such as SAPHO syndrome (synovitis, acne, pustulosis, hyperostosis, and osteitis) of the mandible, in which the histologic appearance may resemble that of osteonecrosis.59

WHAT SHOULD WE TELL OUR PATIENTS?

Several things are worth emphasizing from the published data and guidelines:

  • Many things are unknown about osteonecrosis of the jaw and the risk in people taking bisphosphonates.
  • The best evidence today does not support a cause-and-effect relationship between osteonecrosis of the jaw and bisphosphonate therapy.
  • If bisphosphonates are causative, the risk appears very low in patients without cancer.
  • It is important to distinguish between cancer and noncancer patients because of different risk factors, the markedly higher doses of bisphosphonates used in cancer patients, and the much greater incidence of osteonecrosis of the jaw seen in cancer patients irrespective of the cause.
  • The higher risk in cancer patients is likely modified or confounded by additional risk factors, possibly including long-term use of high-dose intravenous bisphosphonates.
  • About 90% of cases of bisphosphonate-associated osteonecrosis of the jaw have been in cancer patients, in whom a substantial temporal relationship to bisphosphonate therapy has been seen.9–12,15–17,19,49,54–57
  • Prevention will likely be the most effective management strategy because of the significant morbidity associated with and the refractory nature of osteonecrosis of the jaw.
  • Prophylactic dental examinations and any needed repair work are probably best done before starting bisphosphonate therapy in cancer patients; however, studies supporting such a strategy are needed.
  • There is no evidence to support routine dental examinations before starting such therapy for disorders other than cancer, or for stopping such therapy before, during, or after dental surgery. Whether this is true for patients who have been taking these drugs for several years or more is unclear.
  • Good communication between patients and their physicians, dentists, periodontists, and surgeons will help provide them with the best possible care.

Clearly, much further research is needed on the causes, risks, diagnosis, and management of this disorder to optimize patient outcomes.

References
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  20. Freiberger JJ, Padilla-Burgos R, Chhoeu AH, et al. Hyperbaric oxygen treatment and bisphosphonate-induced osteonecrosis of the jaw: a case series. J Oral Maxillofac Surg 2007; 65:13211327.
  21. Fleisch H. Bisphosphonates in Bone Disease. Fourth ed. San Diego, CA: Academic Press; 2000.
  22. Bone Health and Osteoporosis: A Report of the Surgeon General. www.surgeongeneral.gov/library/bonehealth. Accessed 10/1/2008.
  23. Carey JJ. What is a ‘failure’ of bisphosphonate therapy for osteoporosis? Cleve Clin J Med 2005; 72:10331039.
  24. Liberman UA, Weiss SR, Bröll J, et al. Effect of oral alendronate on bone mineral density and the incidence of fractures in postmenopausal osteoporosis. The Alendronate Phase III Osteoporosis Treatment Study Group. N Engl J Med 1995; 333:14371443.
  25. Black DM, Cummings SR, Karpf DB, et al. Randomised trial of effect of alendronate on risk of fracture in women with existing vertebral fractures. Fracture Intervention Trial Research Group. Lancet 1996; 348:15351541.
  26. Harris ST, Watts NB, Genant HK, et al. Effects of risedronate treatment on vertebral and nonvertebral fractures in women with postmenopausal osteoporosis: a randomized controlled trial. Vertebral Efficacy With Risedronate Therapy (VERT) Study Group. JAMA 1999; 282:13441352.
  27. McClung MR, Geusens P, Miller PD, et al; Hip Intervention Program Study Group. Effect of risedronate on the risk of hip fracture in elderly women. N Engl J Med 2001; 344:333340.
  28. Chesnut CH, Skag A, Christiansen C, et al; Oral Ibandronate Osteoporosis Vertebral Fracture Trial in North America and Europe (BONE). Effects of oral ibandronate administered daily or intermittently on fracture risk in postmenopausal osteoporosis. J Bone Miner Res 2004; 19:12411249.
  29. Black DM, Delmas PD, Eastell R, et al; HORIZON Pivotal Fracture Trial. Once-yearly zoledronic acid for treatment of postmenopausal osteoporosis. N Engl J Med 2007; 356:18091822.
  30. Lyles KW, Colón-Emeric CS, Magaziner JS, et al; HORIZON Recurrent Fracture Trial. Zoledronic acid and clinical fractures and mortality after hip fracture. N Engl J Med 2007; 357:17991809.
  31. Reid IR, Miller P, Lyles K, et al. Comparison of a single infusion of zoledronic acid with risedronate for Paget’s disease. N Engl J Med 2005; 353:898908.
  32. Bone HG, Santora AC. Authors Reply. N Engl J Med 2004; 351:191192.
  33. Conte P, Guarneri V. Safety of intravenous and oral bisphosphonates and compliance with dosing regimens. Oncologist 2004; 9(suppl 4):2837.
  34. Walter C, Grötz KA, Kunkel M, Al-Nawas B. Prevalence of bisphosphonate associated osteonecrosis of the jaw within the field of osteonecrosis. Support Care Cancer 2007; 15:197202.
  35. Zervas K, Verrou E, Teleioudis Z, et al. Incidence, risk factors and management of osteonecrosis of the jaws in patients with multiple myeloma: a single-centre experience in 303 patients. Br J Haematol 2006; 134:620623.
  36. Mortensen M, Lawson W, Montazem A. Osteonecrosis of the jaw associated with bisphosphonate use: presentation of seven cases and literature review. Laryngoscope 2007; 117:3034.
  37. Badros A, Weikel D, Salama A, et al. Osteonecrosis of the jaw in multiple myeloma patients: clinical features and risk factors. J Clin Oncol 2006; 24:945952.
  38. Durie BG, Katz M, Crowley J. Osteonecrosis of the jaw and bisphosphonates (letter). N Engl J Med 2005; 353:99100.
  39. Black DM, Schwartz AV, Ensrud KE, et al; FLEX Research Group. Effects of continuing or stopping alendronate after 5 years of treatment: the Fracture Intervention Trial Long-term Extension (FLEX): a randomized trial. JAMA 2006; 296:29272938.
  40. Gordis L. Epidemiology, 3rd ed. Philadelphia, Elsevier Saunders 2004:205.
  41. Fletcher RH, Fletcher SW, Wagner EH. Clinical Epidemiology. The Essentials. 3rd ed. Baltimore, MD; Lippincott, Williams & Wilkins, 1996:245.
  42. Sim J, Wright C. Research in Health Care, 1st ed. Cheltenham, England; Nelson Thornes, 2002.
  43. US Preventive Services Task Force Ratings. Strength of recommendations and quality of evidence. www.ahrq.gov/clinic/3rduspstf/ratings.htm. Accessed 10/1/2008.
  44. Mavrokokki T, Cheng A, Stein B, Goss A. Nature and frequency of bisphosphonate-associated osteonecrosis of the jaws in Australia. J Oral Maxillofac Surg 2007; 65:415423.
  45. Gibbs AE, Kherani A, Weitzel K, et al. Bisphosphonate-associated osteonecrosis: survey of oncologists. J Dent Res 2008; 87(special issue A):abstract #0639.
  46. Bone HG, Hosking D, Devogelaer JP, et al; Alendronate Phase III Osteoporosis Treatment Study Group. Ten years’ experience with alendronate for osteoporosis in postmenopausal women. N Engl J Med 2004; 350:11891199.
  47. Mellström DD, Sörensen OH, Goemaere S, Roux C, Johnson TD, Chines AA. Seven years of treatment with risedronate in women with postmenopausal osteoporosis. Calcif Tissue Int 2004; 75:462468.
  48. Bilezekian JP, Gold DT, Goldring S, et al. Discussions in Osteoporosis Issue 5, Feb 2006 5–7. Adelphia Inc.
  49. Grbic JT, Landesberg R, Lin SQ, et al; Health Outcomes and Reduced Incidence with Zoledronic Acid Once yearly Pivotal Fracture Trial Research Group. Incidence of osteonecrosis of the jaw in women with postmenopausal osteoporosis in the Health Outcomes and Reduced Incidence with Zoledronic Acid Once Yearly Pivotal Fracture Trial. J Am Dent Assoc 2008; 139:3240.
  50. Pazianas M, Blumentals WA, Miller PD. Lack of association between oral bisphosphonates and osteonecrosis using jaw surgery as a surrogate marker. Osteoporos Int 2007; Epub Nov 13.
  51. Cartsos VM, Zhu S, Zavras AI. Bisphosphonate use and the risk of adverse jaw outcomes. J Am Dent Assoc 2008; 139:2330.
  52. National Safety Council. The odds of dying from... www.nsc.org/lrs/statinfo/odds.htm. Accessed 10/1/2008.
  53. Palomo L, Bissada NF, Liu J. Periodontal assessment of postmenopausal women receiving risedronate. Menopause 2005; 12:685690.
  54. Rocha ML, Malacara JM, Sánchez-Marin FJ, Vazquez de la Torre CJ, Fajardo ME. Effect of alendronate on periodontal disease in postmenopausal women: a randomized placebo-controlled trial. J Periodontol 2004; 75:15791585.
  55. Jeffcoat MK, Cizza G, Shih WJ, Genco R, Lombardi A. Efficacy of bisphosphonates for the control of alveolar bone loss in periodontitis. J Int Acad Periodontol 2007; 9:7076.
  56. Little DG, Peat RA, Mcevoy A, Williams PR, Smith EJ, Baldock PA. Zoledronic acid treatment results in retention of femoral head structure after traumatic osteonecrosis in young Wistar rats. J Bone Miner Res 2003; 18:20162022.
  57. Agarwala S, Jain D, Joshi VR, Sule A. Efficacy of alendronate, a bisphosphonate, in the treatment of AVN of the hip. A prospective open-label study. Rheumatology (Oxf) 2005; 44:352359.
  58. Ramachandran M, Ward K, Brown RR, Munns CF, Cowell CT, Little DG. Intravenous bisphosphonate therapy for traumatic osteonecrosis of the femoral head in adolescents. J Bone Joint Surg Am 2007; 89:17271734.
  59. Kopterides P, Pikazis D, Koufos C. Successful treatment of SAPHO syndrome with zoledronic acid. Arthritis Rheum 2004; 50:29702973.
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Assistant Professor of Periodontology, Director of Predoctoral Periodontics, Case Western Reserve University School of Dental Medicine, Cleveland, OH

Address: Dr. John J. Carey, Department of Rheumatology, Unit 3, Merlin Park University Hospital, Galway, Ireland; e-mail [email protected]

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Assistant Professor of Periodontology, Director of Predoctoral Periodontics, Case Western Reserve University School of Dental Medicine, Cleveland, OH

Address: Dr. John J. Carey, Department of Rheumatology, Unit 3, Merlin Park University Hospital, Galway, Ireland; e-mail [email protected]

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Assistant Professor of Periodontology, Director of Predoctoral Periodontics, Case Western Reserve University School of Dental Medicine, Cleveland, OH

Address: Dr. John J. Carey, Department of Rheumatology, Unit 3, Merlin Park University Hospital, Galway, Ireland; e-mail [email protected]

Dr. Carey has indicated that he has received honoraria, consulting fees, or both from Procter and Gamble; Merck, Sharp, and Dohme; and Novartis and has board membership in Merck, Sharp and Dohme and Novartis.

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Recent case reports have linked bisphosphonate drugs to osteonecrosis of the jaw, and these reports have been widely publicized. Many patients receiving these drugs are asking their dentists and doctors whether the drugs do more harm than good, and some have even stopped taking them against medical advice. Health care professionals may be unsure what to tell patients and may be fearful of litigation.

However, most of the cases reported were in cancer patients, who are at significantly higher risk of osteonecrosis of the jaw for several reasons, and who receive much higher doses of bisphosphonates than do patients with osteoporosis or Paget disease of bone.

Moreover, although case reports have clearly documented an association between these drugs and osteonecrosis of the jaw, there is a lack of robust scientific evidence to support a cause-and-effect relationship. In fact, wellcontrolled clinical studies have not shown an increased risk of this complication in patients with osteoporosis or Paget disease of bone who were exposed to these agents, nor have they elucidated definite pathogenic mechanisms by which it might occur.

For these reasons, we believe that patients with osteoporosis should be advised of:

  • Their risk of fracture
  • The significant risk of morbidity and death following such a fracture
  • The effectiveness and excellent safety of bisphosphonate therapy in preventing fractures
  • The evidence that such therapy for osteoporosis and Paget disease poses little or no risk of osteonecrosis of the jaw
  • The need for further research.

WHAT IS OSTEONECROSIS OF THE JAW?

Osteonecrosis—a general loss of bone tissue as a result of cell death1—can occur at any skeletal site, but it typically involves the long bones, ie, the femur, tibia, and humerus.

Osteonecrosis of the jaw is a rare disorder characterized by exposure and loss of bone in the maxillofacial complex. It can result in significant morbidity and can be resistant or refractory to conventional therapy.

This condition is not new, having been described in 19th century factory workers exposed to white phosphorus used in matchstick manufacturing. Known then as “phossy jaw,” it was associated with poor dentition and often resulted in severe disfigurement, disease, and death. Use of white phosphorus, and matches containing it, were subsequently banned in many countries.2

In the early 20th century, radiation therapy for cancers of the head and neck area came into vogue, but its side effects included damage to the skeleton, or osteoradionecrosis.3 In 1950, LaDow4 described a case of osteoradionecrosis of the jaw and reviewed the literature available at that time. He concluded that there were three main causes of osteonecrosis of the jaw, namely, radiation therapy, trauma, and infection.

Although many such cases have since been reported in association with radiation therapy, chemotherapy, or both, and involvement of other skeletal sites is well described,5–8 the actual incidence of osteoradionecrosis in the general population remains unclear because no large epidemiologic studies to elucidate accurate numbers have been published.

BISPHOSPHONATE-ASSOCIATED OSTEONECROSIS OF THE JAW

Bisphosphonate-associated osteonecrosis of the jaw is a relatively new condition, having been first reported in three case series9–11 published in 2003 and 2004. The patients had exposure of areas of alveolar bone, mostly after oral surgery, eg, mucogingival flap elevation procedures (such as tooth extraction), that did not respond or were refractory to conventional treatment. All had received a bisphosphonate drug.

After these articles were published, the number of reported cases rose dramatically, including a case presented by one of us.12 By the end of January 2008, more than 500 papers on this condition were listed in PubMed. More than 60% had been printed since 2003, and approximately 85% concerned the association between osteonecrosis of the jaw and bisphosphonate use (search terms: “osteonecrosis of the jaw” and “bisphosphonate”).13

Although some dentists and oral surgeons claim to have seen many patients with this disorder, physicians who specialize in osteoporosis and metabolic bone disease do not. The medical literature and popular press have suggested that bisphosphonates are the cause of this malady. However, such articles are more perspective than evidence, as they are not scientific studies but rather reports of cases or series, or reviews of these. High-impact journals have given such articles prominent positions, highlighting the issue further, rather than balancing what is known and what is not known.

Thus, medicine safety boards, physicians, dentists, and oral surgeons have become increasingly concerned about the possible risk of this disorder in their patients on long-term bisphosphonate therapy, prompting organizations to issue management guidelines for this disorder and regulatory bodies to mandate warning labels on all drugs in this class about the possible risk.14–18 Funding agencies have highlighted this as an area in need of further investigation.17

However, robust evidence of a causal relationship is lacking. Contributing to the problem, other disorders can have similar presentations.

As a result, the diagnosis requires a dental examination and dental imaging, which are often impossible or impractical in a medical setting. Well-designed studies have relied on blinded panels of dental specialists using clinical and imaging data to adjudicate cases as osteonecrosis of the jaw before including them in published reports; case reports, however, often do not.

 

 

HOW IS OSTEONECROSIS OF THE JAW DIAGNOSED AND MANAGED?

A working definition of osteonecrosis of the jaw has recently emerged, and it will likely continue to evolve as results of further investigation become available.

A confirmed case is defined as an area of exposed bone in the maxillofacial region that does not heal within 8 weeks after being identified by a health care provider, in a patient who is currently receiving or has been exposed to a bisphosphonate and who has not had radiation therapy to the craniofacial region.14,17 This 8-week duration is consistent with the time frame in which soft tissue would be expected to close and exposed bone would be expected to heal under normal conditions after oral surgery such as dental extraction or a flap elevation procedure.

The working definition is one of inclusion and exclusion because the clinical presentation of osteonecrosis of the jaw is very similar to that of other diseases (Table 1).14,17 It is important for health professionals to understand this, since patients who have established osteonecrosis of the jaw or who are deemed to be at risk of it can also present with these other common clinical conditions that should not be confused with it.

Patients may have no symptoms at the time of presentation. However, symptoms can include oral or jaw pain, difficulty chewing, evidence of infection, and dental loss. Bone loss is often apparent radiographically, and it may be focal or generalized. Other imaging studies such as cone beam computed tomography provide greater detail on the extent and nature of the lesions, and thus provide a better assessment.

Histologically, there is evidence of necrosis, cell death, and, usually, concomitant infection.9–12,17

Management can be difficult

Osteonecrosis of the jaw can be difficult to manage, and extensive guidelines have been published.14–17 Its treatment is complicated because resection of the necrotic area often only makes the necrotic area bigger. Unlike in osteoradionecrosis, surgical removal of the affected area often results in necrosis at the margins of resected bone. This creates a potential situation of “chasing” affected bone in procedure after procedure, which results in significant morbidity.

Staging guidelines provide a framework for treatment (Table 2).14,16 Some case studies suggest that mucoperiosteal flap elevation procedures such as bone grafting, the use of bone morphogenic proteins, and alveolar bone decortication can succeed, but no randomized, placebo-controlled trials have been conducted. 19 Treatment with analgesics, antibiotics, surgery, and hyperbarbic oxygen may also be beneficial. Most authors have concluded that prevention is the ideal approach.14–20

A preventive protocol for cancer patients

Most of the cases reported so far have been in cancer patients receiving long-term treatment with potent bisphosphonates in high intravenous doses (12 times the usual dose for osteoporosis) after a mucoperiosteal flap elevation dental procedure (many of which were performed on an emergency basis).9–12,14–20 Authors have thus concluded that a preventive protocol should be followed for all patients being considered for intensive bisphosphonate treatment, similar to that adopted for patients receiving head and neck radiation.

Specifically, all chronic dental and periodontal conditions should be identified and stabilized before starting intensive bisphosphonate therapy. Experts today believe that controlling all chronic dental problems before starting intensive intravenous bisphosphonate therapy may be the best method to avoid dental surgery after bisphosphonate therapy has begun, particularly since the washout period (time to elimination of the drug) for bisphosphonates in alveolar bone is unknown.14–20

Although authors seem to agree that such a preventive protocol is prudent for intensive intravenous therapy, it does not appear to be necessary for patients without cancer.14,17 Indeed, such an approach is impractical, given the huge numbers involved and the lack of evidence to support it.

WHAT ARE BISPHOSPHONATES, AND WHY THE CONCERN?

Bisphosphonates are analogues of pyrophosphates, inorganic compounds developed to remove calcium carbonate from water in industrial pipes and laundry machines. Pyrophosphate use in humans arose from their affinity for calcium phosphate, which proved beneficial in scintigraphic imaging studies and in preventing tartar build-up, resulting in their incorporation into toothpastes. Modifications of the pyrophosphate molecule led to the development of diphosphonate compounds (later known as bisphosphonates), which have gained widespread use in treating a variety of disorders of the skeleton and of calcium metabolism.

These drugs prevent bone resorption by selectively inhibiting osteoclastic activity through several mechanisms (depending on the compound), thus helping prevent bone loss, bone pain, and hypercalcemia in diseases of the skeleton.

 

 

Bisphosphonates are widely used

Today, oral and intravenous bisphosphonates are widely prescribed for several skeletal disorders, including metastatic disease, malignant hypercalcemia, Paget disease of bone, and prevention and treatment of osteoporosis.21–23

More than 10 million Americans and more than 200 million people worldwide may have osteoporosis, which results in more than 1 million fractures each year. The lifetime risk of fracture for a postmenopausal white woman today is approximately 40% (approximately 15% for a 50-year-old man), and her annual risk of fracture is greater than her combined risk of stroke, heart attack, and breast cancer.22 Several bisphosphonates have been shown to safely and significantly reduce the risk of fracture in patients with osteoporosis and to be effective therapies for Paget disease of bone.24–31

Bisphosphonates are the most widely prescribed drugs for osteoporosis,22,23,29 with almost 200 million prescriptions for oral bisphosphonates worldwide. As of 2004, exposure to alendronate (Fosamax) was estimated to be about 20 million patient-years.32 Noncompliance limits their effectiveness in practice, due in part to concerns about adverse effects.

Since bisphosphonates are so widely prescribed, concern has been raised that they may be causing a new epidemic of osteonecrosis of the jaw.9 However, most reported cases have been in cancer patients, who are known to be at increased risk of this condition and who receive doses of bisphosphonates up to 12 times higher than in patients with osteoporosis or Paget disease of bone.9–12,33–38

The optimal duration of bisphosphonate therapy for these diseases to obtain the maximum benefit and minimize cost and harm remains unclear. Although a recent report suggests a bisphosphonate “drug holiday” may be an option when treating postmenopausal osteoporosis, larger, more robust studies of longer duration are needed.39 Outcomes of osteonecrosis of the jaw related to drug holidays have not been investigated.

‘IF I TAKE THIS TO STOP BONE LOSS, WILL IT HURT MY JAWS?’

The recently described association between bisphosphonates and osteonecrosis of the jaw has received considerable attention. Guidelines have been drawn up, some based on the assumption that bisphosphonates cause the osteonecrosis, but not based on scientific research.14–18 More than 90% of reported cases have been in cancer patients, a group known to be at increased risk of osteonecrosis of the jaw and other skeletal sites, for reasons that include radiation therapy, chemotherapy, corticosteroid use, and increased risk of infections.4,6,9–12,33–38 Nevertheless, it has been assumed that these patients are the same as osteoporosis patients, and sometimes that causation is beyond dispute. This is problematic for two main reasons:

  • Since noncompliance and lack of adherence (due to lack of knowledge about the dangers posed by osteoporosis, cost of the drugs, difficulty with dosing regimens, and fear of adverse effects) limit the effectiveness of these therapies in clinical practice, such attention has already persuaded patients to discontinue or refuse therapy (J.J. Carey, personal experience and communications from colleagues); and
  • Patients with osteoporosis and osteoporotic fractures have increased rates of morbidity and mortality and significantly higher fracture risk, which can be prevented with these agents if they are willing to take them.

Association does not prove causation

However, association does not prove causation. A relationship between a drug and a disease may be due to chance alone or to confounding factors.40 To judge the exact nature of this relationship, several issues need to be considered when reviewing the available evidence.

Substantiating that an agent causes a disease requires careful consideration of several aspects of their relationship: temporality, strength, dose-response, reversibility, consistency, biologic plausibility, and specificity.41 Correct interpretation of the strength of the evidence should also incorporate an evaluation of the study design, size, and reporting mechanism. Accordingly, case reports and case series are considered to constitute the weakest evidence, while randomized controlled trials and meta-analyses are usually considered the strongest.

When a true cause-and-effect relationship does exist, the situation can be a simple one in which only a single agent is involved. However, the issue can be decidedly more complex when the cause is an effect-modifier, requiring the interaction of additional factors.

When a cause has been assumed, demonstration of the dose-response relationship is also important: whether the risk is related in a continuous fashion to dose and duration of therapy (all patients), is seen only with particular doses or regimens (such as frequent use of high doses of potent bisphosphonates), or exists only in people who have passed a certain threshold value (for example, it may only occur in those who have received 0.5 g of an intravenous or 10 g of an oral bisphosphonate). Bearing in mind these considerations, the nature of the relationship between an agent and a disease can be better understood.40–43

A cause-and-effect relationship has not been established

A cause-and-effect relationship between bisphosphonates and osteonecrosis of the jaw has not been clearly established.14,17 Although case series highlight a relationship between the two, large controlled trials evaluating the occurrence of osteonecrosis of the jaw as the primary outcome have not been conducted. To date, most cases have been reported as uncontrolled case series, generally considered the weakest form of evidence.43

 

 

Most cases have been in cancer patients

Most cases of osteonecrosis of the jaw were in patients with cancer (particularly breast cancer and multiple myeloma) receiving potent intravenous bisphosphonates in high doses, most of whom had other documented risk factors, including recent dental procedures such as tooth extraction.9–12,15–19,33–38

One of the most compelling studies supporting causation examined the prevalence of osteonecrosis of the jaw in a cohort of 303 myeloma patients from 1991 to 2003. Osteonecrosis of the jaw developed only in those taking bisphosphonates (28 of 254), and the risk appeared greatest in those treated with both zoledronic acid (Zometa) and thalidomide (Thalomid). The importance of additional chemotherapies, concomitant diseases, and baseline dental pathology was not described.35 Biases, including channeling bias (in which patients who appear at increased risk of this rare condition also appear to be most likely to receive this medication), referral bias, and survivor bias, were not addressed in this paper or in others claiming that the risk is related to the type of bisphosphonate used and the duration of its use.15,33–38

A review of all cases of osteonecrosis of the jaw over a 5-year period in one institution (N = 163) found that only 17 (10%) were associated with bisphosphonate use, and all 17 patients had other risk factors, such as concomitant therapy for malignancy and recent dental surgery.34 The authors’ concern that longer follow-up may have shown a higher incidence of this problem is supported by the temporal relationship seen in other reports in which cancer patients with osteonecrosis of the jaw appear to have had higher cumulative doses of intravenous bisphosphonates than those without.9–12,15,34,35,37,38 Unfortunately, only one study had a control group to highlight the incidence of osteonecrosis of the jaw in similar patients not treated with bisphosphonates.35 The incidence in cancer patients treated with intravenous bisphosphonates has been reported as between 0% and 11%, and the incidence is higher following dental procedures and with a greater duration of drug exposure.11,14,15,17,35,38,44

Interestingly, in a recent survey of oncologists prescribing bisphosphonate medications for metastatic indications, two-thirds said they believe their patients probably have undiagnosed chronic oral conditions that could increase the risk of osteonecrosis of the jaw following bisphosphonate therapy and dental surgery procedures. A similar number reported that their patients receive routine dental care (access to and cost of dental care and the difficulty in physician prescreening are cited as obstacles), but only about one-third actually refer their patients to dentists before starting bisphosphonate therapy.45

What recent studies in osteoporosis and Paget disease showed

Controlled scientific studies in osteoporosis and Paget disease of bone have not shown osteonecrosis of the jaw to emerge, even after years of treatment with bisphosphonate drugs.24–31,46–49 To date, more than 50,000 patients have been treated with oral bisphosphonates— more than 100,000 patient-years for each drug: alendronate, risedronate (Actonel), and ibandronate (Boniva)—in clinical trials, and there has not been a single case of bisphosphonate-associated osteonecrosis in any of these studies.48

Recent publications have addressed the results of clinical trials comparing zoledronic acid (the drug most often associated with this condition in published case series) and risedronate in more than 300 patients with Paget disease of bone,31 and with placebo in postmenopausal women with osteoporosis and persons over 50 years of age suffering a hip fracture treated for up to 3 years following their fracture.29,30

In the largest trial, almost 4,000 osteoporotic women were treated with 5 mg of zoledronic acid annually for 3 years, and a similar number received placebo. Despite a rigorous search for any potential cases of bisphosphonate-associated osteonecrosis of the jaw—adjudicated by a blinded panel of ex on the basis of clinical and dental diagnostic imaging—only two possible cases were found: one in the placebo group and one in the treatment group (a case of osteomyelitis that preceded any treatment with zoledronic acid). Both patients recovered following a course of oral antibiotics and debridement. There was no increase in osteonecrosis at other skeletal sites.29,49

Observational studies have yielded conflicting results. An Australian postal survey of oral surgeons and dentists combined with drug adverse events data suggested the frequency of osteonecrosis of the jaw was 1:2,260 to 1:8,470 in patients on weekly alendronate treatment for osteoporosis, and 1:56 to 1:380 in patients with Paget disease. Following dental extractions, this rose to 1:296 to 1:1,130 and 1:7.4 to 1:48, respectively. Results in patients with malignancy were similar to those in other studies.44 The study raises issues similar to those in other studies: lack of an appropriate control group, reporting bias, and the possibility of multiple reportings of the same patients.

Unpublished information from pharmaceutical companies has suggested the incidence of unconfirmed cases of osteonecrosis of the jaw in persons taking alendronate is 0.7/100,000 person-years.14,17 One study using administrative claims data did not find evidence of increased bisphosphonate use in patients undergoing jaw surgery (used as a surrogate for osteonecrosis of the jaw),50 while another actually found that oral bisphosphonates had a protective effect against osteonecrosis of the jaw, inflammatory conditions of the jaw, and need for major jaw surgery.51

 

 

The risk, if any, is probably very small

This information suggests that if these drugs, used at the recommended dose, really do pose a risk, it is probably very small: less than 1 case in 100,000 patient-years if taking an oral bisphosphonate such as alendronate.14,17 This is significantly less than the risk of fracture in these patients (which may be higher than 1 in 10), the risk of death following such a fracture,22–30 or the risk of death from drowning, house fire, or motor vehicle accident.52

The cases of osteonecrosis of the jaw that we have personally seen—all in cancer patients treated with chemotherapy and highdose bisphosphonates—all showed histologic evidence of necrosis and concomitant infections, suggesting the actual diagnosis was osteomyelitis. Bone biopsies from affected but macroscopically normal mandibles at the time of surgical debridement for osteonecrosis of the jaw showed normal or increased osteoclastic activity, in contrast to what one would expect if there were oversuppression of bone turnover (unpublished data, J. Christian, J. Carey, Cleveland Clinic).

Recently, this family of drugs has shown some promise in limiting the progression of alveolar bone loss in periodontal disease (though they are not approved for this indication).53–55 Finally, published studies suggest bisphosphonate therapy may even be beneficial in animals and humans with osteonecrosis,56–58 and in conditions that mimic osteonecrosis such as SAPHO syndrome (synovitis, acne, pustulosis, hyperostosis, and osteitis) of the mandible, in which the histologic appearance may resemble that of osteonecrosis.59

WHAT SHOULD WE TELL OUR PATIENTS?

Several things are worth emphasizing from the published data and guidelines:

  • Many things are unknown about osteonecrosis of the jaw and the risk in people taking bisphosphonates.
  • The best evidence today does not support a cause-and-effect relationship between osteonecrosis of the jaw and bisphosphonate therapy.
  • If bisphosphonates are causative, the risk appears very low in patients without cancer.
  • It is important to distinguish between cancer and noncancer patients because of different risk factors, the markedly higher doses of bisphosphonates used in cancer patients, and the much greater incidence of osteonecrosis of the jaw seen in cancer patients irrespective of the cause.
  • The higher risk in cancer patients is likely modified or confounded by additional risk factors, possibly including long-term use of high-dose intravenous bisphosphonates.
  • About 90% of cases of bisphosphonate-associated osteonecrosis of the jaw have been in cancer patients, in whom a substantial temporal relationship to bisphosphonate therapy has been seen.9–12,15–17,19,49,54–57
  • Prevention will likely be the most effective management strategy because of the significant morbidity associated with and the refractory nature of osteonecrosis of the jaw.
  • Prophylactic dental examinations and any needed repair work are probably best done before starting bisphosphonate therapy in cancer patients; however, studies supporting such a strategy are needed.
  • There is no evidence to support routine dental examinations before starting such therapy for disorders other than cancer, or for stopping such therapy before, during, or after dental surgery. Whether this is true for patients who have been taking these drugs for several years or more is unclear.
  • Good communication between patients and their physicians, dentists, periodontists, and surgeons will help provide them with the best possible care.

Clearly, much further research is needed on the causes, risks, diagnosis, and management of this disorder to optimize patient outcomes.

Recent case reports have linked bisphosphonate drugs to osteonecrosis of the jaw, and these reports have been widely publicized. Many patients receiving these drugs are asking their dentists and doctors whether the drugs do more harm than good, and some have even stopped taking them against medical advice. Health care professionals may be unsure what to tell patients and may be fearful of litigation.

However, most of the cases reported were in cancer patients, who are at significantly higher risk of osteonecrosis of the jaw for several reasons, and who receive much higher doses of bisphosphonates than do patients with osteoporosis or Paget disease of bone.

Moreover, although case reports have clearly documented an association between these drugs and osteonecrosis of the jaw, there is a lack of robust scientific evidence to support a cause-and-effect relationship. In fact, wellcontrolled clinical studies have not shown an increased risk of this complication in patients with osteoporosis or Paget disease of bone who were exposed to these agents, nor have they elucidated definite pathogenic mechanisms by which it might occur.

For these reasons, we believe that patients with osteoporosis should be advised of:

  • Their risk of fracture
  • The significant risk of morbidity and death following such a fracture
  • The effectiveness and excellent safety of bisphosphonate therapy in preventing fractures
  • The evidence that such therapy for osteoporosis and Paget disease poses little or no risk of osteonecrosis of the jaw
  • The need for further research.

WHAT IS OSTEONECROSIS OF THE JAW?

Osteonecrosis—a general loss of bone tissue as a result of cell death1—can occur at any skeletal site, but it typically involves the long bones, ie, the femur, tibia, and humerus.

Osteonecrosis of the jaw is a rare disorder characterized by exposure and loss of bone in the maxillofacial complex. It can result in significant morbidity and can be resistant or refractory to conventional therapy.

This condition is not new, having been described in 19th century factory workers exposed to white phosphorus used in matchstick manufacturing. Known then as “phossy jaw,” it was associated with poor dentition and often resulted in severe disfigurement, disease, and death. Use of white phosphorus, and matches containing it, were subsequently banned in many countries.2

In the early 20th century, radiation therapy for cancers of the head and neck area came into vogue, but its side effects included damage to the skeleton, or osteoradionecrosis.3 In 1950, LaDow4 described a case of osteoradionecrosis of the jaw and reviewed the literature available at that time. He concluded that there were three main causes of osteonecrosis of the jaw, namely, radiation therapy, trauma, and infection.

Although many such cases have since been reported in association with radiation therapy, chemotherapy, or both, and involvement of other skeletal sites is well described,5–8 the actual incidence of osteoradionecrosis in the general population remains unclear because no large epidemiologic studies to elucidate accurate numbers have been published.

BISPHOSPHONATE-ASSOCIATED OSTEONECROSIS OF THE JAW

Bisphosphonate-associated osteonecrosis of the jaw is a relatively new condition, having been first reported in three case series9–11 published in 2003 and 2004. The patients had exposure of areas of alveolar bone, mostly after oral surgery, eg, mucogingival flap elevation procedures (such as tooth extraction), that did not respond or were refractory to conventional treatment. All had received a bisphosphonate drug.

After these articles were published, the number of reported cases rose dramatically, including a case presented by one of us.12 By the end of January 2008, more than 500 papers on this condition were listed in PubMed. More than 60% had been printed since 2003, and approximately 85% concerned the association between osteonecrosis of the jaw and bisphosphonate use (search terms: “osteonecrosis of the jaw” and “bisphosphonate”).13

Although some dentists and oral surgeons claim to have seen many patients with this disorder, physicians who specialize in osteoporosis and metabolic bone disease do not. The medical literature and popular press have suggested that bisphosphonates are the cause of this malady. However, such articles are more perspective than evidence, as they are not scientific studies but rather reports of cases or series, or reviews of these. High-impact journals have given such articles prominent positions, highlighting the issue further, rather than balancing what is known and what is not known.

Thus, medicine safety boards, physicians, dentists, and oral surgeons have become increasingly concerned about the possible risk of this disorder in their patients on long-term bisphosphonate therapy, prompting organizations to issue management guidelines for this disorder and regulatory bodies to mandate warning labels on all drugs in this class about the possible risk.14–18 Funding agencies have highlighted this as an area in need of further investigation.17

However, robust evidence of a causal relationship is lacking. Contributing to the problem, other disorders can have similar presentations.

As a result, the diagnosis requires a dental examination and dental imaging, which are often impossible or impractical in a medical setting. Well-designed studies have relied on blinded panels of dental specialists using clinical and imaging data to adjudicate cases as osteonecrosis of the jaw before including them in published reports; case reports, however, often do not.

 

 

HOW IS OSTEONECROSIS OF THE JAW DIAGNOSED AND MANAGED?

A working definition of osteonecrosis of the jaw has recently emerged, and it will likely continue to evolve as results of further investigation become available.

A confirmed case is defined as an area of exposed bone in the maxillofacial region that does not heal within 8 weeks after being identified by a health care provider, in a patient who is currently receiving or has been exposed to a bisphosphonate and who has not had radiation therapy to the craniofacial region.14,17 This 8-week duration is consistent with the time frame in which soft tissue would be expected to close and exposed bone would be expected to heal under normal conditions after oral surgery such as dental extraction or a flap elevation procedure.

The working definition is one of inclusion and exclusion because the clinical presentation of osteonecrosis of the jaw is very similar to that of other diseases (Table 1).14,17 It is important for health professionals to understand this, since patients who have established osteonecrosis of the jaw or who are deemed to be at risk of it can also present with these other common clinical conditions that should not be confused with it.

Patients may have no symptoms at the time of presentation. However, symptoms can include oral or jaw pain, difficulty chewing, evidence of infection, and dental loss. Bone loss is often apparent radiographically, and it may be focal or generalized. Other imaging studies such as cone beam computed tomography provide greater detail on the extent and nature of the lesions, and thus provide a better assessment.

Histologically, there is evidence of necrosis, cell death, and, usually, concomitant infection.9–12,17

Management can be difficult

Osteonecrosis of the jaw can be difficult to manage, and extensive guidelines have been published.14–17 Its treatment is complicated because resection of the necrotic area often only makes the necrotic area bigger. Unlike in osteoradionecrosis, surgical removal of the affected area often results in necrosis at the margins of resected bone. This creates a potential situation of “chasing” affected bone in procedure after procedure, which results in significant morbidity.

Staging guidelines provide a framework for treatment (Table 2).14,16 Some case studies suggest that mucoperiosteal flap elevation procedures such as bone grafting, the use of bone morphogenic proteins, and alveolar bone decortication can succeed, but no randomized, placebo-controlled trials have been conducted. 19 Treatment with analgesics, antibiotics, surgery, and hyperbarbic oxygen may also be beneficial. Most authors have concluded that prevention is the ideal approach.14–20

A preventive protocol for cancer patients

Most of the cases reported so far have been in cancer patients receiving long-term treatment with potent bisphosphonates in high intravenous doses (12 times the usual dose for osteoporosis) after a mucoperiosteal flap elevation dental procedure (many of which were performed on an emergency basis).9–12,14–20 Authors have thus concluded that a preventive protocol should be followed for all patients being considered for intensive bisphosphonate treatment, similar to that adopted for patients receiving head and neck radiation.

Specifically, all chronic dental and periodontal conditions should be identified and stabilized before starting intensive bisphosphonate therapy. Experts today believe that controlling all chronic dental problems before starting intensive intravenous bisphosphonate therapy may be the best method to avoid dental surgery after bisphosphonate therapy has begun, particularly since the washout period (time to elimination of the drug) for bisphosphonates in alveolar bone is unknown.14–20

Although authors seem to agree that such a preventive protocol is prudent for intensive intravenous therapy, it does not appear to be necessary for patients without cancer.14,17 Indeed, such an approach is impractical, given the huge numbers involved and the lack of evidence to support it.

WHAT ARE BISPHOSPHONATES, AND WHY THE CONCERN?

Bisphosphonates are analogues of pyrophosphates, inorganic compounds developed to remove calcium carbonate from water in industrial pipes and laundry machines. Pyrophosphate use in humans arose from their affinity for calcium phosphate, which proved beneficial in scintigraphic imaging studies and in preventing tartar build-up, resulting in their incorporation into toothpastes. Modifications of the pyrophosphate molecule led to the development of diphosphonate compounds (later known as bisphosphonates), which have gained widespread use in treating a variety of disorders of the skeleton and of calcium metabolism.

These drugs prevent bone resorption by selectively inhibiting osteoclastic activity through several mechanisms (depending on the compound), thus helping prevent bone loss, bone pain, and hypercalcemia in diseases of the skeleton.

 

 

Bisphosphonates are widely used

Today, oral and intravenous bisphosphonates are widely prescribed for several skeletal disorders, including metastatic disease, malignant hypercalcemia, Paget disease of bone, and prevention and treatment of osteoporosis.21–23

More than 10 million Americans and more than 200 million people worldwide may have osteoporosis, which results in more than 1 million fractures each year. The lifetime risk of fracture for a postmenopausal white woman today is approximately 40% (approximately 15% for a 50-year-old man), and her annual risk of fracture is greater than her combined risk of stroke, heart attack, and breast cancer.22 Several bisphosphonates have been shown to safely and significantly reduce the risk of fracture in patients with osteoporosis and to be effective therapies for Paget disease of bone.24–31

Bisphosphonates are the most widely prescribed drugs for osteoporosis,22,23,29 with almost 200 million prescriptions for oral bisphosphonates worldwide. As of 2004, exposure to alendronate (Fosamax) was estimated to be about 20 million patient-years.32 Noncompliance limits their effectiveness in practice, due in part to concerns about adverse effects.

Since bisphosphonates are so widely prescribed, concern has been raised that they may be causing a new epidemic of osteonecrosis of the jaw.9 However, most reported cases have been in cancer patients, who are known to be at increased risk of this condition and who receive doses of bisphosphonates up to 12 times higher than in patients with osteoporosis or Paget disease of bone.9–12,33–38

The optimal duration of bisphosphonate therapy for these diseases to obtain the maximum benefit and minimize cost and harm remains unclear. Although a recent report suggests a bisphosphonate “drug holiday” may be an option when treating postmenopausal osteoporosis, larger, more robust studies of longer duration are needed.39 Outcomes of osteonecrosis of the jaw related to drug holidays have not been investigated.

‘IF I TAKE THIS TO STOP BONE LOSS, WILL IT HURT MY JAWS?’

The recently described association between bisphosphonates and osteonecrosis of the jaw has received considerable attention. Guidelines have been drawn up, some based on the assumption that bisphosphonates cause the osteonecrosis, but not based on scientific research.14–18 More than 90% of reported cases have been in cancer patients, a group known to be at increased risk of osteonecrosis of the jaw and other skeletal sites, for reasons that include radiation therapy, chemotherapy, corticosteroid use, and increased risk of infections.4,6,9–12,33–38 Nevertheless, it has been assumed that these patients are the same as osteoporosis patients, and sometimes that causation is beyond dispute. This is problematic for two main reasons:

  • Since noncompliance and lack of adherence (due to lack of knowledge about the dangers posed by osteoporosis, cost of the drugs, difficulty with dosing regimens, and fear of adverse effects) limit the effectiveness of these therapies in clinical practice, such attention has already persuaded patients to discontinue or refuse therapy (J.J. Carey, personal experience and communications from colleagues); and
  • Patients with osteoporosis and osteoporotic fractures have increased rates of morbidity and mortality and significantly higher fracture risk, which can be prevented with these agents if they are willing to take them.

Association does not prove causation

However, association does not prove causation. A relationship between a drug and a disease may be due to chance alone or to confounding factors.40 To judge the exact nature of this relationship, several issues need to be considered when reviewing the available evidence.

Substantiating that an agent causes a disease requires careful consideration of several aspects of their relationship: temporality, strength, dose-response, reversibility, consistency, biologic plausibility, and specificity.41 Correct interpretation of the strength of the evidence should also incorporate an evaluation of the study design, size, and reporting mechanism. Accordingly, case reports and case series are considered to constitute the weakest evidence, while randomized controlled trials and meta-analyses are usually considered the strongest.

When a true cause-and-effect relationship does exist, the situation can be a simple one in which only a single agent is involved. However, the issue can be decidedly more complex when the cause is an effect-modifier, requiring the interaction of additional factors.

When a cause has been assumed, demonstration of the dose-response relationship is also important: whether the risk is related in a continuous fashion to dose and duration of therapy (all patients), is seen only with particular doses or regimens (such as frequent use of high doses of potent bisphosphonates), or exists only in people who have passed a certain threshold value (for example, it may only occur in those who have received 0.5 g of an intravenous or 10 g of an oral bisphosphonate). Bearing in mind these considerations, the nature of the relationship between an agent and a disease can be better understood.40–43

A cause-and-effect relationship has not been established

A cause-and-effect relationship between bisphosphonates and osteonecrosis of the jaw has not been clearly established.14,17 Although case series highlight a relationship between the two, large controlled trials evaluating the occurrence of osteonecrosis of the jaw as the primary outcome have not been conducted. To date, most cases have been reported as uncontrolled case series, generally considered the weakest form of evidence.43

 

 

Most cases have been in cancer patients

Most cases of osteonecrosis of the jaw were in patients with cancer (particularly breast cancer and multiple myeloma) receiving potent intravenous bisphosphonates in high doses, most of whom had other documented risk factors, including recent dental procedures such as tooth extraction.9–12,15–19,33–38

One of the most compelling studies supporting causation examined the prevalence of osteonecrosis of the jaw in a cohort of 303 myeloma patients from 1991 to 2003. Osteonecrosis of the jaw developed only in those taking bisphosphonates (28 of 254), and the risk appeared greatest in those treated with both zoledronic acid (Zometa) and thalidomide (Thalomid). The importance of additional chemotherapies, concomitant diseases, and baseline dental pathology was not described.35 Biases, including channeling bias (in which patients who appear at increased risk of this rare condition also appear to be most likely to receive this medication), referral bias, and survivor bias, were not addressed in this paper or in others claiming that the risk is related to the type of bisphosphonate used and the duration of its use.15,33–38

A review of all cases of osteonecrosis of the jaw over a 5-year period in one institution (N = 163) found that only 17 (10%) were associated with bisphosphonate use, and all 17 patients had other risk factors, such as concomitant therapy for malignancy and recent dental surgery.34 The authors’ concern that longer follow-up may have shown a higher incidence of this problem is supported by the temporal relationship seen in other reports in which cancer patients with osteonecrosis of the jaw appear to have had higher cumulative doses of intravenous bisphosphonates than those without.9–12,15,34,35,37,38 Unfortunately, only one study had a control group to highlight the incidence of osteonecrosis of the jaw in similar patients not treated with bisphosphonates.35 The incidence in cancer patients treated with intravenous bisphosphonates has been reported as between 0% and 11%, and the incidence is higher following dental procedures and with a greater duration of drug exposure.11,14,15,17,35,38,44

Interestingly, in a recent survey of oncologists prescribing bisphosphonate medications for metastatic indications, two-thirds said they believe their patients probably have undiagnosed chronic oral conditions that could increase the risk of osteonecrosis of the jaw following bisphosphonate therapy and dental surgery procedures. A similar number reported that their patients receive routine dental care (access to and cost of dental care and the difficulty in physician prescreening are cited as obstacles), but only about one-third actually refer their patients to dentists before starting bisphosphonate therapy.45

What recent studies in osteoporosis and Paget disease showed

Controlled scientific studies in osteoporosis and Paget disease of bone have not shown osteonecrosis of the jaw to emerge, even after years of treatment with bisphosphonate drugs.24–31,46–49 To date, more than 50,000 patients have been treated with oral bisphosphonates— more than 100,000 patient-years for each drug: alendronate, risedronate (Actonel), and ibandronate (Boniva)—in clinical trials, and there has not been a single case of bisphosphonate-associated osteonecrosis in any of these studies.48

Recent publications have addressed the results of clinical trials comparing zoledronic acid (the drug most often associated with this condition in published case series) and risedronate in more than 300 patients with Paget disease of bone,31 and with placebo in postmenopausal women with osteoporosis and persons over 50 years of age suffering a hip fracture treated for up to 3 years following their fracture.29,30

In the largest trial, almost 4,000 osteoporotic women were treated with 5 mg of zoledronic acid annually for 3 years, and a similar number received placebo. Despite a rigorous search for any potential cases of bisphosphonate-associated osteonecrosis of the jaw—adjudicated by a blinded panel of ex on the basis of clinical and dental diagnostic imaging—only two possible cases were found: one in the placebo group and one in the treatment group (a case of osteomyelitis that preceded any treatment with zoledronic acid). Both patients recovered following a course of oral antibiotics and debridement. There was no increase in osteonecrosis at other skeletal sites.29,49

Observational studies have yielded conflicting results. An Australian postal survey of oral surgeons and dentists combined with drug adverse events data suggested the frequency of osteonecrosis of the jaw was 1:2,260 to 1:8,470 in patients on weekly alendronate treatment for osteoporosis, and 1:56 to 1:380 in patients with Paget disease. Following dental extractions, this rose to 1:296 to 1:1,130 and 1:7.4 to 1:48, respectively. Results in patients with malignancy were similar to those in other studies.44 The study raises issues similar to those in other studies: lack of an appropriate control group, reporting bias, and the possibility of multiple reportings of the same patients.

Unpublished information from pharmaceutical companies has suggested the incidence of unconfirmed cases of osteonecrosis of the jaw in persons taking alendronate is 0.7/100,000 person-years.14,17 One study using administrative claims data did not find evidence of increased bisphosphonate use in patients undergoing jaw surgery (used as a surrogate for osteonecrosis of the jaw),50 while another actually found that oral bisphosphonates had a protective effect against osteonecrosis of the jaw, inflammatory conditions of the jaw, and need for major jaw surgery.51

 

 

The risk, if any, is probably very small

This information suggests that if these drugs, used at the recommended dose, really do pose a risk, it is probably very small: less than 1 case in 100,000 patient-years if taking an oral bisphosphonate such as alendronate.14,17 This is significantly less than the risk of fracture in these patients (which may be higher than 1 in 10), the risk of death following such a fracture,22–30 or the risk of death from drowning, house fire, or motor vehicle accident.52

The cases of osteonecrosis of the jaw that we have personally seen—all in cancer patients treated with chemotherapy and highdose bisphosphonates—all showed histologic evidence of necrosis and concomitant infections, suggesting the actual diagnosis was osteomyelitis. Bone biopsies from affected but macroscopically normal mandibles at the time of surgical debridement for osteonecrosis of the jaw showed normal or increased osteoclastic activity, in contrast to what one would expect if there were oversuppression of bone turnover (unpublished data, J. Christian, J. Carey, Cleveland Clinic).

Recently, this family of drugs has shown some promise in limiting the progression of alveolar bone loss in periodontal disease (though they are not approved for this indication).53–55 Finally, published studies suggest bisphosphonate therapy may even be beneficial in animals and humans with osteonecrosis,56–58 and in conditions that mimic osteonecrosis such as SAPHO syndrome (synovitis, acne, pustulosis, hyperostosis, and osteitis) of the mandible, in which the histologic appearance may resemble that of osteonecrosis.59

WHAT SHOULD WE TELL OUR PATIENTS?

Several things are worth emphasizing from the published data and guidelines:

  • Many things are unknown about osteonecrosis of the jaw and the risk in people taking bisphosphonates.
  • The best evidence today does not support a cause-and-effect relationship between osteonecrosis of the jaw and bisphosphonate therapy.
  • If bisphosphonates are causative, the risk appears very low in patients without cancer.
  • It is important to distinguish between cancer and noncancer patients because of different risk factors, the markedly higher doses of bisphosphonates used in cancer patients, and the much greater incidence of osteonecrosis of the jaw seen in cancer patients irrespective of the cause.
  • The higher risk in cancer patients is likely modified or confounded by additional risk factors, possibly including long-term use of high-dose intravenous bisphosphonates.
  • About 90% of cases of bisphosphonate-associated osteonecrosis of the jaw have been in cancer patients, in whom a substantial temporal relationship to bisphosphonate therapy has been seen.9–12,15–17,19,49,54–57
  • Prevention will likely be the most effective management strategy because of the significant morbidity associated with and the refractory nature of osteonecrosis of the jaw.
  • Prophylactic dental examinations and any needed repair work are probably best done before starting bisphosphonate therapy in cancer patients; however, studies supporting such a strategy are needed.
  • There is no evidence to support routine dental examinations before starting such therapy for disorders other than cancer, or for stopping such therapy before, during, or after dental surgery. Whether this is true for patients who have been taking these drugs for several years or more is unclear.
  • Good communication between patients and their physicians, dentists, periodontists, and surgeons will help provide them with the best possible care.

Clearly, much further research is needed on the causes, risks, diagnosis, and management of this disorder to optimize patient outcomes.

References
  1. Thomas CL. Taber’s Cyclopedic Medical Dictionary, 17th ed. Philadelphia, FA Davis, 1993.
  2. Donoghue AM. Bisphosphonates and osteonecrosis: analogy to phossy jaw. Med J Aust 2005; 183:163164.
  3. Watson WL, Scarborough JE. Osteoradionecrosis in intraoral cancer. Am J Roentgenol 1938; 40:524534.
  4. LaDow CS. Osteoradionecrosis of the jaw. Oral Surg Oral Med Oral Pathol 1950; 3:582590.
  5. Topazian DS. Prevention of osteoradionecrosis of the jaws. Oral Surg Oral Med Oral Pathol 1959; 21:530538.
  6. Marx RE. Osteoradionecrosis: a new concept of its pathophysiology. J Oral Maxillofac Surg 1983; 41:283288.
  7. Rossleigh MA, Smith J, Straus DJ, Engel IA. Osteonecrosis in patients with malignant lymphoma. A review of 31 cases. Cancer 1986; 58:11121116.
  8. Cook AM, Dzik-Jurasz AS, Padhani AR, Norman A, Huddart RA. The prevalence of avascular necrosis in patients treated with chemotherapy for testicular tumors. Br J Cancer 2001; 85:16241626.
  9. Marx RE. Pamidronate (Aredia) and zoledronate (Zometa) induced avascular necrosis of the jaws: a growing epidemic. J Oral Maxillofac Surg 2003; 61:11151117.
  10. Migliorati CA. Bisphosphonates and oral cavity avascular bone necrosis. J Clin Oncol 2003; 21:42534254.
  11. Ruggiero SL, Mehrotra B, Rosenberg TJ, Engroff SL. Osteonecrosis of the jaws associated with the use of bisphosphonates: a review of 63 cases. J Oral Maxillofac Surg 2004; 62:527534.
  12. Wright MM, Wright BM, Christian J, Carey JJ. A case series of osteonecrosis of the jaw associated with the use of bisphosphonates. Arthritis Rheum 2005; ( suppl Sept): 1984.
  13. National Center for Biotechnology Information. PubMed. www.ncbi.nlm.nih.gov/PubMed. Accessed 10/1/2008.
  14. American Dental Association Council on Scientific Affairs. Dental management of patients receiving oral bisphosphonate therapy: expert panel recommendations. J Am Dent Assoc 2006; 137:11441150.
  15. Woo SB, Hellstein JW, Kalmar JR. Narrative review: bisphosphonates and osteonecrosis of the jaws. Ann Intern Med 2006; 144:753761.
  16. Advisory Task Force on Bisphosphonate-Related Osteonecrosis of the Jaws, American Association of Oral and Maxillofacial Surgeons. American Association of Oral and Maxillofacial Surgeons position paper on bisphosphonate-related osteonecrosis of the jaws. J Oral Maxillofac Surg 2007; 65:369376.
  17. Khosla S, Burr D, Cauley J, et al; American Society for Bone and Mineral Research. Bishosphonate-associated osteonecrosis of the jaw: report of a task force of the American Society for Bone and Mineral Research. J Bone Miner Res 2007; 22:14791491.
  18. Ruggiero S, Gralow J, Marx R, et al. Practical guidelines for the prevention, diagnosis, and treatment of osteonecrosis of the jaw in patients with cancer. J Oncol Pract 2006; 2:714.
  19. Wang HL, Weber D, McCauley LK. Effect of long-term oral bisphosphonates on implant wound healing: literature review and a case report. J Periodontol 2007; 78:584594.
  20. Freiberger JJ, Padilla-Burgos R, Chhoeu AH, et al. Hyperbaric oxygen treatment and bisphosphonate-induced osteonecrosis of the jaw: a case series. J Oral Maxillofac Surg 2007; 65:13211327.
  21. Fleisch H. Bisphosphonates in Bone Disease. Fourth ed. San Diego, CA: Academic Press; 2000.
  22. Bone Health and Osteoporosis: A Report of the Surgeon General. www.surgeongeneral.gov/library/bonehealth. Accessed 10/1/2008.
  23. Carey JJ. What is a ‘failure’ of bisphosphonate therapy for osteoporosis? Cleve Clin J Med 2005; 72:10331039.
  24. Liberman UA, Weiss SR, Bröll J, et al. Effect of oral alendronate on bone mineral density and the incidence of fractures in postmenopausal osteoporosis. The Alendronate Phase III Osteoporosis Treatment Study Group. N Engl J Med 1995; 333:14371443.
  25. Black DM, Cummings SR, Karpf DB, et al. Randomised trial of effect of alendronate on risk of fracture in women with existing vertebral fractures. Fracture Intervention Trial Research Group. Lancet 1996; 348:15351541.
  26. Harris ST, Watts NB, Genant HK, et al. Effects of risedronate treatment on vertebral and nonvertebral fractures in women with postmenopausal osteoporosis: a randomized controlled trial. Vertebral Efficacy With Risedronate Therapy (VERT) Study Group. JAMA 1999; 282:13441352.
  27. McClung MR, Geusens P, Miller PD, et al; Hip Intervention Program Study Group. Effect of risedronate on the risk of hip fracture in elderly women. N Engl J Med 2001; 344:333340.
  28. Chesnut CH, Skag A, Christiansen C, et al; Oral Ibandronate Osteoporosis Vertebral Fracture Trial in North America and Europe (BONE). Effects of oral ibandronate administered daily or intermittently on fracture risk in postmenopausal osteoporosis. J Bone Miner Res 2004; 19:12411249.
  29. Black DM, Delmas PD, Eastell R, et al; HORIZON Pivotal Fracture Trial. Once-yearly zoledronic acid for treatment of postmenopausal osteoporosis. N Engl J Med 2007; 356:18091822.
  30. Lyles KW, Colón-Emeric CS, Magaziner JS, et al; HORIZON Recurrent Fracture Trial. Zoledronic acid and clinical fractures and mortality after hip fracture. N Engl J Med 2007; 357:17991809.
  31. Reid IR, Miller P, Lyles K, et al. Comparison of a single infusion of zoledronic acid with risedronate for Paget’s disease. N Engl J Med 2005; 353:898908.
  32. Bone HG, Santora AC. Authors Reply. N Engl J Med 2004; 351:191192.
  33. Conte P, Guarneri V. Safety of intravenous and oral bisphosphonates and compliance with dosing regimens. Oncologist 2004; 9(suppl 4):2837.
  34. Walter C, Grötz KA, Kunkel M, Al-Nawas B. Prevalence of bisphosphonate associated osteonecrosis of the jaw within the field of osteonecrosis. Support Care Cancer 2007; 15:197202.
  35. Zervas K, Verrou E, Teleioudis Z, et al. Incidence, risk factors and management of osteonecrosis of the jaws in patients with multiple myeloma: a single-centre experience in 303 patients. Br J Haematol 2006; 134:620623.
  36. Mortensen M, Lawson W, Montazem A. Osteonecrosis of the jaw associated with bisphosphonate use: presentation of seven cases and literature review. Laryngoscope 2007; 117:3034.
  37. Badros A, Weikel D, Salama A, et al. Osteonecrosis of the jaw in multiple myeloma patients: clinical features and risk factors. J Clin Oncol 2006; 24:945952.
  38. Durie BG, Katz M, Crowley J. Osteonecrosis of the jaw and bisphosphonates (letter). N Engl J Med 2005; 353:99100.
  39. Black DM, Schwartz AV, Ensrud KE, et al; FLEX Research Group. Effects of continuing or stopping alendronate after 5 years of treatment: the Fracture Intervention Trial Long-term Extension (FLEX): a randomized trial. JAMA 2006; 296:29272938.
  40. Gordis L. Epidemiology, 3rd ed. Philadelphia, Elsevier Saunders 2004:205.
  41. Fletcher RH, Fletcher SW, Wagner EH. Clinical Epidemiology. The Essentials. 3rd ed. Baltimore, MD; Lippincott, Williams & Wilkins, 1996:245.
  42. Sim J, Wright C. Research in Health Care, 1st ed. Cheltenham, England; Nelson Thornes, 2002.
  43. US Preventive Services Task Force Ratings. Strength of recommendations and quality of evidence. www.ahrq.gov/clinic/3rduspstf/ratings.htm. Accessed 10/1/2008.
  44. Mavrokokki T, Cheng A, Stein B, Goss A. Nature and frequency of bisphosphonate-associated osteonecrosis of the jaws in Australia. J Oral Maxillofac Surg 2007; 65:415423.
  45. Gibbs AE, Kherani A, Weitzel K, et al. Bisphosphonate-associated osteonecrosis: survey of oncologists. J Dent Res 2008; 87(special issue A):abstract #0639.
  46. Bone HG, Hosking D, Devogelaer JP, et al; Alendronate Phase III Osteoporosis Treatment Study Group. Ten years’ experience with alendronate for osteoporosis in postmenopausal women. N Engl J Med 2004; 350:11891199.
  47. Mellström DD, Sörensen OH, Goemaere S, Roux C, Johnson TD, Chines AA. Seven years of treatment with risedronate in women with postmenopausal osteoporosis. Calcif Tissue Int 2004; 75:462468.
  48. Bilezekian JP, Gold DT, Goldring S, et al. Discussions in Osteoporosis Issue 5, Feb 2006 5–7. Adelphia Inc.
  49. Grbic JT, Landesberg R, Lin SQ, et al; Health Outcomes and Reduced Incidence with Zoledronic Acid Once yearly Pivotal Fracture Trial Research Group. Incidence of osteonecrosis of the jaw in women with postmenopausal osteoporosis in the Health Outcomes and Reduced Incidence with Zoledronic Acid Once Yearly Pivotal Fracture Trial. J Am Dent Assoc 2008; 139:3240.
  50. Pazianas M, Blumentals WA, Miller PD. Lack of association between oral bisphosphonates and osteonecrosis using jaw surgery as a surrogate marker. Osteoporos Int 2007; Epub Nov 13.
  51. Cartsos VM, Zhu S, Zavras AI. Bisphosphonate use and the risk of adverse jaw outcomes. J Am Dent Assoc 2008; 139:2330.
  52. National Safety Council. The odds of dying from... www.nsc.org/lrs/statinfo/odds.htm. Accessed 10/1/2008.
  53. Palomo L, Bissada NF, Liu J. Periodontal assessment of postmenopausal women receiving risedronate. Menopause 2005; 12:685690.
  54. Rocha ML, Malacara JM, Sánchez-Marin FJ, Vazquez de la Torre CJ, Fajardo ME. Effect of alendronate on periodontal disease in postmenopausal women: a randomized placebo-controlled trial. J Periodontol 2004; 75:15791585.
  55. Jeffcoat MK, Cizza G, Shih WJ, Genco R, Lombardi A. Efficacy of bisphosphonates for the control of alveolar bone loss in periodontitis. J Int Acad Periodontol 2007; 9:7076.
  56. Little DG, Peat RA, Mcevoy A, Williams PR, Smith EJ, Baldock PA. Zoledronic acid treatment results in retention of femoral head structure after traumatic osteonecrosis in young Wistar rats. J Bone Miner Res 2003; 18:20162022.
  57. Agarwala S, Jain D, Joshi VR, Sule A. Efficacy of alendronate, a bisphosphonate, in the treatment of AVN of the hip. A prospective open-label study. Rheumatology (Oxf) 2005; 44:352359.
  58. Ramachandran M, Ward K, Brown RR, Munns CF, Cowell CT, Little DG. Intravenous bisphosphonate therapy for traumatic osteonecrosis of the femoral head in adolescents. J Bone Joint Surg Am 2007; 89:17271734.
  59. Kopterides P, Pikazis D, Koufos C. Successful treatment of SAPHO syndrome with zoledronic acid. Arthritis Rheum 2004; 50:29702973.
References
  1. Thomas CL. Taber’s Cyclopedic Medical Dictionary, 17th ed. Philadelphia, FA Davis, 1993.
  2. Donoghue AM. Bisphosphonates and osteonecrosis: analogy to phossy jaw. Med J Aust 2005; 183:163164.
  3. Watson WL, Scarborough JE. Osteoradionecrosis in intraoral cancer. Am J Roentgenol 1938; 40:524534.
  4. LaDow CS. Osteoradionecrosis of the jaw. Oral Surg Oral Med Oral Pathol 1950; 3:582590.
  5. Topazian DS. Prevention of osteoradionecrosis of the jaws. Oral Surg Oral Med Oral Pathol 1959; 21:530538.
  6. Marx RE. Osteoradionecrosis: a new concept of its pathophysiology. J Oral Maxillofac Surg 1983; 41:283288.
  7. Rossleigh MA, Smith J, Straus DJ, Engel IA. Osteonecrosis in patients with malignant lymphoma. A review of 31 cases. Cancer 1986; 58:11121116.
  8. Cook AM, Dzik-Jurasz AS, Padhani AR, Norman A, Huddart RA. The prevalence of avascular necrosis in patients treated with chemotherapy for testicular tumors. Br J Cancer 2001; 85:16241626.
  9. Marx RE. Pamidronate (Aredia) and zoledronate (Zometa) induced avascular necrosis of the jaws: a growing epidemic. J Oral Maxillofac Surg 2003; 61:11151117.
  10. Migliorati CA. Bisphosphonates and oral cavity avascular bone necrosis. J Clin Oncol 2003; 21:42534254.
  11. Ruggiero SL, Mehrotra B, Rosenberg TJ, Engroff SL. Osteonecrosis of the jaws associated with the use of bisphosphonates: a review of 63 cases. J Oral Maxillofac Surg 2004; 62:527534.
  12. Wright MM, Wright BM, Christian J, Carey JJ. A case series of osteonecrosis of the jaw associated with the use of bisphosphonates. Arthritis Rheum 2005; ( suppl Sept): 1984.
  13. National Center for Biotechnology Information. PubMed. www.ncbi.nlm.nih.gov/PubMed. Accessed 10/1/2008.
  14. American Dental Association Council on Scientific Affairs. Dental management of patients receiving oral bisphosphonate therapy: expert panel recommendations. J Am Dent Assoc 2006; 137:11441150.
  15. Woo SB, Hellstein JW, Kalmar JR. Narrative review: bisphosphonates and osteonecrosis of the jaws. Ann Intern Med 2006; 144:753761.
  16. Advisory Task Force on Bisphosphonate-Related Osteonecrosis of the Jaws, American Association of Oral and Maxillofacial Surgeons. American Association of Oral and Maxillofacial Surgeons position paper on bisphosphonate-related osteonecrosis of the jaws. J Oral Maxillofac Surg 2007; 65:369376.
  17. Khosla S, Burr D, Cauley J, et al; American Society for Bone and Mineral Research. Bishosphonate-associated osteonecrosis of the jaw: report of a task force of the American Society for Bone and Mineral Research. J Bone Miner Res 2007; 22:14791491.
  18. Ruggiero S, Gralow J, Marx R, et al. Practical guidelines for the prevention, diagnosis, and treatment of osteonecrosis of the jaw in patients with cancer. J Oncol Pract 2006; 2:714.
  19. Wang HL, Weber D, McCauley LK. Effect of long-term oral bisphosphonates on implant wound healing: literature review and a case report. J Periodontol 2007; 78:584594.
  20. Freiberger JJ, Padilla-Burgos R, Chhoeu AH, et al. Hyperbaric oxygen treatment and bisphosphonate-induced osteonecrosis of the jaw: a case series. J Oral Maxillofac Surg 2007; 65:13211327.
  21. Fleisch H. Bisphosphonates in Bone Disease. Fourth ed. San Diego, CA: Academic Press; 2000.
  22. Bone Health and Osteoporosis: A Report of the Surgeon General. www.surgeongeneral.gov/library/bonehealth. Accessed 10/1/2008.
  23. Carey JJ. What is a ‘failure’ of bisphosphonate therapy for osteoporosis? Cleve Clin J Med 2005; 72:10331039.
  24. Liberman UA, Weiss SR, Bröll J, et al. Effect of oral alendronate on bone mineral density and the incidence of fractures in postmenopausal osteoporosis. The Alendronate Phase III Osteoporosis Treatment Study Group. N Engl J Med 1995; 333:14371443.
  25. Black DM, Cummings SR, Karpf DB, et al. Randomised trial of effect of alendronate on risk of fracture in women with existing vertebral fractures. Fracture Intervention Trial Research Group. Lancet 1996; 348:15351541.
  26. Harris ST, Watts NB, Genant HK, et al. Effects of risedronate treatment on vertebral and nonvertebral fractures in women with postmenopausal osteoporosis: a randomized controlled trial. Vertebral Efficacy With Risedronate Therapy (VERT) Study Group. JAMA 1999; 282:13441352.
  27. McClung MR, Geusens P, Miller PD, et al; Hip Intervention Program Study Group. Effect of risedronate on the risk of hip fracture in elderly women. N Engl J Med 2001; 344:333340.
  28. Chesnut CH, Skag A, Christiansen C, et al; Oral Ibandronate Osteoporosis Vertebral Fracture Trial in North America and Europe (BONE). Effects of oral ibandronate administered daily or intermittently on fracture risk in postmenopausal osteoporosis. J Bone Miner Res 2004; 19:12411249.
  29. Black DM, Delmas PD, Eastell R, et al; HORIZON Pivotal Fracture Trial. Once-yearly zoledronic acid for treatment of postmenopausal osteoporosis. N Engl J Med 2007; 356:18091822.
  30. Lyles KW, Colón-Emeric CS, Magaziner JS, et al; HORIZON Recurrent Fracture Trial. Zoledronic acid and clinical fractures and mortality after hip fracture. N Engl J Med 2007; 357:17991809.
  31. Reid IR, Miller P, Lyles K, et al. Comparison of a single infusion of zoledronic acid with risedronate for Paget’s disease. N Engl J Med 2005; 353:898908.
  32. Bone HG, Santora AC. Authors Reply. N Engl J Med 2004; 351:191192.
  33. Conte P, Guarneri V. Safety of intravenous and oral bisphosphonates and compliance with dosing regimens. Oncologist 2004; 9(suppl 4):2837.
  34. Walter C, Grötz KA, Kunkel M, Al-Nawas B. Prevalence of bisphosphonate associated osteonecrosis of the jaw within the field of osteonecrosis. Support Care Cancer 2007; 15:197202.
  35. Zervas K, Verrou E, Teleioudis Z, et al. Incidence, risk factors and management of osteonecrosis of the jaws in patients with multiple myeloma: a single-centre experience in 303 patients. Br J Haematol 2006; 134:620623.
  36. Mortensen M, Lawson W, Montazem A. Osteonecrosis of the jaw associated with bisphosphonate use: presentation of seven cases and literature review. Laryngoscope 2007; 117:3034.
  37. Badros A, Weikel D, Salama A, et al. Osteonecrosis of the jaw in multiple myeloma patients: clinical features and risk factors. J Clin Oncol 2006; 24:945952.
  38. Durie BG, Katz M, Crowley J. Osteonecrosis of the jaw and bisphosphonates (letter). N Engl J Med 2005; 353:99100.
  39. Black DM, Schwartz AV, Ensrud KE, et al; FLEX Research Group. Effects of continuing or stopping alendronate after 5 years of treatment: the Fracture Intervention Trial Long-term Extension (FLEX): a randomized trial. JAMA 2006; 296:29272938.
  40. Gordis L. Epidemiology, 3rd ed. Philadelphia, Elsevier Saunders 2004:205.
  41. Fletcher RH, Fletcher SW, Wagner EH. Clinical Epidemiology. The Essentials. 3rd ed. Baltimore, MD; Lippincott, Williams & Wilkins, 1996:245.
  42. Sim J, Wright C. Research in Health Care, 1st ed. Cheltenham, England; Nelson Thornes, 2002.
  43. US Preventive Services Task Force Ratings. Strength of recommendations and quality of evidence. www.ahrq.gov/clinic/3rduspstf/ratings.htm. Accessed 10/1/2008.
  44. Mavrokokki T, Cheng A, Stein B, Goss A. Nature and frequency of bisphosphonate-associated osteonecrosis of the jaws in Australia. J Oral Maxillofac Surg 2007; 65:415423.
  45. Gibbs AE, Kherani A, Weitzel K, et al. Bisphosphonate-associated osteonecrosis: survey of oncologists. J Dent Res 2008; 87(special issue A):abstract #0639.
  46. Bone HG, Hosking D, Devogelaer JP, et al; Alendronate Phase III Osteoporosis Treatment Study Group. Ten years’ experience with alendronate for osteoporosis in postmenopausal women. N Engl J Med 2004; 350:11891199.
  47. Mellström DD, Sörensen OH, Goemaere S, Roux C, Johnson TD, Chines AA. Seven years of treatment with risedronate in women with postmenopausal osteoporosis. Calcif Tissue Int 2004; 75:462468.
  48. Bilezekian JP, Gold DT, Goldring S, et al. Discussions in Osteoporosis Issue 5, Feb 2006 5–7. Adelphia Inc.
  49. Grbic JT, Landesberg R, Lin SQ, et al; Health Outcomes and Reduced Incidence with Zoledronic Acid Once yearly Pivotal Fracture Trial Research Group. Incidence of osteonecrosis of the jaw in women with postmenopausal osteoporosis in the Health Outcomes and Reduced Incidence with Zoledronic Acid Once Yearly Pivotal Fracture Trial. J Am Dent Assoc 2008; 139:3240.
  50. Pazianas M, Blumentals WA, Miller PD. Lack of association between oral bisphosphonates and osteonecrosis using jaw surgery as a surrogate marker. Osteoporos Int 2007; Epub Nov 13.
  51. Cartsos VM, Zhu S, Zavras AI. Bisphosphonate use and the risk of adverse jaw outcomes. J Am Dent Assoc 2008; 139:2330.
  52. National Safety Council. The odds of dying from... www.nsc.org/lrs/statinfo/odds.htm. Accessed 10/1/2008.
  53. Palomo L, Bissada NF, Liu J. Periodontal assessment of postmenopausal women receiving risedronate. Menopause 2005; 12:685690.
  54. Rocha ML, Malacara JM, Sánchez-Marin FJ, Vazquez de la Torre CJ, Fajardo ME. Effect of alendronate on periodontal disease in postmenopausal women: a randomized placebo-controlled trial. J Periodontol 2004; 75:15791585.
  55. Jeffcoat MK, Cizza G, Shih WJ, Genco R, Lombardi A. Efficacy of bisphosphonates for the control of alveolar bone loss in periodontitis. J Int Acad Periodontol 2007; 9:7076.
  56. Little DG, Peat RA, Mcevoy A, Williams PR, Smith EJ, Baldock PA. Zoledronic acid treatment results in retention of femoral head structure after traumatic osteonecrosis in young Wistar rats. J Bone Miner Res 2003; 18:20162022.
  57. Agarwala S, Jain D, Joshi VR, Sule A. Efficacy of alendronate, a bisphosphonate, in the treatment of AVN of the hip. A prospective open-label study. Rheumatology (Oxf) 2005; 44:352359.
  58. Ramachandran M, Ward K, Brown RR, Munns CF, Cowell CT, Little DG. Intravenous bisphosphonate therapy for traumatic osteonecrosis of the femoral head in adolescents. J Bone Joint Surg Am 2007; 89:17271734.
  59. Kopterides P, Pikazis D, Koufos C. Successful treatment of SAPHO syndrome with zoledronic acid. Arthritis Rheum 2004; 50:29702973.
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Bisphosphonates and osteonecrosis of the jaw: Innocent association or significant risk?
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KEY POINTS

  • Recently published data do not support the hypothesis that these drugs cause osteonecrosis of the jaw.
  • There is no evidence to support routine dental examinations for all patients before starting bisphosphonate therapy for osteoporosis or Paget disease, but heightened concern seems warranted for cancer patients.
  • Clinical experience suggests that dental work by experienced dentists and surgeons can be carried out safely with very little risk to patients taking bisphosphonates.
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Parkinson disease: Not just a movement disorder

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Parkinson disease: Not just a movement disorder

Parkinson disease is characterized by tremor, rigidity, bradykinesia, and postural instability, but if we focus on these easily identified motor signs we risk overlooking the many nonmotor symptoms that coexist with them (Table 1).

These nonmotor symptoms—sensory, autonomic, and behavioral—are important to recognize, as they can lead to even more serious complications and impair quality of life.

COMMON, TROUBLESOME, AND UNDERDIAGNOSED

Nonmotor symptoms are very common. In fact, up to 60% of patients suffer from more than one nonmotor symptom, and 25% have four or more,1 including autonomic dysfunction, sensory symptoms, and cognitive and behavioral problems.2

Nonmotor symptoms can be primary complaints and, for some patients and family members, can cause greater disability than motor symptoms.3,4 For instance, depression and cognitive problems contribute to a decline in quality of life regardless of the degree of motor impairment.

Yet these symptoms are often underdiagnosed. 5 A delay in diagnosis may reflect the tendency of clinicians, patients, and family members to focus on the more apparent motor features of Parkinson disease, a lack of awareness of the nonmotor symptoms, or both. Consequently, patient education is essential. Identifying and treating these symptoms requires a multidisciplinary clinical team approach and an ongoing dialogue with the patient and family.

VARIOUS SYMPTOMS, VARIOUS CAUSES

Some nonmotor symptoms (eg, impaired sense of smell, depression, anxiety, fatigue, and constipation) can precede the motor symptoms of Parkinson disease and may be symptoms of the disease itself. Perhaps accounting for these observations, recent pathologic studies described diffuse Lewy body deposition in areas outside of nigral dopaminergic neurons,6,7 and the olfactory bulb, medulla, and pontine tegmentum may be involved before the substantia nigra.

Other symptoms, such as orthostatic hypotension, sedation, psychosis, confusion, and impulsiveness, may be adverse effects of medical therapy or may worsen with it.

Nonmotor symptoms can also emerge as a “wearing-off” phenomenon with standard treatment.2,8 The “off period” is a term primarily used to describe the reemergence of motor symptoms as a dose of levodopa wears off and before the patient receives the next dose. However, nonmotor symptoms, in particular depression and anxiety, can also occur in this period.

To treat nonmotor symptoms, one needs to identify and treat the primary symptom or the comorbid illnesses that may worsen it (eg, confusion in the setting of dehydration and infection), assess the possibility of adverse drug effects (a particular problem with many anti-Parkinson drugs), and try to reduce off periods with changes in dopaminergic therapy.

SENSORY SYMPTOMS

Off-period pain, paresthesia

Pain that cannot be attributed to muscle spasms, dystonia, somatic disease, autonomic dysfunction, or peripheral nerve disease occurs in up to 38% of patients with Parkinson disease.9,10 The pain is often diffuse and aching. Paresthesia-like complaints include numbness, tingling, and change in temperature.

Some sensory symptoms occur mostly during off periods and may respond to dopaminergic therapy. Examples are limb paresthesia, truncal pain, trigeminal neuralgia-like pain, and vaginal or perineal pain.9–11

Impaired sense of smell, vision

Impaired sense of smell can precede motor symptoms and is being investigated as a possible screening symptom for early diagnosis.12,13

Altered vision is a less recognized symptom of Parkinson disease. Many patients have difficulty reading even if they have normal visual acuity. Part of their difficulty stems from oculomotor defects such as impairment in visual saccadic movements and muscle rigidity.14 Visual pathways can be affected, as evidenced by abnormal visual evoked potentials that correlate with disease severity and by impairment in contrast sensitivity, color perception, and judgment of line orientation.15

It is unclear how these visual abnormalities contribute to everyday symptoms in Parkinson disease. Certainly, visual scanning activities such as reading are impaired.

Patients also suffer from drug-induced visual illusions and hallucinations, which are often colorful. Diederich et al16 found that contrast discrimination and color perception were significantly more impaired in Parkinson patients who have visual hallucinations, which suggests that it is important to correct visual abnormalities.

AUTONOMIC SYMPTOMS

In general, autonomic problems increase with age, disease severity, medication use, postural instability, cognitive decline, and visual hallucinations.17,18

Orthostatic hypotension

Almost half of patients with Parkinson disease have orthostatic hypotension.19 Of concern, patients with postural instability are at greater risk of orthostatic hypotension, thereby further increasing their risk of falling and injuring themselves.20

Postprandial hypotension is more common in Parkinson disease and is more often associated with midday meals, perhaps owing to a higher carbohydrate content and its effect on insulin release21 (many patients reserve high-protein meals for the evening and eat a greater proportion of carbohydrates during the day).

Home blood pressure monitoring is especially helpful, since blood pressure can fluctuate significantly and office readings may not reveal the problem.

Orthostatic hypotension can be both a drug side effect and a manifestation of the disease. Although all dopaminergic drugs can worsen orthostatic hypotension, the motor benefits of these drugs should be reviewed in relation to this risk. Dopaminergic agonists and amantadine (Symmetrel) should be used with caution in patients with significant orthostatic hypotension.

Treatment should include fluids, a highsalt diet, elastic stockings, fludrocortisone (Florinef), pyridostigmine (Mestinon), and perhaps the selective alpha 1 agonist midodrine (Proamatine). However, midodrine can cause supine hypertension and must be used cautiously in patients with advanced disease who take daytime naps because of fatigue. If postprandial hypotension is a problem, altering the patient's diet to include smaller but more frequent meals may help.

 

 

Cold limbs, sweating

Complaints related to temperature regulation include cold limbs and excessive sweating. Off-period drenching sweats occur as an endof- dose symptom thought to be related to subtherapeutic plasma dopamine levels and may respond to dopaminergic therapy aimed at reducing motor fluctuations and off periods.22

Gastrointestinal symptoms

Dysphagia (difficulty swallowing), sialorrhea (excessive salivation), nausea, constipation, and defecatory dysfunction are more common in patients with Parkinson disease than in agematched controls, even after controlling for factors such as drugs, autonomic dysfunction, diet, and exercise.23 These problems can cause malnutrition (necessitating a gastrostomy tube), aspiration pneumonia, and difficulty in swallowing and retaining pills,24 all of which can lead to problems that are even more serious. Although gastrointestinal symptoms occur in all stages of Parkinson disease, patients with advanced disease are at greater risk.

Dysphagia. James Parkinson described dysphagia and sialorrhea in his original 1816 monograph.25 The prevalence of dysphagia increases with severity of disease.23 Dysphagia is usually due to altered pharyngeal contraction, resulting in difficulty propelling food into the pharynx and retention of food in the pyriform sinuses and valleculae, but esophageal dilatation and dysmotility, spasms, gastroesophageal reflux, and increased transit time also contribute.24,26,27

Constipation may affect more than half of patients.28 One study reported a higher risk of developing Parkinson disease in men with infrequent bowel movements.29

Constipation and defecatory dysfunction can be severe enough to result in colonic dilatation and pseudo-obstruction.30 Altered gastrointestinal transit time may contribute to erratic absorption of medications.

Causes of constipation include slow colonic transit, weak abdominal muscles, decreased phasic contraction, and a paradoxical increase in puborectalis muscle and anal sphincter activity with straining, consistent with pelvic muscle dystonia.31

Treatment includes reducing off periods, limiting anticholinergic agents, prescribing a proper bowel regimen, and encouraging fluids and exercise. In addition, daily stool softeners, fiber, and polyethylene glycol are effective. Botulinum toxin injection into the puborectalis muscle may improve outlet obstruction.32

Risk of aspiration. Dysphagia, in association with respiratory symptoms, should prompt an evaluation for aspiration. Thickening liquids and early referral to a swallowing specialist may lessen the risk of aspiration.

Drooling is bothersome and embarrassing for many patients. Treatment historically included antimuscarinic agents, but these can cause constipation and confusion in patients with advanced disease. More recently, botulinum toxin injections into the parotid and submandibular glands have been shown to be effective in patients with excessive drooling.33

Urinary problems

Urologic abnormalities can be divided into dysfunction of the bladder, dysfunction of the urethral sphincter, and other causes of outflow obstruction such as prostate enlargement in men. The most common complaint is nocturia, followed by frequency and urgency.34

Nocturnal polyuria and urinary hesitancy and urgency are embarrassing but treatable. Urinary incontinence is a common reason for nursing home placement, and nocturia is a common cause of falls, as patients attempt to get up to urinate.35,36

Treatment of urinary incontinence should begin with an assessment for urinary tract infection, stress incontinence in women, and prostate enlargement in men. Urinary urgency due to detrusor hyperreflexia or spastic bladder can improve with anticholinergic antispasmodic agents. However, these should be used with caution in patients who are experiencing hallucinations or cognitive problems.

Sexual dysfunction

Sexual dysfunction, including decreased libido and erectile dysfunction, is in part related to autonomic dysfunction.

Treatment is complex, as these problems are multifactorial. Contributing factors include physical disability, the stress of living with a progressive illness, drug effects, depression, pain, difficulty in communication, caregiver stress, and impact on intimacy. The phosphodiesterase inhibitor sildenafil (Viagra) can improve erectile dysfunction, but must be used cautiously in patients with orthostatic hypotension.37 Other drugs of this class are available but have not been tested in this population.

COGNITIVE-BEHAVIORAL PROBLEMS

Neuropsychiatric disorders are common in Parkinson disease and at times can be more distressing to the patient and family than the motor symptoms. These include mood disorders, apathy, anxiety, impulse control disorders, psychosis, and dementia.

Dopaminergic medications used to treat movement can precipitate or exacerbate these neuropsychiatric problems. Therefore, treatment requires a balance between motor and neuropsychiatric benefits, with close dialogue with the patient and family about primary goals of treatment.

Depression

Depression is among the most common neuropsychiatric symptoms in Parkinson disease, occurring to some degree in up to 50% of patients.38 Diagnosing it is critical, because it can worsen physical symptoms, cognitive status, quality of life, and caregiver distress.39

However, depression can be difficult to recognize, because many of its features (eg, fatigue, psychomotor slowing, flattened affect, sleep difficulties) can also be manifestations of Parkinson disease. One should specifically ascertain whether the patient has a depressed mood or loss of interest in pleasurable activities. The Beck Depression Inventory is sensitive for depression in Parkinson disease and thus may be a reasonable screening tool.40

Treatment. Psychotherapy may help and may even be a first-line treatment in patients who cannot tolerate antidepressant drugs. Practical recommendations include relaxation techniques, a sleep hygiene regimen, engaging in meaningful activities to achieve a sense of purpose, and caregiver education.41

We have little evidence-based guidance on drug treatment of depression in patients with Parkinson disease. A recent meta-analysis found only two placebo-controlled studies in the past 40 years that monitored outcome based on a standardized rating scale of depression in patients with Parkinson disease.42

In preliminary studies, dopamine agonists have shown some efficacy in treating depression without Parkinson disease.43 However, the antidepressant contributions of anti-Parkinson drugs have not been well established.

Selective serotonin reuptake inhibitors (SSRIs) appear to be safe and well tolerated.44 Venlafaxine (Effexor) and mirtazapine (Remeron) are also reasonable initial options. Tricyclic antidepressants should be used with caution because they can cause anticholinergic side effects, especially confusion, in this population.

All serotonergic agents should be used with caution when given in combination with monoamine oxidase inhibitors, which are often used to treat motor symptoms in Parkinson disease, because of the risk of serotonin syndrome, which is characterized by fever, altered mental status, myoclonus, tremor, hyperreflexia, and diaphoresis and may be fatal.

Electroconvulsive therapy can be reserved for the treatment of severe refractory depression in patients with Parkinson disease without complex medical issues.45

 

 

Apathy

Apathy is present in approximately 30% of patients with Parkinson disease.46

Apathy can be very difficult to differentiate from depression, as the two disorders can occur together. Apathy can also be present without signs or symptoms of depressed mood. Apathy is commonly conceptualized as involving three domains: cognitive (lack of interest), behavioral (lack of initiation and drive), and affective (lack of emotion). The possibility of a primary apathy syndrome should be considered if the patient does not respond to standard treatments for depression. This is critical, as the treatment of the two syndromes may differ.47

Although efficacy data are limited, bupropion (Wellbutrin) and methylphenidate (Ritalin)48 can be tried for their activating or stimulant properties.

Anxiety disorders

Anxiety disorders commonly accompany depression in Parkinson disease, but they can also occur independently. They most often present in the setting of wearing-off or on-off fluctuations associated with medication status. Anxiety disorders in patients with Parkinson disease include generalized anxiety and panic attacks, which are responsive to SSRIs and benzodiazepines.49 Benzodiazepines are effective, and clonazepam (Klonopin) may be preferred because it has a long half-life, thereby minimizing anxiety associated with wearingoff or unpredictable off periods. Conversely, a long half-life and depressive effects may limit its use in advanced age.

Classic obsessive-compulsive disorder is less common, but obsessive behaviors and impulse control difficulties can occur in up to 7% of patients with Parkinson disease and presumably reflect dopamine dysregulation, most often associated with dopamine agonists.50 Impulsive behavior can include gambling, hypersexuality, and bingeing.

One form of obsessive-compulsive disorder is punding, a behavior characterized by intense fascination with repetitive handling and examining of objects, most often mechanical objects.51 Behaviors can include assembling and disassembling, collecting, or sorting of objects.

Visual hallucinations

Many patients with Parkinson disease have visual hallucinations as a side effect of dopaminergic drugs. At first, the patient realizes that they are hallucinations, but this insight may be lost as the disease progresses. The clinician should also consider other potential causes such as dementia, systemic illness, or psychosocial stress.

If visual hallucinations present early in the course of the disease and are accompanied by loss of insight and by cognitive fluctuations, the patient may actually have Lewy body dementia.52 Its features include parkinsonian symptoms, visual hallucinations, a fluctuating level of consciousness, and neuroleptic sensitivity.

Psychosis

The first-line treatment for psychosis in patients with Parkinson disease should involve:

  • Searching for a systemic illness such as urinary tract infection, aspiration pneumonia, or dehydration;
  • Stopping or lowering the dose of drugs that act on the central nervous system; and
  • If possible, stopping or lowering the dose of anti-Parkinson drugs that have the greatest risk of cognitive side effects. In many cases, this is not a realistic option, and adding an antipsychotic drug may be necessary.

Monitoring and treating psychosis is paramount, as it is a major risk factor for nursing home placement.53

Conventional neuroleptics such as haloperidol (Haldol) should be avoided because they can exacerbate parkinsonian symptoms.

Two atypical neuroleptics, clozapine (Clozaril) and quetiapine (Seroquel), appear to be the best tolerated in Parkinson disease patients. Clozapine is the only neuroleptic found to be more efficacious than placebo in patients with Parkinson disease.54 However, of the two, clozapine has a higher risk of side effects and requires frequent blood monitoring, making it difficult to use. Quetiapine has been shown to be as efficacious as clozapine,55 but it failed to show efficacy in a recent controlled study.56 Nevertheless, it is considered the first-line treatment option, since it is safer.40

Other atypical antipsychotics appear to exacerbate Parkinson disease or have not been adequately studied and should therefore be used with caution.

Dementia

Estimates of the prevalence of dementia in patients with Parkinson disease vary widely, most likely reflecting differences in populations studied and methods used. The best estimates indicate that 20% to 30% of patients with Parkinson disease develop dementia.57

Parkinson dementia is one of the classic subcortical dementias, characterized by slow thinking and by difficulties in working memory and problem-solving due to disruption of frontal-subcortical circuits.58 Its most common neuropsychiatric symptoms are hallucinations and depression, with less agitation, disinhibition, and irritability than in Alzheimer dementia.59

Anti-Parkinson drugs, especially anticholinergics, can exacerbate cognitive impairments in patients with Parkinson disease. An acute change in cognitive abilities or visual hallucinations is often associated with an un derlying medical illness such as infection (eg, a urinary tract infection or aspiration pneumonia) or dehydration.

Anticholinesterase inhibitors such as rivastigmine (Exelon) are indicated in patients with Parkinson dementia but may provide only a modest benefit.60

 

 

SLEEP DISORDERS

Excessive daytime sleepiness

Fatigue and hypersomnolence often impair quality of life.61 Daytime hypersomnolence is often multifactorial: it can be caused by the disease itself,62 by dopaminergic therapy,63,64 by a comorbid illness, or by nighttime sleep problems.

Sudden and uncontrollable episodes of sleep are an extreme form of hypersomnolence and are worrisome, especially with activities such as driving.65 Greater sleepiness (measured by the Epworth Sleepiness Scale), longer duration of Parkinson disease, and use of dopaminergic agonists increase the risk of such attacks.66 In general, very few patients experience such attacks without warning signs of sedation.

Treatment must include a comprehensive evaluation of current medications, the effect of dopaminergic agents (especially agonists), and nighttime factors that influence sleep (some of which are described below). Modafinil (Provigil), effective in narcolepsy, helped in some studies67 but not in others68; it could be tried in moderate to severe cases of excessive daytime sleepiness.

Sleep apnea contributes to daytime hypersomnolence. An evaluation for sleep apnea should be considered even in patients who are not overweight, as some evidence suggests that this disorder is common in Parkinson disease and correlates with disease severity.69

Insomnia

Sleep is impaired in up to 74% of Parkinson patients.70,71 A sleep study may show a low total sleep time, many awakenings, a short rapid-eye movement (REM) latency, and short slow-wave sleep (stages III and IV); the patient experiences the problem as light sleep with frequent awakenings.72 A variety of problems related to Parkinson disease can directly affect sleep patterns: eg, pain, stiffness, tremor, problems turning over in bed, dystonia, dementia, nocturia,73 depression, and anxiety.74

Restless legs syndrome

Restless legs syndrome is an uncomfortable, sometimes painful feeling in the legs or other body parts during rest (especially at night) that improves with movement.75 It may be more common in patients with Parkinson disease than in the general population76,77 and can precede the diagnosis of Parkinson disease.78

Iron supplementation with ferrous sulfate can help if iron deficiency (ferritin < 50 μg/L or iron saturation < 16%) is present but is ineffective in its absence. Levodopa and the dopaminergic agonists ropinirole (Requip)70 and pramipexole (Mirapex)80 are effective Parkinson disease treatments that also treat restless legs syndrome. In addition, opioids, clonazepam, and gabapentin (Gabarone) may help.81

Vivid dreams

Parkinson patients often describe very vivid, intense, frightening, and unpleasant dreams,73 which may be a precursor to psychosis.82

REM sleep behavior disorder is characterized by sustained phasic muscle activity in place of normal atonia during REM or dream sleep. The patient's bed partner may describe him or her behaving in an aggressive way as if acting out his or her dreams, ie, hitting, yelling, or kicking. Upon awakening, the patient's recall of the dream content is consistent with the nocturnal behavior.

REM sleep behavior disorder may actually precede the motor symptoms of Parkinson disease,83,84 and as many as 20% of patents with REM sleep behavior disorder eventually develop Parkinson disease.85 The possible link between the two disorders is strengthened by a case report describing a patient with REM sleep behavior disorder, no signs of Parkinson disease on examination, but brain pathology similar to that found in Parkinson disease.86

Clonazepam is an effective treatment for REM sleep behavior disorder and should be considered if sleep is disrupted or patient safety becomes a concern.87

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  73. van Hilten JJ, Weggeman M, van der Velde EA, Kerkhof GA, van Dijk JG, Roos RA. Sleep, excessive daytime sleepiness and fatigue in Parkinson's disease. J Neural Transm Park Dis Dement Sect 1993; 5:235244.
  74. Borek LL, Kohn R, Friedman JH. Mood and sleep in Parkinson's disease. J Clin Psychiatry 2006; 67:958963.
  75. Walters AS, Hening W. Clinical presentation and neuropharmacology of restless legs syndrome. Clin Neuropharmacol 1987; 10:225237.
  76. Krishnan PR, Bhatia M, Behari M. Restless leg syndrome in Parkinson's disease: a case-controlled study. Mov Disord 2003; 18:181185.
  77. Ondo WG, Vuong KD, Jankovic J. Exploring the relationship between Parkinson disease and restless legs syndrome. Arch Neurol 2002; 59:421424.
  78. Lang AE. Restless legs syndrome and Parkinson's disease: insights into pathophysiology. Clin Neuropharmacol 1987; 10:476478.
  79. Bogan RK, Fry JM, Schmidt MH, Carson SW, Ritchie SY; TREAT RLS US Study Group. Ropinirole in the treatment of patients with restless legs syndrome: a US-based randomized, double-blind, placebo-controlled clinical trial. Mayo Clin Proc 2006; 81:1727.
  80. Winkelman JW, Sethi KD, Kushida CA, et al. Efficacy and safety of pramipexole in restless legs syndrome. Neurology 2006; 67:10341039.
  81. Thorpy MJ. New paradigms in the treatment of restless legs syndrome. Neurology 2005; 64(supp 3):S28S33.
  82. Moskovitz C, Hoses H, Klawans H. Levodopa-induced psychosis: a kindling phenomenon. Am J Psychiatry 1978; 135:669675.
  83. Hickey MM, Demaerschalk BM, Casaelli RJ, Parish JM, Wingerchuk DM. “Idiopathic” rapid-eye-movement (REM) sleep behavior disorder is associated with future development of neurodegenerative diseases. Neurologist 2007; 13:98101.
  84. Tan A, Salgado M, Fahn S. Rapid eye movement sleep behavior disorder preceding Parkinson's disease with therapeutic response to levodopa. Mov Disord 1996; 11:214216.
  85. Schenck CH, Bundlie SR, Mahowald MW. Delayed emergence of a parkinsonian disorder in 38% of 29 older men initially diagnosed with idiopathic rapid eye movement sleep behavior disorder. Neurology 1996; 46:388393.
  86. Uchiyama M, Isse K, Tanaka K, et al. Incidental Lewy body disease in patients with REM sleep behavior disorder. Neurology 1995; 45:709712.
  87. Iranzo A, Santamaria J, Rye DB, et al. Characteristics of idiopathic REM sleep behavior disorder and that associated with MSA and Parkinson disease. Neurology 2005; 65:247252.
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Monique L. Giroux, MD
Booth Gardner Parkinson's Care Center, Evergreen Hospital, Kirkland, WA

Address: Monique L. Giroux, MD, Booth Gardner Parkinson’s Care Center, Evergreen Hospital, 13030 121st Way NE Suite 203, Kirkland, WA 98034; e-mail [email protected]

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Booth Gardner Parkinson's Care Center, Evergreen Hospital, Kirkland, WA

Address: Monique L. Giroux, MD, Booth Gardner Parkinson’s Care Center, Evergreen Hospital, 13030 121st Way NE Suite 203, Kirkland, WA 98034; e-mail [email protected]

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Monique L. Giroux, MD
Booth Gardner Parkinson's Care Center, Evergreen Hospital, Kirkland, WA

Address: Monique L. Giroux, MD, Booth Gardner Parkinson’s Care Center, Evergreen Hospital, 13030 121st Way NE Suite 203, Kirkland, WA 98034; e-mail [email protected]

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Parkinson disease is characterized by tremor, rigidity, bradykinesia, and postural instability, but if we focus on these easily identified motor signs we risk overlooking the many nonmotor symptoms that coexist with them (Table 1).

These nonmotor symptoms—sensory, autonomic, and behavioral—are important to recognize, as they can lead to even more serious complications and impair quality of life.

COMMON, TROUBLESOME, AND UNDERDIAGNOSED

Nonmotor symptoms are very common. In fact, up to 60% of patients suffer from more than one nonmotor symptom, and 25% have four or more,1 including autonomic dysfunction, sensory symptoms, and cognitive and behavioral problems.2

Nonmotor symptoms can be primary complaints and, for some patients and family members, can cause greater disability than motor symptoms.3,4 For instance, depression and cognitive problems contribute to a decline in quality of life regardless of the degree of motor impairment.

Yet these symptoms are often underdiagnosed. 5 A delay in diagnosis may reflect the tendency of clinicians, patients, and family members to focus on the more apparent motor features of Parkinson disease, a lack of awareness of the nonmotor symptoms, or both. Consequently, patient education is essential. Identifying and treating these symptoms requires a multidisciplinary clinical team approach and an ongoing dialogue with the patient and family.

VARIOUS SYMPTOMS, VARIOUS CAUSES

Some nonmotor symptoms (eg, impaired sense of smell, depression, anxiety, fatigue, and constipation) can precede the motor symptoms of Parkinson disease and may be symptoms of the disease itself. Perhaps accounting for these observations, recent pathologic studies described diffuse Lewy body deposition in areas outside of nigral dopaminergic neurons,6,7 and the olfactory bulb, medulla, and pontine tegmentum may be involved before the substantia nigra.

Other symptoms, such as orthostatic hypotension, sedation, psychosis, confusion, and impulsiveness, may be adverse effects of medical therapy or may worsen with it.

Nonmotor symptoms can also emerge as a “wearing-off” phenomenon with standard treatment.2,8 The “off period” is a term primarily used to describe the reemergence of motor symptoms as a dose of levodopa wears off and before the patient receives the next dose. However, nonmotor symptoms, in particular depression and anxiety, can also occur in this period.

To treat nonmotor symptoms, one needs to identify and treat the primary symptom or the comorbid illnesses that may worsen it (eg, confusion in the setting of dehydration and infection), assess the possibility of adverse drug effects (a particular problem with many anti-Parkinson drugs), and try to reduce off periods with changes in dopaminergic therapy.

SENSORY SYMPTOMS

Off-period pain, paresthesia

Pain that cannot be attributed to muscle spasms, dystonia, somatic disease, autonomic dysfunction, or peripheral nerve disease occurs in up to 38% of patients with Parkinson disease.9,10 The pain is often diffuse and aching. Paresthesia-like complaints include numbness, tingling, and change in temperature.

Some sensory symptoms occur mostly during off periods and may respond to dopaminergic therapy. Examples are limb paresthesia, truncal pain, trigeminal neuralgia-like pain, and vaginal or perineal pain.9–11

Impaired sense of smell, vision

Impaired sense of smell can precede motor symptoms and is being investigated as a possible screening symptom for early diagnosis.12,13

Altered vision is a less recognized symptom of Parkinson disease. Many patients have difficulty reading even if they have normal visual acuity. Part of their difficulty stems from oculomotor defects such as impairment in visual saccadic movements and muscle rigidity.14 Visual pathways can be affected, as evidenced by abnormal visual evoked potentials that correlate with disease severity and by impairment in contrast sensitivity, color perception, and judgment of line orientation.15

It is unclear how these visual abnormalities contribute to everyday symptoms in Parkinson disease. Certainly, visual scanning activities such as reading are impaired.

Patients also suffer from drug-induced visual illusions and hallucinations, which are often colorful. Diederich et al16 found that contrast discrimination and color perception were significantly more impaired in Parkinson patients who have visual hallucinations, which suggests that it is important to correct visual abnormalities.

AUTONOMIC SYMPTOMS

In general, autonomic problems increase with age, disease severity, medication use, postural instability, cognitive decline, and visual hallucinations.17,18

Orthostatic hypotension

Almost half of patients with Parkinson disease have orthostatic hypotension.19 Of concern, patients with postural instability are at greater risk of orthostatic hypotension, thereby further increasing their risk of falling and injuring themselves.20

Postprandial hypotension is more common in Parkinson disease and is more often associated with midday meals, perhaps owing to a higher carbohydrate content and its effect on insulin release21 (many patients reserve high-protein meals for the evening and eat a greater proportion of carbohydrates during the day).

Home blood pressure monitoring is especially helpful, since blood pressure can fluctuate significantly and office readings may not reveal the problem.

Orthostatic hypotension can be both a drug side effect and a manifestation of the disease. Although all dopaminergic drugs can worsen orthostatic hypotension, the motor benefits of these drugs should be reviewed in relation to this risk. Dopaminergic agonists and amantadine (Symmetrel) should be used with caution in patients with significant orthostatic hypotension.

Treatment should include fluids, a highsalt diet, elastic stockings, fludrocortisone (Florinef), pyridostigmine (Mestinon), and perhaps the selective alpha 1 agonist midodrine (Proamatine). However, midodrine can cause supine hypertension and must be used cautiously in patients with advanced disease who take daytime naps because of fatigue. If postprandial hypotension is a problem, altering the patient's diet to include smaller but more frequent meals may help.

 

 

Cold limbs, sweating

Complaints related to temperature regulation include cold limbs and excessive sweating. Off-period drenching sweats occur as an endof- dose symptom thought to be related to subtherapeutic plasma dopamine levels and may respond to dopaminergic therapy aimed at reducing motor fluctuations and off periods.22

Gastrointestinal symptoms

Dysphagia (difficulty swallowing), sialorrhea (excessive salivation), nausea, constipation, and defecatory dysfunction are more common in patients with Parkinson disease than in agematched controls, even after controlling for factors such as drugs, autonomic dysfunction, diet, and exercise.23 These problems can cause malnutrition (necessitating a gastrostomy tube), aspiration pneumonia, and difficulty in swallowing and retaining pills,24 all of which can lead to problems that are even more serious. Although gastrointestinal symptoms occur in all stages of Parkinson disease, patients with advanced disease are at greater risk.

Dysphagia. James Parkinson described dysphagia and sialorrhea in his original 1816 monograph.25 The prevalence of dysphagia increases with severity of disease.23 Dysphagia is usually due to altered pharyngeal contraction, resulting in difficulty propelling food into the pharynx and retention of food in the pyriform sinuses and valleculae, but esophageal dilatation and dysmotility, spasms, gastroesophageal reflux, and increased transit time also contribute.24,26,27

Constipation may affect more than half of patients.28 One study reported a higher risk of developing Parkinson disease in men with infrequent bowel movements.29

Constipation and defecatory dysfunction can be severe enough to result in colonic dilatation and pseudo-obstruction.30 Altered gastrointestinal transit time may contribute to erratic absorption of medications.

Causes of constipation include slow colonic transit, weak abdominal muscles, decreased phasic contraction, and a paradoxical increase in puborectalis muscle and anal sphincter activity with straining, consistent with pelvic muscle dystonia.31

Treatment includes reducing off periods, limiting anticholinergic agents, prescribing a proper bowel regimen, and encouraging fluids and exercise. In addition, daily stool softeners, fiber, and polyethylene glycol are effective. Botulinum toxin injection into the puborectalis muscle may improve outlet obstruction.32

Risk of aspiration. Dysphagia, in association with respiratory symptoms, should prompt an evaluation for aspiration. Thickening liquids and early referral to a swallowing specialist may lessen the risk of aspiration.

Drooling is bothersome and embarrassing for many patients. Treatment historically included antimuscarinic agents, but these can cause constipation and confusion in patients with advanced disease. More recently, botulinum toxin injections into the parotid and submandibular glands have been shown to be effective in patients with excessive drooling.33

Urinary problems

Urologic abnormalities can be divided into dysfunction of the bladder, dysfunction of the urethral sphincter, and other causes of outflow obstruction such as prostate enlargement in men. The most common complaint is nocturia, followed by frequency and urgency.34

Nocturnal polyuria and urinary hesitancy and urgency are embarrassing but treatable. Urinary incontinence is a common reason for nursing home placement, and nocturia is a common cause of falls, as patients attempt to get up to urinate.35,36

Treatment of urinary incontinence should begin with an assessment for urinary tract infection, stress incontinence in women, and prostate enlargement in men. Urinary urgency due to detrusor hyperreflexia or spastic bladder can improve with anticholinergic antispasmodic agents. However, these should be used with caution in patients who are experiencing hallucinations or cognitive problems.

Sexual dysfunction

Sexual dysfunction, including decreased libido and erectile dysfunction, is in part related to autonomic dysfunction.

Treatment is complex, as these problems are multifactorial. Contributing factors include physical disability, the stress of living with a progressive illness, drug effects, depression, pain, difficulty in communication, caregiver stress, and impact on intimacy. The phosphodiesterase inhibitor sildenafil (Viagra) can improve erectile dysfunction, but must be used cautiously in patients with orthostatic hypotension.37 Other drugs of this class are available but have not been tested in this population.

COGNITIVE-BEHAVIORAL PROBLEMS

Neuropsychiatric disorders are common in Parkinson disease and at times can be more distressing to the patient and family than the motor symptoms. These include mood disorders, apathy, anxiety, impulse control disorders, psychosis, and dementia.

Dopaminergic medications used to treat movement can precipitate or exacerbate these neuropsychiatric problems. Therefore, treatment requires a balance between motor and neuropsychiatric benefits, with close dialogue with the patient and family about primary goals of treatment.

Depression

Depression is among the most common neuropsychiatric symptoms in Parkinson disease, occurring to some degree in up to 50% of patients.38 Diagnosing it is critical, because it can worsen physical symptoms, cognitive status, quality of life, and caregiver distress.39

However, depression can be difficult to recognize, because many of its features (eg, fatigue, psychomotor slowing, flattened affect, sleep difficulties) can also be manifestations of Parkinson disease. One should specifically ascertain whether the patient has a depressed mood or loss of interest in pleasurable activities. The Beck Depression Inventory is sensitive for depression in Parkinson disease and thus may be a reasonable screening tool.40

Treatment. Psychotherapy may help and may even be a first-line treatment in patients who cannot tolerate antidepressant drugs. Practical recommendations include relaxation techniques, a sleep hygiene regimen, engaging in meaningful activities to achieve a sense of purpose, and caregiver education.41

We have little evidence-based guidance on drug treatment of depression in patients with Parkinson disease. A recent meta-analysis found only two placebo-controlled studies in the past 40 years that monitored outcome based on a standardized rating scale of depression in patients with Parkinson disease.42

In preliminary studies, dopamine agonists have shown some efficacy in treating depression without Parkinson disease.43 However, the antidepressant contributions of anti-Parkinson drugs have not been well established.

Selective serotonin reuptake inhibitors (SSRIs) appear to be safe and well tolerated.44 Venlafaxine (Effexor) and mirtazapine (Remeron) are also reasonable initial options. Tricyclic antidepressants should be used with caution because they can cause anticholinergic side effects, especially confusion, in this population.

All serotonergic agents should be used with caution when given in combination with monoamine oxidase inhibitors, which are often used to treat motor symptoms in Parkinson disease, because of the risk of serotonin syndrome, which is characterized by fever, altered mental status, myoclonus, tremor, hyperreflexia, and diaphoresis and may be fatal.

Electroconvulsive therapy can be reserved for the treatment of severe refractory depression in patients with Parkinson disease without complex medical issues.45

 

 

Apathy

Apathy is present in approximately 30% of patients with Parkinson disease.46

Apathy can be very difficult to differentiate from depression, as the two disorders can occur together. Apathy can also be present without signs or symptoms of depressed mood. Apathy is commonly conceptualized as involving three domains: cognitive (lack of interest), behavioral (lack of initiation and drive), and affective (lack of emotion). The possibility of a primary apathy syndrome should be considered if the patient does not respond to standard treatments for depression. This is critical, as the treatment of the two syndromes may differ.47

Although efficacy data are limited, bupropion (Wellbutrin) and methylphenidate (Ritalin)48 can be tried for their activating or stimulant properties.

Anxiety disorders

Anxiety disorders commonly accompany depression in Parkinson disease, but they can also occur independently. They most often present in the setting of wearing-off or on-off fluctuations associated with medication status. Anxiety disorders in patients with Parkinson disease include generalized anxiety and panic attacks, which are responsive to SSRIs and benzodiazepines.49 Benzodiazepines are effective, and clonazepam (Klonopin) may be preferred because it has a long half-life, thereby minimizing anxiety associated with wearingoff or unpredictable off periods. Conversely, a long half-life and depressive effects may limit its use in advanced age.

Classic obsessive-compulsive disorder is less common, but obsessive behaviors and impulse control difficulties can occur in up to 7% of patients with Parkinson disease and presumably reflect dopamine dysregulation, most often associated with dopamine agonists.50 Impulsive behavior can include gambling, hypersexuality, and bingeing.

One form of obsessive-compulsive disorder is punding, a behavior characterized by intense fascination with repetitive handling and examining of objects, most often mechanical objects.51 Behaviors can include assembling and disassembling, collecting, or sorting of objects.

Visual hallucinations

Many patients with Parkinson disease have visual hallucinations as a side effect of dopaminergic drugs. At first, the patient realizes that they are hallucinations, but this insight may be lost as the disease progresses. The clinician should also consider other potential causes such as dementia, systemic illness, or psychosocial stress.

If visual hallucinations present early in the course of the disease and are accompanied by loss of insight and by cognitive fluctuations, the patient may actually have Lewy body dementia.52 Its features include parkinsonian symptoms, visual hallucinations, a fluctuating level of consciousness, and neuroleptic sensitivity.

Psychosis

The first-line treatment for psychosis in patients with Parkinson disease should involve:

  • Searching for a systemic illness such as urinary tract infection, aspiration pneumonia, or dehydration;
  • Stopping or lowering the dose of drugs that act on the central nervous system; and
  • If possible, stopping or lowering the dose of anti-Parkinson drugs that have the greatest risk of cognitive side effects. In many cases, this is not a realistic option, and adding an antipsychotic drug may be necessary.

Monitoring and treating psychosis is paramount, as it is a major risk factor for nursing home placement.53

Conventional neuroleptics such as haloperidol (Haldol) should be avoided because they can exacerbate parkinsonian symptoms.

Two atypical neuroleptics, clozapine (Clozaril) and quetiapine (Seroquel), appear to be the best tolerated in Parkinson disease patients. Clozapine is the only neuroleptic found to be more efficacious than placebo in patients with Parkinson disease.54 However, of the two, clozapine has a higher risk of side effects and requires frequent blood monitoring, making it difficult to use. Quetiapine has been shown to be as efficacious as clozapine,55 but it failed to show efficacy in a recent controlled study.56 Nevertheless, it is considered the first-line treatment option, since it is safer.40

Other atypical antipsychotics appear to exacerbate Parkinson disease or have not been adequately studied and should therefore be used with caution.

Dementia

Estimates of the prevalence of dementia in patients with Parkinson disease vary widely, most likely reflecting differences in populations studied and methods used. The best estimates indicate that 20% to 30% of patients with Parkinson disease develop dementia.57

Parkinson dementia is one of the classic subcortical dementias, characterized by slow thinking and by difficulties in working memory and problem-solving due to disruption of frontal-subcortical circuits.58 Its most common neuropsychiatric symptoms are hallucinations and depression, with less agitation, disinhibition, and irritability than in Alzheimer dementia.59

Anti-Parkinson drugs, especially anticholinergics, can exacerbate cognitive impairments in patients with Parkinson disease. An acute change in cognitive abilities or visual hallucinations is often associated with an un derlying medical illness such as infection (eg, a urinary tract infection or aspiration pneumonia) or dehydration.

Anticholinesterase inhibitors such as rivastigmine (Exelon) are indicated in patients with Parkinson dementia but may provide only a modest benefit.60

 

 

SLEEP DISORDERS

Excessive daytime sleepiness

Fatigue and hypersomnolence often impair quality of life.61 Daytime hypersomnolence is often multifactorial: it can be caused by the disease itself,62 by dopaminergic therapy,63,64 by a comorbid illness, or by nighttime sleep problems.

Sudden and uncontrollable episodes of sleep are an extreme form of hypersomnolence and are worrisome, especially with activities such as driving.65 Greater sleepiness (measured by the Epworth Sleepiness Scale), longer duration of Parkinson disease, and use of dopaminergic agonists increase the risk of such attacks.66 In general, very few patients experience such attacks without warning signs of sedation.

Treatment must include a comprehensive evaluation of current medications, the effect of dopaminergic agents (especially agonists), and nighttime factors that influence sleep (some of which are described below). Modafinil (Provigil), effective in narcolepsy, helped in some studies67 but not in others68; it could be tried in moderate to severe cases of excessive daytime sleepiness.

Sleep apnea contributes to daytime hypersomnolence. An evaluation for sleep apnea should be considered even in patients who are not overweight, as some evidence suggests that this disorder is common in Parkinson disease and correlates with disease severity.69

Insomnia

Sleep is impaired in up to 74% of Parkinson patients.70,71 A sleep study may show a low total sleep time, many awakenings, a short rapid-eye movement (REM) latency, and short slow-wave sleep (stages III and IV); the patient experiences the problem as light sleep with frequent awakenings.72 A variety of problems related to Parkinson disease can directly affect sleep patterns: eg, pain, stiffness, tremor, problems turning over in bed, dystonia, dementia, nocturia,73 depression, and anxiety.74

Restless legs syndrome

Restless legs syndrome is an uncomfortable, sometimes painful feeling in the legs or other body parts during rest (especially at night) that improves with movement.75 It may be more common in patients with Parkinson disease than in the general population76,77 and can precede the diagnosis of Parkinson disease.78

Iron supplementation with ferrous sulfate can help if iron deficiency (ferritin < 50 μg/L or iron saturation < 16%) is present but is ineffective in its absence. Levodopa and the dopaminergic agonists ropinirole (Requip)70 and pramipexole (Mirapex)80 are effective Parkinson disease treatments that also treat restless legs syndrome. In addition, opioids, clonazepam, and gabapentin (Gabarone) may help.81

Vivid dreams

Parkinson patients often describe very vivid, intense, frightening, and unpleasant dreams,73 which may be a precursor to psychosis.82

REM sleep behavior disorder is characterized by sustained phasic muscle activity in place of normal atonia during REM or dream sleep. The patient's bed partner may describe him or her behaving in an aggressive way as if acting out his or her dreams, ie, hitting, yelling, or kicking. Upon awakening, the patient's recall of the dream content is consistent with the nocturnal behavior.

REM sleep behavior disorder may actually precede the motor symptoms of Parkinson disease,83,84 and as many as 20% of patents with REM sleep behavior disorder eventually develop Parkinson disease.85 The possible link between the two disorders is strengthened by a case report describing a patient with REM sleep behavior disorder, no signs of Parkinson disease on examination, but brain pathology similar to that found in Parkinson disease.86

Clonazepam is an effective treatment for REM sleep behavior disorder and should be considered if sleep is disrupted or patient safety becomes a concern.87

Parkinson disease is characterized by tremor, rigidity, bradykinesia, and postural instability, but if we focus on these easily identified motor signs we risk overlooking the many nonmotor symptoms that coexist with them (Table 1).

These nonmotor symptoms—sensory, autonomic, and behavioral—are important to recognize, as they can lead to even more serious complications and impair quality of life.

COMMON, TROUBLESOME, AND UNDERDIAGNOSED

Nonmotor symptoms are very common. In fact, up to 60% of patients suffer from more than one nonmotor symptom, and 25% have four or more,1 including autonomic dysfunction, sensory symptoms, and cognitive and behavioral problems.2

Nonmotor symptoms can be primary complaints and, for some patients and family members, can cause greater disability than motor symptoms.3,4 For instance, depression and cognitive problems contribute to a decline in quality of life regardless of the degree of motor impairment.

Yet these symptoms are often underdiagnosed. 5 A delay in diagnosis may reflect the tendency of clinicians, patients, and family members to focus on the more apparent motor features of Parkinson disease, a lack of awareness of the nonmotor symptoms, or both. Consequently, patient education is essential. Identifying and treating these symptoms requires a multidisciplinary clinical team approach and an ongoing dialogue with the patient and family.

VARIOUS SYMPTOMS, VARIOUS CAUSES

Some nonmotor symptoms (eg, impaired sense of smell, depression, anxiety, fatigue, and constipation) can precede the motor symptoms of Parkinson disease and may be symptoms of the disease itself. Perhaps accounting for these observations, recent pathologic studies described diffuse Lewy body deposition in areas outside of nigral dopaminergic neurons,6,7 and the olfactory bulb, medulla, and pontine tegmentum may be involved before the substantia nigra.

Other symptoms, such as orthostatic hypotension, sedation, psychosis, confusion, and impulsiveness, may be adverse effects of medical therapy or may worsen with it.

Nonmotor symptoms can also emerge as a “wearing-off” phenomenon with standard treatment.2,8 The “off period” is a term primarily used to describe the reemergence of motor symptoms as a dose of levodopa wears off and before the patient receives the next dose. However, nonmotor symptoms, in particular depression and anxiety, can also occur in this period.

To treat nonmotor symptoms, one needs to identify and treat the primary symptom or the comorbid illnesses that may worsen it (eg, confusion in the setting of dehydration and infection), assess the possibility of adverse drug effects (a particular problem with many anti-Parkinson drugs), and try to reduce off periods with changes in dopaminergic therapy.

SENSORY SYMPTOMS

Off-period pain, paresthesia

Pain that cannot be attributed to muscle spasms, dystonia, somatic disease, autonomic dysfunction, or peripheral nerve disease occurs in up to 38% of patients with Parkinson disease.9,10 The pain is often diffuse and aching. Paresthesia-like complaints include numbness, tingling, and change in temperature.

Some sensory symptoms occur mostly during off periods and may respond to dopaminergic therapy. Examples are limb paresthesia, truncal pain, trigeminal neuralgia-like pain, and vaginal or perineal pain.9–11

Impaired sense of smell, vision

Impaired sense of smell can precede motor symptoms and is being investigated as a possible screening symptom for early diagnosis.12,13

Altered vision is a less recognized symptom of Parkinson disease. Many patients have difficulty reading even if they have normal visual acuity. Part of their difficulty stems from oculomotor defects such as impairment in visual saccadic movements and muscle rigidity.14 Visual pathways can be affected, as evidenced by abnormal visual evoked potentials that correlate with disease severity and by impairment in contrast sensitivity, color perception, and judgment of line orientation.15

It is unclear how these visual abnormalities contribute to everyday symptoms in Parkinson disease. Certainly, visual scanning activities such as reading are impaired.

Patients also suffer from drug-induced visual illusions and hallucinations, which are often colorful. Diederich et al16 found that contrast discrimination and color perception were significantly more impaired in Parkinson patients who have visual hallucinations, which suggests that it is important to correct visual abnormalities.

AUTONOMIC SYMPTOMS

In general, autonomic problems increase with age, disease severity, medication use, postural instability, cognitive decline, and visual hallucinations.17,18

Orthostatic hypotension

Almost half of patients with Parkinson disease have orthostatic hypotension.19 Of concern, patients with postural instability are at greater risk of orthostatic hypotension, thereby further increasing their risk of falling and injuring themselves.20

Postprandial hypotension is more common in Parkinson disease and is more often associated with midday meals, perhaps owing to a higher carbohydrate content and its effect on insulin release21 (many patients reserve high-protein meals for the evening and eat a greater proportion of carbohydrates during the day).

Home blood pressure monitoring is especially helpful, since blood pressure can fluctuate significantly and office readings may not reveal the problem.

Orthostatic hypotension can be both a drug side effect and a manifestation of the disease. Although all dopaminergic drugs can worsen orthostatic hypotension, the motor benefits of these drugs should be reviewed in relation to this risk. Dopaminergic agonists and amantadine (Symmetrel) should be used with caution in patients with significant orthostatic hypotension.

Treatment should include fluids, a highsalt diet, elastic stockings, fludrocortisone (Florinef), pyridostigmine (Mestinon), and perhaps the selective alpha 1 agonist midodrine (Proamatine). However, midodrine can cause supine hypertension and must be used cautiously in patients with advanced disease who take daytime naps because of fatigue. If postprandial hypotension is a problem, altering the patient's diet to include smaller but more frequent meals may help.

 

 

Cold limbs, sweating

Complaints related to temperature regulation include cold limbs and excessive sweating. Off-period drenching sweats occur as an endof- dose symptom thought to be related to subtherapeutic plasma dopamine levels and may respond to dopaminergic therapy aimed at reducing motor fluctuations and off periods.22

Gastrointestinal symptoms

Dysphagia (difficulty swallowing), sialorrhea (excessive salivation), nausea, constipation, and defecatory dysfunction are more common in patients with Parkinson disease than in agematched controls, even after controlling for factors such as drugs, autonomic dysfunction, diet, and exercise.23 These problems can cause malnutrition (necessitating a gastrostomy tube), aspiration pneumonia, and difficulty in swallowing and retaining pills,24 all of which can lead to problems that are even more serious. Although gastrointestinal symptoms occur in all stages of Parkinson disease, patients with advanced disease are at greater risk.

Dysphagia. James Parkinson described dysphagia and sialorrhea in his original 1816 monograph.25 The prevalence of dysphagia increases with severity of disease.23 Dysphagia is usually due to altered pharyngeal contraction, resulting in difficulty propelling food into the pharynx and retention of food in the pyriform sinuses and valleculae, but esophageal dilatation and dysmotility, spasms, gastroesophageal reflux, and increased transit time also contribute.24,26,27

Constipation may affect more than half of patients.28 One study reported a higher risk of developing Parkinson disease in men with infrequent bowel movements.29

Constipation and defecatory dysfunction can be severe enough to result in colonic dilatation and pseudo-obstruction.30 Altered gastrointestinal transit time may contribute to erratic absorption of medications.

Causes of constipation include slow colonic transit, weak abdominal muscles, decreased phasic contraction, and a paradoxical increase in puborectalis muscle and anal sphincter activity with straining, consistent with pelvic muscle dystonia.31

Treatment includes reducing off periods, limiting anticholinergic agents, prescribing a proper bowel regimen, and encouraging fluids and exercise. In addition, daily stool softeners, fiber, and polyethylene glycol are effective. Botulinum toxin injection into the puborectalis muscle may improve outlet obstruction.32

Risk of aspiration. Dysphagia, in association with respiratory symptoms, should prompt an evaluation for aspiration. Thickening liquids and early referral to a swallowing specialist may lessen the risk of aspiration.

Drooling is bothersome and embarrassing for many patients. Treatment historically included antimuscarinic agents, but these can cause constipation and confusion in patients with advanced disease. More recently, botulinum toxin injections into the parotid and submandibular glands have been shown to be effective in patients with excessive drooling.33

Urinary problems

Urologic abnormalities can be divided into dysfunction of the bladder, dysfunction of the urethral sphincter, and other causes of outflow obstruction such as prostate enlargement in men. The most common complaint is nocturia, followed by frequency and urgency.34

Nocturnal polyuria and urinary hesitancy and urgency are embarrassing but treatable. Urinary incontinence is a common reason for nursing home placement, and nocturia is a common cause of falls, as patients attempt to get up to urinate.35,36

Treatment of urinary incontinence should begin with an assessment for urinary tract infection, stress incontinence in women, and prostate enlargement in men. Urinary urgency due to detrusor hyperreflexia or spastic bladder can improve with anticholinergic antispasmodic agents. However, these should be used with caution in patients who are experiencing hallucinations or cognitive problems.

Sexual dysfunction

Sexual dysfunction, including decreased libido and erectile dysfunction, is in part related to autonomic dysfunction.

Treatment is complex, as these problems are multifactorial. Contributing factors include physical disability, the stress of living with a progressive illness, drug effects, depression, pain, difficulty in communication, caregiver stress, and impact on intimacy. The phosphodiesterase inhibitor sildenafil (Viagra) can improve erectile dysfunction, but must be used cautiously in patients with orthostatic hypotension.37 Other drugs of this class are available but have not been tested in this population.

COGNITIVE-BEHAVIORAL PROBLEMS

Neuropsychiatric disorders are common in Parkinson disease and at times can be more distressing to the patient and family than the motor symptoms. These include mood disorders, apathy, anxiety, impulse control disorders, psychosis, and dementia.

Dopaminergic medications used to treat movement can precipitate or exacerbate these neuropsychiatric problems. Therefore, treatment requires a balance between motor and neuropsychiatric benefits, with close dialogue with the patient and family about primary goals of treatment.

Depression

Depression is among the most common neuropsychiatric symptoms in Parkinson disease, occurring to some degree in up to 50% of patients.38 Diagnosing it is critical, because it can worsen physical symptoms, cognitive status, quality of life, and caregiver distress.39

However, depression can be difficult to recognize, because many of its features (eg, fatigue, psychomotor slowing, flattened affect, sleep difficulties) can also be manifestations of Parkinson disease. One should specifically ascertain whether the patient has a depressed mood or loss of interest in pleasurable activities. The Beck Depression Inventory is sensitive for depression in Parkinson disease and thus may be a reasonable screening tool.40

Treatment. Psychotherapy may help and may even be a first-line treatment in patients who cannot tolerate antidepressant drugs. Practical recommendations include relaxation techniques, a sleep hygiene regimen, engaging in meaningful activities to achieve a sense of purpose, and caregiver education.41

We have little evidence-based guidance on drug treatment of depression in patients with Parkinson disease. A recent meta-analysis found only two placebo-controlled studies in the past 40 years that monitored outcome based on a standardized rating scale of depression in patients with Parkinson disease.42

In preliminary studies, dopamine agonists have shown some efficacy in treating depression without Parkinson disease.43 However, the antidepressant contributions of anti-Parkinson drugs have not been well established.

Selective serotonin reuptake inhibitors (SSRIs) appear to be safe and well tolerated.44 Venlafaxine (Effexor) and mirtazapine (Remeron) are also reasonable initial options. Tricyclic antidepressants should be used with caution because they can cause anticholinergic side effects, especially confusion, in this population.

All serotonergic agents should be used with caution when given in combination with monoamine oxidase inhibitors, which are often used to treat motor symptoms in Parkinson disease, because of the risk of serotonin syndrome, which is characterized by fever, altered mental status, myoclonus, tremor, hyperreflexia, and diaphoresis and may be fatal.

Electroconvulsive therapy can be reserved for the treatment of severe refractory depression in patients with Parkinson disease without complex medical issues.45

 

 

Apathy

Apathy is present in approximately 30% of patients with Parkinson disease.46

Apathy can be very difficult to differentiate from depression, as the two disorders can occur together. Apathy can also be present without signs or symptoms of depressed mood. Apathy is commonly conceptualized as involving three domains: cognitive (lack of interest), behavioral (lack of initiation and drive), and affective (lack of emotion). The possibility of a primary apathy syndrome should be considered if the patient does not respond to standard treatments for depression. This is critical, as the treatment of the two syndromes may differ.47

Although efficacy data are limited, bupropion (Wellbutrin) and methylphenidate (Ritalin)48 can be tried for their activating or stimulant properties.

Anxiety disorders

Anxiety disorders commonly accompany depression in Parkinson disease, but they can also occur independently. They most often present in the setting of wearing-off or on-off fluctuations associated with medication status. Anxiety disorders in patients with Parkinson disease include generalized anxiety and panic attacks, which are responsive to SSRIs and benzodiazepines.49 Benzodiazepines are effective, and clonazepam (Klonopin) may be preferred because it has a long half-life, thereby minimizing anxiety associated with wearingoff or unpredictable off periods. Conversely, a long half-life and depressive effects may limit its use in advanced age.

Classic obsessive-compulsive disorder is less common, but obsessive behaviors and impulse control difficulties can occur in up to 7% of patients with Parkinson disease and presumably reflect dopamine dysregulation, most often associated with dopamine agonists.50 Impulsive behavior can include gambling, hypersexuality, and bingeing.

One form of obsessive-compulsive disorder is punding, a behavior characterized by intense fascination with repetitive handling and examining of objects, most often mechanical objects.51 Behaviors can include assembling and disassembling, collecting, or sorting of objects.

Visual hallucinations

Many patients with Parkinson disease have visual hallucinations as a side effect of dopaminergic drugs. At first, the patient realizes that they are hallucinations, but this insight may be lost as the disease progresses. The clinician should also consider other potential causes such as dementia, systemic illness, or psychosocial stress.

If visual hallucinations present early in the course of the disease and are accompanied by loss of insight and by cognitive fluctuations, the patient may actually have Lewy body dementia.52 Its features include parkinsonian symptoms, visual hallucinations, a fluctuating level of consciousness, and neuroleptic sensitivity.

Psychosis

The first-line treatment for psychosis in patients with Parkinson disease should involve:

  • Searching for a systemic illness such as urinary tract infection, aspiration pneumonia, or dehydration;
  • Stopping or lowering the dose of drugs that act on the central nervous system; and
  • If possible, stopping or lowering the dose of anti-Parkinson drugs that have the greatest risk of cognitive side effects. In many cases, this is not a realistic option, and adding an antipsychotic drug may be necessary.

Monitoring and treating psychosis is paramount, as it is a major risk factor for nursing home placement.53

Conventional neuroleptics such as haloperidol (Haldol) should be avoided because they can exacerbate parkinsonian symptoms.

Two atypical neuroleptics, clozapine (Clozaril) and quetiapine (Seroquel), appear to be the best tolerated in Parkinson disease patients. Clozapine is the only neuroleptic found to be more efficacious than placebo in patients with Parkinson disease.54 However, of the two, clozapine has a higher risk of side effects and requires frequent blood monitoring, making it difficult to use. Quetiapine has been shown to be as efficacious as clozapine,55 but it failed to show efficacy in a recent controlled study.56 Nevertheless, it is considered the first-line treatment option, since it is safer.40

Other atypical antipsychotics appear to exacerbate Parkinson disease or have not been adequately studied and should therefore be used with caution.

Dementia

Estimates of the prevalence of dementia in patients with Parkinson disease vary widely, most likely reflecting differences in populations studied and methods used. The best estimates indicate that 20% to 30% of patients with Parkinson disease develop dementia.57

Parkinson dementia is one of the classic subcortical dementias, characterized by slow thinking and by difficulties in working memory and problem-solving due to disruption of frontal-subcortical circuits.58 Its most common neuropsychiatric symptoms are hallucinations and depression, with less agitation, disinhibition, and irritability than in Alzheimer dementia.59

Anti-Parkinson drugs, especially anticholinergics, can exacerbate cognitive impairments in patients with Parkinson disease. An acute change in cognitive abilities or visual hallucinations is often associated with an un derlying medical illness such as infection (eg, a urinary tract infection or aspiration pneumonia) or dehydration.

Anticholinesterase inhibitors such as rivastigmine (Exelon) are indicated in patients with Parkinson dementia but may provide only a modest benefit.60

 

 

SLEEP DISORDERS

Excessive daytime sleepiness

Fatigue and hypersomnolence often impair quality of life.61 Daytime hypersomnolence is often multifactorial: it can be caused by the disease itself,62 by dopaminergic therapy,63,64 by a comorbid illness, or by nighttime sleep problems.

Sudden and uncontrollable episodes of sleep are an extreme form of hypersomnolence and are worrisome, especially with activities such as driving.65 Greater sleepiness (measured by the Epworth Sleepiness Scale), longer duration of Parkinson disease, and use of dopaminergic agonists increase the risk of such attacks.66 In general, very few patients experience such attacks without warning signs of sedation.

Treatment must include a comprehensive evaluation of current medications, the effect of dopaminergic agents (especially agonists), and nighttime factors that influence sleep (some of which are described below). Modafinil (Provigil), effective in narcolepsy, helped in some studies67 but not in others68; it could be tried in moderate to severe cases of excessive daytime sleepiness.

Sleep apnea contributes to daytime hypersomnolence. An evaluation for sleep apnea should be considered even in patients who are not overweight, as some evidence suggests that this disorder is common in Parkinson disease and correlates with disease severity.69

Insomnia

Sleep is impaired in up to 74% of Parkinson patients.70,71 A sleep study may show a low total sleep time, many awakenings, a short rapid-eye movement (REM) latency, and short slow-wave sleep (stages III and IV); the patient experiences the problem as light sleep with frequent awakenings.72 A variety of problems related to Parkinson disease can directly affect sleep patterns: eg, pain, stiffness, tremor, problems turning over in bed, dystonia, dementia, nocturia,73 depression, and anxiety.74

Restless legs syndrome

Restless legs syndrome is an uncomfortable, sometimes painful feeling in the legs or other body parts during rest (especially at night) that improves with movement.75 It may be more common in patients with Parkinson disease than in the general population76,77 and can precede the diagnosis of Parkinson disease.78

Iron supplementation with ferrous sulfate can help if iron deficiency (ferritin < 50 μg/L or iron saturation < 16%) is present but is ineffective in its absence. Levodopa and the dopaminergic agonists ropinirole (Requip)70 and pramipexole (Mirapex)80 are effective Parkinson disease treatments that also treat restless legs syndrome. In addition, opioids, clonazepam, and gabapentin (Gabarone) may help.81

Vivid dreams

Parkinson patients often describe very vivid, intense, frightening, and unpleasant dreams,73 which may be a precursor to psychosis.82

REM sleep behavior disorder is characterized by sustained phasic muscle activity in place of normal atonia during REM or dream sleep. The patient's bed partner may describe him or her behaving in an aggressive way as if acting out his or her dreams, ie, hitting, yelling, or kicking. Upon awakening, the patient's recall of the dream content is consistent with the nocturnal behavior.

REM sleep behavior disorder may actually precede the motor symptoms of Parkinson disease,83,84 and as many as 20% of patents with REM sleep behavior disorder eventually develop Parkinson disease.85 The possible link between the two disorders is strengthened by a case report describing a patient with REM sleep behavior disorder, no signs of Parkinson disease on examination, but brain pathology similar to that found in Parkinson disease.86

Clonazepam is an effective treatment for REM sleep behavior disorder and should be considered if sleep is disrupted or patient safety becomes a concern.87

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References
  1. Shulman LM, Taback RL, Bean J, Weiner WJ. Comorbidity of the nonmotor symptoms of Parkinson's disease. Mov Disord 2001; 16:507510.
  2. Hillen ME, Sage JI. Nonmotor fluctuations in patients with Parkinson's disease. Neurology 1996; 47:11801183.
  3. Witjas T, Kaphan E, Azulay JP, et al. Nonmotor fluctuations in Parkinson's disease: frequent and disabling. Neurology 2002; 59:408413.
  4. Adler CH. Nonmotor complications in Parkinson's disease. Mov Disord 2005; 20(suppl 11):S23S29.
  5. Shulman LM, Taback RL, Rabinstein AA, Weiner WJ. Non-recognition of depression and other non-motor symptoms in Parkinson's disease. Parkinsonism Relat Disord 2002; 8:193197.
  6. Braak H, Ghebremedhin E, Rüb U, Bratzke H, Del Tredici K. Stages in the development of Parkinson's disease-related pathology. Cell Tissue Res 2004; 318:121134.
  7. Wolters ECh, Braak H. Parkinson's disease: premotor clinico-pathological correlations. J Neural Transmiss Suppl 2006; 70:309319.
  8. Gunal DI, Nurichalichi K, Tuncer N, Bekiroglu N, Aktan S. The clinical profile of nonmotor fluctuations in Parkinson's disease patients. Can J Neurol Sci 2002; 29:6164.
  9. Snider SR, Fahn S, Isgreen WP, Cote LJ. Primary sensory symptoms in parkinsonism. Neurology 1976; 26:423429.
  10. Koller WC. Sensory symptoms in Parkinson's disease. Neurology 1984; 34:957959.
  11. Ford B, Louis ED, Geene P, Fahn S. Oral and genital pain syndromes in Parkinson's disease. Mov Disord 1996: 11:421426.
  12. Haehner A, Hummel T, Hummel C, et al. Olfactory loss may be the first sign of idiopathic Parkinson's disease. Mov Disord 2007; 22:839842.
  13. Suchowersky O, Reich S, Perlmutter J, Zesiewicz T, Gronseth G, Weiner WJ; Quality Standards Subcommittee of the American Academy of Neurology. Practice parameter: diagnosis and prognosis of new onset Parkinson's disease (an evidence-based review): report of the Quality Standards Subcommittee of the American Academy of Neurology. Neurology 2006; 66:968975.
  14. Hunt LA, Sadun AA, Bassi CJ. Review of the visual system in Parkinson's disease. Optom Vis Sci 1995; 72:9299.
  15. Rodnitzky RL. Visual dysfunction in Parkinson's disease. Clin Neurosci 1998; 5:102106.
  16. Diederich N, Goetz G, Pappert E. Primary deficits in visual discrimination is a risk factor for visual hallucinations in Parkinson's disease [abstract]. Neurology 1997; 48:A181.
  17. Oka H, Yoshioka M, Onouchi K, et al. Characteristics of orthostatic hypotension in Parkinson's disease. Brain 2007; 130:24252432.
  18. Verbaan D, Marinus J, Visser M, van Rooden SM, Stiggelbout AM, van Hilten JJ. Patient-reported autonomic symptoms in Parkinson's disease. Neurology 2007; 69:323341.
  19. Allcock LdM, Ullyart K, Kenny RA, Burn DJ. Frequency of orthostatic hypotension in a community based cohort of patients with Parkinson's disease. J Neurol Neurosurg Psychiatry 2004; 75:14701471.
  20. Allcock LM, Kenny RA, Burn DJ. Clinical phenotype of subjects with Parkinson's disease and orthostatic hypotension: autonomic symptom and demographic comparison. Mov Disord 2006; 21:18511855.
  21. Micieli G, Martignoni E, Cavallini A, Sandrini G, Nappi G. Postprandial and orthostatic hypotension in Parkinson's disease. Neurology 1987; 37:386393.
  22. Sage JI, Mark MH. Drenching sweats as an off phenomenon in Parkinson's disease: treatment and relationship to plasma levodopa profile. Ann Neurol 1995; 37:120122.
  23. Edwards LL, Pfeiffer RF, Quigley EM, Hofman R, Balluff M. Gastrointestinal symptoms in Parkinson's disease. Mov Disord 1991; 6:151156.
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  42. Weintraub D, Morales KH, Moberg PJ, et al. Antidepressant studies in Parkinson's disease: a review and meta-analysis. Mov Disord 2005; 20:11611169.
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  45. Fall P, Granérus AK. Maintenance ECT in Parkinson's disease. J Neural Transm 1999; 106:737741.
  46. Kirsch-Darrow L, Fernandez HH, Marsiske M, Okun MS, Bowers D. Dissociating apathy and depression in Parkinson disease. Neurology 2006; 67:3338.
  47. van Reekum R, Stuss DT, Ostrander L. Apathy: why care? J Neuropsychiatry Clin Neurosci 2005; 17:719.
  48. Chatterjee A, Fahn S. Methylphenidate treats apathy in Parkinson's disease. J Neuropsychiatry Clin Neurosci 2002; 14:461462.
  49. Richard IH. Anxiety disorders in Parkinson's disease. Adv Neurol 2005; 96:4255.
  50. Weintraub D, Siderowf AD, Potenza MN, et al. Association of dopamine agonist use with impulse control disorders in Parkinson disease. Arch Neurol 2006; 63:969973.
  51. Fernandez HH, Friedman JH. Punding on L-dopa. Mov Disord 1999; 14:836838.
  52. McKeith IG. Consensus guidelines for the clinical and pathologic diagnosis of dementia with Lewy bodies (DLB): report of the Consortium on DLB International Workshop. J Alzheimers Dis 2006; 9(suppl 3):417423.
  53. Goetz CG, Stebbins GT. Risk factors for nursing home placement in advanced Parkinson's disease. Neurology 1993; 43:22272229.
  54. Frieling H, Hillemacher T, Ziegenbein M, Neundörfer B, Bleich S. Treating dopamimetic psychosis in Parkinson's disease: structured review and meta-analysis. Eur Neuropsychopharmacol 2007; 17:165171.
  55. Morgante L, Epifanio A, Spina E, et al. Quetiapine versus clozapine: a preliminary report of comparative effects on dopaminergic psychosis in patients with Parkinson's disease. Neurol Sci 2002; 23(suppl 2):S89S90.
  56. Rabey JM, Prokhorov T, Moniovitz A, Dobronevsky E, Klein C. Effect of quetiapine in psychotic Parkinson's disease patients: a double-blind labeled study of 3 months' duration. Mov Disord 2007; 22:313318.
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  59. Aarsland D, Cummings JL, Larsen JP. Neuropsychiatric differences between Parkinson's disease with dementia and Alzheimer's disease. Int J Geriatr Psychiatry 2001; 16:184191.
  60. Emre M, Aarsland D, Albanese A, et al. Rivastigmine for dementia associated with Parkinson's disease. N Engl J Med 2004; 351:25092518.
  61. Martinez-Martin P, Catalan MJ, Benito-Leon J, et al. Impact of fatigue in Parkinson's disease: the Fatigue Impact Scale for Daily Use (D-FIS). Qual Life Res 2006; 15:597606.
  62. Arnulf I, Konofal E, Merino-Andreu M, et al. Parkinson's disease and sleepiness: an integral part of Parkinson disease. Neurology 2002; 58:10191024.
  63. Ondo WG, Dat Vong K, Khan H, Atassi F, Kwak C, Jankovic J. Daytime sleepiness and other sleep disorders in Parkinson's disease. Neurology 2001; 57:13921396.
  64. O'Suilleabhain PE, Dewey RB. Contributions of dopaminergic drugs and disease severity to daytime sleepiness in Parkinson's disease. Arch Neurol 2002; 59:986989.
  65. Fucht S, Rogers JD, Greene PE, Gordon MF, Fahn S. Falling asleep at the wheel: motor vehicle mishaps in persons taking pramipexole and ropinirole. Neurology 1999; 52:19081910.
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KEY POINTS

  • Nonmotor symptoms can be due to the disease itself, to its treatment, or to on-off fluctuations in motor status as doses of medication wear off.
  • Impaired sense of smell, depression, anxiety, fatigue, and constipation can precede the motor symptoms of Parkinson disease and may be symptoms of the disease itself.
  • Orthostatic hypotension, sedation, psychosis, confusion, and impulsiveness may be adverse effects of medical therapy or may worsen with it.
  • Depression occurs in up to 50% of patients with Parkinson disease, although it may be difficult to recognize because many of its physical features can also be manifestations of Parkinson disease itself.
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Carcinoid tumors: What should increase our suspicion?

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Carcinoid tumors: What should increase our suspicion?

Carcinoid tumors, also known as gastroenteropancreatic neuroendocrine tumors, are neoplasms of neuroendocrine origin. Traditionally considered slow-growing, they are now known to vary in their aggressiveness. Many patients with carcinoid tumors have no symptoms or present with symptoms that have broad differential diagnoses. Unless the primary care physician suspects that the patient has a carcinoid tumor, the appropriate testing is seldom ordered. In addition, these patients are at higher risk of developing other cancers of the genitourinary, gastrointestinal, and respiratory tracts; this makes close follow-up, especially by the primary care provider, extremely important.

This article reviews the epidemiology, pathogenesis, clinical features, management, and prognosis of carcinoid tumors. A better knowledge of these tumors among physicians will facilitate recognition, early diagnosis, and improved outcomes for these patients.

INCIDENCE IS INCREASING

The overall incidence of carcinoid tumors has increased over the last 30 years, due at least in part to improvements in ways to diagnose them.1,2 The incidence over the last decade has been between 2.47 and 4.48 per 100,000 population, depending on race and sex, with the highest rates in black men.1,3

The small intestine is the most frequent location, followed by the lungs/bronchi, rectum, appendix, and stomach3; 67.5% of carcinoid tumors occur somewhere in the gastrointestinal system.

The cause of carcinoid tumors is unknown, but genetic factors may play a role, since these tumors often occur as part of genetic disorders such as multiple endocrine neoplasia type 1, von Hippel-Lindau disease, and neurofibromatosis type 1.1–3

SEROTONERGIC EFFECTS DEPEND ON LOCATION

Carcinoid tumors are classified on the basis of their embryologic origin:

  • Foregut (lungs, bronchi, stomach)
  • Midgut (small intestine, appendix, proximal large bowel)
  • Hindgut (distal large bowel, rectum). Tumors from each of these origins differ clinically, biochemically, and histologically.

Carcinoid tumors secrete several bioactive compounds, including serotonin and bradykinin, and the secretory pattern varies depending on the location of the tumor. Most foregut carcinoid tumors secrete low levels of serotonin, being deficient in the enzyme needed to convert 5-hydroxytryptophan to serotonin. Midgut tumors secrete high levels of serotonin, whereas most hindgut tumors do not secrete 5-hydroxytryptophan or serotonin. These differences in secretory patterns are responsible for the different clinical manifestations and biochemical characteristics of these tumors.

Carcinoid syndrome

The systemic effects of the bioactive compounds secreted by carcinoid tumors are responsible for carcinoid syndrome, which has features that can include bronchospasm (possibly mediated by serotonin or bradykinin), diarrhea (likely mediated by serotonin), cutaneous flushing (which has multiple possible mediators), and right-sided valvular heart lesions (possibly mediated by serotonin).2,4 However, the secretory products of midgut carcinoids are normally inactivated by enzymes in the liver before they enter the systemic circulation. Thus, patients with midgut carcinoid tumors develop the carcinoid syndrome only if they have hepatic metastases.4

In contrast, patients with foregut (bronchial and extraintestinal) carcinoids can present with carcinoid syndrome without hepatic metastases, since their secretory products normally bypass the liver and enter the systemic circulation directly.

Hindgut tumors seldom produce this syndrome, since they do not secrete these products.

Fibrosis

Another effect of carcinoid tumors is desmoplasia, or fibrosis.

The pathogenesis of this phenomenon is poorly understood. Serotonin was thought to mediate this effect, but serotonin antagonists are ineffective in treating it, casting doubt on this hypothesis.2,4 More recently, growth factors such as transforming growth factor beta, platelet-derived growth factor, and basic fibroblast growth factor have been implicated.4

 

 

SYMPTOMS ARE OFTEN ABSENT OR NONSPECIFIC

Carcinoid tumors are often clinically silent. Signs and symptoms, when present, represent local effects of the tumor, tumor-induced fibrosis, biological effects of secreted products, or metastases.

When symptomatic, carcinoid tumors can mimic a variety of more common conditions (Table 1). For this reason, the average delay between symptom onset and diagnosis exceeds 9 years.5,6 Still, one should consider these other causes before pursuing an evaluation for carcinoid tumor.

Local effects can include abdominal pain, intestinal obstruction, appendicitis, rectal bleeding, and peptic ulcer disease, depending on the site of the tumor. Intestinal obstruction can be caused by intussusception, by the intraluminal effects of the tumor, or by adhesions due to tumor-induced fibrosis.7

Tumor-induced fibrosis can be retroperitoneal and have a myriad of manifestations, for example2,5:

  • Hydronephrosis from ureteral obstruction
  • Mesenteric ischemia from vascular trapping
  • Peyronie disease (an acquired fibrosis of the penis that produces bending or pain of the erect penis).

Classic carcinoid syndrome, caused by the entry of bioactive compounds secreted by the tumor into the systemic circulation, occurs in fewer than 10% of patients with carcinoid tumors.2,6 Most patients who present with this syndrome have a midgut carcinoid tumor.

The hallmark is cutaneous flushing, which typically affects the face, neck, and upper body and lasts from 30 seconds to 30 minutes. This reaction can be unprovoked, but it is often precipitated by foods (eg, bananas, tomatoes, eggplant, kiwi, pineapple, cheese), by alcohol consumption, by exercise, by emotional stimuli, or by anesthesia.4,8 Other symptoms of this syndrome include bronchospasm, secretory diarrhea, and venous telangiectasia.

Carcinoid syndrome variants, caused by differences in secretory products, are seen in some patients with bronchial and gastric carcinoid tumors. Patients with gastric carcinoid variants have flushing that is pruritic and well demarcated, and they have an increased incidence of peptic ulcer. In contrast, flushing in patients with bronchial carcinoid variants can last days and is often associated with changes in mental status.2,9

Carcinoid heart disease refers to endocardial fibrotic plaques that occur in patients with carcinoid tumors, especially those with hepatic metastases. The right side of the heart is generally affected, as the left side is protected by inactivation of the bioactive compounds in the lungs. Tricuspid valve regurgitation is the most common finding, but tricuspid stenosis, pulmonary valve regurgitation, and pulmonary valve stenosis can also occur.10 Left-sided lesions can occur in patients with pulmonary metastases.

Hypoalbuminemia and pellagra. The amino acid tryptophan is a precursor of serotonin and niacin (vitamin B3). In patients with widely metastatic carcinoid tumors, increased conversion of tryptophan to serotonin by the tumor cells can lead to tryptophan deficiency and niacin deficiency.1,2 These manifest as hypoalbuminemia and pellagra (glossitis, scaly skin, and confusion).

IF YOU DON’T THINK ABOUT THEM, YOU WON’T LOOK FOR THEM

Many carcinoid tumors are discovered incidentally during surgery or diagnostic procedures. However, an evaluation for a carcinoid tumor is often prompted by symptoms that suggest the carcinoid syndrome. Of importance, since these symptoms can often be erroneously attributed to other, more common causes (Table 1), a very high level of suspicion is required on the part of the primary care physician to initiate the evaluation for carcinoid tumors.

When evaluating a patient who presents with flushing, the clinician should obtain a detailed history, noting the pattern of flushing, precipitating factors, duration, and associated symptoms, such as diarrhea and bronchospasm. 11

Often, patient recall can be improved by asking the patient to keep a symptom diary. If the diary does not offer any clues to the diagnosis, a trial of abstinence from foods and drugs that increase urinary 5-hydroxyindoleacetic acid (5-HIAA) should be attempted. If the flushing resolves, the foods and drugs can be reintroduced one at a time to identify the culprit.11 However, if symptoms persist, a more extensive workup should be undertaken, including screening for carcinoid tumor.

Biochemical assays

Biochemical screening for carcinoid tumors is performed using an assay for bioamines secreted by the tumor.

Plasma chromogranin A is the preferred screening test because it is very sensitive12; however, it is not very specific. Several conditions (including essential hypertension, proton pump inhibitor use, chronic atrophic gastritis, heart failure, renal failure, and pheochromocytoma) can be associated with elevated levels of chromogranin A. Its specificity for diagnosing carcinoid tumors can be increased to about 84% by raising the cut-off value to 31 or 32 U/L. Its specificity can be increased to 95% by using 84 to 87 U/L as the cut-off value, but this comes at the cost of diminishing its sensitivity (from 75% to about 55%).13 Significantly elevated levels of chromogranin A (> 5,000 U/L) independently predict a poor prognosis.13

5-HIAA, a renally excreted product of serotonin metabolism, is a useful alternative when screening for carcinoid tumors. Measurement of urinary excretion of 5-HIAA requires 24-hour urine collection; importantly, starting at least 3 days before the urine collection begins and throughout the 24-hour collection period, patients must avoid ingesting foods, beverages, and drugs that elevate or suppress urinary excretion of 5-HIAA (Table 2).1,2

Urinary 5-HIAA levels also vary depending on the origin of the carcinoid tumor and are therefore useful in locating the site of the tumor. Foregut tumors lack the decarboxylase enzyme necessary to convert 5-hydroxytryptophan to serotonin, resulting in minimal to no elevation in urinary 5-HIAA levels. Midgut tumors secrete serotonin, resulting in high levels of urinary 5-HIAA. Hindgut tumors secrete neither 5-hydroxytryptophan nor serotonin and thus do not raise urinary 5-HIAA levels.

Other less sensitive markers include bradykinin, human chorionic gonadotropin, and neuropeptide PP.14

 

 

Provocative tests

Provocative tests such as the pentagastrin test can be considered if other screening test results are equivocal.12 Such testing must occur in a closely monitored, controlled environment, with intravenous somatostatin available in case of a “carcinoid crisis” (see discussion further below).

Patients with equivocal results from biochemical assays or provocative testing should be followed annually without further testing or evaluated for other causes of their symptoms. If the results of biochemical or provocative testing are abnormal, the tumor topography should be identified with an imaging study.

Imaging tests

Topographic localization of carcinoid tumors is done using various imaging tests, depending on the suspected site of the primary tumor.6

Somatostatin receptor scintigraphy, the preferred imaging test, is based on the principle that some carcinoid tumors have high concentrations of somatostatin receptors. Thus, a radiolabeled form of octreotide, a somatostatin analogue, is used to image these primary tumors and metastases.

Other imaging studies:

  • Barium studies
  • Computed tomography
  • Endoscopy
  • Endoscopic ultrasonography.

On imaging studies, in general, the tumor may appear as a smooth submucosal mass, as a target lesion (if it ulcerates), as wall-thickening, or as a cystic or calcified mass.6

MANAGEMENT IS MULTIDISCIPLINARY

Any patient with a carcinoid tumor should be referred to a medical and surgical oncologist once the diagnosis is established. Referral to additional specialists, such as a gastroenterologist or an interventional radiologist, is based on the location and extent of disease.

Surgery is the cornerstone of therapy

Figure 1.
Patients with limited disease may need only surgical resection, but those with more extensive disease require additional management based on the presence and location of metastases (Figure 1).15

Drug therapy

Somatostatin analogues such as octreotide (Sandostatin) and lanreotide (Somatuline) are useful for treating carcinoid syndrome16 and also have a role in treating systemic metastases. These agents are effective in controlling flushing and diarrhea in 70% to 80% of patients.17 There are data, albeit limited, supporting a role for these agents in inhibiting tumor growth.18 They are the treatment of choice for carcinoid crisis (see discussion below). Important adverse effects include nausea, cramps, diarrhea; cholelithiasis; hypoglycemia or hyperglycemia; cardiac arrhythmias; and gastric atony.16

Interferon alfa is useful as an additive therapy when symptoms of carcinoid syndrome do not resolve with a somatostatin analogue alone. The addition of interferon alfa in these patients is useful for both symptom control (seen in 40% to 50% of those treated) and tumor stabilization (in 20% to 40% of those treated).19 However, it is still unclear whether combination drug therapy is more effective than a somatostatin analogue alone as the initial therapy for carcinoid syndrome.20 Adverse effects of interferon alfa include myelosuppression, depression, flu-like symptoms, and thyroid disturbances.

Supportive therapies

In patients with hepatic metastases who are not candidates for surgery, hepatic artery embolization with chemotherapy or particles can be used as palliative therapy. Severe adverse effects of this procedure include renal failure, hepatic failure, carcinoid crisis, and hepatic abscess and are seen in about 10% of patients.1

Conventional chemotherapy and molecularly targeted therapy are used for patients with rapidly progressive and widely metastatic disease. The precise role and efficacy of these therapies need further study.

Other supportive therapies for patients with carcinoid disease include dietary supplementation with vitamin B3, bronchodilators for bronchospasm, antidiarrheals, diuretics, and valve replacement for carcinoid heart disease.

 

 

LONG-TERM PROGNOSIS IS GENERALLY GOOD

The prognosis for patients with carcinoid tumors depends on the location and extent of disease. Tumors of the appendix and rectum have the best prognosis, with 5-year survival rates approaching 100% for localized carcinoid tumors of the appendix.3,21 In contrast, tumors of the small bowel, especially the ileum, are more aggressive and have the worst prognosis (a 5-year survival rate of about 60% to 65%).21

COMPLICATIONS

Other primary malignancies

Carcinoid tumors are often associated with the development of other tumors, not always in the gastrointestinal tract. As many as 52% of patients with small-bowel carcinoid tumors develop another primary tumor.22 This effect is thought to be related to the tumorigenic properties of the bioactive compounds secreted by carcinoid tumors. The other primary malignancy can be synchronous (diagnosed at the same time) or metachronous (diagnosed 1 to 7 years after the carcinoid) and generally arises from the gastrointestinal, genitourinary, or respiratory tract. Adenocarcinoma of the colon is reported as the most common second primary malignancy in patients with carcinoid tumors.22

The best strategy for surveillance in these patients is still unclear. Screening for tumors of the colon, small bowel, lung, cervix, and ovaries at the time of carcinoid tumor diagnosis followed by surveillance for these malignancies has been suggested as a possible approach; however, this comes at the cost of increased patient anxiety, cost, and morbidity from testing. 3

Carcinoid crisis

Carcinoid crisis is a life-threatening emergency caused by release of large amounts of vasoactive compounds from the carcinoid tumor, either spontaneously or provoked by tumor manipulation, surgery, chemotherapy, or hepatic artery embolization.2,5 The syndrome manifests as cardiovascular collapse (severe hypotension or hypertension), tachycardia, and altered mental status.

Treatment differs from those for other causes of shock in that catecholamines and calcium should not be used since they trigger the release of larger amounts of bioactive chemicals from the tumor. In addition, the shock in this situation is refractory to fluid. The mainstay of treatment is the infusion of octreotide and plasma. This crisis can be prevented by giving octreotide before manipulating the tumor.1,2,5

References
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  19. Bajetta E, Zilembo N, Di Bartolomeo M, et al. Treatment of metastatic carcinoids and other neuroendocrine tumors with recombinant interferon-alpha-2a. A study by the Italian Trials in Medical Oncology Group. Cancer 1993; 72:30993105.
  20. Faiss S, Pape UF, Bohmig M, et al. Prospective, randomized, multicenter trial on the antiproliferative effect of lanreotide, interferon-alfa, and their combination for therapy of metastatic neuroendocrine gastroenteropancreatic tumors—the International Lanreotide and Interferon Alfa Study Group. J Clin Oncol 2003; 21:26892696.
  21. Helland SK, Prosch AM, Viste A. Carcinoid tumors in the gastrointestinal tract—a population-based study from Western Norway. Scand J Surg 2006; 95:158161.
  22. Habal N, Sims C, Bilchik AJ. Gastrointestinal carcinoid tumors and second primary malignancies. J Surg Oncol 2000; 75:310316.
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Kamil Obideen, MD
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Mohammad Wehbi, MD
Department of Medicine and Division of Digestive Diseases, Emory University, and Atlanta Veterans Affairs Medical Center, Atlanta, GA

Address: Gaurav Aggarwal, MD, MS, Department of Medicine, Emory University, 1364 Clifton Road, Atlanta, GA 30322; [email protected]

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Department of Medicine and Division of Digestive Diseases, Emory University, and Atlanta Veterans Affairs Medical Center, Atlanta, GA

Address: Gaurav Aggarwal, MD, MS, Department of Medicine, Emory University, 1364 Clifton Road, Atlanta, GA 30322; [email protected]

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Department of Medicine, Emory University, Atlanta, GA

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Mohammad Wehbi, MD
Department of Medicine and Division of Digestive Diseases, Emory University, and Atlanta Veterans Affairs Medical Center, Atlanta, GA

Address: Gaurav Aggarwal, MD, MS, Department of Medicine, Emory University, 1364 Clifton Road, Atlanta, GA 30322; [email protected]

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Carcinoid tumors, also known as gastroenteropancreatic neuroendocrine tumors, are neoplasms of neuroendocrine origin. Traditionally considered slow-growing, they are now known to vary in their aggressiveness. Many patients with carcinoid tumors have no symptoms or present with symptoms that have broad differential diagnoses. Unless the primary care physician suspects that the patient has a carcinoid tumor, the appropriate testing is seldom ordered. In addition, these patients are at higher risk of developing other cancers of the genitourinary, gastrointestinal, and respiratory tracts; this makes close follow-up, especially by the primary care provider, extremely important.

This article reviews the epidemiology, pathogenesis, clinical features, management, and prognosis of carcinoid tumors. A better knowledge of these tumors among physicians will facilitate recognition, early diagnosis, and improved outcomes for these patients.

INCIDENCE IS INCREASING

The overall incidence of carcinoid tumors has increased over the last 30 years, due at least in part to improvements in ways to diagnose them.1,2 The incidence over the last decade has been between 2.47 and 4.48 per 100,000 population, depending on race and sex, with the highest rates in black men.1,3

The small intestine is the most frequent location, followed by the lungs/bronchi, rectum, appendix, and stomach3; 67.5% of carcinoid tumors occur somewhere in the gastrointestinal system.

The cause of carcinoid tumors is unknown, but genetic factors may play a role, since these tumors often occur as part of genetic disorders such as multiple endocrine neoplasia type 1, von Hippel-Lindau disease, and neurofibromatosis type 1.1–3

SEROTONERGIC EFFECTS DEPEND ON LOCATION

Carcinoid tumors are classified on the basis of their embryologic origin:

  • Foregut (lungs, bronchi, stomach)
  • Midgut (small intestine, appendix, proximal large bowel)
  • Hindgut (distal large bowel, rectum). Tumors from each of these origins differ clinically, biochemically, and histologically.

Carcinoid tumors secrete several bioactive compounds, including serotonin and bradykinin, and the secretory pattern varies depending on the location of the tumor. Most foregut carcinoid tumors secrete low levels of serotonin, being deficient in the enzyme needed to convert 5-hydroxytryptophan to serotonin. Midgut tumors secrete high levels of serotonin, whereas most hindgut tumors do not secrete 5-hydroxytryptophan or serotonin. These differences in secretory patterns are responsible for the different clinical manifestations and biochemical characteristics of these tumors.

Carcinoid syndrome

The systemic effects of the bioactive compounds secreted by carcinoid tumors are responsible for carcinoid syndrome, which has features that can include bronchospasm (possibly mediated by serotonin or bradykinin), diarrhea (likely mediated by serotonin), cutaneous flushing (which has multiple possible mediators), and right-sided valvular heart lesions (possibly mediated by serotonin).2,4 However, the secretory products of midgut carcinoids are normally inactivated by enzymes in the liver before they enter the systemic circulation. Thus, patients with midgut carcinoid tumors develop the carcinoid syndrome only if they have hepatic metastases.4

In contrast, patients with foregut (bronchial and extraintestinal) carcinoids can present with carcinoid syndrome without hepatic metastases, since their secretory products normally bypass the liver and enter the systemic circulation directly.

Hindgut tumors seldom produce this syndrome, since they do not secrete these products.

Fibrosis

Another effect of carcinoid tumors is desmoplasia, or fibrosis.

The pathogenesis of this phenomenon is poorly understood. Serotonin was thought to mediate this effect, but serotonin antagonists are ineffective in treating it, casting doubt on this hypothesis.2,4 More recently, growth factors such as transforming growth factor beta, platelet-derived growth factor, and basic fibroblast growth factor have been implicated.4

 

 

SYMPTOMS ARE OFTEN ABSENT OR NONSPECIFIC

Carcinoid tumors are often clinically silent. Signs and symptoms, when present, represent local effects of the tumor, tumor-induced fibrosis, biological effects of secreted products, or metastases.

When symptomatic, carcinoid tumors can mimic a variety of more common conditions (Table 1). For this reason, the average delay between symptom onset and diagnosis exceeds 9 years.5,6 Still, one should consider these other causes before pursuing an evaluation for carcinoid tumor.

Local effects can include abdominal pain, intestinal obstruction, appendicitis, rectal bleeding, and peptic ulcer disease, depending on the site of the tumor. Intestinal obstruction can be caused by intussusception, by the intraluminal effects of the tumor, or by adhesions due to tumor-induced fibrosis.7

Tumor-induced fibrosis can be retroperitoneal and have a myriad of manifestations, for example2,5:

  • Hydronephrosis from ureteral obstruction
  • Mesenteric ischemia from vascular trapping
  • Peyronie disease (an acquired fibrosis of the penis that produces bending or pain of the erect penis).

Classic carcinoid syndrome, caused by the entry of bioactive compounds secreted by the tumor into the systemic circulation, occurs in fewer than 10% of patients with carcinoid tumors.2,6 Most patients who present with this syndrome have a midgut carcinoid tumor.

The hallmark is cutaneous flushing, which typically affects the face, neck, and upper body and lasts from 30 seconds to 30 minutes. This reaction can be unprovoked, but it is often precipitated by foods (eg, bananas, tomatoes, eggplant, kiwi, pineapple, cheese), by alcohol consumption, by exercise, by emotional stimuli, or by anesthesia.4,8 Other symptoms of this syndrome include bronchospasm, secretory diarrhea, and venous telangiectasia.

Carcinoid syndrome variants, caused by differences in secretory products, are seen in some patients with bronchial and gastric carcinoid tumors. Patients with gastric carcinoid variants have flushing that is pruritic and well demarcated, and they have an increased incidence of peptic ulcer. In contrast, flushing in patients with bronchial carcinoid variants can last days and is often associated with changes in mental status.2,9

Carcinoid heart disease refers to endocardial fibrotic plaques that occur in patients with carcinoid tumors, especially those with hepatic metastases. The right side of the heart is generally affected, as the left side is protected by inactivation of the bioactive compounds in the lungs. Tricuspid valve regurgitation is the most common finding, but tricuspid stenosis, pulmonary valve regurgitation, and pulmonary valve stenosis can also occur.10 Left-sided lesions can occur in patients with pulmonary metastases.

Hypoalbuminemia and pellagra. The amino acid tryptophan is a precursor of serotonin and niacin (vitamin B3). In patients with widely metastatic carcinoid tumors, increased conversion of tryptophan to serotonin by the tumor cells can lead to tryptophan deficiency and niacin deficiency.1,2 These manifest as hypoalbuminemia and pellagra (glossitis, scaly skin, and confusion).

IF YOU DON’T THINK ABOUT THEM, YOU WON’T LOOK FOR THEM

Many carcinoid tumors are discovered incidentally during surgery or diagnostic procedures. However, an evaluation for a carcinoid tumor is often prompted by symptoms that suggest the carcinoid syndrome. Of importance, since these symptoms can often be erroneously attributed to other, more common causes (Table 1), a very high level of suspicion is required on the part of the primary care physician to initiate the evaluation for carcinoid tumors.

When evaluating a patient who presents with flushing, the clinician should obtain a detailed history, noting the pattern of flushing, precipitating factors, duration, and associated symptoms, such as diarrhea and bronchospasm. 11

Often, patient recall can be improved by asking the patient to keep a symptom diary. If the diary does not offer any clues to the diagnosis, a trial of abstinence from foods and drugs that increase urinary 5-hydroxyindoleacetic acid (5-HIAA) should be attempted. If the flushing resolves, the foods and drugs can be reintroduced one at a time to identify the culprit.11 However, if symptoms persist, a more extensive workup should be undertaken, including screening for carcinoid tumor.

Biochemical assays

Biochemical screening for carcinoid tumors is performed using an assay for bioamines secreted by the tumor.

Plasma chromogranin A is the preferred screening test because it is very sensitive12; however, it is not very specific. Several conditions (including essential hypertension, proton pump inhibitor use, chronic atrophic gastritis, heart failure, renal failure, and pheochromocytoma) can be associated with elevated levels of chromogranin A. Its specificity for diagnosing carcinoid tumors can be increased to about 84% by raising the cut-off value to 31 or 32 U/L. Its specificity can be increased to 95% by using 84 to 87 U/L as the cut-off value, but this comes at the cost of diminishing its sensitivity (from 75% to about 55%).13 Significantly elevated levels of chromogranin A (> 5,000 U/L) independently predict a poor prognosis.13

5-HIAA, a renally excreted product of serotonin metabolism, is a useful alternative when screening for carcinoid tumors. Measurement of urinary excretion of 5-HIAA requires 24-hour urine collection; importantly, starting at least 3 days before the urine collection begins and throughout the 24-hour collection period, patients must avoid ingesting foods, beverages, and drugs that elevate or suppress urinary excretion of 5-HIAA (Table 2).1,2

Urinary 5-HIAA levels also vary depending on the origin of the carcinoid tumor and are therefore useful in locating the site of the tumor. Foregut tumors lack the decarboxylase enzyme necessary to convert 5-hydroxytryptophan to serotonin, resulting in minimal to no elevation in urinary 5-HIAA levels. Midgut tumors secrete serotonin, resulting in high levels of urinary 5-HIAA. Hindgut tumors secrete neither 5-hydroxytryptophan nor serotonin and thus do not raise urinary 5-HIAA levels.

Other less sensitive markers include bradykinin, human chorionic gonadotropin, and neuropeptide PP.14

 

 

Provocative tests

Provocative tests such as the pentagastrin test can be considered if other screening test results are equivocal.12 Such testing must occur in a closely monitored, controlled environment, with intravenous somatostatin available in case of a “carcinoid crisis” (see discussion further below).

Patients with equivocal results from biochemical assays or provocative testing should be followed annually without further testing or evaluated for other causes of their symptoms. If the results of biochemical or provocative testing are abnormal, the tumor topography should be identified with an imaging study.

Imaging tests

Topographic localization of carcinoid tumors is done using various imaging tests, depending on the suspected site of the primary tumor.6

Somatostatin receptor scintigraphy, the preferred imaging test, is based on the principle that some carcinoid tumors have high concentrations of somatostatin receptors. Thus, a radiolabeled form of octreotide, a somatostatin analogue, is used to image these primary tumors and metastases.

Other imaging studies:

  • Barium studies
  • Computed tomography
  • Endoscopy
  • Endoscopic ultrasonography.

On imaging studies, in general, the tumor may appear as a smooth submucosal mass, as a target lesion (if it ulcerates), as wall-thickening, or as a cystic or calcified mass.6

MANAGEMENT IS MULTIDISCIPLINARY

Any patient with a carcinoid tumor should be referred to a medical and surgical oncologist once the diagnosis is established. Referral to additional specialists, such as a gastroenterologist or an interventional radiologist, is based on the location and extent of disease.

Surgery is the cornerstone of therapy

Figure 1.
Patients with limited disease may need only surgical resection, but those with more extensive disease require additional management based on the presence and location of metastases (Figure 1).15

Drug therapy

Somatostatin analogues such as octreotide (Sandostatin) and lanreotide (Somatuline) are useful for treating carcinoid syndrome16 and also have a role in treating systemic metastases. These agents are effective in controlling flushing and diarrhea in 70% to 80% of patients.17 There are data, albeit limited, supporting a role for these agents in inhibiting tumor growth.18 They are the treatment of choice for carcinoid crisis (see discussion below). Important adverse effects include nausea, cramps, diarrhea; cholelithiasis; hypoglycemia or hyperglycemia; cardiac arrhythmias; and gastric atony.16

Interferon alfa is useful as an additive therapy when symptoms of carcinoid syndrome do not resolve with a somatostatin analogue alone. The addition of interferon alfa in these patients is useful for both symptom control (seen in 40% to 50% of those treated) and tumor stabilization (in 20% to 40% of those treated).19 However, it is still unclear whether combination drug therapy is more effective than a somatostatin analogue alone as the initial therapy for carcinoid syndrome.20 Adverse effects of interferon alfa include myelosuppression, depression, flu-like symptoms, and thyroid disturbances.

Supportive therapies

In patients with hepatic metastases who are not candidates for surgery, hepatic artery embolization with chemotherapy or particles can be used as palliative therapy. Severe adverse effects of this procedure include renal failure, hepatic failure, carcinoid crisis, and hepatic abscess and are seen in about 10% of patients.1

Conventional chemotherapy and molecularly targeted therapy are used for patients with rapidly progressive and widely metastatic disease. The precise role and efficacy of these therapies need further study.

Other supportive therapies for patients with carcinoid disease include dietary supplementation with vitamin B3, bronchodilators for bronchospasm, antidiarrheals, diuretics, and valve replacement for carcinoid heart disease.

 

 

LONG-TERM PROGNOSIS IS GENERALLY GOOD

The prognosis for patients with carcinoid tumors depends on the location and extent of disease. Tumors of the appendix and rectum have the best prognosis, with 5-year survival rates approaching 100% for localized carcinoid tumors of the appendix.3,21 In contrast, tumors of the small bowel, especially the ileum, are more aggressive and have the worst prognosis (a 5-year survival rate of about 60% to 65%).21

COMPLICATIONS

Other primary malignancies

Carcinoid tumors are often associated with the development of other tumors, not always in the gastrointestinal tract. As many as 52% of patients with small-bowel carcinoid tumors develop another primary tumor.22 This effect is thought to be related to the tumorigenic properties of the bioactive compounds secreted by carcinoid tumors. The other primary malignancy can be synchronous (diagnosed at the same time) or metachronous (diagnosed 1 to 7 years after the carcinoid) and generally arises from the gastrointestinal, genitourinary, or respiratory tract. Adenocarcinoma of the colon is reported as the most common second primary malignancy in patients with carcinoid tumors.22

The best strategy for surveillance in these patients is still unclear. Screening for tumors of the colon, small bowel, lung, cervix, and ovaries at the time of carcinoid tumor diagnosis followed by surveillance for these malignancies has been suggested as a possible approach; however, this comes at the cost of increased patient anxiety, cost, and morbidity from testing. 3

Carcinoid crisis

Carcinoid crisis is a life-threatening emergency caused by release of large amounts of vasoactive compounds from the carcinoid tumor, either spontaneously or provoked by tumor manipulation, surgery, chemotherapy, or hepatic artery embolization.2,5 The syndrome manifests as cardiovascular collapse (severe hypotension or hypertension), tachycardia, and altered mental status.

Treatment differs from those for other causes of shock in that catecholamines and calcium should not be used since they trigger the release of larger amounts of bioactive chemicals from the tumor. In addition, the shock in this situation is refractory to fluid. The mainstay of treatment is the infusion of octreotide and plasma. This crisis can be prevented by giving octreotide before manipulating the tumor.1,2,5

Carcinoid tumors, also known as gastroenteropancreatic neuroendocrine tumors, are neoplasms of neuroendocrine origin. Traditionally considered slow-growing, they are now known to vary in their aggressiveness. Many patients with carcinoid tumors have no symptoms or present with symptoms that have broad differential diagnoses. Unless the primary care physician suspects that the patient has a carcinoid tumor, the appropriate testing is seldom ordered. In addition, these patients are at higher risk of developing other cancers of the genitourinary, gastrointestinal, and respiratory tracts; this makes close follow-up, especially by the primary care provider, extremely important.

This article reviews the epidemiology, pathogenesis, clinical features, management, and prognosis of carcinoid tumors. A better knowledge of these tumors among physicians will facilitate recognition, early diagnosis, and improved outcomes for these patients.

INCIDENCE IS INCREASING

The overall incidence of carcinoid tumors has increased over the last 30 years, due at least in part to improvements in ways to diagnose them.1,2 The incidence over the last decade has been between 2.47 and 4.48 per 100,000 population, depending on race and sex, with the highest rates in black men.1,3

The small intestine is the most frequent location, followed by the lungs/bronchi, rectum, appendix, and stomach3; 67.5% of carcinoid tumors occur somewhere in the gastrointestinal system.

The cause of carcinoid tumors is unknown, but genetic factors may play a role, since these tumors often occur as part of genetic disorders such as multiple endocrine neoplasia type 1, von Hippel-Lindau disease, and neurofibromatosis type 1.1–3

SEROTONERGIC EFFECTS DEPEND ON LOCATION

Carcinoid tumors are classified on the basis of their embryologic origin:

  • Foregut (lungs, bronchi, stomach)
  • Midgut (small intestine, appendix, proximal large bowel)
  • Hindgut (distal large bowel, rectum). Tumors from each of these origins differ clinically, biochemically, and histologically.

Carcinoid tumors secrete several bioactive compounds, including serotonin and bradykinin, and the secretory pattern varies depending on the location of the tumor. Most foregut carcinoid tumors secrete low levels of serotonin, being deficient in the enzyme needed to convert 5-hydroxytryptophan to serotonin. Midgut tumors secrete high levels of serotonin, whereas most hindgut tumors do not secrete 5-hydroxytryptophan or serotonin. These differences in secretory patterns are responsible for the different clinical manifestations and biochemical characteristics of these tumors.

Carcinoid syndrome

The systemic effects of the bioactive compounds secreted by carcinoid tumors are responsible for carcinoid syndrome, which has features that can include bronchospasm (possibly mediated by serotonin or bradykinin), diarrhea (likely mediated by serotonin), cutaneous flushing (which has multiple possible mediators), and right-sided valvular heart lesions (possibly mediated by serotonin).2,4 However, the secretory products of midgut carcinoids are normally inactivated by enzymes in the liver before they enter the systemic circulation. Thus, patients with midgut carcinoid tumors develop the carcinoid syndrome only if they have hepatic metastases.4

In contrast, patients with foregut (bronchial and extraintestinal) carcinoids can present with carcinoid syndrome without hepatic metastases, since their secretory products normally bypass the liver and enter the systemic circulation directly.

Hindgut tumors seldom produce this syndrome, since they do not secrete these products.

Fibrosis

Another effect of carcinoid tumors is desmoplasia, or fibrosis.

The pathogenesis of this phenomenon is poorly understood. Serotonin was thought to mediate this effect, but serotonin antagonists are ineffective in treating it, casting doubt on this hypothesis.2,4 More recently, growth factors such as transforming growth factor beta, platelet-derived growth factor, and basic fibroblast growth factor have been implicated.4

 

 

SYMPTOMS ARE OFTEN ABSENT OR NONSPECIFIC

Carcinoid tumors are often clinically silent. Signs and symptoms, when present, represent local effects of the tumor, tumor-induced fibrosis, biological effects of secreted products, or metastases.

When symptomatic, carcinoid tumors can mimic a variety of more common conditions (Table 1). For this reason, the average delay between symptom onset and diagnosis exceeds 9 years.5,6 Still, one should consider these other causes before pursuing an evaluation for carcinoid tumor.

Local effects can include abdominal pain, intestinal obstruction, appendicitis, rectal bleeding, and peptic ulcer disease, depending on the site of the tumor. Intestinal obstruction can be caused by intussusception, by the intraluminal effects of the tumor, or by adhesions due to tumor-induced fibrosis.7

Tumor-induced fibrosis can be retroperitoneal and have a myriad of manifestations, for example2,5:

  • Hydronephrosis from ureteral obstruction
  • Mesenteric ischemia from vascular trapping
  • Peyronie disease (an acquired fibrosis of the penis that produces bending or pain of the erect penis).

Classic carcinoid syndrome, caused by the entry of bioactive compounds secreted by the tumor into the systemic circulation, occurs in fewer than 10% of patients with carcinoid tumors.2,6 Most patients who present with this syndrome have a midgut carcinoid tumor.

The hallmark is cutaneous flushing, which typically affects the face, neck, and upper body and lasts from 30 seconds to 30 minutes. This reaction can be unprovoked, but it is often precipitated by foods (eg, bananas, tomatoes, eggplant, kiwi, pineapple, cheese), by alcohol consumption, by exercise, by emotional stimuli, or by anesthesia.4,8 Other symptoms of this syndrome include bronchospasm, secretory diarrhea, and venous telangiectasia.

Carcinoid syndrome variants, caused by differences in secretory products, are seen in some patients with bronchial and gastric carcinoid tumors. Patients with gastric carcinoid variants have flushing that is pruritic and well demarcated, and they have an increased incidence of peptic ulcer. In contrast, flushing in patients with bronchial carcinoid variants can last days and is often associated with changes in mental status.2,9

Carcinoid heart disease refers to endocardial fibrotic plaques that occur in patients with carcinoid tumors, especially those with hepatic metastases. The right side of the heart is generally affected, as the left side is protected by inactivation of the bioactive compounds in the lungs. Tricuspid valve regurgitation is the most common finding, but tricuspid stenosis, pulmonary valve regurgitation, and pulmonary valve stenosis can also occur.10 Left-sided lesions can occur in patients with pulmonary metastases.

Hypoalbuminemia and pellagra. The amino acid tryptophan is a precursor of serotonin and niacin (vitamin B3). In patients with widely metastatic carcinoid tumors, increased conversion of tryptophan to serotonin by the tumor cells can lead to tryptophan deficiency and niacin deficiency.1,2 These manifest as hypoalbuminemia and pellagra (glossitis, scaly skin, and confusion).

IF YOU DON’T THINK ABOUT THEM, YOU WON’T LOOK FOR THEM

Many carcinoid tumors are discovered incidentally during surgery or diagnostic procedures. However, an evaluation for a carcinoid tumor is often prompted by symptoms that suggest the carcinoid syndrome. Of importance, since these symptoms can often be erroneously attributed to other, more common causes (Table 1), a very high level of suspicion is required on the part of the primary care physician to initiate the evaluation for carcinoid tumors.

When evaluating a patient who presents with flushing, the clinician should obtain a detailed history, noting the pattern of flushing, precipitating factors, duration, and associated symptoms, such as diarrhea and bronchospasm. 11

Often, patient recall can be improved by asking the patient to keep a symptom diary. If the diary does not offer any clues to the diagnosis, a trial of abstinence from foods and drugs that increase urinary 5-hydroxyindoleacetic acid (5-HIAA) should be attempted. If the flushing resolves, the foods and drugs can be reintroduced one at a time to identify the culprit.11 However, if symptoms persist, a more extensive workup should be undertaken, including screening for carcinoid tumor.

Biochemical assays

Biochemical screening for carcinoid tumors is performed using an assay for bioamines secreted by the tumor.

Plasma chromogranin A is the preferred screening test because it is very sensitive12; however, it is not very specific. Several conditions (including essential hypertension, proton pump inhibitor use, chronic atrophic gastritis, heart failure, renal failure, and pheochromocytoma) can be associated with elevated levels of chromogranin A. Its specificity for diagnosing carcinoid tumors can be increased to about 84% by raising the cut-off value to 31 or 32 U/L. Its specificity can be increased to 95% by using 84 to 87 U/L as the cut-off value, but this comes at the cost of diminishing its sensitivity (from 75% to about 55%).13 Significantly elevated levels of chromogranin A (> 5,000 U/L) independently predict a poor prognosis.13

5-HIAA, a renally excreted product of serotonin metabolism, is a useful alternative when screening for carcinoid tumors. Measurement of urinary excretion of 5-HIAA requires 24-hour urine collection; importantly, starting at least 3 days before the urine collection begins and throughout the 24-hour collection period, patients must avoid ingesting foods, beverages, and drugs that elevate or suppress urinary excretion of 5-HIAA (Table 2).1,2

Urinary 5-HIAA levels also vary depending on the origin of the carcinoid tumor and are therefore useful in locating the site of the tumor. Foregut tumors lack the decarboxylase enzyme necessary to convert 5-hydroxytryptophan to serotonin, resulting in minimal to no elevation in urinary 5-HIAA levels. Midgut tumors secrete serotonin, resulting in high levels of urinary 5-HIAA. Hindgut tumors secrete neither 5-hydroxytryptophan nor serotonin and thus do not raise urinary 5-HIAA levels.

Other less sensitive markers include bradykinin, human chorionic gonadotropin, and neuropeptide PP.14

 

 

Provocative tests

Provocative tests such as the pentagastrin test can be considered if other screening test results are equivocal.12 Such testing must occur in a closely monitored, controlled environment, with intravenous somatostatin available in case of a “carcinoid crisis” (see discussion further below).

Patients with equivocal results from biochemical assays or provocative testing should be followed annually without further testing or evaluated for other causes of their symptoms. If the results of biochemical or provocative testing are abnormal, the tumor topography should be identified with an imaging study.

Imaging tests

Topographic localization of carcinoid tumors is done using various imaging tests, depending on the suspected site of the primary tumor.6

Somatostatin receptor scintigraphy, the preferred imaging test, is based on the principle that some carcinoid tumors have high concentrations of somatostatin receptors. Thus, a radiolabeled form of octreotide, a somatostatin analogue, is used to image these primary tumors and metastases.

Other imaging studies:

  • Barium studies
  • Computed tomography
  • Endoscopy
  • Endoscopic ultrasonography.

On imaging studies, in general, the tumor may appear as a smooth submucosal mass, as a target lesion (if it ulcerates), as wall-thickening, or as a cystic or calcified mass.6

MANAGEMENT IS MULTIDISCIPLINARY

Any patient with a carcinoid tumor should be referred to a medical and surgical oncologist once the diagnosis is established. Referral to additional specialists, such as a gastroenterologist or an interventional radiologist, is based on the location and extent of disease.

Surgery is the cornerstone of therapy

Figure 1.
Patients with limited disease may need only surgical resection, but those with more extensive disease require additional management based on the presence and location of metastases (Figure 1).15

Drug therapy

Somatostatin analogues such as octreotide (Sandostatin) and lanreotide (Somatuline) are useful for treating carcinoid syndrome16 and also have a role in treating systemic metastases. These agents are effective in controlling flushing and diarrhea in 70% to 80% of patients.17 There are data, albeit limited, supporting a role for these agents in inhibiting tumor growth.18 They are the treatment of choice for carcinoid crisis (see discussion below). Important adverse effects include nausea, cramps, diarrhea; cholelithiasis; hypoglycemia or hyperglycemia; cardiac arrhythmias; and gastric atony.16

Interferon alfa is useful as an additive therapy when symptoms of carcinoid syndrome do not resolve with a somatostatin analogue alone. The addition of interferon alfa in these patients is useful for both symptom control (seen in 40% to 50% of those treated) and tumor stabilization (in 20% to 40% of those treated).19 However, it is still unclear whether combination drug therapy is more effective than a somatostatin analogue alone as the initial therapy for carcinoid syndrome.20 Adverse effects of interferon alfa include myelosuppression, depression, flu-like symptoms, and thyroid disturbances.

Supportive therapies

In patients with hepatic metastases who are not candidates for surgery, hepatic artery embolization with chemotherapy or particles can be used as palliative therapy. Severe adverse effects of this procedure include renal failure, hepatic failure, carcinoid crisis, and hepatic abscess and are seen in about 10% of patients.1

Conventional chemotherapy and molecularly targeted therapy are used for patients with rapidly progressive and widely metastatic disease. The precise role and efficacy of these therapies need further study.

Other supportive therapies for patients with carcinoid disease include dietary supplementation with vitamin B3, bronchodilators for bronchospasm, antidiarrheals, diuretics, and valve replacement for carcinoid heart disease.

 

 

LONG-TERM PROGNOSIS IS GENERALLY GOOD

The prognosis for patients with carcinoid tumors depends on the location and extent of disease. Tumors of the appendix and rectum have the best prognosis, with 5-year survival rates approaching 100% for localized carcinoid tumors of the appendix.3,21 In contrast, tumors of the small bowel, especially the ileum, are more aggressive and have the worst prognosis (a 5-year survival rate of about 60% to 65%).21

COMPLICATIONS

Other primary malignancies

Carcinoid tumors are often associated with the development of other tumors, not always in the gastrointestinal tract. As many as 52% of patients with small-bowel carcinoid tumors develop another primary tumor.22 This effect is thought to be related to the tumorigenic properties of the bioactive compounds secreted by carcinoid tumors. The other primary malignancy can be synchronous (diagnosed at the same time) or metachronous (diagnosed 1 to 7 years after the carcinoid) and generally arises from the gastrointestinal, genitourinary, or respiratory tract. Adenocarcinoma of the colon is reported as the most common second primary malignancy in patients with carcinoid tumors.22

The best strategy for surveillance in these patients is still unclear. Screening for tumors of the colon, small bowel, lung, cervix, and ovaries at the time of carcinoid tumor diagnosis followed by surveillance for these malignancies has been suggested as a possible approach; however, this comes at the cost of increased patient anxiety, cost, and morbidity from testing. 3

Carcinoid crisis

Carcinoid crisis is a life-threatening emergency caused by release of large amounts of vasoactive compounds from the carcinoid tumor, either spontaneously or provoked by tumor manipulation, surgery, chemotherapy, or hepatic artery embolization.2,5 The syndrome manifests as cardiovascular collapse (severe hypotension or hypertension), tachycardia, and altered mental status.

Treatment differs from those for other causes of shock in that catecholamines and calcium should not be used since they trigger the release of larger amounts of bioactive chemicals from the tumor. In addition, the shock in this situation is refractory to fluid. The mainstay of treatment is the infusion of octreotide and plasma. This crisis can be prevented by giving octreotide before manipulating the tumor.1,2,5

References
  1. Modlin IM, Oberg K, Chung DC, et al. Gastroenteropancreatic neuroendocrine tumors. Lancet Oncol 2008; 9:6172.
  2. Modlin IM, Kidd M, Latich I, Zikusoka MN, Shapiro MD. Current status of gastrointestinal carcinoids. Gastroenterology 2005; 128:17171751.
  3. Modlin IM, Lye KD, Kidd M. A 5-decade analysis of 13,715 carcinoid tumors. Cancer 2003; 97:934959.
  4. DeVries H, Verschueren R, Willemse P, Kema I, DeVries E. Diagnostic, surgical, and medical aspect of midgut carcinoids. Cancer Treat Rev 2002; 28:1125.
  5. Robertson RG, Griger WJ, Davis NB. Carcinoid tumors. Am Fam Physician 2006; 74:429434.
  6. Horton KM, Kamel I, Hofman L, Fishman EK. Carcinoid tumors of the small bowel: a multitechnique imaging approach. AJR Am J Roentgenol 2004; 182:559567.
  7. Kulke MH, Mayer RJ. Carcinoid tumors. N Engl J Med 1999; 340:858868.
  8. Bendelow J, Apps E, Jones LE, Poston GJ. Carcinoid syndrome. Eur J Surg Oncol 2008; 34:289296.
  9. Fink G, Krelbaum T, Yellin A, et al. Pulmonary carcinoid: presentation, diagnosis, and outcome in 142 cases in Israel and review of 640 cases from the literature. Chest 2001; 119:16471651.
  10. Bhattacharyya S, Toumpanakis C, Caplin ME, Davar J. Analysis of 150 patients with carcinoid syndrome seen in a single year at one institution in the first decade of the twenty-first century. Am J Cardiol 2008; 101:378381.
  11. Nasr C. Flushing: is it carcinoid or something else?Cleveland Clinic Disease Management Project, 2004. Available at http://www.clevelandclinicmeded.com/medicalpubs/diseasemanagement/endocrinology/flushing/flushing.htm. Accessed 10/25/08.
  12. Modlin IM, Tang LH. Approaches to the diagnosis of gut neuroendocrine tumors: the last word (today). Gastroenterology 1997; 112:583590.
  13. Campana D, Nori F, Piscitelli L, et al. Chromogranin A: is it a useful marker of neuroendocrine tumors? J Clin Oncol 2007; 25:19671973.
  14. Eriksson B, Oberg K. Peptide hormones as tumor markers in neuroendocrine gastrointestinal tumors. Acta Oncol 1991; 30:477483.
  15. National Comprehensive Cancer Network. Carcinoid tumors. http://www.nccn.org/professionals/physician_gls/PDF/neuroendocrine.pdf. Accessed 10/25/08.
  16. Oberg K, Kvols L, Caplin M, et al. Consensus report on the use of somatostatin analogs for the management of neuroendocrine tumors of the gastroenteropancreatic system. Ann Oncol 2004; 15:966973.
  17. Welin SV, Janson ET, Sundin A, et al. High-dose treatment with long-acting somatostatin analogue in patients with advanced midgut carcinoid tumours. Eur J Endocrinol 2004; 151:107112.
  18. Arnold R, Trautmann ME, Creutzfeldt W, et al. Somatostatin analogue octreotide and inhibition of tumor growth in metastatic endocrine gastroenteropancreatic tumors. Gut 1996; 38:430438.
  19. Bajetta E, Zilembo N, Di Bartolomeo M, et al. Treatment of metastatic carcinoids and other neuroendocrine tumors with recombinant interferon-alpha-2a. A study by the Italian Trials in Medical Oncology Group. Cancer 1993; 72:30993105.
  20. Faiss S, Pape UF, Bohmig M, et al. Prospective, randomized, multicenter trial on the antiproliferative effect of lanreotide, interferon-alfa, and their combination for therapy of metastatic neuroendocrine gastroenteropancreatic tumors—the International Lanreotide and Interferon Alfa Study Group. J Clin Oncol 2003; 21:26892696.
  21. Helland SK, Prosch AM, Viste A. Carcinoid tumors in the gastrointestinal tract—a population-based study from Western Norway. Scand J Surg 2006; 95:158161.
  22. Habal N, Sims C, Bilchik AJ. Gastrointestinal carcinoid tumors and second primary malignancies. J Surg Oncol 2000; 75:310316.
References
  1. Modlin IM, Oberg K, Chung DC, et al. Gastroenteropancreatic neuroendocrine tumors. Lancet Oncol 2008; 9:6172.
  2. Modlin IM, Kidd M, Latich I, Zikusoka MN, Shapiro MD. Current status of gastrointestinal carcinoids. Gastroenterology 2005; 128:17171751.
  3. Modlin IM, Lye KD, Kidd M. A 5-decade analysis of 13,715 carcinoid tumors. Cancer 2003; 97:934959.
  4. DeVries H, Verschueren R, Willemse P, Kema I, DeVries E. Diagnostic, surgical, and medical aspect of midgut carcinoids. Cancer Treat Rev 2002; 28:1125.
  5. Robertson RG, Griger WJ, Davis NB. Carcinoid tumors. Am Fam Physician 2006; 74:429434.
  6. Horton KM, Kamel I, Hofman L, Fishman EK. Carcinoid tumors of the small bowel: a multitechnique imaging approach. AJR Am J Roentgenol 2004; 182:559567.
  7. Kulke MH, Mayer RJ. Carcinoid tumors. N Engl J Med 1999; 340:858868.
  8. Bendelow J, Apps E, Jones LE, Poston GJ. Carcinoid syndrome. Eur J Surg Oncol 2008; 34:289296.
  9. Fink G, Krelbaum T, Yellin A, et al. Pulmonary carcinoid: presentation, diagnosis, and outcome in 142 cases in Israel and review of 640 cases from the literature. Chest 2001; 119:16471651.
  10. Bhattacharyya S, Toumpanakis C, Caplin ME, Davar J. Analysis of 150 patients with carcinoid syndrome seen in a single year at one institution in the first decade of the twenty-first century. Am J Cardiol 2008; 101:378381.
  11. Nasr C. Flushing: is it carcinoid or something else?Cleveland Clinic Disease Management Project, 2004. Available at http://www.clevelandclinicmeded.com/medicalpubs/diseasemanagement/endocrinology/flushing/flushing.htm. Accessed 10/25/08.
  12. Modlin IM, Tang LH. Approaches to the diagnosis of gut neuroendocrine tumors: the last word (today). Gastroenterology 1997; 112:583590.
  13. Campana D, Nori F, Piscitelli L, et al. Chromogranin A: is it a useful marker of neuroendocrine tumors? J Clin Oncol 2007; 25:19671973.
  14. Eriksson B, Oberg K. Peptide hormones as tumor markers in neuroendocrine gastrointestinal tumors. Acta Oncol 1991; 30:477483.
  15. National Comprehensive Cancer Network. Carcinoid tumors. http://www.nccn.org/professionals/physician_gls/PDF/neuroendocrine.pdf. Accessed 10/25/08.
  16. Oberg K, Kvols L, Caplin M, et al. Consensus report on the use of somatostatin analogs for the management of neuroendocrine tumors of the gastroenteropancreatic system. Ann Oncol 2004; 15:966973.
  17. Welin SV, Janson ET, Sundin A, et al. High-dose treatment with long-acting somatostatin analogue in patients with advanced midgut carcinoid tumours. Eur J Endocrinol 2004; 151:107112.
  18. Arnold R, Trautmann ME, Creutzfeldt W, et al. Somatostatin analogue octreotide and inhibition of tumor growth in metastatic endocrine gastroenteropancreatic tumors. Gut 1996; 38:430438.
  19. Bajetta E, Zilembo N, Di Bartolomeo M, et al. Treatment of metastatic carcinoids and other neuroendocrine tumors with recombinant interferon-alpha-2a. A study by the Italian Trials in Medical Oncology Group. Cancer 1993; 72:30993105.
  20. Faiss S, Pape UF, Bohmig M, et al. Prospective, randomized, multicenter trial on the antiproliferative effect of lanreotide, interferon-alfa, and their combination for therapy of metastatic neuroendocrine gastroenteropancreatic tumors—the International Lanreotide and Interferon Alfa Study Group. J Clin Oncol 2003; 21:26892696.
  21. Helland SK, Prosch AM, Viste A. Carcinoid tumors in the gastrointestinal tract—a population-based study from Western Norway. Scand J Surg 2006; 95:158161.
  22. Habal N, Sims C, Bilchik AJ. Gastrointestinal carcinoid tumors and second primary malignancies. J Surg Oncol 2000; 75:310316.
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KEY POINTS

  • Bioactive compounds secreted by carcinoid tumors cause carcinoid syndrome—ie, bronchospasm, diarrhea, cutaneous flushing, and right-sided valvular heart lesions.
  • Endocardial fibrotic plaques can occur in patients with carcinoid tumors. The right side of the heart is affected more often than the left, as the left side is protected by inactivation of the bioactive compounds in the lungs. Tricuspid valve regurgitation is the most common finding.
  • Since carcinoid tumors have high concentrations of somatostatin receptors, octreotide scanning offers a distinct advantage in imaging them: use of radiolabeled octreotide, a somatostatin analogue, enables imaging of primary tumors and metastases.
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Black hairy tongue

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Black hairy tongue

A 71-year-old man presents for evaluation of an asymptomatic black discoloration of the tongue that he noticed several days earlier. The tongue does not itch or hurt, and the patient is otherwise well, although he is concerned about potential malignancy.

He has a history of hypertension, hyperuricemia, and type 2 diabetes treated with oral glucose-lowering drugs, and he has had no recent changes in his medications. He drinks coffee and uses tobacco. His oral hygiene is poor, with intense halitosis.

Figure 1. Elongation of the filiform papillae with a blackish discoloration on the dorsal surface of the tongue.
Physical examination shows a black coloration of the tongue that appears as an elongation of the filiform papillae on the dorsal surface, with no other abnormalities (Figure 1). The physical examination is otherwise normal. Culture of the dorsal surface of the tongue shows no bacterial or fungal overgrowth.

Q: What is the most likely diagnosis?

  • Oral leukoplakia
  • Epidermoid carcinoma of the tongue
  • Malignant melanoma of the tongue
  • Mucosal candidiasis
  • Black hairy tongue

A: Black hairy tongue is correct. A simple treatment consisting of brushing the tongue daily with a soft toothbrush enhanced by previous application of 30% urea is recommended to the patient, and the discoloration resolves completely within 4 weeks. He is educated on correct oral hygiene and discontinues smoking, with no clinical relapses after 2 years of follow-up.

THE CAUSES AND THE COURSE

Black hairy tongue, also known as lingua villosa nigra, is a painless, benign disorder caused by defective desquamation and reactive hypertrophy of the filiform papillae of the tongue. The hairy appearance is due to elongation of keratinized filiform papillae, which may have different colors, varying from white to yellowish brown to black depending on extrinsic factors (eg, tobacco, coffee, tea, food) and intrinsic factors (ie, chromogenic organisms in normal flora).1

The exact pathogenesis is unclear. Precipitating factors include poor oral hygiene, use of the antipsychotic drug olanzapine1 (Zyprexa) or a broad-spectrum antibiotic such as erythromycin,2 and therapeutic radiation of the head and the neck. Tobacco use and drinking coffee and tea are also contributory factors. Neurologic conditions such as trigeminal neuropathy may be associated. 3 Manabe et al4 applied a panel of antikeratin probes, showing that defective desquamation of the cells in the central column of filiform papillae resulted in the formation of highly elongated, cornified spines or “hairs”—the hallmark of lingua villosa nigra.

PRESENTATION AND DIAGNOSIS

Black hairy tongue is usually asymptomatic. However, symptoms such as altered (metallic) taste, nausea, or halitosis may be noted. Most patients with hairy tongue drink coffee or tea, often in addition to tobacco use.

The diagnosis is based on filiform papillae that are elongated more than 3 mm on the dorsal surface of the tongue. Cultures may be taken to rule out a superimposed oral candidiasis or other suspected oral infection.

MANAGEMENT

Although frightening to the patient, black hairy tongue is completely harmless. In most cases, treatment does not require drugs. If fungal overgrowth is present, a topical antifungal can be used when the condition is symptomatic.

Empirical approaches such as brushing or scraping the tongue, improving oral hygiene, and eliminating potential offending factors (eg, tobacco, candies, strong mouthwashes, antibiotics) is usually sufficient to resolve the lesions.5

In our experience, educating the patient about proper oral hygiene (including discontinuing smoking) and encouraging routine tongue brushing are the best preventive and therapeutic measures.

References
  1. Tamam L, Annagur BB. Black hairy tongue associated with olanzapine treatment: a case report. Mt Sinai J Med 2006; 73:891894.
  2. Pigatto PD, Spadari F, Meroni L, Guzzi G. Black hairy tongue associated with long-term oral erythromycin use. J Eur Acad Dermatol Venereol 2008; 22:12691270.
  3. Chesire WP. Unilateral black hairy tongue in trigeminal neuralgia. Headache 2004; 44:908910.
  4. Manabe M, Lim HW, Winzer M, Loomis CA. Architectural organization of filiform papillae in normal and black hairy tongue epithelium: dissection of differentiation pathways in a complex human epithelium according to their patterns of keratin expression. Arch Dermatol 1999; 135:177181.
  5. Sarti GM, Haddy RI, Schaffer D, Kihm J. Black hairy tongue. Am Fam Physician 1990; 41:17511755.
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Sergio Vañó-Galván, 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

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

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 71-year-old man presents for evaluation of an asymptomatic black discoloration of the tongue that he noticed several days earlier. The tongue does not itch or hurt, and the patient is otherwise well, although he is concerned about potential malignancy.

He has a history of hypertension, hyperuricemia, and type 2 diabetes treated with oral glucose-lowering drugs, and he has had no recent changes in his medications. He drinks coffee and uses tobacco. His oral hygiene is poor, with intense halitosis.

Figure 1. Elongation of the filiform papillae with a blackish discoloration on the dorsal surface of the tongue.
Physical examination shows a black coloration of the tongue that appears as an elongation of the filiform papillae on the dorsal surface, with no other abnormalities (Figure 1). The physical examination is otherwise normal. Culture of the dorsal surface of the tongue shows no bacterial or fungal overgrowth.

Q: What is the most likely diagnosis?

  • Oral leukoplakia
  • Epidermoid carcinoma of the tongue
  • Malignant melanoma of the tongue
  • Mucosal candidiasis
  • Black hairy tongue

A: Black hairy tongue is correct. A simple treatment consisting of brushing the tongue daily with a soft toothbrush enhanced by previous application of 30% urea is recommended to the patient, and the discoloration resolves completely within 4 weeks. He is educated on correct oral hygiene and discontinues smoking, with no clinical relapses after 2 years of follow-up.

THE CAUSES AND THE COURSE

Black hairy tongue, also known as lingua villosa nigra, is a painless, benign disorder caused by defective desquamation and reactive hypertrophy of the filiform papillae of the tongue. The hairy appearance is due to elongation of keratinized filiform papillae, which may have different colors, varying from white to yellowish brown to black depending on extrinsic factors (eg, tobacco, coffee, tea, food) and intrinsic factors (ie, chromogenic organisms in normal flora).1

The exact pathogenesis is unclear. Precipitating factors include poor oral hygiene, use of the antipsychotic drug olanzapine1 (Zyprexa) or a broad-spectrum antibiotic such as erythromycin,2 and therapeutic radiation of the head and the neck. Tobacco use and drinking coffee and tea are also contributory factors. Neurologic conditions such as trigeminal neuropathy may be associated. 3 Manabe et al4 applied a panel of antikeratin probes, showing that defective desquamation of the cells in the central column of filiform papillae resulted in the formation of highly elongated, cornified spines or “hairs”—the hallmark of lingua villosa nigra.

PRESENTATION AND DIAGNOSIS

Black hairy tongue is usually asymptomatic. However, symptoms such as altered (metallic) taste, nausea, or halitosis may be noted. Most patients with hairy tongue drink coffee or tea, often in addition to tobacco use.

The diagnosis is based on filiform papillae that are elongated more than 3 mm on the dorsal surface of the tongue. Cultures may be taken to rule out a superimposed oral candidiasis or other suspected oral infection.

MANAGEMENT

Although frightening to the patient, black hairy tongue is completely harmless. In most cases, treatment does not require drugs. If fungal overgrowth is present, a topical antifungal can be used when the condition is symptomatic.

Empirical approaches such as brushing or scraping the tongue, improving oral hygiene, and eliminating potential offending factors (eg, tobacco, candies, strong mouthwashes, antibiotics) is usually sufficient to resolve the lesions.5

In our experience, educating the patient about proper oral hygiene (including discontinuing smoking) and encouraging routine tongue brushing are the best preventive and therapeutic measures.

A 71-year-old man presents for evaluation of an asymptomatic black discoloration of the tongue that he noticed several days earlier. The tongue does not itch or hurt, and the patient is otherwise well, although he is concerned about potential malignancy.

He has a history of hypertension, hyperuricemia, and type 2 diabetes treated with oral glucose-lowering drugs, and he has had no recent changes in his medications. He drinks coffee and uses tobacco. His oral hygiene is poor, with intense halitosis.

Figure 1. Elongation of the filiform papillae with a blackish discoloration on the dorsal surface of the tongue.
Physical examination shows a black coloration of the tongue that appears as an elongation of the filiform papillae on the dorsal surface, with no other abnormalities (Figure 1). The physical examination is otherwise normal. Culture of the dorsal surface of the tongue shows no bacterial or fungal overgrowth.

Q: What is the most likely diagnosis?

  • Oral leukoplakia
  • Epidermoid carcinoma of the tongue
  • Malignant melanoma of the tongue
  • Mucosal candidiasis
  • Black hairy tongue

A: Black hairy tongue is correct. A simple treatment consisting of brushing the tongue daily with a soft toothbrush enhanced by previous application of 30% urea is recommended to the patient, and the discoloration resolves completely within 4 weeks. He is educated on correct oral hygiene and discontinues smoking, with no clinical relapses after 2 years of follow-up.

THE CAUSES AND THE COURSE

Black hairy tongue, also known as lingua villosa nigra, is a painless, benign disorder caused by defective desquamation and reactive hypertrophy of the filiform papillae of the tongue. The hairy appearance is due to elongation of keratinized filiform papillae, which may have different colors, varying from white to yellowish brown to black depending on extrinsic factors (eg, tobacco, coffee, tea, food) and intrinsic factors (ie, chromogenic organisms in normal flora).1

The exact pathogenesis is unclear. Precipitating factors include poor oral hygiene, use of the antipsychotic drug olanzapine1 (Zyprexa) or a broad-spectrum antibiotic such as erythromycin,2 and therapeutic radiation of the head and the neck. Tobacco use and drinking coffee and tea are also contributory factors. Neurologic conditions such as trigeminal neuropathy may be associated. 3 Manabe et al4 applied a panel of antikeratin probes, showing that defective desquamation of the cells in the central column of filiform papillae resulted in the formation of highly elongated, cornified spines or “hairs”—the hallmark of lingua villosa nigra.

PRESENTATION AND DIAGNOSIS

Black hairy tongue is usually asymptomatic. However, symptoms such as altered (metallic) taste, nausea, or halitosis may be noted. Most patients with hairy tongue drink coffee or tea, often in addition to tobacco use.

The diagnosis is based on filiform papillae that are elongated more than 3 mm on the dorsal surface of the tongue. Cultures may be taken to rule out a superimposed oral candidiasis or other suspected oral infection.

MANAGEMENT

Although frightening to the patient, black hairy tongue is completely harmless. In most cases, treatment does not require drugs. If fungal overgrowth is present, a topical antifungal can be used when the condition is symptomatic.

Empirical approaches such as brushing or scraping the tongue, improving oral hygiene, and eliminating potential offending factors (eg, tobacco, candies, strong mouthwashes, antibiotics) is usually sufficient to resolve the lesions.5

In our experience, educating the patient about proper oral hygiene (including discontinuing smoking) and encouraging routine tongue brushing are the best preventive and therapeutic measures.

References
  1. Tamam L, Annagur BB. Black hairy tongue associated with olanzapine treatment: a case report. Mt Sinai J Med 2006; 73:891894.
  2. Pigatto PD, Spadari F, Meroni L, Guzzi G. Black hairy tongue associated with long-term oral erythromycin use. J Eur Acad Dermatol Venereol 2008; 22:12691270.
  3. Chesire WP. Unilateral black hairy tongue in trigeminal neuralgia. Headache 2004; 44:908910.
  4. Manabe M, Lim HW, Winzer M, Loomis CA. Architectural organization of filiform papillae in normal and black hairy tongue epithelium: dissection of differentiation pathways in a complex human epithelium according to their patterns of keratin expression. Arch Dermatol 1999; 135:177181.
  5. Sarti GM, Haddy RI, Schaffer D, Kihm J. Black hairy tongue. Am Fam Physician 1990; 41:17511755.
References
  1. Tamam L, Annagur BB. Black hairy tongue associated with olanzapine treatment: a case report. Mt Sinai J Med 2006; 73:891894.
  2. Pigatto PD, Spadari F, Meroni L, Guzzi G. Black hairy tongue associated with long-term oral erythromycin use. J Eur Acad Dermatol Venereol 2008; 22:12691270.
  3. Chesire WP. Unilateral black hairy tongue in trigeminal neuralgia. Headache 2004; 44:908910.
  4. Manabe M, Lim HW, Winzer M, Loomis CA. Architectural organization of filiform papillae in normal and black hairy tongue epithelium: dissection of differentiation pathways in a complex human epithelium according to their patterns of keratin expression. Arch Dermatol 1999; 135:177181.
  5. Sarti GM, Haddy RI, Schaffer D, Kihm J. Black hairy tongue. Am Fam Physician 1990; 41:17511755.
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