Chemoprophylaxis

Chemoprevention (also Chemoprophylaxis) refers to the administration of a medication for the purpose of preventing disease or infection.[1] Antibiotics, for example, may be administered to patients with disorders of immune system function to prevent bacterial infections (particularly opportunistic infection).[2] Antibiotics may also be administered to healthy individuals to limit the spread of an epidemic, or to patients who have repeated infections (such as urinary tract infections) to prevent recurrence. It may also refer to the administration of heparin to prevent deep venous thrombosis in hospitalized patients.

In some cases, chemoprophylaxis is initiated to prevent the spread of an existing infection in an individual to a new organ system, as when intrathecal chemotherapy is administered in patients with malignancy to prevent further infection.

The use of chemoprophylaxis is limited primarily by two factors: risk and financial costs.

Specific diseases

Using chemoprophylaxis as a treatment against early signs of tuberculosis has proven to be effective. In familial adenomatous polyposis physicians observed polyps regression with NSAIDs for anti-inflammatory therapy. Chemoprophylaxis is also used to treat several different varieties of meningococcal infections for close contact exposure to Neisseria meningitidis.

See also

References

  1. Woolf, Steven H.; Jonas, Steven; Kaplan-Liss, Evonne (2008), Health Promotion and Disease Prevention in Clinical Practice, Lippincott Williams & Wilkins, pp. 346–358, ISBN 078177599X.
  2. Golan, David E. (2008), Principles of Pharmacology: The Pathophysiologic Basis of Drug Therapy, Lippincott Williams & Wilkins, p. 578, ISBN 0781783550.
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