PST06106 Basic Pharmacotherapy – Complete Full Notes

NTA Level 6 • Semester 1 • PST06106

Basic Pharmacotherapy – Complete Full Notes

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PST 06106

BASIC PHARMACOTHERAPY

Session 1: Introduction to Pharmacotherapy

Learning objectives

By the end of this session students are expected to be able to:

Define terminologies used in Pharmacotherapy

Describe principles and concepts applied in Pharmacotherapy

Explain importance of Pharmacotherapy in the management of common diseases

Definition of Common Terminologies used in Pharmacotherapy

Pharmacotherapy

is application of knowledge in making therapeutic decisions that are most likely to have maximum positive benefit for a specific patient.

Pharmacotherapy specialist:

is an individual who is specialized in administering and prescribing medication, and requires extensive academic knowledge in pharmacotherapy.

Pharmaceutical

personel

are experts in pharmacotherapy and are responsible for ensuring the safe, appropriate, and economical use of pharmaceutical drugs.

Definition of Common Terminologies used in Pharmacotherapy Cont.…..

Pathophysiology

is the physiology of abnormal states; specifically: the functional changes that accompany a particular syndrome or disease.

Also is the study of changes in the way the body works that result from disease or injury

Pharmaceutical care involves the process through which a pharmacist/ other pharmaceutical personnel cooperates with a patient and other professionals in designing, implementing, and monitoring a therapeutic plan that will produce specific therapeutic outcomes for the patient

Principles

and Concepts applied in pharmacotherapy

There

are

three

steps that are involved in the Pharmacotherapy process which are

;

Patient assessment

Development of the pharmacotherapy care plan

Evaluation of the impact or results of the care plan

Principles and Concepts applied in pharmacotherapy

Cont

…..

Fig 1.1 Patient Care Process in the Pharmacotherapy

Patient Assessment

The focus

is on drug therapy problems in which case it is important to assess if the patient’s problem(s) is/are be caused by drug therapy and can be managed by a change in drug therapy

The following is the list of drug therapy problems that should be identified;

Inappropriate drug

selection,

Need for additional drug therapy

Unnecessary drug therapy

Incorrect drug regimen

Therapeutic

duplication

Drug allergy/adverse drug event

Drug Interactions

Medication adherence issues

Patient Assessment

Cont

…..

Once a drug therapy problem is identified and categorized, it is then necessary to identify the cause of the problem, thereby leading to potential solutions.

The process of drug therapy problem identification is to assessing the patient’s drug therapy needs and ensuring appropriateness, effectiveness and safety of medications, and the patient’s adherence

Pharmacotherapy

Care Plan

The

pharmacotherapy care plan is important in order to achieve improved pharmacotherapy outcomes.

It

is the action plan developed from assessment of patient described

above.

Each

item in the patient’s problem list must be addressed in the care plan, and the care plan should be prioritized in the same way as the problem list.

The pharmacotherapy care plan has several key components for each

problem:

Current

drug regimen

Drug

therapy

problems

Therapy

goals, desired endpoints

Pharmacotherapy Care Plan

Cont

The

goals of therapy must be achievable and realistic for the

patien

Drug

therapy may aim to

cure a disease;

reduce or eliminate signs and/or symptoms

slow or halt the progression of a disease

prevent a disease

normalize laboratory values

and/or

assist in the diagnostic process

Therapeutic recommendations

Rationale

Therapeutic alternatives

Monitoring

Pharmacotherapy Care Plan

C

ont

Monitoring

helps in determining whether treatment goals and endpoints (achieving positive goals and avoiding negative endpoints) are being reached.

An effective monitoring plan must be realistic for the patient setting and include

specific monitoring parameters (clinical and laboratory/diagnostic test)

frequency of monitoring, and

When the patient needs to be seen again for follow-up.

Patient

education

Evaluation

The

patient care process involves continuous follow-up.

As

the pharmacotherapy care plan is implemented, the patient’s response to

therapy is

monitored, and changes in therapy may be necessary.

Changes in previous problems or the development of new signs and symptoms will require the assessment process and changes in the pharmacotherapy care plan

During the Pharmacotherapy process, it is important to consider/review the following factors for optimal therapeutic outcome

;

Evaluation

Cont

…….

Patient

Dermographics

—name, age, etc.

Chief Complaint—why the patient is seeking help, in the patient’s own words

History of Present Illness (HPI)—the patient’s story about why they are seeking help

Past Medical History (PMH)—including all significant illnesses, surgical procedures, injuries

Family History—age and health of immediate family (parents, siblings, children); for deceased relatives, the age and cause of death are included; any hereditary diseases should be noted

E

valuation

Cont

…….

Social

History—may include where the patient is from or lives, ethnicity/race, marital status, number of children, educational background, occupation, diet

Tobacco/Alcohol/Substance

Use

Allergy/Intolerances/Adverse

Drug Events (ADEs)—a common area where information from the patient is missing or

incomplete

Medication

History—should include current (or medications prior to admission if hospitalized) and previous medications; the list should include what the patient actually is taking, not just what is prescribed, and must include OTC drugs and dietary supplements (including herbal and complementary/alternative products

).

Evaluation

Cont

…….

Signs

and symptoms

Laboratory

and Other Diagnostic Tests

Diagnosis

.

Treatment

(Drug) plan

Follow-up plan

Activity: Small Group Discussion

What is the importance of Pharmacotherapy?

Importance of pharmacotherapy

Helps in optimization of drug treatment in complex pharmacotherapy patients such as;

Patients with multiple medications

Patients with multiple disease states or conditions

Patients on narrow therapeutic index medications

Patients on medications requiring laboratory monitoring

Helps in optimization of drug therapy in patients with high risk for loss of continuity of care such as;

Patients with multiple prescribers

Patients with recent transitions of care (e.g., hospital discharge, rehabilitation, skilled nursing facility discharge)

Importance of pharmacotherapy cont…

Helps in reduction of medication nonadherence especially in patients with;

Irregular refill history

History of failure to pick up new prescriptions

Stockpiling or incorrect pill counts

Financial burden (e.g., uninsured or underinsured)

Low health literacy

Patient’s beliefs indicate resistance to treatment

High-cost regimens

Noticeable decline in the health or functionality

Improves patients-pharmaceutical personnel relationship which is important for better therapeutic

outcome

Key Points

Pharmacotherapy

is the therapy that is provided using pharmaceutical

Pharmacotherapy comprises the safe, applicable, and cost-effective use of pharmaceutical drugs.

Steps that are involved in the Pharmacotherapy process which are Patient assessment, Development of the pharmacotherapy care plan and Evaluation of the impact or results of the care plan.

Pharmacotherapy helps in improving quality of patient care through optimal medication management based on sound

pharmacotherapeutic

principles.

Evaluation

What

is pharmacotherapy?

What are the steps involved in the pharmacotherapy process?

What is importance of pharmacotherapy?

References

Wells

BG,

DiPiro

J,

Schwinghammer

T (2013),

Pharmacotherapy Handbook

(6

th

Ed). New York, NY: McGraw-Hill.

DiPiro

JT, Talbert RL, Yee GC, Matzke GR, Wells BG, Posey ML, (2008):

Pharmacotherapy: A Pathophysiologic Approach

(7

th

ed

): New York, NY: McGraw-Hill.

Katz M D., Matthias KR., Chisholm-Burns M A., Pharmacotherapy(2011)

Principles & Practice Study Guide: A Case-Based Care Plan Approach

: New York, NY: McGraw-Hill.

Schwinghammer

TL, Koehler JM (2009)

Pharmacotherapy Casebook: A Patient-Focused Approach

(7

th

ed

): New York, NY: McGraw-Hill.

PST 06106

Basic

Pharmacotherapy

Session 2: Therapeutic Drug Monitoring (TDM)

Learning Tasks

By the end of this session students are expected to be able to:

Define therapeutic drug monitoring

List principles and outline concepts of therapeutic drug monitoring

Outline criteria for therapeutic drug monitoring

List drugs that qualify for therapeutic drug

monotoring

Explain clinical significance of therapeutic drug monitoring

List limitations of therapeutic drug monitoring

Principles and Concepts of Therapeutic Drug Monitoring

Therapeutic

drug monitoring (TDM)

is defined as the use of drug concentration measurements in plasma as an aid to the management of drug therapy for the cure, alleviation or prevention of

disease. TDM

enables the assessment of the efficacy and safety of a particular medication in a variety of clinical settings

.

TDM aims at improving patient care by adjusting the dose of drugs for which clinical experience or clinical trial have shown it improved outcome in the general or special populations

Principles and Concepts of Therapeutic Drug Monitoring

Cont

…..

Therapeutic Drug Monitoring aims to individualize therapeutic regimens for optimal patient benefit and avoid both

sub therapeutic

and toxic plasma drug concentrations.

Specifically, TDM is a practice applied to a small group of drugs in which there is a direct relation between plasma drug concentration and pharmacological response

Therefore, close relationship between the plasma level of the drug and its clinical effect is essential.

If such a relationship does not exit TDM is of little value.

The measurement of plasma level is justified only when the information provided is of potential therapeutic benefit.

Principles and Concepts of Therapeutic Drug Monitoring

Cont.…..

In summary, TDM process involves the following;

Administration of a predetermined dose of drug

Collection of blood samples

Determination/measurements of blood samples using analytical procedures

Evaluation of Clinical effect of drug

Development/Adjustment

of dosage

regimen

Activity: Buzzing

What

are the criteria for therapeutic drug monitoring?

Criteria for therapeutic drug monitoring

The drug in question has a narrow therapeutic range,

eg

: Lithium, phenytoin, and digoxin

A direct relationship exists between the drug or drug metabolite levels in plasma and the pharmacological or toxic effects,

The therapeutic effect can not be readily assessed by the clinical observation,

Large individual variability in steady state plasma concentration exits at any given dose

Appropriate analytic techniques are available to determine the drug and metabolite

levels

Criteria for therapeutic drug

monitoring

Cont

Drugs for which relationship between dose and plasma concentration is unpredictable,

e.g

Phenytoin

Non compliance

Therapeutic failure

Major organ failure

Prevention of adverse drug effects

Drugs that qualify for therapeutic drug monitoring

Cardio

active drugs

amiodarone,

digoxin,

digitoxin

disopyramide

,

lignocaine,

procainamide,

propranolol and

quinidine

Drugs that qualify for therapeutic drug

monitoring Cont.….

Aminoglycoside

gentamycin,

A

mikacin

and tobramycin

Anti Cancer

methotrexate

Antidepressants

:

lithium

tricyclic

antidepressants

Drugs that qualify for therapeutic drug monitoring Cont.….

Antiepileptic

drugs

Phenytoin,

phenobarbitone

benzodiazepines,

carbamazepine,

Valproic

acid and

ethosuximide

Bronchodilators :

theophylline

Therapeutic drug monitoring process

Fig 2.1: Summary of TDM Process

Clinical significance of Therapeutic drug monitoring

Drug levels from TDM are used in conjunction with other clinical data to assist practitioners in determining how a patient is responding.

Drug levels provide a basis for individualizin

g

patient dosage regimens.

Drug levels assist in determining if a change in patient-specific

pharmacokinetics

has occurred during a course of treatment, whether as a result of a change in physiological state, a change in diet, or addition of other drugs.

Clinical significance of Therapeutic drug

monitoring Cont.

Maximizes drug efficacy

Helps in avoidance of drug toxicity

Identifies therapeutic failure due to

subtherapeutic

level

May help to identifies patients who are non compliant

Limitation of Therapeutic

D

rug

M

onitoring(TDM)

There may be some factors that may lead to incorrect interpretation of plasma drug levels such as;

Non-compliance of patient leading to low plasma drug levels

Low dose administered which leads to

subtharapapeutic

concentrations

Patient suffer from mal-absorption

Drug with low bioavailability may also lead to

subtherapeutic

concentrations

Concomitant drugs that could affect the plasma levels of the drug in question

Limitation of Therapeutic Drug Monitoring(TDM

) Cont.….

Hepatic or renal dysfunction

Diseases related to genetic factors affecting drug metabolism

.Time of administration of the drug is not accurate.

Dose administration error.

Inaccurate time of sampling, or timing was before steady-state is reached

Wrong site of sampling.

Lab assay error.

Limitation of Therapeutic Drug Monitoring(TDM) Cont.….

Effect of age

There is a great variability in response to drugs at extremes of age.

As an example, elderly patients are more sensitive to the CNS depressant effect of drugs but are less sensitive to cardiovascular effects of Propranolol.

It is well known that children are more sensitive to morphine.

Pregnancy

Many drugs can be affected by pregnancy state.

As an example, drug levels of phenytoin and

phenobarbitone

are lower during pregnancy

Key Points

TDM is a very important and widely used technique throughout the treatment process.

TDM is used when there is a sufficient relationship between the plasma level of the drug and its clinical effect

Evaluation

What is therapeutic drug monitoring?

What are steps involved during therapeutic drug monitoring?

What are criteria for therapeutic drug monitoring

What the clinical significance of therapeutic drug monitoring

References

Wells

BG,

DiPiro

J,

Schwinghammer

T (2013), Pharmacotherapy Handbook (6th Ed). New York, NY: McGraw-Hill.

DiPiro

JT, Talbert RL, Yee GC, Matzke GR, Wells BG, Posey ML, (2008): Pharmacotherapy: A Pathophysiologic Approach (7th

ed

): New York, NY: McGraw-Hill.

Katz M D., Matthias KR., Chisholm-Burns M A., Pharmacotherapy(2011) Principles & Practice Study Guide: A Case-Based Care Plan Approach: New York, NY: McGraw-Hill.

Schwinghammer

TL, Koehler JM (2009) Pharmacotherapy Casebook: A Patient-Focused Approach (7th

ed

): New York, NY: McGraw-Hill.

PST 06106

Basic Pharmacotherapy

Session 3: Pharmacotherapy of Malaria

Learning Objectives

By the end of this session students are expected to be able to:

Define malaria

Explain pathophysiology of malaria

Explain the clinical presentation of malaria

Outline diagnosis of malaria

Describe pharmacological treatment of malaria

Describe monitoring malaria therapy

Activity: Buzzing

What is the disease status of a patient with malaria?

Definition of Malaria

Uncomplicated malaria

: defined as symptomatic malaria without signs of severity or evidence (clinical or laboratory) of vital organ dysfunction.

It has the following features; fever, headache, joint pains, malaise, vomiting, diarrhoea, body ache, body weakness, poor appetite, pallor, enlarged spleen

Severe malaria:

In a patient with P. falciparum asexual

parasitemia

and no other obvious cause of symptoms the presence of one or more of features listed below classify the patient as suffering from severe malaria

It has the following features; prostration/extreme weakness, impaired consciousness, change of behaviour, convulsions, respiratory distress (due to lactic acidosis and/or pulmonary oedema), bleeding tendency, jaundice, circulatory collapse, vomiting everything, inability to drink or breast feed

Pathophysiology of Malaria

The

Plasmodium species that infect humans are

P. falciparum, P. vivax, P. ovale, P. malariae and P. knowlesi

(rarely).

The

basic elements of the life cycle are the same for all Plasmodium

sp

Transmission begins when a female Anopheles mosquito feeds on a person with malaria and ingests blood containing gametocytes.

During the following 1 to 2

wk

, gametocytes inside the mosquito reproduce sexually and produce infective

sporozoites

.

When

the mosquito feeds on another human,

sporozoites

are inoculated and quickly reach the liver and infect hepatocytes.

Pathophysiology of Malaria

cont

….

The parasites mature into tissue

schizonts

within hepatocytes. Each

schizont

produces 10,000 to 30,000

merozoites

, which are released into the bloodstream 1 to 3

wk

later when the hepatocyte ruptures.

Each

merozoite

can invade an RBC and there transform into a

trophozoite

Trophozoites

grow, and most develop into erythrocyte

schizonts

;

schizonts

produce further

merozoites

, which 48 to 72 h later rupture the RBC and are released in plasma.

Pathophysiology

of Malaria

cont.….

These

merozoites

then rapidly invade new RBCs, repeating the cycle

Some

trophozoites

develop into gametocytes, which are ingested by an

Anopheles

mosquito

They undergo sexual union in the gut of the mosquito, develop into oocysts, and release infective

sporozoites

, which migrate to the salivary glands

Plasmodium Life Cycle

Clinical Presentation Of Malaria

Signs and symptoms of uncomplicated Malaria

Fever

Headache

Malaise

Joint pains

Vomiting /diarrhoea

Body ache

Poor appetite

Body weakness

Pallor

Enlarged spleen

Signs

and symptoms of Severe Malaria

Extreme

weakness

Impaired consciousness

Change of behaviour ( hallucinations, delusions, agitation, and acute state of confusion)

Respiratory distress

Bleeding tendency

Jaundice

Circulatory collapse/ shock

Vomiting everything

Inability to drink or

breastfeed

Diagnosis of Malaria

Parasite-based diagnosis is recommended for all patients presenting with signs and symptoms of malaria.

The recommended investigations are: malaria microscopy and malaria rapid diagnostic tests (

mRDTs

)

In severe malaria, blood slide (BS) is a recommended malaria test as it quantifies parasitemia.

Activity: Small Group Discussion

What is pharmacological treatment of

malaria

?

Pharmacological Treatment of Malaria

Management OF Uncomplicated

M

alaria

Drug

of choice for treatment of uncomplicated malaria is Artemether-Lumefantrine (AL), which is a fixed formulation of artemether 20mg and lumefantrine 120mg or dispersible tablets for paediatric

use.

Dosage regimen of ALU

Pharmacological Treatment of Malaria Cont.…..

Use of

Artemether-lumefantrine

(

ALu

) in Pregnancy

Presently, Artemisinin compounds cannot be recommended for treatment of malaria in the first trimester of pregnancy.

In the first trimester of pregnancy quinine should be used as first line treatment.

After the first trimester

ALu

tablets is first line medicine.

Use of

Artemether-lumefantrine

(

ALu

) in Lactation

Due to the long elimination half-life of

Lumefantrine

(up to 10 days), it is not recommended in mothers breast-feeding children below 5kgs.

In this case quinine should be used

.

Pharmacological Treatment of Malaria Cont.…..

Management of Severe Malaria

Parenteral

artesunate

Dosage: 2.4 mg/kg in body weight. IV or IM given on admission (time = 0 hour), then at 12 hours and 24 hours for a minimum of 3 injections in 24 hours regardless of patient’s recovery
Alternatively; Injectable Artemether should be administered in a dose of 3.2mg/kg body weight loading dose IM stat then 1.6mg/kg

bwt

(time= 0 hrs, then 24hrs then 48 hrs)

Major Anti Malarial Drugs

Monitoring Of Malaria Therapy

It is important to monitor Malaria therapy in order to evaluate if it is effective

Patients can be monitored clinically and/or by using laboratory test to confirm for absence/presence of malaria parasite in their blood

A follow-up period after the completion of the Malaria therapy varies according to the drugs used.

Follow-up periods longer than 14 days are appropriate for

amodiaquine

, chloroquine and SP which is 28 days

For

lumefantrine+artemether

is 42 days,

For

mefloquine

is 63 days

Monitoring Of Malaria Therapy

Cont

This allows drug levels in the blood to fall below the minimum therapeutic threshold.

Any recrudescence of parasites before this threshold is reached would be due to drug resistance

Recrudescence after this threshold is reached is not necessarily related to resistance (even sensitive parasites could recrudesce if blood drug levels are

subtherapeutic

).

Shorter follow-up (i.e. <14 days) will underestimate overall treatment failure rates

It is also important for patient to report any adverse reaction of the drugs that may occurs during Malaria therapy.

Key Points

P

. falciparum

causes microvascular obstruction and tissue ischemia, particularly in the brain, kidneys, lungs, and GI tract of nonimmune infants and adults; patients may die within days of their initial symptoms.

P.

vivax

, P.

ovale

, and

P.

malariae

typically do not compromise vital organs; mortality is rare.

Clinical

maanifestations

include recurrent fever and rigor, headache, myalgia, and nausea; hemolytic anemia and splenomegaly are common.

Treatment with antimalarial drugs is based on the species (if known) and drug resistance patterns in the area in which infection was acquired

Artemisinin

-based combination therapy (

eg

,

artemether

/lumefantrine) is the most rapidly active therapy and is available worldwide

Evaluation

What

is the disease status of a patient with Malaria?

What is the pathophysiology of malaria?

What is the diagnosis of malaria?

What parameters can be used to monitor malaria therapy

References

Wells BG,

DiPiro

J,

Schwinghammer

T (2013), Pharmacotherapy Handbook (6th Ed). New York, NY: McGraw-Hill.

DiPiro

JT, Talbert RL, Yee GC, Matzke GR, Wells BG, Posey ML, (2008): Pharmacotherapy: A Pathophysiologic Approach (7th

ed

): New York, NY: McGraw-Hill.

Katz M D., Matthias KR., Chisholm-Burns M A., Pharmacotherapy(2011) Principles & Practice Study Guide: A Case-Based Care Plan Approach: New York, NY: McGraw-Hill.

Schwinghammer

TL, Koehler JM (2009) Pharmacotherapy Casebook: A Patient-Focused Approach (7th

ed

): New York, NY: McGraw-Hill.

PST 06106

Basic Pharmacotherapy

Session 4: Pharmacotherapy of HIV/AIDS

Learning Objective

By the end of this session students are expected to be able to:

Define HIV/AIDS

Explain pathophysiology of HIV/AIDS

Explain the clinical presentation of HIV/AIDS

Outline diagnosis of HIV/AIDS

Describe pharmacological treatment of HIV/AIDS

Describe the monitoring of HIV/AIDS Therapy

Activity: Buzzing

What is HIV/AIDS?

INTRODUCTION

AIDs is a set of symptoms (or syndrome) caused by Human Immunodeficiency Virus (HIV). The clinical features may be due to HIV per se or as a result of immune system destruction.

It has the following features:

Fever, diarrhoea, weight loss, skin rashes, sores, generalized

pruritis

, altered mental status, persistent severe headache, oral thrush or Kaposi’s sarcoma may be found in patients with advanced disease

Most patients, however, present with symptoms due to opportunistic infections such as tuberculosis, candidiasis and pyogenic infections

Human immunodeficiency virus

Pathophysiology of HIV/AIDS

The virus through its envelope proteins attaches to the CD4 receptor and co-receptors found on the surface of T lymphocytes and macrophage to gain entry to the host cells.

Following entry of the HIV into a susceptible host cell using the enzyme reverse transcriptase, the viral genome copies itself from RNA to DNA genetic material.

The viral DNA copy enters the nucleus of the host cell and becomes intimately incorporated into the host cell’s own DNA using the enzyme integrase.

Pathophysiology of

HIV/AIDS CONT…

The virus thus becomes a permanent part of an infected person’s nuclear proteins.

There follows a latent period during which the provirus in the infected nucleus waits for an external stimulus to start reproducing.

CD4+ T lymphocytes, when stimulated by new HIV, other infections and infestations which would normally result in the CD4+ T lymphocyte reproducing itself, now responds to these stimuli by manufacturing HIV.

As more and more viruses are produced and leave the host cell, the cell membrane weakens leading eventually to the death of the infected CD4+ T lymphocytes

37

Pathophysiology of

HIV/AIDS CONT

The

multiple steps in replication of HIV provide multiple opportunities for intervention.

Therapeutic regimens may be directed at one or several of the following stages essential for viral replication:

Attachment of HIV to the host cell;

Reverse transcription of viral RNA to DNA;

Integration of the pro-viral DNA into the host cells’ DNA; or

Expression of the viral gene after it has been integrated into host cell DNA, including the transcription of more viral RNA and the translation of viral proteins

.

Clinical Presentation Of HIV/AIDS

In the absence of ART, disease progression goes through the following clinical

stages

Primary Infection or becoming HIV Infected

Most primary infection, i.e. new infection with HIV, usually is not immediately noticed.

It presents with short illnesses and flu-like symptoms such as fever, malaise, enlarged lymph nodes, sore throat, skin rash, and/or joint pain soon after being infected.

It may last for a few weeks.

This acute febrile illness is accompanied by widespread dissemination of the virus to different tissues, especially the lymphoid system. This is called

sero

-conversion illness.

Clinical Presentation Of HIV/AIDS

Cont

….

Clinically

Asymptomatic Stage

This stage is free of symptoms, except for the possibility of swollen glands: persistent generalized lymphadenopathy – Persistent Generalized Lymphadenopathy (PGL).

However, this is the stage where there is ongoing extensive immunologic fighting/changes and rapid viral replication begins.

This may last for an average of eight to ten years.

However, disease progression in children and elderly is faster due to high set point.

This is WHO Stage1

Clinical Presentation Of HIV/AIDS

Cont

Symptomatic HIV

Over time, the immune system loses the struggle to contain HIV, resulting in extensive destruction of CD4 cells

This is characterised by the occurrence of opportunistic infections (OIs), which is when) symptoms develop

The most common symptoms include fever, respiratory infections, cough, TB tuberculosis, weight loss, skin diseases, viral infections, oral thrush, pain, and lymphadenopathy

This is WHO Stage 2 or 3, depending on the particular OI

seen

Clinical Presentation Of HIV/AIDS

Cont

Acquired Immune Deficiency Syndrome (AIDS)

AIDS is defined as a point when a person with HIV develops severe immunosuppression, OIs, or malignancies/cancers.

Such conditions are: severe weight loss, Kaposi’s sarcoma, Cryptococcus meningitis, PCP, toxoplasmosis, CMV (Cytomegalovirus) retinitis, etc.

This is WHO Stage 4

Diagnosis of HIV/AIDS

ELISA Test

— ELISA, which stands for enzyme-linked immunosorbent assay, is used to detect HIV infection (detects antibodies against HIV-1)and is both highly sensitive and specific

If an

ELISA test is positive, the Western blot test is usually administered to confirm the diagnosis. If an ELISA test is negative, but you think you may have HIV, you should be tested again in one to three months

ELISA is quite sensitive in chronic HIV infection, but because antibodies aren't produced immediately upon infection, you may test negative during a window of a few weeks to a few months after being infected.

Viral Load Test

— This test measures the amount of HIV in your blood. It quantifies viremia by measuring the amount of viral RNA. Generally, it's used to monitor treatment progress or detect early HIV infection. Three technologies measure HIV viral load in the blood: reverse transcription polymerase chain reaction (RT-PCR), branched DNA (

bDNA

) and nucleic acid sequence-based amplification assay (NASBA). The basic principles of these tests are similar. HIV is detected using DNA sequences that bind specifically to those in the virus

Western Blot

— This is a very sensitive blood test used to confirm a positive ELISA test result

Activity: Small Group Discussion

•What explanations can you give on monitoring therapy for HIV/AIDS?

Pharmacological treatment of HIV/AIDS

Early initiation of combination treatment (ART) is associated with health benefits in terms of reduced morbidity and mor­tality in all age groups.

In addition, ART is effective for pre­venting HIV transmission.

It also helps to drastically reduce TB incidences.

Therefore, all patients diagnosed with HIV should be initiated ART regardless of CD4 cell count and clinical stage

The most effective means to accomplish durable suppression of HIV replication is the simultaneous initiation of combinations of effective anti HIV drugs with which the patient has not been previously treated and that are not cross resistant with antiretroviral agents with which the patient has been treated previously

Each of the antiretroviral drugs used in combination therapy regimens should always be used according to optimum schedules and dosages

Antiretroviral Agents

The

recommended antiretroviral drugs to be used fall into the following main categories:

Nucleotide reverse transcriptase inhibitors (NRTIs)

Nucleoside reverse transcriptase inhibitors (NRTIs)

Non-nucleoside reverse transcriptase inhibitors (NNRTIs)

Protease inhibitors (

Pls

)

Integrase strand transfer inhibitors (INSTI)/ Integrase inhibitors

Fusion inhibitors

Chemokine receptor inhibitors/CCR5 inhibitors

First Line ART

Triple therapy consisting of 2 NRTI + 1 NNRTI

Pharmacological treatment of

HIV/AIDS Cont..

NOTE:

Clients on TDF/3TC/EFV600 can be switched to TDF/3TC/ EFV400 (when available) to reduce CNS related toxicity with exception of Pregnant women and TB-HIV Co-infected pa­tients

TDF 300mg based regimens should not be initiated on patients with weight less than 35kg.

EFV400 based regimens should not be initiated on patients with weight below 20Kg

Pharmacological treatment of HIV/AIDS Cont..

Second-line Antiretroviral Therapy in Adults and Adolescents

Treatment failure will be based on

virological

criteria of more than 1000copies /ml after two successive tests, at least three months apart with assurance of good adherence, in areas where there is access to routine viral load monitoring.

Drugs used as the second line in Tanzania include

Pharmacological treatment of

HIV/AIDS Cont..

NRTIs/

NtRIs

Zidovudine (AZT)

Tenofovir

(TDF)

Abacavir

(ABC)

Lamivudine (3TC)

Emtricitabine

(FTC)

PIs

Atazanavir

boosted by Ritonavir (ATV/r)

Lopinavir

boosted by Ritonavir (LPV/r)

INSTIs

Dolutegravir

(DTG

)

Pharmacological treatment of HIV/AIDS Cont..

The second line NRTI choice for adults and adolescents de­pends on the first line regimen

For patients on TDF based regimens in first line, the preferred second line option is AZT plus 3TC combined with a ritonavir-boosted PI, preferably ATV/r because it is dosed once daily and has fewer metabolic complications and side

effects

Pharmacological treatment of HIV/AIDS Cont..

Third-Line Art Treatment

Patients failing 2nd line regimens may have extensive NRTI and NNRTIs associated resistance mutations (RAMS) which preclude/minimise their use in third-line regimens.

Therefore, 3rd line regimens, in order to have at least two or preferably three effective drugs, need to be constructed using other new classes of drugs or second generation formulations of previous drugs

These second generation drugs usually have a higher genetic barrier to resistance and their efficacy is not compromised by RAMs associated with the first generation formulations. Therefore, the following are used:

Pharmacological treatment of HIV/AIDS Cont..

Integrase Inhibitors:

Dolutegravir

50mg (DTG) and

Raltegravir

400mg (RAL),

Second generation PIs:

Darunavir

800mg /Ritonavir 100mg (DRV/r)

Second generation NNRTI:

Etravirine

200g (ETV

Monitoring Of Antiretroviral Therapy

Tests for Monitoring responses to Antiretroviral treatment and diagnosis of treatment failure/toxicity are important

Clinical assessment and laboratory tests play a key role in assessing individuals before ART is initiated, monitoring treatment response and possible toxicity of ARV drugs.

The following laboratory tests are recommended:

HIV Viral Load test is a preferred monitoring approach to diagnose and confirm early treatment failure.

HVL for adults and adolescents should be done 6 months after initiation of ART

Successful antiretroviral therapy result in decrease of HIV viral load, immune recovery and therefore increase in number of CD4 cells

.

Monitoring Of Antiretroviral Therapy

Cont

CD4 T lymphocytes count should also be done at base­line for all clients.

CD4 cells progressively decrease as HIV advances and immune status deteriorates. Measurements of CD4 cells counts are important immunological markers of the disease progression.

CD4 cells counts are reported in percentage (%).

CD4 testing will be measured as a baseline test and for suspected treatment failure for those clients on ART

Monitoring of cd4 count

Monitoring Of Antiretroviral Therapy

Cont

A complete blood count (If not available, conduct hemo­globin test for patients on AZT based regimens)

Urinalysis to exclude proteinuria (HIV associated ne­phropathy or HIVAN) and glycosuria (Diabetes Mellitus).

Tests to rule out active TB (sputum AFB,

GeneXpert

, CXR) in cases where there is suspected TB from the screening tool

Urine pregnancy test (to women of reproductive age) in order to identify PLHIV requiring EFV 600mg.

Liver function tests (serum alanine aminotransferase, ALT) if on anti-TB drugs or requiring NVP based treat­ment

Renal function tests (serum creatinine, blood urea nitro­gen (BUN)) for patients requiring TDF based regimens

Lipids test (for clients requiring PIs)

Key Points

HIV/AIDs

is a set of symptoms (or syndrome) caused by Human Immunodeficiency Virus (HIV)

HIV is commonly transmitted via unprotected sexual activity,

blood

transfusions, hypodermic needles, and from mother to child.

Upon acquisition of the virus, the virus replicates inside and kills T helper cells, which are required for almost all adaptive immune responses.

Diagnosis of HIV/AIDS is commonly done by ELISA, Viral load and Western blot tests

Treatment of HIV/AIDS is initiated

regarless

of CD4 count

Varieties of tests are done in order to monitor ART therapy

Evaluation

What

is the disease status of a patient with HIV/AIDS?

What is the pathophysiology of HIV/AIDS?

What is the diagnosis of HIV/AIDS?

What are the first line treatment regimes for HIV/AIDS?

What laboratory tests are used to monitor ART?

References

Wells

BG,

DiPiro

J,

Schwinghammer

T (2013),

Pharmacotherapy Handbook

(6

th

Ed). New York, NY: McGraw-Hill.

DiPiro

JT, Talbert RL, Yee GC, Matzke GR, Wells BG, Posey ML, (2008):

Pharmacotherapy: A Pathophysiologic Approach

(7

th

ed

): New York, NY: McGraw-Hill.

Katz M D., Matthias KR., Chisholm-Burns M A., Pharmacotherapy(2011)

Principles & Practice Study Guide: A Case-Based Care Plan Approach

: New York, NY: McGraw-Hill.

Schwinghammer

TL, Koehler JM (2009)

Pharmacotherapy Casebook: A Patient-Focused Approach

(7

th

ed

): New York, NY: McGraw-Hill.

BASIC PHARMACOTHERAPY

Pharmacotherapy of Tuberculosis

Complete learning session

1 / 20

Basic Pharmacotherapy

Learning outcomes

• Define Pharmacotherapy of Tuberculosis.
• Explain its main principles and classifications.
• Apply the concept safely in pharmaceutical practice.
• Recognise common errors and appropriate corrective action.

2 / 20

Basic Pharmacotherapy

Why this topic matters

• Tuberculosis is caused by organisms in the Mycobacterium tuberculosis complex.
• Combination therapy reduces treatment failure and selection of resistance.
• Correct understanding supports safe, effective and accountable practice.

3 / 20

Basic Pharmacotherapy

Core definition

• Pharmacotherapy of Tuberculosis is studied as a structured concept within Basic Pharmacotherapy.
• Tuberculosis is caused by organisms in the Mycobacterium tuberculosis complex.
• Use precise terms before attempting application or calculation.

4 / 20

Basic Pharmacotherapy

Foundational principles

• Combination therapy reduces treatment failure and selection of resistance.
• Adherence support is essential because treatment continues for months.
• Each principle should be linked to a practical decision.

5 / 20

Basic Pharmacotherapy

Key components

• Tuberculosis is caused by organisms in the Mycobacterium tuberculosis complex.
• Adherence support is essential because treatment continues for months.
• Drug interactions and adverse effects require active monitoring.

6 / 20

Basic Pharmacotherapy

Classification and organisation

• Group the subject by function, structure, source, risk or stage as appropriate.
• Use one classification system consistently.
• State the feature that separates one category from another.

7 / 20

Basic Pharmacotherapy

How the process works

• Combination therapy reduces treatment failure and selection of resistance.
• Adherence support is essential because treatment continues for months.
• Follow the sequence from input or cause to outcome.

8 / 20

Basic Pharmacotherapy

Professional terminology

• Distinguish related terms that are often confused.
• Use names, units and abbreviations consistently.
• Define technical words before using them in explanations.

9 / 20

Basic Pharmacotherapy

Practical application

• Drug interactions and adverse effects require active monitoring.
• Prepare the required materials, information or records before starting.
• Complete each step in order and document important observations.

10 / 20

Basic Pharmacotherapy

Quality requirements

• Persistent severe symptoms or treatment complications require clinical review.
• Check identity, accuracy, completeness and fitness for purpose.
• Record deviations and take corrective action promptly.

11 / 20

Basic Pharmacotherapy

Safety and risk control

• Identify hazards before beginning the task.
• Use appropriate protective, ethical and legal safeguards.
• Stop and refer when the situation exceeds competence or available resources.

12 / 20

Basic Pharmacotherapy

Common errors

• Using an incorrect definition, unit, category or sequence.
• Skipping verification, documentation or a final reasonableness check.
• Applying a general rule without considering the patient, material or research context.

13 / 20

Basic Pharmacotherapy

Preventing avoidable mistakes

• Use a written procedure or checklist.
• Independently verify high-risk calculations and decisions.
• Communicate unclear or abnormal findings before proceeding.

14 / 20

Basic Pharmacotherapy

Worked application

• Start with a clearly stated problem related to Pharmacotherapy of Tuberculosis.
• Select the correct principle from the earlier slides.
• Show the decision or calculation step by step.
• Confirm that the final answer is reasonable and professionally usable.

15 / 20

Basic Pharmacotherapy

Practice scenario

• A routine situation requires the learner to apply Pharmacotherapy of Tuberculosis.
• Identify the information that must be collected first.
• Explain the safest action and the record that should be completed.

16 / 20

Basic Pharmacotherapy

Decision points

• What finding confirms that the chosen approach is suitable?
• What warning sign requires correction, referral or further investigation?
• What evidence must be documented to support the decision?

17 / 20

Basic Pharmacotherapy

Connection to patient care

• Accurate practice reduces preventable harm.
• Clear communication helps patients and colleagues use information correctly.
• Monitoring outcomes shows whether the intended benefit was achieved.

18 / 20

Basic Pharmacotherapy

Session summary

• Tuberculosis is caused by organisms in the Mycobacterium tuberculosis complex.
• Combination therapy reduces treatment failure and selection of resistance.
• Adherence support is essential because treatment continues for months.
• Drug interactions and adverse effects require active monitoring.
• Persistent severe symptoms or treatment complications require clinical review.

19 / 20

Basic Pharmacotherapy

Self-check questions

• Define Pharmacotherapy of Tuberculosis in your own words.
• List three important principles or components.
• Describe one practical application and one common error.
• Explain one quality or safety control.

20 / 20

PST 06106

Basic Pharmacotherapy

Session 6: Pharmacotherapy of Leprosy

11/11/2020

Pharmacotherapy of Leprosy

Learning Task

By the end of this session students are expected to be able to:

Define leprosy

Explain pathophysiology of leprosy

Explain the clinical presentation of leprosy

Outline diagnosis of leprosy

Describe pharmacological treatment of leprosy

Describe monitoring of leprosy therapy

11/11/2020

Pharmacotherapy of Leprosy

Activity: Small Group Discussion

What

is the first line treatment of Pneumonia?

Definition of Leprosy

Leprosy is a chronic infectious disease caused by

Mycobacterium

leprae

(M.

leprae

).

It mainly affects the

skin, peripheral nerves, and mucous membranes.

It is a disease mainly of human beings, which affects

people of all races, all ages, and both sexes.

Similar to TB, leprosy bacilli are mainly transmitted through

infectious droplets that are spread by an infectious individual through coughing and sneezing.

11/11/2020

Pharmacotherapy of Leprosy

Definition

of Leprosy

Cont.…

Patients

carrying many leprosy bacilli are called multibacillary (MB) patients. They are the main source of infection.

People may carry the bacilli but not develop the disease.

These people, called healthy carriers, are also probably able to transmit the bacilli to others.

Individuals with few bacilli in their body are called paucibacillary (PB).

Like healthy carriers, they are not a significant source of infection

11/11/2020

Pharmacotherapy of Leprosy

Pathophysiology of Leprosy

Onset of leprosy is insidious.

The disease affects nerves, skin and eyes.

It may also affect mucosa (mouth, nose, pharynx), testes, kidney, voluntary/smooth muscles,

reticulo

-endothelial system, and vascular endothelium.

Bacilli enter the body usually through respiratory system.

It has low

pathogenicity,

only a small proportion of infected people develop signs of the disease.

Though infected, majority of the population do not develop the disease.

11/11/2020

Pharmacotherapy of Leprosy

Pathophysiology of

Leprosy Cont.…..

After entering the body, bacilli migrate towards the neural tissue and enter the Schwann cells. Bacteria can also be found in, macrophages, muscle cells and endothelial cells of blood vessels. After entering the Schwann cells /macrophage; fate of the bacterium depends on the resistance of the infected individual towards the infecting organism.

Bacilli start multiplying slowly (about 12-14 days for one bacterium to divide into two) within the cells, get liberated from the destroyed cells and enter other unaffected cells.

Till this stage person remains free from signs and symptoms of leprosy

.

11/11/2020

Pharmacotherapy of Leprosy

Pathophysiology of

Leprosy Cont

.…..

As the bacilli multiply, bacterial load increases in the body and infection is recognized by the immunological system.

Lymphocytes and

histiocytes

(macrophages) invade the infected tissue.

At this stage clinical manifestation may appear as involvement of nerves with impairment of sensation &/ or skin patch.

If it is not diagnosed and treated in the early stages, further progress of the diseases is determined by the strength of the patient’s immune response

11/11/2020

Pharmacotherapy of Leprosy

Pathophysiology of Leprosy Cont.…..

Specific and effective cell mediated immunity (CMI) provides protection to a person against leprosy.

When specific CMI is effective in eliminating/ controlling the infection in the body, lesions heal spontaneously or it produces

pauci

-bacillary (PB) type of leprosy.

If CMI is deficient; the disease spreads uncontrolled and produces multi bacillary (MB) leprosy with multiple system involvement.

Some times, the immune response is abruptly altered, either following multiple drug treatment (MDT) or due to improvement of immunological status, which results in – 12 – the inflammation of skin or / and nerves and even others tissue, called as leprosy reaction

11/11/2020

Pharmacotherapy of Leprosy

Clinical presentation and Diagnosis of Leprosy

The diagnosis of leprosy

The diagnosis of leprosy relies on both passive and active case-finding.

Clinical diagnosis.

This is achieved through observation of signs or symptoms of leprosy which includes;

One or more pale or reddish, hypo-pigmented patch(

es

) on the skin with diminished or loss of sensation.

Painless swelling or lumps in the face and/or earlobes.

Enlarged and/or tender nerves.

11/11/2020

Pharmacotherapy of Leprosy

Clinical presentation

Cont.….

Burning sensation of the skin.

Numbness or tingling of hands and/or feet.

Weakness of eyelids, hands, and/or feet.

Painless wounds or burns on the hands and/or feet.

11/11/2020

Pharmacotherapy of Leprosy

Clinical presentation and Diagnosis of

Leprosy Cont.…

Examination of other organs

:

Leprosy can affect a few organs other than skin and peripheral nerves.

Depending on the duration of the disease and the spread of leprosy through the body, various other organs may show signs typical for leprosy

11/11/2020

Pharmacotherapy of Leprosy

Activity: Small Group Discussion

What

is the first line treatment of Leprosy??

Pharmacological Treatment Of Leprosy

Treatment regimens

The drugs and dosages for PB and MB for both adults and children are shown below

:

Adults (MB)

Monthly treatment: Day 1

Rifampicin 600 mg (2 x 300 mg)

Clofazimine

300 mg (3 x 100 mg)

Dapsone

100

mg

11/11/2020

Pharmacotherapy of Leprosy

Pharmacological Treatment Of

Leprosy Cont.….

Daily treatment: Days 2–28

Clofazimine

50 mg

Dapsone

100 mg

Duration of treatment

12 blister packs to be taken within a period of 12-18 months

11/11/2020

Pharmacotherapy of Leprosy

Pharmacological Treatment Of

Leprosy

Cont

Children 10-14 years (MB)

Monthly treatment: Day 1

Rifampicin 450 mg (3 x 150 mg)

Clofazimine

150 mg (3 x 50 mg)

Dapsone

50 mg

Daily treatment: Days 2–28

Clofazimine

50 mg every other day

Dapsone

50 mg daily

Duration of treatment

12 blister packs to be taken within a period of 12-18 months

11/11/2020

Pharmacotherapy of Leprosy

Pharmacological Treatment Of Leprosy

Cont

Adults (PB)

Monthly treatment: Day 1

Rifampicin 600 mg (2 x 300 mg)

Dapsone

100 mg

Daily treatment: Days 2–28

Dapsone

100 mg

Duration of treatment

Six blister packs

to be taken within a period of 6–9 months.

11/11/2020

Pharmacotherapy of Leprosy

Pharmacological Treatment Of Leprosy

Cont

Children 10-14 years (PB)

Monthly treatment: Day 1

Rifampicin 450 mg (3 x 150 mg)

Dapsone

50 mg

Daily Treatment: Days 2–28

Dapsone

50 mg

Duration of treatment

Six blister packs to be taken within a period of 6–9 months.

Note:

Adjust the dose appropriately for a child (PB) younger than 10 years. For example,

dapsone

25 mg daily and rifampicin 300 mg given once a month under supervision.

11/11/2020

Pharmacotherapy of Leprosy

11/11/2020

Pharmacotherapy of Leprosy

Monitoring of Leprosy Therapy

Treatment monitoring

Multi Drug Therapy

(MDT)

should be provided to the patient as close to the patient’s home as possible

Based

on

the geographic distribution of health facilities, the availability of trained staff, and the patient’s wish, the health worker and/or

District Tuberculosis and Leprosy Coordinator(DTLC)

decides where

Multi Drug Therapy

should be delivered. In principle, every health facility should be able to provide MDT

Staff need to be trained on leprosy management as described in the

National Tuberculosis and Leprosy Programme(NTLP)

training

manual for

health workers

11/11/2020

Pharmacotherapy of Leprosy

Monitoring of Leprosy

Therapy Cont.…

Patients should have access to treatment on any day immediately after finishing the blister pack, but they should be given an appointment to attend a fixed clinic day in order to be reviewed and assessed by a trained health worker or DTLC

The trained health worker or DTLC should arrange leprosy clinics every three months

The DTLC, in collaboration with the district pharmacist, is responsible for the supply of MDT drugs and drugs for treating reactions

11/11/2020

Pharmacotherapy of Leprosy

Monitoring of Leprosy Therapy Cont.…

There should always be a minimum of three blister packs in stock for every patient attending the clinic at any given time

Under normal circumstances patients should not be given more than a one-month drug supply (one blister pack)

Those patients who cannot come on monthly basis to a health facility due to problems such as long distance, impassable roads during the rainy season, nomadic lifestyle, etc., may be given drugs for more than one month, sufficient to cover the expected period of absence

Under exceptional circumstances, a full course supply can be

given

11/11/2020

Pharmacotherapy of Leprosy

Monitoring of Leprosy Therapy Cont.…

When patients are given more than a one-month supply, it is better to involve a formal or informal community leader or relative who will then be oriented to support the patient to complete the full course of treatment (accompanied MDT

Each

time a patient comes to a health facility to collect an MDT blister pack, a health worker should ask the patient about new complaints regarding nerve function impairment.

If there are any complaints, the health worker should conduct nerve function tests to assess for

damage

11/11/2020

Pharmacotherapy of Leprosy

Monitoring of Leprosy Therapy Cont.…

If there are indications of nerve damage, the patient should be managed appropriately

In case of uncertainty, the health worker should refer the patient to the DTLC

The health staff is also responsible for tracing a patient who does not attend for two consecutive months

When the patient is found, she/he should be persuaded to continue with treatment

11/11/2020

Pharmacotherapy of Leprosy

Key Points

Leprosy

is caused by a slow-growing type of bacteria called Mycobacterium

leprae

(M.

leprae

)

The disease mainly affects the skin, the peripheral nerves, mucosal surfaces of the upper respiratory tract and the eyes.

The main symptom of leprosy is disfiguring skin sores, lumps, or bumps that do not go away after several weeks or months. The skin sores are pale-colored.

The disease was transmitted by contact between cases of leprosy and healthy persons.

Leprosy is curable with a combination of drugs known as multidrug therapy (MDT)

11/11/2020

Pharmacotherapy of Leprosy

Evaluation

What

is Leprosy?

What are the signs and symptoms of Leprosy?

What is the pathophysiology of Leprosy?

What is the treatment of leprosy?

11/11/2020

Pharmacotherapy of Leprosy

References

Wells

BG,

DiPiro

J,

Schwinghammer

T (2013),

Pharmacotherapy Handbook

(6

th

Ed). New York, NY: McGraw-Hill.

DiPiro

JT, Talbert RL, Yee GC, Matzke GR, Wells BG, Posey ML, (2008):

Pharmacotherapy: A Pathophysiologic Approach

(7

th

ed

): New York, NY: McGraw-Hill.

Katz

M D.,

Matthias KR.,

Chisholm-Burns M A.,

Pharmacotherapy(2011)

Principles & Practice Study Guide: A Case-Based Care Plan Approach

:

New York, NY:

McGraw-Hill.

Schwinghammer

TL, Koehler JM (2009)

Pharmacotherapy Casebook: A Patient-Focused Approach

(7

th

ed

): New York, NY: McGraw-Hill

.

11/11/2020

Pharmacotherapy of Leprosy

End

11/11/2020

Pharmacotherapy of Leprosy

PST 06106

Basic Pharmacotherapy

Session 7: Pharmacotherapy of Pharyngitis, Sinusitis, and Otitis Media

Learning objectives

By the end of this session students are expected to be able to:

Define pharyngitis, sinusitis, and otitis media

Explain pathophysiology of pharyngitis, sinusitis, and otitis media

Explain the clinical presentation of pharyngitis, sinusitis, and otitis media

Outline diagnosis of pharyngitis, sinusitis, and otitis media

Describe pharmacological treatment of pharyngitis, sinusitis, and otitis media

Describe monitoring of pharyngitis, sinusitis, and otitis media therapy

Activity: Buzzing

What

is pharyngitis??

Definition of Pharyngitis, Sinusitis, and Otitis Media

Pharyngitis

is an acute infection of the oropharynx or nasopharynx.

It is caused by virus and bacteria

Viruses cause the majority of acute pharyngitis cases

Specific etiologies include rhinovirus, coronavirus, adenovirus, herpes simplex virus, influenza virus, parainfluenza virus, and Epstein-Barr virus

Group A

β

–hemolytic streptococci (GAS; also known as

S.

pyogenes

),

is the

primary

bacterial

cause.

Other, less-common causes of acute pharyngitis are groups C and G

Streptococcus, Corynebacterium

diphtheriae

, Neisseria gonorrhoeae, Mycoplasma pneumoniae,

Arcanobacterium

haemolyticum

, Yersinia

enterocolitica

, and Chlamydia pneumonia

Pathophysiology Of Pharyngitis

The mechanism by which

Group A beta haemolytic streptococci (GAS)

causes pharyngitis is not well defined

Asymptomatic pharyngeal carriers of the organism may have an alteration in host immunity (e.g., a breach in the pharyngeal mucosa) and the bacteria of the oropharynx, allowing colonization to become an infection

Pathogenic factors associated with the organism itself may also play a role

These include pyrogenic toxins,

hemolysins

, streptokinase, and

proteinase.

Clinical presentation and Diagnosis of Pharyngitis

General

A sore throat of sudden onset that is mostly self-limited

Fever and constitutional symptoms resolving in about 3 to 5 days

Clinical signs and symptoms are similar for viral causes and

nonstreptococcal

bacterial

causes

Clinical presentation and Diagnosis of

Pharyngitis

Cont

Signs and Symptoms

Sore throat ( pain or irritation in the throat that occurs with/without swallowing)

Pain on swallowing

Fever

Headache, nausea, vomiting, and abdominal pain (especially children)

Erythema/inflammation of the tonsils and pharynx with or without patchy exudates

Enlarged, tender lymph nodes

Red swollen uvula,

petechiae

on the soft palate, and a

scarlatiniform

rash

Several symptoms that are not suggestive of group A streptococci are cough, conjunctivitis,

coryza

, and diarrhea

Clinical presentation and Diagnosis of Pharyngitis

Cont

Signs Suggestive of Viral Origin for Pharyngitis

Conjunctivitis

Coryza (irritation and swelling of the mucous membrane in the nose)

Cough

Diarrhea

Laboratory Tests

Throat swab and culture

Rapid antigen detection testing (RADT)

Activity: Small Group Discussion

What

is the first line treatment of

Pharyngitis ?

Pharmacological treatment of Pharyngitis

The goals of treatment for pharyngitis are to;

Improve clinical signs and symptoms,

M

inimize

adverse drug reactions,

Prevent

transmission to close contacts, and

P

revent

acute rheumatic fever and suppurative complications, such as

peritonsillar

abscess, cervical lymphadenitis, and

mastoiditis

Pharmacological treatment of Pharyngitis

For recurrent

pharyngitis

Monitoring of Pharyngitis Therapy

Most pharyngitis cases are self-limited; however, antibiotics hasten resolution when given early for proven cases of

Group A beta hemolytic streptococci (GAS) pharyngitis

.

Generally, fever and other symptoms resolve within 3 or 4 days of onset without antibiotics; however, symptoms will improve 16 hours to 2 days earlier with antibiotic therapy.

Follow-up testing is generally not necessary for index cases or in asymptomatic contacts of the index patient.

However, for patients who remain symptomatic or when symptoms recur despite completion of treatment, posttreatment throat cultures 2 to 7 days after completion of antibiotics should be done

.

Key Points

Acute

pharyngitis is characterized by the rapid onset of sore throat and pharyngeal inflammation (with or without exudate). .

It can be caused by a variety of viral and bacterial pathogens, including group A Streptococcus (GAS),

Diagnosis can be done clinically especially and by using lab test

Most of the time the condition is self limiting, but antibiotics may be needed

Evaluation

What

is pharyngitis?

What are the signs and symptoms of pharyngitis?

How is pharyngitis diagnosed?

How is the treatment of pharyngitis

REFER Students to Handout 7.1: Pharmacotherapy of

Sinusitis

REFER Students to Handout 7.2: Pharmacotherapy of Otitis Media

References

Wells

BG,

DiPiro

J,

Schwinghammer

T (2013),

Pharmacotherapy Handbook

(6

th

Ed). New York, NY: McGraw-Hill.

DiPiro

JT, Talbert RL, Yee GC, Matzke GR, Wells BG, Posey ML, (2008):

Pharmacotherapy: A Pathophysiologic Approach

(7

th

ed

): New York, NY: McGraw-Hill.

Katz M D., Matthias KR., Chisholm-Burns M A., Pharmacotherapy(2011)

Principles & Practice Study Guide: A Case-Based Care Plan Approach

: New York, NY: McGraw-Hill.

Schwinghammer

TL, Koehler JM (2009)

Pharmacotherapy Casebook: A Patient-Focused Approach

(7

th

ed

): New York, NY: McGraw-Hill.

PST 06106

Basic Pharmacotherapy

Session 8: Pharmacotherapy of Pneumonia

Learning objectives

By the end of this session students are expected to be able to:

Define pneumonia

Explain pathophysiology of pneumonia

Explain the clinical presentation of bronchitis and pneumonia

Outline diagnosis of bronchitis and pneumonia

Describe pharmacological treatment of bronchitis and pneumonia

Describe monitoring of bronchitis and pneumonia therapy

Activity: Buzzing

What

is Pneumonia?

Definition of Pneumonia

Pneumonia

Pneumonia is the inflammation of the lung tissue.

Pneumonia can either be primary (to the causing organism) or secondary to pathological damage in the respiratory system

It occurs in persons of all ages, although the clinical manifestations are most severe in the very young, the elderly, and the chronically ill

.

The most prominent pathogen causing community-acquired pneumonia (CAP) in otherwise healthy adults is S. pneumonia and accounts for up to 75% of all acute cases.

Other common pathogens include M.

pneumoniae

, Legionella species, C.

pneumoniae

, H.

influenzae

, and a variety of viruses including influenza.

Pathophysiology of Pneumonia

Microorganisms gain access to the lower respiratory tract by three routes.

Through inhalation as aerosolized particles, or

via the bloodstream from an

extra pulmonary

site of infection;

Aspiration of oropharyngeal contents which is a common occurrence in both healthy and ill persons during sleep is the major mechanism by which pulmonary pathogens gain access to the normally sterile lower airways and alveoli.

Pathophysiology of Pneumonia CONT…..

When pulmonary defense mechanisms are functioning optimally, aspirated microorganisms are cleared from the region before infection can become established;

However, aspiration of potential pathogens from the oropharynx can result in pneumonia if lung defenses are impaired

Factors that promote aspiration, such as altered sensorium and neuromuscular disease, may result in an increase in the size of the inoculum delivered to the lower respiratory tract, thereby overwhelming local defense mechanisms.

Pathophysiology of Pneumonia CONT…..

Lung

infections with viruses suppress the antibacterial activity of the lung by impairing alveolar macrophage function and mucociliary clearance, thus setting the stage for secondary bacterial pneumonia.

Mucociliary transport is also depressed by ethanol and narcotics and by obstruction of a bronchus by mucus, tumor, or extrinsic compression.

All these factors can severely impair pulmonary clearance of aspirated bacteria hence causing infection in the

lung.

Clinical Presentation And Diagnosis Of Pneumonia

Signs and symptoms

Abrupt onset of fever, chills, dyspnea, and productive cough

Rust-colored sputum or hemoptysis

Pleuritic chest

pain

Clinical Presentation And Diagnosis Of Pneumonia CONT…

Physical examination

Tachypnea and tachycardia

Dullness to percussion

Increased tactile fremitus, whisper

pectoriloquy

, and

egophony

Chest wall retractions and grunting respirations

Diminished breath sounds over affected area

Inspiratory crackles during lung expansion

Clinical Presentation And Diagnosis Of Pneumonia CONT…

Chest radiograph

Dense lobar or segmental infiltrate

Laboratory tests

Leukocytosis with predominance of

polymorphonuclear

cells

Low oxygen saturation on arterial blood gas or pulse oximetry

Sign and symptoms of pneumonia

Activity: Small Group Discussion

What is the first line treatment of Pneumonia?

Pharmacological Treatment Of Pneumonia

Treatment goals of pneumonia includes:

Eradication of the offending organism through selection of the appropriate antibiotic and complete clinical cure

Therapy should minimize associated morbidity, including reversible or irreversible disease and drug-induced organ toxicity (e.g., renal, lung, or hepatic dysfunction).

Most cases of viral pneumonia are self-limiting, although therapy of influenza pneumonia with specific antiviral agents (oseltamivir and

zanamivir

) may hasten recovery

.

Treatment of Pneumonia in Adults

First- line

Treatment of Atypical Community Acquired Pneumonias

Pharmacological Treatment Of Pneumonia In Children

Non-severe pneumonia

A: Amoxicillin 25 mg/kg 8 hourly for 5 days
Plus A: Paracetamol suppositories 10–15mg/kg (if there is fever)

OR B:

Ibuprofen 15mg/kg 12 hourly for 5 days

Give the first dose at the clinic and teach the mother how to give the other doses at home.

And

Encourage breasting and feeding.

Pharmacological Treatment Of Pneumonia In Children

Severe Pneumonia

A: Benzyl Penicillin 50000 units/kg IV or IM every 6 hours for at least 3 days
THEN A: Amoxicillin 40 mg/kg 8 hourly for 7 days.

OR

A:

Ampicillin 50 mg/kg IV/IM every 6 hourly

AND

A: Gentamicin (7.5 mg/kg IV/IM once a day) for 5 days;

then, If child responds well, complete treatment at home or in hospital with

A: Amoxicillin 30 mg/kg 8 hourly for 7 days.

Pharmacological Treatment Of Pneumonia In Children

Cont

…..

Very severe Pneumonia:

A:

Ampicillin 50 mg/kg IV/IM every 6 hours

AND

A

:

Gentamicin (7.5 mg/kg IV/IM once a day) for 5 days; then, If child responds well, complete treatment at home or in hospital with

A

:

Amoxicillin (40 mg/kg12 hourly 10 days

Alternatively,

A:

Ceftriaxone 80 mg/kg IV or IM once daily for 10 days.

Monitoring Of Pneumonia Therapy

After therapy has been instituted, appropriate clinical parameters such as signs and symptoms and other laboratory markers should be monitored to ensure the efficacy and safety of the therapeutic regimen.

For patients with CAP or pneumonia from any source of mild to moderate clinical severity, the time to resolution of cough, decreasing sputum production, and fever, as well as other constitutional symptoms of malaise, nausea, vomiting, and lethargy, should be noted.

Monitoring Of Pneumonia Therapy Cont.….

Initial resolution should be observed within the first 2 days and progression to complete resolution within 5 to 7 days but usually no more than 10 days.

For patients with HAP, substantial underlying diseases, or both, additional parameters can be followed, including the magnitude and character of the peripheral blood WBC count, chest radiograph, and blood gas determinations.

Monitoring Of Pneumonia Therapy cont.

.

Similar to patients with less severe disease, some resolution of symptoms should be observed within 2 days of instituting antibiotic therapy.

If no resolution of symptoms is observed within 2 days of starting seemingly appropriate

antibiotic therapy or if the patient’s clinical status is deteriorating, the appropriateness of initial antibiotic therapy should be critically reassessed.

The patient should be evaluated carefully for deterioration of underlying concurrent disease(s).

Monitoring Of Pneumonia Therapy cont

.….

Additionally, the caregiver should consider the possibility of changing the initial antibiotic therapy to expand antimicrobial coverage not included in the original regimen (e.g.

Mycoplasma, Legionella,

and anaerobes).

Furthermore, the need for antifungal therapy (lipid-based amphotericin B) should be considered.

Some resolution of symptoms should be observed within 2 days of starting proper antibiotic therapy, with complete resolution expected within 10 to 14 days

Key Points

Pneumonia

is an infection of the lung tissue whereby the air sacs in the lungs become infected with microorganisms, fluid and inflammatory cells and hence they lungs fail to work properly.

Diagnosis of pneumonia is based on symptoms and signs of an acute lower respiratory tract infection, and can be confirmed by a chest X-ray showing new shadowing that is not due to any other cause

Penicillins as well as other antibiotics can be used for treatment of Pneumonia as indicated

Evaluation

What

is pneumonia?

What are the signs and symptoms of pneumonia?

How is pneumonia diagnosed?

How is the treatment of pneumonia in adult and children?

Which clinical parameters can be used to monitor pneumonia therapy?

REFER Students to

Handout 8.1:

Classification of Pneumonia and Risk Factors

References

Wells

BG,

DiPiro

J,

Schwinghammer

T (2013),

Pharmacotherapy Handbook

(6

th

Ed). New York, NY: McGraw-Hill.

DiPiro

JT, Talbert RL, Yee GC, Matzke GR, Wells BG, Posey ML, (2008):

Pharmacotherapy: A Pathophysiologic Approach

(7

th

ed

): New York, NY: McGraw-Hill.

Katz M D., Matthias KR., Chisholm-Burns M A., Pharmacotherapy(2011)

Principles & Practice Study Guide: A Case-Based Care Plan Approach

: New York, NY: McGraw-Hill.

Schwinghammer

TL, Koehler JM (2009)

Pharmacotherapy Casebook: A Patient-Focused Approach

(7

th

ed

): New York, NY: McGraw-Hill.

PST 06106

Basic Pharmacotherapy

Session 9: Pharmacotherapy of Bronchitis

12/3/2020

Pharmacotherapy of Leprosy

Learning objectives

By the end of this session, you are expected to be able to:

Define bronchitis

Explain pathophysiology of bronchitis

Explain the clinical presentation of bronchitis

Outline diagnosis of bronchitis

Describe pharmacological treatment of bronchitis

Describe the monitoring of bronchitis

therapy

Activity: Buzzing

•What

is Chronic Bronchitis??

Definition of Bronchitis

Bronchitis is an infection resulting from the inflammation of the lining of the lungs/bronchioles

It is subdivided into two types

Acute

Bronchitis

Chronic Bronchitis

Acute bronchitis

is one of the most common conditions associated with antibiotic misuse.

Respiratory viruses are by far the most common infectious agents associated with acute

bronchitis

Chronic bronchitis

It defined by a chronic productive cough for three months in each of two successive years in a patient in whom other causes of chronic cough have been excluded.

Chronic Bronchitis

It defined by a chronic productive cough for three months in each of two successive years in a patient in whom other causes of chronic cough have been excluded.

Patients may get secondary bacterial infection with development of fever and production of thick smelly sputum.

The disease is a result of several contributing factors; the most prominent include;

cigarette smoking,

exposure to occupational dusts, fumes, and environmental pollution; and

Host factors [e.g., genetic factors and bacterial (and possibly viral) infections

].

Pathophysiology of Chronic Bronchitis

Microorganisms gain access to the lower respiratory tract by three routes.

Through inhalation as aerosolized particles, or

via the bloodstream from an

extra pulmonary

site of infection;

Aspiration of oropharyngeal contents which is a common occurrence in both healthy and ill persons during sleep is the major mechanism by which pulmonary pathogens gain access to the normally sterile lower airways and alveoli.

When pulmonary defense mechanisms are functioning optimally, aspirated microorganisms are cleared from the region before infection can become established;

However, aspiration of potential pathogens from the oropharynx can result in pneumonia if lung defenses are impaired

Pathophysiology of Chronic

Bronchitis Cont..

Factors that promote aspiration, such as altered sensorium and neuromuscular disease, may result in an increase in the size of the inoculum delivered to the lower respiratory tract, thereby overwhelming local defense mechanisms.

Lung infections with viruses suppress the antibacterial activity of the lung by impairing alveolar macrophage function and mucociliary clearance, thus setting the stage for secondary bacterial pneumonia.

Mucociliary transport is also depressed by ethanol and narcotics and by obstruction of a bronchus by mucus, tumor, or extrinsic compression.

All these factors can severely impair pulmonary clearance of aspirated bacteria hence causing infection in the lung

Clinical Presentation And Diagnosis Of Chronic Bronchitis

Signs and symptoms

Excessive sputum expectoration

Cyanosis (advanced disease)

Obesity

Clinical Presentation And Diagnosis Of Chronic

Bronchitis

Cont

….

Physical examination

Chest auscultation usually reveals inspiratory and expiratory rates,

Rhonchi(Sound generated by the movement of air through the respiratory system), and mild wheezing with an expiratory phase that is frequently prolonged;

H

yper resonance

on percussion(Too much air present within the lung) with obliteration of the area of cardiac dullness(dense tissue)

Normal vesicular breathing sounds are diminished

Clubbing of digits (advanced disease)—- enlargement of the tip of the lung and change in angle, present in bronchitis but not in asthma and pneumonia

Clinical Presentation And Diagnosis Of Chronic Bronchitis

Cont

….

Chest radiograph

Increase in anteroposterior diameter of the thoracic cage (observed as a barrel chest

)—rib cage broadened as in the middle of deep breath, person find hard to breath

Depressed diaphragm with limited

mobility

Laboratory tests

Erythrocytosis

(advanced disease

)—-Too many red blood cells to carry oxygen to your organ and tissue.

Pulmonary function tests

Decreased vital capacity

Prolonged expiratory

flow (person’s maximum speed of expiration as measured with a peak flow meter)

Activity: Small Group Discussion

What

is the first line treatment

of

Pneumonia?

Treatment of chronic Bronchitis

The goals of therapy for chronic bronchitis are:

T

o

reduce the severity of chronic symptoms and

T

o

ameliorate acute exacerbations and achieve prolonged infection-free

intervals

Treatment of chronic

Bronchitis

Cont

Non-Pharmacological Treatment

Stop smoking and/or remove from hazardous environment

Prompt treatment of infective exacerbations

Antibiotics as above in case of secondary bacterial infection

Controlled oxygen therapy

Physiotherapy

Treatment of chronic

Bronchitis

Cont

……

Pharmacological Treatment

Inhaler

Salbutamol (PO) 100

μg

two puff 6 hourly

OR

Salbutamol (PO) 4mg 8 hourly

OR

Ipratropium bromide aerosol 20–80mg, 6–8 hourly

Trial of steroids if there is possibility of reversible airways obstructions

Prednisolone (PO) 20mg once daily for 5 days

Treatment of chronic Bronchitis

Cont

……

Pharmacological

Treatment..

Antibiotics

are probably helpful only in acute exacerbations of chronic bronchitis

Common current clinical practice is to promptly use antibiotics empirically in patients who demonstrate a fever or a change in sputum character.

Such therapy should be directed against streptococcal species, Haemophilus species and

Moraxella

catarrhalis

.

Treatment of chronic Bronchitis

Cont

……

Monitoring of Chronic Bronchitis Therapy

After therapy has been instituted, appropriate clinical parameters such as signs and symptoms and other laboratory markers such as lung function tests should be monitored to ensure the efficacy and safety of the therapeutic regimen.

Key Points

Pneumonia

is an infection of the lung tissue whereby the air sacs in the lungs become infected with microorganisms, fluid and inflammatory cells and hence they lungs fail to work properly.

Diagnosis of pneumonia is based on symptoms and signs of an acute lower respiratory tract infection, and can be confirmed by a chest X-ray showing new shadowing that is not due to any other cause

Penicillins as well as other antibiotics can be used for treatment of Pneumonia as indicated

Evaluation

What

is Chronic Bronchitis?

What are the signs and symptoms of Chronic Bronchitis?

How is Chronic Bronchitis diagnosed?

How is the treatment of Chronic Bronchitis?

REFER Students to Handout 9.1: Pharmacotherapy of Acute Bronchitis

References

Wells

BG,

DiPiro

J,

Schwinghammer

T (2013),

Pharmacotherapy Handbook

(6

th

Ed). New York, NY: McGraw-Hill.

DiPiro

JT, Talbert RL, Yee GC, Matzke GR, Wells BG, Posey ML, (2008):

Pharmacotherapy: A Pathophysiologic Approach

(7

th

ed

): New York, NY: McGraw-Hill.

Katz M D.,

Matthias KR.,

Chisholm-Burns M A.,

Pharmacotherapy(2011)

Principles & Practice Study Guide: A Case-Based Care Plan Approach

:

New York, NY: McGraw-Hill.

Schwinghammer

TL, Koehler JM (2009)

Pharmacotherapy Casebook: A Patient-Focused Approach

(7

th

ed

): New York, NY: McGraw-Hill.

PST 06106

Basic Pharmacotherapy

Session 10: Pharmacotherapy of Typhoid Fever

Learning Objectives

By the end of this session students are expected to be able to:

Define typhoid fever

Explain pathophysiology of typhoid fever

Explain the clinical presentation of typhoid fever

Outline diagnosis of typhoid fever

Describe pharmacological treatment of typhoid fever

Describe monitoring of typhoid fever therapy

Activity: Buzzing

• What

is typhoid fever?

Definition of Typhoid Fever

Typhoid Fever

Typhoid fever, also called enteric fever, is caused by a bacterial infection with

Salmonella enterica

subspecies enterica serotype

Typhi

or serotypes

Paratyphi A, B or C

.

Infection is acquired through ingestion of contaminated food and water.

Humans are the only known hosts of

Salmonella Typhi

.

Bacteria are shed in the faeces of an infected person and transmitted from person to person via ingestion of food or water contaminated by these faeces (faecaloral route).

Definition of Typhoid Fever

Cont.….

Large outbreaks of typhoid fever are often associated with contamination of a drinking water.

The organism can survive for several days in fresh water (e.g. ground water, pond-water) and seawater.

Furthermore, the organism can survive for prolonged periods (up to several months) in contaminated foods

Pathophysiology Of Typhoid Fever

Once ingested and successfully beyond host defense mechanisms such as low gastric pH and bile salts, organisms can attach and invade the distal ileum and proximal colon.

Gastroenteritis often is characterized by massive neutrophil infiltration followed by lymphocytes and macrophages.

The serotypes that are responsible for human illness cause intestinal epithelial

cellsto

secrete interleukin 8, a potent neutrophil chemo-tactic factor.

Degranulation and release of toxic substances by neutrophils may contribute to inflammation and result in tissue damage, fluid secretion, or leakage across the intestinal mucosa

Clinical Presentation Of Typhoid Fever

Few clinical features reliably distinguish typhoid fever from other causes of febrile illnesses(temporary increase in average body temperature). Infection in the absence of treatment manifests after an average incubation period of 10-14 days (range 5-21 days) as a multistage febrile illness

.

Acute typhoid fever:

Systemic illness characterised by:

Fever: remittent during the first week, rising in a stepwise fashion and becomes sustained (lasting > 48 hours) after the first week.

Headache

Clinical Presentation Of Typhoid

Fever

Cont

….

Gastrointestinal symptoms including:

Abdominal pain/cramps

Nausea and vomiting (usually not severe), and/or

Constipation or diarrhoea (diarrhoea is more frequent in children and HIV infected adults).

Clinical presentation

cont.

Relative bradycardia

(slower heart rate)

Hepatosplenomegaly (23-65

%).——liver and spleen swell beyond normal size

Leukopenia (16-46

%).—— Low white blood count

Nonspecific symptoms, such as chills, diaphoresis, anorexia, cough, weakness, sore throat,

Dizziness, and muscle pains, are frequent before the onset of fever.

Severe illness and extra-intestinal complications may include;

gastrointestinal bleeding ,

intestinal perforation,

Septic shock or acidosis.

Blood culture is the diagnostic test of choice

Activity

: Small Group Discussion

• What

is the first line treatment of Typhoid Fever??

Pharmacological Treatment Of Typhoid Fever

Monitoring of Typhoid fever Therapy

After therapy has been instituted, appropriate clinical parameters such as signs and symptoms and other laboratory markers should be monitored to ensure the efficacy and safety of the therapeutic regimen

Key

Points

It

is an acute systemic disease resulting from infection by Salmonella

typhi

and

S.paratyphi

,

serovar

group A and B respectively.

Infection is acquired through ingestion of contaminated food and water.

Patients may complain of nausea and vomiting followed by abdominal cramps, headache, fever, and diarrhea

Ciprofloxacin (PO) 500mg 12 hourly for 10 days

OR

Azithromycin (PO) Adult 500mg for 7 days can be used for treatment

Evaluation

What

is typhoid fever?

What is the pathophysiology of typhoid fever?

What are the signs and symptoms of acute typhoid fever?

How is the treatment of typhoid fever?

References

Wells

BG,

DiPiro

J,

Schwinghammer

T (2013),

Pharmacotherapy Handbook

(6

th

Ed). New York, NY: McGraw-Hill.

DiPiro

JT, Talbert RL, Yee GC, Matzke GR, Wells BG, Posey ML, (2008):

Pharmacotherapy: A Pathophysiologic Approach

(7

th

ed

): New York, NY: McGraw-Hill.

Katz M D.,

Matthias KR.,

Chisholm-Burns M A.,

Pharmacotherapy(2011)

Principles & Practice Study Guide: A Case-Based Care Plan Approach

:

New York, NY: McGraw-Hill.

Schwinghammer

TL, Koehler JM (2009)

Pharmacotherapy Casebook: A Patient-Focused Approach

(7

th

ed

): New York, NY: McGraw-Hill.

PST 06106

Basic Pharmacotherapy

Session 11: Pharmacotherapy of

Amoebiasis

Learning Objectives

By the end of this session students are expected to be able to:

Define of amebiasis and

ameobic

liver abscess

Explain pathophysiology of amebiasis and

ameobic

liver abscess

Explain the clinical presentation of amebiasis and

ameobic

liver abscess

Outline diagnosis of amebiasis and

ameobic

liver abscess

Describe pharmacological treatment of amebiasis and

ameobic

liver abscess

Describe the monitoring of amebiasis and

ameobic

liver abscess therapy

Activity: Buzzing

• What

is

Amoebiasis?

Definition of Amebiasis

Amebiasis

Amoebiasis is an infection caused by the protozoa organism

Entamoeba histolytica,

which can cause colitis and other extra-intestinal manifestations.

The infection is primarily acquired through ingestion of contaminated food and water and occasionally can be acquired through oral-anal sexual practices.

Amoebic Liver Abscess

It is the most frequent extra-intestinal manifestation of

Entamoeba histolytica

infection which results from the invasion of the portal venous system from the colon leading to inflammation and subsequently abscess formation particularly involving the right lobe of the liver.

Pathophysiology Of Amoebiasis

E histolytica

invades mucosal cells of colonic epithelium, producing the classic flask-shaped ulcer in the submucosa.

The trophozoite has a

cytolethal

effect on cells through a toxin.

If the trophozoite gets into the portal circulation, it will be carried to the liver, where it produces abscess and

periportal

fibrosis.

Amebic ulcerations can affect the colon, perineum, and genitalia, and abscesses may occur in the lung and brain.

Clinical Presentation Of Amoebiasis

Intestinal disease

Vague abdominal discomfort, malaise to severe abdominal cramps, flatulence,

bloody diarrhea (

heme

-positive in 100% of cases) with mucus

Eosinophilia is usually absent, although moderate leukocytosis is not unusual

Evidence of motile

trophozoites

or cysts on saline wet mount from a stool specimen

Clinical Presentation Of Amoebiasis Cont.…

Amebic liver abscess

High fever, rigors(sudden feeling of cold and shivering) and profuse sweating,

significant leukocytosis with left shift,

elevated alkaline phosphatase, and liver tenderness on palpation

Right-upper-quadrant pain, hepatomegaly, and liver tenderness, with referred

painto

the left or right shoulder

Erosion of liver abscesses may also present as peritonitis(inflammation of the membrane lining the

abnominal

wall and covering the

abnominal

organs).

Positive imaging evidence of liver abscess and Serological evidence of

E.

histolytica

antibodies or antigens.

Activity

: Small Group Discussion

• What

is the

treatments

of

amebiasis?

Pharmacological treatment and diagnosis of Amoebiasis

Monitoring Of Amoebiasis Therapy

Follow up in patients with amebiasis should include;

repeat stool examination, serology, colonoscopy (for colitis), or

Computed tomography (CT) (for liver abscess) between days 5 and 7, at the end of the course of therapy, and a month after the end of therapy.

Most patients with either intestinal amebiasis or colitis will respond in 3 to 5 days with amelioration of symptoms.

Monitoring Of Amoebiasis

Therapy Cont.…

Patients with liver abscesses may take from 7 to 10 days to respond;

Patients not responding during this period may require aspiration of abscesses or exploratory laparotomy.

Serial liver scans have demonstrated healing of liver abscesses over 4 to 8 months after adequate therapy.

Key

Points

Amebiasis

is a parasitic infection of the intestines caused by the protozoan Entamoeba histolytica, or E. histolytica.

Infection

by Entamoeba histolytica occurs by ingestion of mature cysts

infecally

contaminated food, water, or hands

The

symptoms of amebiasis include loose stool, abdominal cramping, and stomach

pain

Treatment for uncomplicated cases of amebiasis generally consists of a course of

metronidazole

or

tinidazole

Evaluation

What

is Amebiasis?

What is the pathophysiology of amebiasis?

What are the signs and symptoms of Amebiasis?

How is the treatment of Amebiasis?

References

Wells

BG,

DiPiro

J,

Schwinghammer

T (2013),

Pharmacotherapy Handbook

(6

th

Ed). New York, NY: McGraw-Hill.

DiPiro

JT, Talbert RL, Yee GC, Matzke GR, Wells BG, Posey ML, (2008):

Pharmacotherapy: A Pathophysiologic Approach

(7

th

ed

): New York, NY: McGraw-Hill.

Katz M D., Matthias KR., Chisholm-Burns M A., Pharmacotherapy(2011)

Principles & Practice Study Guide: A Case-Based Care Plan Approach

: New York, NY: McGraw-Hill.

Schwinghammer

TL, Koehler JM (2009)

Pharmacotherapy Casebook: A Patient-Focused Approach

(7

th

ed

): New York, NY: McGraw-

PST 06106

Basic Pharmacotherapy

Session 12: Pharmacotherapy of Trypanosomiasis

Learning objectives

By the end of this session students are expected to be able to:

Define trypanosomiasis

Explain the clinical presentation of trypanosomiasis

Outline diagnosis of trypanosomiasis

Describe pharmacological treatment of trypanosomiasis

Describe monitoring of trypanosomiasis therapy

Activity: Buzzing

What is Trypanosomiasis?

Definition of Trypanosomiasis

Two distinct forms of the genus

Trypanosoma

occur in humans.

One is associated with African trypanosomiasis (sleeping sickness) and the other with American trypanosomiasis (Chagas disease)

Human African trypanosomiasis, also known as sleeping sickness, is a vector-borne parasitic disease.

The parasites concerned are protozoa belonging to the Trypanosoma genus.

They are transmitted to humans by tsetse fly (

Glossina

genus) bites which have acquired their infection from human beings or from animals harbouring the human pathogenic

parasites

Definition of Trypanosomiasis

Cont

Two forms of the disease exist.

The slow-progressing form, caused by

Trypanosoma

brucei

gambiense

, is found in Western and Central Africa.

The faster progressing form, caused by T. b.

rhodesiense

, is found in Eastern and Southern Africa

Mother-to-child infection: the trypanosome can cross the placenta and infect the

fetus

.

Mechanical transmission through other blood sucking insects is possible.

Accidental infections have occurred in laboratories due to pricks from contaminated needles.

Clinical presentation of Trypanosomiasis

In the first stage, the trypanosomes multiply in subcutaneous tissues, blood and lymph.

This is known as a

haemolymphatic

phase, which entails bouts of fever, headaches, joint pains and itching.

After their inoculation, parasites proliferate at the site of infection, leading to an inflammatory nodule or ulcer.

This trypanosomal chancre arises in about 50% of all rhodesiense—but rarely in gambiense—infections.

After 3–4 weeks, the chancre usually heals with overlying desquamation, sometimes with altered pigmentation.

Parasites spread to the draining lymph node and reach the bloodstream, initiating the

haemolymphatic

stage of the disease.

This stage is characterised by general malaise, headache, and fever of an undulating type.

In rhodesiense infection, with its more acute course,

pancarditis

with congestive heart failure, pericardial effusion, and pulmonary oedema can cause fatalities at this early stage, whereas gambiense infection shows a more insidious development that is frequently unrecognised or misdiagnosed.

A typical sign of

gambiense

human African

trypanosomiasis

is generalised lymphadenopathy that develops after several weeks, frequently in the posterior triangle of the neck

Clinical

presentation of Trypanosomiasis

cont.

In the second stage the parasites cross the blood-brain barrier to infect the central nervous system.

This is known as the neurological phase.

In general this is when more obvious signs and symptoms of the disease appear: changes of behaviour, confusion, sensory disturbances and poor coordination.

Disturbance of the sleep cycle, which gives the disease its name, is an important feature of the second stage of the disease.

Diagnosis of Trypanosomiasis

The diagnosis of African Trypanosomiasis is made through laboratory methods, because the clinical features of infection are not sufficiently specific.

The diagnosis rests on finding the parasite in body fluid or tissue by microscopy.

The parasite load in

T. b. rhodesiense

infection is substantially higher than the level in

T. b. gambiense

infection.

T. b. rhodesiense

parasites can easily be found in blood.

Diagnosis of Trypanosomiasis

Cont

They can also be found in lymph node fluid or in fluid or biopsy of a chancre.

The classic method for diagnosing

T. b. gambiense

infection is by microscopic examination of lymph node aspirate, usually from a posterior cervical node.

It is often difficult to detect

T. b. gambiense

in blood. Concentration techniques and serial examinations are frequently needed.

Serologic testing is available outside the U.S. for

T. b. gambiense

; however, it normally is used for screening purposes only and the definitive diagnosis rests on microscopic

Diagnosis of Trypanosomiasis

Cont

All patients diagnosed with African trypanosomiasis must have their cerebrospinal fluid examined to determine whether there is involvement of the central nervous system, since the choice of treatment drug(s) will depend on the disease stage.

The World Health Organization criteria for central nervous system involvement include increased protein in cerebrospinal fluid and a white cell count of more than 5.

Trypanosomes can often be observed in cerebrospinal fluid in persons with second stage infection

.

Activity

: Small Group Discussion

What

is the

treatment

of Trypanosomiasis?

Pharmacological treatment of Trypanosomiasis

The type of treatment depends on the stage of the disease.

The drugs used in the first stage of the disease are of lower toxicity and easier to administer.

The earlier the disease is identified, the better the prospect of a cure.

Treatment success in the second stage depends on a drug that can cross the blood-brain barrier to reach the parasite.

Such drugs are toxic and complicated to administer.

Monitoring of Trypanosomiasis Therapy

Monitor clinically and by using laboratory test

In both early- and late-stage trypanosomiasis, symptoms usually resolve after treatment, and the

parasitemia

clears on repeat blood smears.

Patients who have recovered from late-stage East African trypanosomiasis should undergo

lumbar punctures

every 3 months for the first year.

Patients who have recovered from West African trypanosomiasis should undergo lumbar punctures every 6 months for 2 years

.

Monitoring of Trypanosomiasis

Therapy

Cont

….

If symptoms return, the CSF WBC count is higher than 20/µL, CSF

pleocytosis

occurs((presence of an abnormally large number lymphocytes in cerebrospinal fluid), or trypanosomes are still present in blood or CSF, a relapse is suggested.

However, a persistently elevated CSF WBC count may also be observed in recovering patients; thus, the change (increase or decrease) in the WBC count is more diagnostically helpful than the count by itself.

If a relapse is noted, repeat treatment with

melarsoprol

or

eflornithine

may be considered

Key Points

Human

African trypanosomiasis, also known as sleeping sickness, is a vector-borne parasitic disease.

It is caused by infection with protozoan parasites belonging to the genus

Trypanosoma

.

They are transmitted to humans by tsetse fly (

Glossina

genus) bites which have acquired their infection from human beings or from animals harbouring human pathogenic parasites.

The type of treatment depends on the disease stage whereby drugs used in the first stage are safer and easier to administer than those for second stage.

Also, the earlier the disease is identified, the better the prospect of a cure

.

Evaluation

What

is trypanosomiasis?

What is the pathophysiology of trypanosomiasis?

What are the signs and symptoms of trypanosomiasis?

How is the treatment of trypanosomiasis?

References

Wells

BG,

DiPiro

J,

Schwinghammer

T (2013),

Pharmacotherapy Handbook

(6

th

Ed). New York, NY: McGraw-Hill.

DiPiro

JT, Talbert RL, Yee GC, Matzke GR, Wells BG, Posey ML, (2008):

Pharmacotherapy: A Pathophysiologic Approach

(7

th

ed

): New York, NY: McGraw-Hill.

Katz M D.,

Matthias KR.,

Chisholm-Burns M A.,

Pharmacotherapy(2011)

Principles & Practice Study Guide: A Case-Based Care Plan Approach

:

New York, NY: McGraw-Hill.

Schwinghammer

TL, Koehler JM (2009)

Pharmacotherapy Casebook: A Patient-Focused Approach

(7

th

ed

): New York, NY: McGraw-Hill.

PST 06106

Basic Pharmacotherapy

Session 13: Pharmacotherapy of Schistosomiasis

Learning tasks

By the end of this session students are expected to be able to:

Define

schistosomiasis

Explain pathophysiology of schistosomiasis

Explain the clinical presentation of schistosomiasis

Outline diagnosis of schistosomiasis

Describe pharmacological treatment of schistosomiasis

Describe monitoring of schistosomiasis therapy

Activity: Buzzing

What

is

Schistosomiasis

?

Definition of Schistosomiasis

Schistosomiasis

Schistosomiasis is an acute and chronic parasitic disease caused by blood flukes (trematode worms) of the genus

Schistosoma

.

Definition of Schistosomiasis

Cont

There are 2 major forms of schistosomiasis which are intestinal and urogenital caused by 5 main species of blood fluke as follows

;

Definition of Schistosomiasis

Cont

….

Infection happens when larval forms of the parasite released by freshwater snails penetrate the skin during contact with infested water.

Transmission occurs when infected individual from schistosomiasis contaminate freshwater sources with their excreta containing parasite eggs, which hatch in water.

In the body, the larvae develop into adult

schistosomes

.

Adult worms live in the blood vessels where the females release eggs.

Some of the eggs are passed out of the body in the

faeces

or urine to continue the parasite’s lifecycle.

Others become trapped in body tissues, causing immune reactions and progressive damage to organs

.

Pathophysiology and Symptoms of Schistosomiasis

In schistosomiasis, adult worms reside in the mesenteric and pelvic venules in various sites where they lay eggs

These sites tend to be specific for each species (e.g.

S.

japonicum

prefers the superior mesenteric veins draining to the small intestine, while

S.

mansoni

prefers the superior mesenteric veins of the large intestine)

Many eggs are carried upstream where they get lodged in various organs, especially in the liver, bowel, and genitourinary tract

Acute disease may trigger a cell-driven inflammatory response (involving tumour necrosis factor, interleukin-1, and interleukin-6 cytokines) and cause febrile illness

Pathophysiology and Symptoms of Schistosomiasis

Cont..

As mature female worms lay eggs, products of worm and egg metabolism induce formation of immune complexes resulting to a serum like-sickness called Katayama syndrome

In chronic disease, eggs are the cause of pathology; they evoke a Thelper type 2 (Th2) cell-driven granulomatous reaction (involving interleukin-4, interleukin-5, and interleukin-13 cytokines) resulting in tissue fibrosis and chronic morbidity

Gastrointestinal schistosomiasis due to S.

mansoni

, S.

japonicum

and S.

mekongi

can cause bowel lesions such as ulceration,

pseudopolyps

(masses of scar tissue during healing), and

microabcesses

.

These manifest clinically as abdominal pain, altered bowel habits, and blood in stools

Pathophysiology and Symptoms of Schistosomiasis

Cont

The

classic sign of urogenital schistosomiasis is haematuria and is specifically noted with

S.

haematobium

Bladder, ureter fibrosis and kidney damage are sometimes seen in advanced cases

The urogenital form may present with genital lesions (e.g. vulvar nodules), vaginal bleeding,

dyspareunia(painful intercourse) ,

and fallopian tube damage (in the late stages) in females

Genital infection in males may

result in

damage to seminal vesicles, prostate and other related organs; this may lead to irreversible infertility

Clinical Presentation of Schistosomiasis

Symptoms of schistosomiasis are caused by the body’s reaction to the worms' eggs.

Intestinal schistosomiasis can result in abdominal pain,

diarrhoea

, and blood in the stool.

Liver enlargement is common in advanced cases, and is frequently associated with an accumulation of fluid in the peritoneal cavity and hypertension of the abdominal blood vessels.

In such cases there may also be enlargement of the spleen.

The classic sign of urogenital schistosomiasis is

haematuria

(blood in urine).

Clinical Presentation of Schistosomiasis

Cont

Fibrosis of the bladder and ureter, and kidney damage are sometimes diagnosed in advanced cases.

Bladder cancer is another possible complication in the later stages. In women, urogenital schistosomiasis may present with genital lesions, vaginal bleeding, pain during sexual intercourse, and nodules in the vulva.

In men, urogenital schistosomiasis can induce pathology of the seminal vesicles, prostate, and other organs.

This disease may also have other long-term irreversible consequences, including infertility.

Diagnosis of Schistosomiasis

Schistosomiasis is diagnosed through the detection of parasite eggs in stool or urine specimens

Antibodies and/or antigens detected in blood or urine samples are also indications of infection

For urogenital schistosomiasis, a filtration technique using nylon, paper or polycarbonate filters is the standard diagnostic technique

Children with

S.

haematobium

almost always have microscopic blood in their urine which can be detected by chemical reagent

strips

Diagnosis of

Schistosomiasis

Cont

The eggs of intestinal schistosomiasis can be detected in

faecal

specimens through a technique using methylene blue-stained cellophane soaked in

glycerine

or glass slides, known as the Kato-Katz technique

For people living in non-endemic or low-transmission areas, serological and immunological tests may be useful in showing exposure to infection and the need for thorough examination, treatment and follow-up

Activity

: Small Group Discussion

• What

is the

treatment

of Schistosomiasis?

Pharmacological Treatment of Schistosomiasis

Praziquantel (PO) 40mg/kg as a single dose or in 2 divided doses

The control of schistosomiasis is based on large-scale treatment of at-risk population groups, access to safe water, improved sanitation, hygiene education, and snail control.

The WHO strategy for schistosomiasis control focuses on reducing disease through periodic, targeted treatment with

praziquantel

through the large-scale treatment (preventive chemotherapy) of affected populations.

It involves regular treatment of all at-risk groups.

Groups targeted for treatment are:

School-aged children in endemic areas.

Pharmacological Treatment of

Schistosomiasis

Cont

Adults considered to be at risk in endemic areas, and people with occupations involving contact with infested water, such as fishermen, farmers, irrigation workers, and women whose domestic tasks bring them in contact with infested water.

Entire communities living in highly endemic areas.

In high-transmission areas, treatment may have to be repeated every year for a number of years.

Monitoring is essential to determine the impact of control interventions

.

Monitoring Of Schistosomiasis Therapy

Follow-up of treatment response in schistosomiasis needs to be guided by active disease parameters, such as suggestive symptoms, raised eosinophil count, or parasitological/histological evidence of viable eggs

If symptoms such as hematuria or bloody diarrhea persist for weeks after treatment, urine or stool samples should be tested for parasite eggs and appropriate action should be taken depending on the results

Serological assays of the levels of anti-

schistosome

-egg antibodies can also be used in the post-treatment monitoring to confirm

for

treatment

success or failure

from

praziquentel

.

Key Points

Schistosomiasis

is an acute and chronic parasitic disease caused by blood flukes (trematode worms) of the genus

Schistosoma

.

People become infected when larval forms of the parasite are released by freshwater snails and then penetrate the skin during contact with infested water.

Transmission occurs when people suffering from schistosomiasis contaminate freshwater sources with their excreta containing parasite eggs, which hatch in water.

The classic sign of urogenital schistosomiasis is haematuria (blood in urine

Praziquantel is the recommended treatment against all forms of schistosomiasis

Evaluation

What

is Schistosomiasis?

What is the pathophysiology of

Schistosomiasis?

What are the signs and symptoms of Schistosomiasis?

How is the treatment of Schistosomiasis

?

References

Wells

BG,

DiPiro

J,

Schwinghammer

T (2013),

Pharmacotherapy Handbook

(6

th

Ed). New York, NY: McGraw-Hill.

DiPiro

JT, Talbert RL, Yee GC, Matzke GR, Wells BG, Posey ML, (2008):

Pharmacotherapy: A Pathophysiologic Approach

(7

th

ed

): New York, NY: McGraw-Hill.

Katz M D., Matthias KR., Chisholm-Burns M A., Pharmacotherapy(2011)

Principles & Practice Study Guide: A Case-Based Care Plan Approach

: New York, NY: McGraw-Hill.

Schwinghammer

TL, Koehler JM (2009)

Pharmacotherapy Casebook: A Patient-Focused Approach

(7

th

ed

): New York, NY: McGraw-Hill.

PST 06106

Basic Pharmacotherapy

Session 14: Pharmacotherapy

of

Gonorrhea

Learning Objective

By the end of this session students are expected to be able to:

Define

gonorrhoea

Explain pathophysiology of gonorrhoea

Explain the clinical presentation of gonorrhoea

Outline diagnosis of gonorrhoea

Describe pharmacological treatment of gonorrhoea

Describe monitoring of gonorrhoea

therapy

Activity: Buzzing

•What

is

Gonorrhoea

?

Definition of

Gonorrhea

Gonorrhea

is a

sexually transmitted disease (

STD)

caused

by infection with the bacterium

Neisseria gonorrhoeae

.

It tends to infect warm, moist areas of the body, including the:

U

rethra

(the tube that drains urine from the urinary bladder)

E

yes

T

hroat

V

agina

A

nus

F

emale

reproductive tract

(the fallopian tubes, cervix, and uterus)

Definition of Gonorrhea

Gonorrhea is transmitted from person to person through unprotected oral, anal, or vaginal sex.

People with numerous sexual partners or those who don’t use a condom are at greatest risk of infection

.

Pathophysiology of

Gonorrhea

On contact with a mucosal surface lined by columnar, cuboidal, or

noncornified

squamous epithelial cells, the gonococci attach to cell membranes by means of surface pili and are then

pinocytosed

.

The virulence of the organism is mediated primarily by the presence of pili and other outer membrane proteins.

After mucosal damage is established,

polymorphonuclear

(PMN) leukocytes invade the tissue, submucosal abscesses form, and purulent exudates are secreted

.

Clinical Presentation of Gonorrhea

Individuals infected with gonorrhea can be;

symptomatic or asymptomatic,

have complicated or uncomplicated infections, and

Have infections involving several anatomic sites.

Complications

associated with untreated gonorrhea appear more pronounced in women, because most of them are asymptomatic

As a result, most of these patients develop serious complications, such as;

pelvic inflammatory disease (PID),

Infertility and ectopic pregnancies.

In other patients the gonococci invade the bloodstream and produce disseminated disease

Diagnosis of

Gonorrhea

Diagnosis of gonococcal infections can be made by ;

gram-stained smears,

culture, or

Methods based on the detection of cellular components of the gonococcus such as Enzyme immunoassay, DNA probe techniques, and nucleic acid amplification techniques (NAATs) are also used in clinical specimens.

Various stains have been used to identify gonococci microscopically, with the Gram stain the most widely used in clinical practice.

Gram-stained smears are positive for gonococci when gram-negative diplococci of typical kidney bean morphology are identified within PMN leukocytes.

Activity

: Small Group Discussion

What

is the

treatment

of Gonorrhoea?

Pharmacological treatment of gonorrhea

Uncomplicated gonococcal infection

Recommended Regimen

Ceftriaxone 250mg IM in a single dose

PLUS

Azithromycin 1g orally in a single dose

Alternative regimen

If ceftriaxone is not available.

Cefixime

400mg orally in a single dose

plus

Azithromycin 1g orally in a single dose

Treatment of various forms of

Gonorrhea

Infection

Monitoring Of Gonorrhea Therapy

It is recommended to obtain follow-up cultures at least 3 days after treatment

However the combination gonorrhea and chlamydial therapy rarely results in treatment failures, and routine follow-up of patients treated with a regimen is not necessary.

Persistence of symptoms following any treatment requires culture of the site(s) of gonorrheal infection, as well as susceptibility testing if gonococci are isolated.

Monitoring Of Gonorrhea

Therapy Cont..

In most cases, the presence of gonococci indicates reinfection rather than treatment failure and reflects the need for improved patient education and sex partner referral.

Persistence of symptoms also can be caused by other infectious causes, such as C. trachomatis

Key Points

Gonorrhea

is a sexually transmitted disease (STD).

It’s

caused by infection with the bacterium Neisseria

gonorrhoeae

Gonorrhea

passes from person to person through unprotected oral, anal, or vaginal

sex.

First

line drug treatment with

Cetriaxone

and Azithromycin is recommended

Evaluation

What

is Gonorrhoea?

What is the pathophysiology of Gonorrhoea?

What are the signs and symptoms of Gonorrhoea?

How is the treatment of Gonorrhoea?

References

Wells

BG,

DiPiro

J,

Schwinghammer

T (2013),

Pharmacotherapy Handbook

(6

th

Ed). New York, NY: McGraw-Hill.

DiPiro

JT, Talbert RL, Yee GC, Matzke GR, Wells BG, Posey ML, (2008):

Pharmacotherapy: A Pathophysiologic Approach

(7

th

ed

): New York, NY: McGraw-Hill.

Katz M D., Matthias KR., Chisholm-Burns M A., Pharmacotherapy(2011)

Principles & Practice Study Guide: A Case-Based Care Plan Approach

: New York, NY: McGraw-Hill.

Schwinghammer

TL, Koehler JM (2009)

Pharmacotherapy Casebook: A Patient-Focused Approach

(7

th

ed

): New York, NY: McGraw-Hill.

PST 06106

Basic Pharmacotherapy

Session 15: Pharmacotherapy of Syphilis

Learning Task

By the end of this session students are expected to be able to:

Define syphilis

Explain the clinical presentation of syphilis

Outline diagnosis of syphilis

Describe pharmacological treatment of syphilis

Describe the monitoring of syphilis

therapy

.

Activity: Buzzing

• What

is syphilis??

Definition of Syphilis

Syphilis

Syphilis is an infectious venereal disease caused by the spirochete

Treponema pallidum

.

Syphilis is transmissible by sexual contact with infectious lesions, from mother to fetus in utero, via blood product transfusion, and occasionally through breaks in the skin that come into contact with infectious lesions.

If untreated, it progresses through 4 stages: primary, secondary, latent, and tertiary

Clinical Presentation

Primary Syphilis

The primary stage, characterized by the appearance of a chancre on cutaneous or mucocutaneous tissue exposed to the organism, is highly infectious.

Even without treatment, chancres persist only for 1 to 8 weeks before healing spontaneously. Because syphilitic chancres can be confused with other infectious etiologies, appropriate diagnostic testing is important

.

Clinical

Presentation

Cont

Secondary Syphilis

The secondary stage of syphilis is characterized by a variety of mucocutaneous eruptions resulting from widespread

hematogenous

and lymphatic spread of

T. pallidum

.

Skin lesions can be either generalized or localized to a small portion of the body and, with the exception of follicular lesions, are

nonpruritic

.

Generalized lymphadenopathy also is seen in the majority of patients, as are nonspecific symptoms such as mild and transitory malaise, fever, pharyngitis, headache, anorexia, and arthralgia.

If untreated, secondary syphilis disappears in 4 to 10 weeks; however, lesions can recur at any time within 4 years.

Clinical Presentation

Cont

Latent Syphilis

These are persons with a positive serologic test for syphilis but with no other evidence of disease.

Latent syphilis is further divided into early and late latency.

During early latency, the patient is considered potentially infectious.

Early latency is

defined as 1 year from the onset of infection, up to 2 to 4 years.

Late latency is considered noninfectious, although the patient remains a host.

Most untreated patients with late latent syphilis have no further sequelae; however, approximately 25% to 30% progress either to neurosyphilis or to late syphilis with clinical manifestations other than neurosyphilis.

Treatment of all patients with latent syphilis is essential because there is no way to predict which patients will have progression of their disease

Clinical Presentation

Cont

Tertiary Syphilis and

Neurosyphilis

If

left untreated, syphilis can slowly produce an inflammatory reaction in virtually any organ in the body.

Manifestations of this disease progression are referred to as

tertiary syphilis.

These clinical manifestations are differentiated into two subgroups based on the presence or absence of central nervous system (CNS) involvement which are neurosyphilis or tertiary syphilis (i.e., gumma and cardiovascular syphilis).

The gumma, a nonspecific granulomatous lesion, is the classic lesion of late syphilis and develops in 50% of patients with disease progression.

These chronic, destructive lesions characteristically infiltrate the skin, bone, soft tissue, and liver but can be found in any organ or tissue.

Gummas of critical organs, such as the heart or brain, can be fatal

Clinical Presentation Of Syphilis

Diagnosis Of Syphilis

Syphilis diagnosis is based on the;

patient’s history,

physical examination,

laboratory testing and

Radiology

Diagnosis of

Sphilis

Cont

The available laboratory tests for diagnosis of syphilis include

D

irect

detection methods (i.e.

dark field

microscopy, direct fluorescent antibody test and nucleic acid amplification test),

S

erology

tests such as;

Treponemal tests which include the Treponema pallidum

haem- agglutination

assay (TPHA), the Treponema pallidum particle agglutination assay (TPPA) and the fluorescent treponemal antibody absorbed (FTA-ABS) tests

Non-treponemal tests (the microscopic Venereal Diseases Research Laboratory -VDRL and the macroscopic rapid plasma

reagin

–RPR tests),

Examination of cerebrospinal fluids

Rapid diagnostic tests (RDTs) for treponemal antibodies in syphilis infection

Activity

: Small Group Discussion

• What

is the

treatment

of

Syphilis

?

Pharmacological Treatment

Parenteral penicillin G is the treatment of choice for all stages of syphilis.

Because

T. pallidum

multiplies slowly, single doses of short- or intermediate-acting penicillins do not provide the prolonged, low-level exposure to penicillin required for eradication of the

treponeme

.

A result, benzathine penicillin G is the only penicillin effective for single-dose therapy.

The recommended treatment for syphilis of less than 1 year’s duration is benzathine penicillin G 2.4 million units as a single dose.

Units can be administered once a week for 2 consecutive weeks.

In patients with syphilis of longer than 1 year’s duration and normal CSF examination, benzathine penicillin G is administered weekly for three successive doses

Monitoring Of Syphilis Therapy

Non treponemal tests should be performed at 6 and 12 months in all patients

treated

for

primary and secondary syphilis and at 6, 12, and 24 months for early and late latent disease.

More frequent monitoring of HIV-infected individuals (i.e., 3, 6, 9, 12, and 24 months after therapy) should be done

In general, the time to reach seronegativity is proportional to the duration of the

disease.

Despite adequate therapy, some patients can remain seropositive based on

non- treponemal

test results.

In these cases, stabilization of low antibody titers is indicative of adequate therapy.

For women treated during pregnancy, monthly quantitative

non-treponemal

tests are recommended in those at high risk of reinfection.

Key Points

Syphilis

is a systemic disease from the outset and is caused by the

spirochaete

,

Treponema

pallidum (T. pallidum)

The infection can be classified as congenital (transmitted from mother to child in utero) or acquired (through sex or blood transfusion)

Acquired syphilis is divided into early and late syphilis

Early syphilis comprises the primary, secondary and early latent stages while late syphilis refers to late latent syphilis,

gummatous

, neurological and cardiovascular syphilis

Long-acting benzathine

benzylpenicillin

provides optimal

treponemicidal

penicillinaemia

and is recommended for syphilis treatment

Evaluation

What

is Syphilis?

What are the signs and symptoms of syphilis?

What is the treatment of Syphilis?

How will you monitor patient on syphilis therapy

References

Wells

BG,

DiPiro

J,

Schwinghammer

T (2013),

Pharmacotherapy Handbook

(6

th

Ed). New York, NY: McGraw-Hill.

DiPiro

JT, Talbert RL, Yee GC, Matzke GR, Wells BG, Posey ML, (2008):

Pharmacotherapy: A Pathophysiologic Approach

(7

th

ed

): New York, NY: McGraw-Hill.

Katz M D., Matthias KR., Chisholm-Burns M A., Pharmacotherapy(2011)

Principles & Practice Study Guide: A Case-Based Care Plan Approach

: New York, NY: McGraw-Hill.

Schwinghammer

TL, Koehler JM (2009)

Pharmacotherapy Casebook: A Patient-Focused Approach

(7

th

ed

): New York, NY: McGraw-Hill.

PST 06106

Basic Pharmacotherapy

Session 16: Pharmacotherapy of Chlamydial Genital Tract Infections

Learning Tasks

By the end of this session students are expected to be able to

:

Define

chlamydial genital tract infections

Explain pathophysiology of chlamydial genital tract infections

Explain the clinical presentation of chlamydial genital tract infections

Outline diagnosis of chlamydial genital tract infections

Describe pharmacological treatment of chlamydial genital tract infections

Describe the monitoring of chlamydial genital tract infections therapy

Activity: Buzzing

What

is Chlamydial Genital Tract Infections?

Definition of Chlamydial Genital Tract Infections

Chlamydial Genital Tract Infections

Chlamydial Genital Tract Infections is a sexually transmissible infection caused by bacterium

Chlamydia

t

rachomatis

Persons infected with the bacterium may not have symptoms of infection but can still transmit the bacterium.

Chlamydia can affect the urethra (the urine passage), cervix (the neck of the womb), rectum and anus, throat, and eyes

.

Pathophysiology of Chlamydial Genital Tract Infections

C. trachomatis

is an obligate intracellular parasite that shares properties of both viruses and bacteria.

Like viruses,

chlamydiae

require cellular material from host cells for replication; however, unlike viruses,

chlamydiae

maintain their cellular identity throughout development.

Although

C. trachomatis

lacks a cell-wall peptidoglycan, its major outer membrane is similar to gram-negative bacteria.

At least 18

serovars

(subspecies) of

C. trachomatis

exist, of which only the lymphogranuloma venereum strains produce potentially invasive infections.

The remaining

serovars

are involved primarily with superficial infection of epithelial cells

.

Pathophysiology of Chlamydial Genital Tract

Infections Cont

..

Chlamydia have the ability to establish long-term associations with host cells.

When an infected host cell is starved for various nutrients such as amino acids (for example, tryptophan), iron, or vitamins, this has a negative consequence for Chlamydiae since the organism is dependent on the host cell for these nutrients.

The starved

Chlamydiae

enter a persistent growth state wherein they stop cell division and become morphologically aberrant by increasing in size.

Persistent organisms remain viable as they are capable of returning to a normal growth state once conditions in the host cell improve and causing chronic

Clinical

Presentation of Chlamydial Genital Tract Infections

In comparison with gonorrhea, chlamydial genital tract infections are more frequently asymptomatic, and when present, symptoms tend to be less noticeable.

Urethral discharge usually is less profuse and more mucoid or watery than the urethral discharge associated with gonorrhea.

Diagnosis of Chlamydia Genital tract infection

A sample of urine can be collected and analyzed in the laboratory to investigate the presence of this infection.

A swab of the discharge can be collected for culture or antigen testing for chlamydia.

Nucleic Acid Amplification Tests

(NAAT), such

as

Polymerase Chain Reaction

(PCR

),

Transcription Mediated Amplification

(

TMA), and the DNA

Strand Displacement Amplification

(SDA) now are the mainstays.

NAAT for chlamydia may be performed on swab specimens sampled from the cervix (women) or urethra (men), on self-collected vaginal swabs, or on voided urine

Activity

: Small Group Discussion

What

is the treatment of Chlamydial Genital Tract Infections?

Pharmacological treatment of Chlamydial Genital Tract infection

Monitoring of chlamydial Genital Tract Infections Therapy

Treatment of chlamydial infections with the recommended regimens is highly effective; therefore, post-treatment laboratory testing is not recommended routinely unless symptoms persist or there are other specific concerns (e.g., pregnancy).

Post-treatment tests should not be performed for at least 3 weeks following

completion

of

therapy.

When post-treatment tests are positive, they usually represent noncompliance, failure to treat sexual partners, or laboratory error rather than inadequate therapy or resistance to therapy.

Infants with pneumonitis should receive follow-up testing because erythromycin is only 80% effective, and a second course of therapy can be necessary

Key

Points

Chlamydia

is a sexually transmissible infection caused by bacterium

Chlamydia

t

rachomatis

Persons infected with the bacterium may not have symptoms of infection but can still transmit the bacterium.

Azithromycin is drug of choice for the treatment of chlamydia infection

Evaluation

What

is

Chlamydia

infection?

What is the pathophysiology of

Chlamydial

infection?

What are the signs and symptoms of

Chlamydia

infection?

How is the treatment of

Chlamydia

Infection?

References

Wells

BG,

DiPiro

J,

Schwinghammer

T (2013),

Pharmacotherapy Handbook

(6

th

Ed). New York, NY: McGraw-Hill.

DiPiro

JT, Talbert RL, Yee GC, Matzke GR, Wells BG, Posey ML, (2008):

Pharmacotherapy: A Pathophysiologic Approach

(7

th

ed

): New York, NY: McGraw-Hill.

Katz M D., Matthias KR., Chisholm-Burns M A., Pharmacotherapy(2011)

Principles & Practice Study Guide: A Case-Based Care Plan Approach

: New York, NY: McGraw-Hill.

Schwinghammer

TL, Koehler JM (2009)

Pharmacotherapy Casebook: A Patient-Focused Approach

(7

th

ed

): New York, NY: McGraw-Hill.

PST 06106

Basic Pharmacotherapy

Session 17: Pharmacotherapy of Genital Herpes

Learning Tasks

By the end of this session students are expected to be able to:

Define genital herpes

Explain pathophysiology of genital herpes

Explain the clinical presentation of genital herpes

Outline diagnosis of genital herpes

Describe pharmacological treatment of genital herpes

Describe the monitoring of genital herpes

therapy

Activity: Buzzing

• What

is Genital

Herpes?

Definition of Genital Herpes

Genital Herpes

Genital herpes is a common sexually transmitted infection caused by the herpes simplex virus (HSV).

Sexual contact is the primary way that the virus spreads.

There are two types of Herpes Simplex viruses; herpes simplex virus type 1 (HSV-1) and herpes simplex virus type 2 (HSV-2).

HSV-1 is associated most commonly with oropharyngeal disease, and HSV-2 is associated most closely with genital disease;

However, each virus is capable of causing clinically indistinguishable infections in both anatomic areas.

Definition of Genital Herpes

Cont.….

Humans are the sole known reservoir for HSV.

Infection is transmitted via inoculation of virus from infected secretions onto mucosal surfaces (e.g., urethra, oropharynx, cervix, and conjunctivae) or through abraded skin.

The cycle of HSV infection occurs in five stages: primary muco-cutaneous infection, infection of the ganglia, establishment of latency, reactivation, and recurrent infection

Pathophysiology Of Genital Herpes

After viral inoculation, HSV infection is associated with cytoplasmic

granulation(condensed areas of cellular material that may be bounded by a membrane),

ballooning degeneration of

cells (cells undergoing this form of death increase in size(balloon),

and production of

mononucleated

giant

cells ( cells formed by fusion of monocytes/macrophage)

Initially, the cellular response is predominantly

polymorph nuclear,

followed by a lymphocytic response.

Replication occurs with viral spread to contiguous cells and peripheral sensory nerves. Latency then is established in sensory or autonomic nerve root ganglia.

Latency appears to be lifelong, interrupted only by reactivation of the viral infection.

It is unclear what factors are important in maintaining latency, but immune responses and emotional and physical stresses appear important in reactivating latent virus.

Clinical Presentation Of Genital Herpes

The signs and symptoms of genital herpes infection are

influenced by

many factors, including previous exposure to HSV, viral type, and host factors such as age and site of infection.

High percentage of initial and recurrent infections are asymptomatic,

Viral shedding can occur in the absence of apparent lesions or symptoms

A summary of the clinical presentation of genital herpes is provided in Table

Diagnosis Of Genital Herpes

A presumptive diagnosis of genital herpes commonly is made based on the presence of

dark-field negative

, vesicular, or ulcerative genital lesions.

A prior history of similar lesions or recent sexual contact with an individual with similar lesions also is useful in making the diagnosis

Viral culture. This test involves taking a tissue sample or scraping of the sores for examination in the laboratory

.

Diagnosis Of Genital

Herpes

Cont

….

Polymerase chain reaction (PCR) test. PCR is used to copy patient DNA from a blood sample, tissue from a sore or spinal fluid.

The DNA can then be tested to establish the presence of HSV and determine which type of HSV you have.

Blood test. This test analyzes a sample of blood for the presence of HSV antibodies to detect a past herpes infection.

Several serologic tests capable of distinguishing HSV-1 and HSV-2 antibodies are available.

These tests detect antibodies to type-specific HSV-1 and HSV-2 proteins gG-1 and gG-2, respectively

Activity

: Small Group Discussion

What

is the treatment of Genital Herpes?

Pharmacological Treatment of Genital Herpes

The most achievable goals in the management of genital herpes are to relieve symptoms and to shorten the clinical course, to prevent complications and recurrences, and to decrease disease transmission.

Although research has focused primarily on the treatment of active infection and suppression of recurrences, increasing emphasis is being placed on various approaches, including immunotherapy that might provide protection from disease transmission or possibly eliminate established latency.

.

Pharmacological Treatment of Genital Herpes

Oral formulations of acyclovir,

famciclovir

, and

valacyclovir

have demonstrated efficacy in reducing viral shedding, duration of symptoms, and time to healing of first-episode genital herpes infections, with maximal benefits seen when therapy is initiated at the earliest stages of infection

Pharmacological Treatment of Genital Herpes

Monitoring of Genital Herpes Therapy

Available antiviral compounds are of greatest benefit in patients experiencing first-episode primary infections, immunocompromised patients, and patients with frequent or severe recurrent infections.

Antivirals, however, are palliative and not curative, and patients receiving these agents should be monitored closely for adverse drug effects.

Discontinuation of suppressive therapy after 1 year should be considered to assess for possible changes in the patient’s intrinsic pattern of recurrence.

In many patients, decreases in recurrence rates and the severity of symptoms occur over time. However, it is also

preferred

to continue suppressive therapy indefinitely because it significantly reduces asymptomatic viral shedding, a potential benefit in reducing the risk of disease transmission to uninfected sexual partners

Key

Points

Genital

herpes is a common sexually transmitted infection caused by the herpes simplex virus (HSV).

Infection is transmitted via inoculation of virus from infected secretions onto mucosal surfaces (e.g., urethra, oropharynx, cervix, and conjunctivae) or through abraded skin

The signs and symptoms of genital herpes infection are

influencedby

many factors, including previous exposure to HSV, viral type, and host factors such as age and site of infection

Oral formulations of acyclovir,

famciclovir

, and

valacyclovir

have demonstrated efficacy in the treatment of genital herpes

Evaluation

What

is genital herpes?

What is the pathophysiology of

genital herpes?

What are the signs and symptoms of genital herpes?

How is the treatment of genital herpes?

References

Wells

BG,

DiPiro

J,

Schwinghammer

T (2013),

Pharmacotherapy Handbook

(6

th

Ed). New York, NY: McGraw-Hill.

DiPiro

JT, Talbert RL, Yee GC, Matzke GR, Wells BG, Posey ML, (2008):

Pharmacotherapy: A Pathophysiologic Approach

(7

th

ed

): New York, NY: McGraw-Hill.

Katz M D.,

Matthias KR.,

Chisholm-Burns M A.,

Pharmacotherapy(2011)

Principles & Practice Study Guide: A Case-Based Care Plan Approach

:

New York, NY: McGraw-Hill.

Schwinghammer

TL, Koehler JM (2009)

Pharmacotherapy Casebook: A Patient-Focused Approach

(7

th

ed

): New York, NY: McGraw-Hill.

PST 06106

Basic Pharmacotherapy

Session 18:

Pharmacotherapy of Urinary Tract Infections

Learning Objectives

By the end of this session students are expected to be able to

:

Define

urinary tract infections

Explain pathophysiology of urinary tract infections

Explain the clinical presentation of urinary tract infections

Outline diagnosis of urinary tract infections

Describe pharmacological treatment of urinary tract infections

Describe the monitoring of urinary tract infections

therapy

Activity: Buzzing

What

is Urinary Tract Infections?

Definition of Urinary Tract Infections

Urinary Tract Infections (UTI

)

UTI is defined as the presence of microorganisms in the urinary tract that cannot be accounted for by contamination.

The organisms present have the potential to invade the tissues of the urinary tract and adjacent structures.

Infection may be limited to the growth of bacteria in the urine, which frequently may not produce symptoms.

A UTI can present as several syndromes associated with an inflammatory response to microbial invasion and can range from asymptomatic bacteriuria to pyelonephritis with bacteremia or sepsis.

Definition of Urinary Tract Infections

Cont.….

UTIs are classified by lower and upper urinary tract infections.

Upper tract infection include pyelonephritis (an infection involving the kidneys) represents

Lower

tract infections correspond to cystitis (bladder),

Also, UTIs are designated as uncomplicated or complicated.

Uncomplicated infections occur in individuals who lack structural or functional abnormalities of the urinary tract that interfere with the normal flow of urine or voiding mechanism.

Definition of Urinary Tract Infections

Cont.….

These infections occur in females of child-bearing age (15 to 45 years) who are otherwise

normal healthy individuals.

Complicated UTIs are the result of a predisposing lesion of the urinary tract, such as a congenital abnormality or distortion of the urinary tract, a stone, indwelling catheter, prostatic hypertrophy, obstruction, or neurologic deficit that interferes with the normal

Classification of UTI

Pathophysiology of Urinary Tract Infections

The bacteria causing UTIs usually originate from bowel flora of the host.

Although virtually every organism is associated with UTIs, certain organisms predominate as a result of specific virulence factors.

The most common cause of UTIs is

Escherichia coli

, which accounts for 80% to 90% of community-acquired

infections.

Additional causative organisms in uncomplicated infections

include

Staphylococcus

saprophyticus

,

Klebsiella

pneumoniae, Proteus

spp.,

Pseudomonas aeruginosa

, and

Enterococcus

spp.

Pathophysiology

cont

Pathogenic organisms have differing degrees of pathogenicity (virulence), which play a role in the development and severity of infection.

Bacteria that adhere to the epithelium of the urinary tract are associated with colonization and infection

The mechanism of adhesion of gram-negative bacteria, particularly E. coli, is related to bacterial fimbriae that are rigid, hair-like appendages of the cell wall

These

fimbriae adhere to specific glycolipid components on epithelial cells

The most common type of fimbriae is type 1, which binds to mannose residues present in glycoproteins

Pathophysiology

Cont.

Glycosaminoglycan and Tamm-

Horsfall

protein are rich in mannose residues that readily trap those organisms that contain type 1 fimbriae, which are then washed out of the bladder.

Other fimbriae are mannose resistant and are associated more frequently with pyelonephritis, such as P fimbriae, which bind avidly to specific glycolipid receptors on

uroepithelial

cells

These bacteria are resistant to washout or removal by glycosaminoglycan and are able to multiply and invade tissue, and causing infection

Clinical Presentation of UTIs

Signs and symptoms

Lower UTI: dysuria, urgency, frequency,

nocturia

, suprapubic heaviness

Gross hematuria

Upper UTI: flank pain, fever, nausea, vomiting,

malaise

Physical examination

Upper UTI: costovertebral

tenderness

Clinical

Presentation of

UTIs

Cont

Laboratory tests

Bacteriuria

Pyuria (white blood cell count >10/mm 3 )

Nitrite-positive urine (with nitrite reducers)

Leukocyte esterase-positive urine

Antibody-coated bacteria (upper UTI

)

Diagnosis of UTIs

Symptoms alone are unreliable for the diagnosis of bacterial UTIs.

The key to the diagnosis of UTI is the ability to demonstrate significant numbers of microorganisms in an appropriate urine specimen to distinguish contamination from infection.

Diagnosis of

UTIs Cont.…

Urine testing

The gold standard for a urine test is to perform a bacteriological urine culture, with identification of the pathogen, with quantification and sensitivity testing.

To test whether the patient has a UTI at all, orientating indirect methods are often used in practice to detect the bacteria or inflammation (dip sticks).

The bacterial count may be assessed by urine microscopy and immersion culture media.

Midstream urine is normally collected

Diagnosis of

UTIs Cont.…

Dip sticks

Urine dip sticks are one of the most frequently used instruments for diagnostic testing if there is clinical evidence that a patient is suffering from UTI.

Multistix

are most often used, which may be able to detect nitrite (a metabolic product of typical pathogens of the urinary tract), leukocyte esterase, protein and blood (as a marker of inflammation

).

Diagnosis of UTIs Cont.…

Dip

sticks……

If

nitrite is detected, this increases the probability of a urinary tract infection, with a likelihood ratio [LR] of 2.6 to 10.6.

However, the sensitivity is relatively low.

In contrast, the detection of leukocyte esterase increases the probability to a lesser degree (LR 1.0 to 2.6). The detection of blood is admittedly highly sensitive, but the specificity is low.

Activity

: Small Group Discussion

What

is the treatment of

UTI

?

Pharmacological Treatment of UTIs

The management of a patient with a UTI includes;

Initial evaluation,

Selection of an antibacterial agent and duration of therapy, and

Follow-up

evaluation.

The initial selection of an antimicrobial agent for the treatment of UTI is based primarily on;

The severity of the presenting signs and symptoms,

The site of infection, and

Whether the infection is determined to be uncomplicated or complicated.

Other considerations include antibiotic susceptibility, side-effect potential, cost, and the comparative inconvenience of different

therapies

.

Empirical

Treatment of UTIs

Treatment

of UTI according to Pathogen

Monitoring of UTI Therapy

In asymptomatic post-treatment patients routine urinalysis and/or urine culture is not recommended

In patients with persistent symptoms, microbiological screening is recommended.

In women whose symptoms do not resolve by end of treatment, and in those whose symptoms resolve but recur within two weeks, urine culture and antimicrobial susceptibility testing should be performed

For therapy in this situation, one should assume that the infecting organism is not susceptible to the agent originally used.

Retreatment with a seven day regimen using another agent should be considered

Antibiotic treatments may be repeated with a more prolonged course, higher dosage and/or different compounds for patients with recurrent

infections

Key Points

UTI

is defined as the presence of microorganisms in the urinary tract that cannot be accounted for by contamination.

UTIs are classified by lower and upper urinary tract infections.

The most common cause of UTIs is

Escherichia coli

, which accounts for 80% to 90% of community-acquired

infections

Signs and Symptoms of UTI include

dysuria, urgency, frequency,

nocturia

, suprapubic heaviness

Variety of antibiotics can be used for the treatment of UTI

Evaluation

What

is UTIs?

What is the pathophysiology of

UTIs?

What are the signs and symptoms of uncomplicated UTI?

How is the treatment of Uncomplicated UTI?

References

Wells

BG,

DiPiro

J,

Schwinghammer

T (2013),

Pharmacotherapy Handbook

(6

th

Ed). New York, NY: McGraw-Hill.

DiPiro

JT, Talbert RL, Yee GC, Matzke GR, Wells BG, Posey ML, (2008):

Pharmacotherapy: A Pathophysiologic Approach

(7

th

ed

): New York, NY: McGraw-Hill.

Katz M D.,

Matthias KR.,

Chisholm-Burns M A.,

Pharmacotherapy(2011)

Principles & Practice Study Guide: A Case-Based Care Plan Approach

:

New York, NY: McGraw-Hill.

Schwinghammer

TL, Koehler JM (2009)

Pharmacotherapy Casebook: A Patient-Focused Approach

(7

th

ed

): New York, NY: McGraw-Hill.

PST 06106

Basic Pharmacotherapy

Session 19: Pharmacotherapy of Folliculitis,

Furunculosis

and

Carbuncles

Learning Objectives

By the end of this session students are expected to be able to:

Define folliculitis,

furunculosis

and carbuncles

Explain pathophysiology of folliculitis,

furunculosis

and carbuncles

Explain the clinical presentation of folliculitis,

furunculosis

and carbuncles

Outline diagnosis of folliculitis,

furunculosis

and carbuncles

Describe pharmacological treatment of folliculitis,

furunculosis

and carbuncles

Describe the monitoring of folliculitis,

furunculosis

and carbuncles

therapy

Activity: Buzzing

What are Folliculitis, Furunculosis and Carbuncles?

Definition of Folliculitis, Furunculosis and Carbuncles

Folliculitis

, Furunculosis and Carbuncles

Folliculitis is inflammation of the hair follicle and is caused by physical injury, chemical irritation, or infection.

Infection occurring at the base of the eyelid is referred to as a stye.

Folliculitis is a superficial infection with pus present only in the dermis

,

Furuncles and carbuncles occur when a follicular infection extends from around the hair shaft to involve deeper areas of the skin.

A furuncle, commonly known as an

abscess

or

boil,

is a walled-off mass of purulent material arising from a hair follicle.

Definition of Folliculitis, Furunculosis and Carbuncles

The lesions are called

carbuncles

when they coalesce and extend to the

subcutaneous tissue

.

This aggregate of infected hair follicles forms deep masses that generally open and drain through multiple sinus tracts.

S. aureus

is the most common cause of folliculitis, furuncles, and carbuncles.

Inadequate chlorine levels in whirlpools, hot tubs, and swimming pools have been responsible for outbreaks of folliculitis caused by

P. aeruginosa

.

Pathophysiology of Folliculitis, Furunculosis and Carbuncles

The skin and subcutaneous tissues normally are extremely resistant to infection but may become susceptible under certain conditions.

Even when high concentrations of bacteria are applied topically or injected into the soft tissue, resulting infections are rare.

Several host factors act together to confer protection against skin infections.

Because the surface of the skin is relatively dry and has a pH of approximately 5.6, it is not conducive to bacterial growth.

Continuous renewal of the epidermal layer results in the shedding of

keratocytes

, as well as skin bacteria.

In addition, sebaceous secretions are hydrolyzed to form free fatty acids that strongly inhibit the growth of many bacteria and fungi.

Pathophysiology of Folliculitis, Furunculosis and Carbuncles

Conditions that may predispose a patient to the development of skin infections include

H

igh

concentrations of bacteria (>10 5 microorganisms),

E

xcessive

moisture of the skin,

I

nadequate

blood supply,

A

vailability

of bacterial nutrients, and

Damage to the corneal layer allowing for bacterial penetration.

The majority of Skin and Soft Tissue Infections result from the disruption of normal host defenses by processes such as skin puncture, abrasion, or underlying diseases (e.g., diabetes).

The nature and severity of the infection depend on both the type of microorganism present and the site of

inoculation

Clinical presentation and diagnosis of Folliculitis, Furunculosis and Carbuncles

Folliculitis

Pruritic, erythematous papules typically appear within 48 hours (range: 6 to 72 hours) of exposure to large numbers of organisms.

Papules evolve into pustules that generally heal in several days.

Systemic signs such as fever and malaise are uncommon, although they have been reported in cases caused by

P. aeruginosa

Clinical presentation and diagnosis of Folliculitis, Furunculosis and Carbuncles Cont.…

Furuncles/

Furunculosis

Furuncles can occur anywhere on hairy skin but generally develop in areas subject to friction and perspiration.

Furuncles are discrete lesions, whether occurring as singular or multiple nodules.

The lesion starts as a firm, tender, red nodule that becomes painful and fluctuant.

Lesions often drain spontaneously.

Lesions caused by CA-MRSA often have necrotic centers characteristic of “spider bites.”

Culture of lesion for laboratory investigation to conform the

presence

and the type of the pathogen

Clinical presentation and diagnosis of Folliculitis, Furunculosis and

Carbuncles Cont.…

Carbuncles

Carbuncles are broad, swollen, erythematous, deep, and painful follicular masses.

Carbuncles commonly develop on the back of the neck and are more likely to occur in patients with diabetes.

Unlike folliculitis and furuncles, carbuncles are commonly associated with fever, chills, and malaise.

Bacteremia with secondary spread to other tissues is common

Culture of lesion for laboratory investigation to conform the

prensence

and the type of the pathogen

Activity

: Small Group Discussion

What is the treatment of Folliculitis, Furunculosis and Carbuncles?

Pharmacological treatment of Folliculitis, Furunculosis and Carbuncles

Treatment of folliculitis generally requires only local measures, such as warm moist compresses or topical therapy (e.g., clindamycin, erythromycin, mupirocin

,

or benzoyl peroxide).

Topical agents generally are applied two to four times daily for 7 days.

Small furuncles generally can be treated with moist heat, which promotes localization and drainage of pus.

Large and/or multiple furuncles and carbuncles require incision and drainage.

Systemic antibiotics are usually not necessary unless accompanied by fever or extensive cellulitis.

Treatment of more severe infections generally consists of a penicillinase-resistant penicillin (such as

dicloxacillin

) or a first-generation cephalosporin (such as cephalexin) for 5 to 10 days

Drug Treatment

Monitoring of Folliculitis , Furuncles and Carbuncles Therapy

Many follicular infections resolve spontaneously without medical or surgical intervention.

Lesions should be incised if they do not respond to a few days of moist heat and nonprescription topical agents.

Following drainage, most lesions begin to heal within several days without antimicrobial therapy.

Any patient who is unresponsive to several days of therapy with a penicillinase-resistant penicillin or first-generation cephalosporin should have a culture and

sensitivity

Performed

because of the increasing frequency of MRSA.

Key Points

Folliculitis

is inflammation of the hair follicle and is caused by physical injury, chemical irritation, or infection

Symptoms of Folliculitis include Pruritic, erythematous papules typically appear within 48 hours (range: 6 to 72 hours) of exposure to large numbers of organisms

Treatment of folliculitis generally requires only local measures, such as warm moist compresses or topical therapy

Evaluation

What

are Folliculitis, Furuncles and Carbuncles?

What is the pathophysiology of

Folliculitis, Furuncles and Carbuncles?

What are the signs and symptoms of Folliculitis, Furuncles and Carbuncles?

How is the treatment of Folliculitis, Furuncles and Carbuncles?

References

Wells

BG,

DiPiro

J,

Schwinghammer

T (2013),

Pharmacotherapy Handbook

(6

th

Ed). New York, NY: McGraw-Hill.

DiPiro

JT, Talbert RL, Yee GC, Matzke GR, Wells BG, Posey ML, (2008):

Pharmacotherapy: A Pathophysiologic Approach

(7

th

ed

): New York, NY: McGraw-Hill.

Katz M D.,

Matthias KR.,

Chisholm-Burns M A.,

Pharmacotherapy(2011)

Principles & Practice Study Guide: A Case-Based Care Plan Approach

:

New York, NY: McGraw-Hill.

Schwinghammer

TL, Koehler JM (2009)

Pharmacotherapy Casebook: A Patient-Focused Approach

(7

th

ed

): New York, NY: McGraw-Hill.

PST 06106

Basic Pharmacotherapy

Session 20: Pharmacotherapy of Vulvovaginal Candidiasis

Learning Objectives

By the end of this session students are expected to be able to:

Define vulvovaginal candidiasis

Explain pathophysiology of vulvovaginal candidiasis

Explain the clinical presentation of vulvovaginal candidiasis

Outline diagnosis of vulvovaginal candidiasis

Describe pharmacological treatment of vulvovaginal candidiasis

Describe the monitoring of vulvovaginal candidiasis therapy

Activity: Buzzing

What is Vulvovaginal

Candidiasis ?

Definition of Vulvovaginal Candidiasis

Vulvovaginal Candidiasis

Vulvovaginal candidiasis

(VVC) refers to infections in individuals with or without symptoms who have positive vaginal cultures for

Candida

species.

Depending on episodic frequency, VVC can be classified as either;

Sporadic or

Recurrent.

This classification is essential to understanding the pathophysiology, as well as

the

pharmacotherapy of

VVC.

Definition of Vulvovaginal

Candidiasis Cont.…

VVC may also be classified as;

uncomplicated, which refers to sporadic infections that are susceptible to all forms of antifungal therapy regardless of the duration of treatment, or

Complicated, in which consideration of factors affecting the host, microorganism, and pharmacotherapy all have an essential role in successful treatment.

Complicated VVC includes recurrent VVC, severe disease, non–

Candida albicans

candidiasis, and host factors, including diabetes mellitus, immunosuppression,

and pregnancy

Pathophysiology of Vulvovaginal Candidiasis

Candida albicans

is the major pathogen responsible for VVC, accounting for 80% to 92% of symptomatic episodes.

The remainders are caused by non–

C. albicans

species, with

Candida

glabrata

dominating.

The number of cases of non–

C. albicans

candidiasis appears to be increasing, possibly related to the use of nonprescription vaginal antifungal preparations and short-course therapy and/ or the increased use of long-term maintenance therapy in preventing recurrent infections.

Candida

species can act as commensal members of the vaginal flora.

Asymptomatic colonization with

Candida

species has been found in 10% to 20% of women of reproductive age.

Pathophysiology of Vulvovaginal

Candidiasis

Cont

Candida

organisms are dimorphic;

blastospores

are believed to be responsible for colonization (transmission and spread), whereas

Germinated Candida forms are associated with tissue invasion and symptomatic infections.

To colonize the vagina,

Candida

species must be able to attach to the mucosa. The attachment process is complex.

Not only are

candidal

surface structures important for attachment, but appropriate receptors for attachment must be present in the epithelial tissue.

Pathophysiology of Vulvovaginal Candidiasis

Cont.…

Not all women have the same range of receptors, which may explain variation in colonization.

Changes in the host’s vaginal environment or response are necessary to induce a symptomatic infection.

Unfortunately, in most cases of symptomatic VVC, no precipitating factor can be identified

C

linical presentation of Vulvovaginal candidiasis

General

Often involves both the vulva and the

vagina

Symptoms

Intense vulvar itching, soreness, irritation, burning on urination, and

dyspareunia

Signs

Erythema,

fissuring (crack),

curdy “cheese”-like discharge, satellite lesions,

edema

Laboratory tests

Vaginal pH—normal, saline and 10% KOH microscopy—

blastospores

or

pseudohyphae

Other diagnostic tests

Candida

cultures not recommended unless classic signs and symptoms with normal vaginal pH and microscopy are inconclusive or recurrence is suspected

Activity

: Small Group Discussion

What is the treatment of Vulvovaginal

Candidiasis ?

Treatment of Uncomplicated

Vulvovaginal candidiasis

Pharmacological Treatment of Vulvovaginal Candidiasis

Complicated Vulvovaginal Candidiasis

Complicated VVC occurs in patients who are immunocompromised or have uncontrolled diabetes mellitus and pregnant.

These

individuals need

a more aggressive treatment plan.

Current recommendations are to lengthen therapy to 10 to 14 days regardless of the

route of

administration.

Therapeutic options include those listed in Table

however

, regimens should be continued for 10 to 14 days.

It is also recommended to repeat 150 mg dose of fluconazole 72 hours after the initial dose for better therapeutic outcomes

Pharmacological Treatment of Vulvovaginal Candidiasis

Cont.….

Antifungal-Resistant Vulvovaginal Candidiasis

Resistance to azole antifungals should be considered in individuals who have persistently positive yeast cultures and fail to respond to therapy despite adherence to prescribed regimens.

These infections can be treated with;

Boric acid Boric acid administered as a 600 mg intravaginal capsule daily for 14 days of induction therapy, followed by a maintenance regimen of one capsule

intravaginal

twice weekly.

Boric acid should not be administered orally, as it is

toxic.

OR

5-Flucytosine cream is administered vaginally, 1,000 mg inserted nightly for 7 days.

Pharmacological Treatment of Vulvovaginal Candidiasis Cont.….

Monitoring of Vulvovaginal Candidiasis Therapy

Efficacy of the antifungal agent is partly influenced by patient adherence to the medication regimen.

Patients must be counseled on proper administration and dosing

Safety end points include monitoring for occurrence of the relevant drug side effects and drug interactions

It is still prudent to monitor for hypersensitivity reactions and side effects

that

might

occur with any medication.

Monitoring of Vulvovaginal Candidiasis

Therapy Cont.…..

GI intolerance is more associated with the oral azoles.

Hepatotoxicity can occur when azole therapy is prolonged beyond 7 to 10 days or high doses are used.

Periodic monitoring of liver enzymes (alanine transaminase and aspartate amino-transferase) should be considered, especially if prolonged therapy (longer than 21 days) is anticipated.

Patients who are receiving IV amphotericin B require daily monitoring by the pharmacist.

Key Points

Vulvovaginal

candidiasis

(VVC) refers to infections in individuals with or without symptoms who have positive vaginal cultures for

Candida

species

Symptoms include intense vulvar itching, soreness, irritation, burning on urination, and dyspareunia

Azole antifungals and other topical antifungals are drug of choice for

culvovaginal

candidiasis

Evaluation

What

is Vulvovaginal Candidiasis?

What is the pathophysiology of

Vulvovaginal Candidiasis?

What are the signs and symptoms of Vulvovaginal Candidiasis?

How is the treatment of Vulvovaginal Candidiasis?

References

Wells

BG,

DiPiro

J,

Schwinghammer

T (2013),

Pharmacotherapy Handbook

(6

th

Ed). New York, NY: McGraw-Hill.

DiPiro

JT, Talbert RL, Yee GC, Matzke GR, Wells BG, Posey ML, (2008):

Pharmacotherapy: A Pathophysiologic Approach

(7

th

ed

): New York, NY: McGraw-Hill.

Katz M D., Matthias KR., Chisholm-Burns M A., Pharmacotherapy(2011)

Principles & Practice Study Guide: A Case-Based Care Plan Approach

: New York, NY: McGraw-Hill.

Schwinghammer

TL, Koehler JM (2009)

Pharmacotherapy Casebook: A Patient-Focused Approach

(7

th

ed

): New York, NY: McGraw-Hill.

PST 06106

Basic Pharmacotherapy

Session 21: Pharmacotherapy of Asthma

Learning Objectives

By the end of this session students are expected to be able to:

Define asthma

Explain pathophysiology of asthma

Explain the clinical presentation of asthma

Outline diagnosis asthma

Describe pharmacological treatment of asthma

Describe the monitoring of

asthma

Activity: Buzzing

What is

Asthma

?

Definition of Asthma

Asthma is a common, chronic respiratory disease

of the airways of the lung characterized by either the intermittent or persistent presence of highly variable degrees of airflow obstruction from airway wall inflammation and bronchial smooth muscle constriction.

People with asthma experience episodes of wheezing, breathlessness and chest tightness due to widespread narrowing of the airways.

The cause of

Asthma

is

unknown

but the risk if associated with genetics and

environmental

factors.

Genetic factors account for 60% to 80% of the susceptibility.

Asthma represents a complex genetic disorder in that the asthma phenotype is likely a result of polygenic inheritance or different combinations of genes

Definition of

Asthma Cont.…..

Environmental risk factors for the development of asthma include;

S

ocioeconomic

status,

F

amily

size,

E

xposure

to secondhand tobacco smoke in infancy and in utero,

A

llergen

exposure

U

rbanization

,

R

espiratory

syncytial virus infection, and

E

xposure

to common childhood infectious

agents

List of agents and events Triggering Asthma

Pathophysiology Of Asthma

The major characteristics of asthma include a variable degree of airflow obstruction (related to bronchospasm, edema, and mucus hypersecretion) and airways inflammation

To understand the pathogenetic mechanisms that underlies the many phenotypes of asthma, it is critical to identify factors that initiate, intensify, and modulate the inflammatory response of the airways and to determine how these processes produce the characteristic airway abnormalities

.

Pathophysiology Of Asthma

Cont

….

The immunohistopathologic features of asthma include inflammatory cell infiltration:

Neutrophils (especially in sudden-onset, fatal asthma exacerbations; occupational asthma, and patients who smoke)

Eosinophils

Lymphocytes

Mast cell activation

Epithelial cell injury

P

athophysiology

of Asthma cont.

Airway inflammation contributes to airway

hyper responsiveness,

airflow limitation, respiratory symptoms, and disease chronicity.

In some patients, persistent changes in airway structure occur, including sub-basement fibrosis, mucus hypersecretion, injury to epithelial cells, smooth muscle hypertrophy, and angiogenesis.

Gene-by-environment interactions are important to the expression of asthma.

Atopy, the genetic predisposition for the development of an immunoglobulin E (

IgE

)-mediated response to common aeroallergens, is the strongest identifiable predisposing factor for developing asthma

.

Viral respiratory infections are one of the most important causes of asthma exacerbation and may also contribute to the development of asthma

Clinical Presentation And Diagnosis Of Asthma

Clinical Presentation is divided into

Acute Asthma

Chronic

asthma

Acute asthma

General

An episode can progress over several days or hours (usual scenario) or progresses rapidly over 1 to 2 hours

.

Clinical Presentation And Diagnosis Of Asthma

Acute

asthma…..

Symptoms

The patient is anxious in acute distress and complains of severe dyspnea , shortness of breath, chest tightness, or burning and wheezing sound

The patient is only able to say a few words with each breath.

Symptoms are unresponsive to usual measures (

shortacting

inhaled

β

2 –agonist administration).

Clinical Presentation And Diagnosis Of

Asthma

Cont

Acute

asthma…..

Signs

Signs

include expiratory and inspiratory wheezing on auscultation (breath sounds may be diminished with very severe obstruction),

D

ry

hacking cough,

T

achypnea

,

T

achycardia

,

P

ale

or cyanotic skin,

Hyper inflated

chest with intercostal and supraclavicular retractions, and

Hypoxic seizures if very severe

Clinical Presentation And Diagnosis Of Asthma

Cont

Acute

asthma……

Laboratory

PEF(peak expiratory flow)

and/or

FEV(Forced expiratory volume 1)

less than 40% of normal predicted values.

Decreased arterial oxygen (

PaO

2 ), and O 2 saturations by pulse oximetry (

SaO

2 less than 90% on room air is severe).

Increased

arterial or capillary CO 2 if mild, but in the normal range or increased in moderate to severe obstruction

.

Clinical Presentation And Diagnosis Of Asthma

Cont

Acute

asthma…

Other

Diagnostic Tests

Blood gases to assess metabolic acidosis (lactic acidosis) in severe obstruction.

Complete blood count if there are signs of infection (fever and purulent sputum).

Serum electrolytes as therapy with

β

2 -agonist and corticosteroids can lower serum potassium, magnesium, and phosphate, and increase glucose.

Chest radiograph if signs of consolidation on auscultation

Clinical Presentation And Diagnosis Of Asthma

Cont

Chronic Asthma

General

Asthma is a disease of exacerbation and remission, so the patient may not have any signs or symptoms at the time of exam.

Symptoms

The patient may complain of episodes of dyspnea, chest tightness, coughing (particularly at night), wheezing, or a whistling sound when breathing.

These often occur in association with exercise, but also occur spontaneously or in association with known allergens

.

Clinical Presentation And Diagnosis Of Asthma

Cont

Chronic

Asthma….

Signs

Expiratory wheezing on auscultation, dry hacking cough, or signs of atopy (allergic rhinitis and/or eczema) may occur.

Laboratory

Spirometry demonstrates obstruction (reduced FEV 1 /FVC(forced vital capacity) with reversibility following inhaled

β

2 -agonist administration (at least a 12% improvement in FEV 1).

Clinical Presentation And Diagnosis Of Asthma

Cont

Chronic

Asthma…..

Other

Diagnostic Tests

A

fall in FEV 1 of at least 15% following 6 minutes of near maximal exercise.

Elevated eosinophil count and

IgE

concentration in blood.

Positive methacholine challenge (PC 20 FEV 1 less than 12.5 mg/mL) or mannitol challenge (FEV 1 decrease of at least 15% from baseline after 635 mg or less

).

Activity

: Small Group Discussion

What is the treatment of

Asthma ?

Pharmacological Treatment of Asthma

Acute Severe Asthma

The primary goal is prevention of life-threatening asthma by early recognition of signs of deterioration and early intervention.

The principal goals of treatment include:

Correction of significant

hypoxemia ( A low level of oxygen in the blood)

Rapid reversal of airflow obstruction

Reduction of the likelihood of relapse of the exacerbation or future recurrence of severe airflow obstruction

Treatment of asthma according to severity

Pharmacological Treatment of

Asthma Cont..

Chronic Asthma in Adults

The assessment of the frequency of daytime and nighttime symptoms and limitation of physical activity determines whether asthma is intermittent or persistent.

There are 4 categories.

Therapy is step-wise (Step 1–4) based on the category of asthma and consists of:

Preventing the inflammation leading to bronchospasm (controllers)

Relieving bronchospasm (relievers)

Controller medicines in asthma

Inhaled corticosteroids e.g. Beclomethasone

Reliever medicines in asthma

β2 agonists e.g. Salbutamol (short-acting)

Treatment

of Chronic Asthma According to

Severity

Monitoring Of Asthma Therapy

Lung function, either

spirometry

or peak flow measurements, should be monitored 5 to 10 minutes after each treatment.

Oxygen saturations can be easily monitored continuously with pulse oximetry.

For young children and infants, pulse oximetry, lung auscultation, and observation of the presence of supraclavicular retractions are useful.

The majority of patients will respond within the first hour of initial inhaled

β

2 -agonists regardless of history of home administration of drug.

Patients not achieving an initial response should be monitored every half hour to 1 hour.

Depending on whether there is a standard ED or a special unit for acute severe asthma, the decision to admit to the hospital should be made within 4 to 6 hours of entry to the emergency

department

Key Points

Asthma

is a common, chronic respiratory disease

of the airways of the lung characterized by either the intermittent or persistent presence of highly variable degrees of airflow obstruction from airway wall inflammation and bronchial smooth muscle constriction.

Symptoms of Asthma include

severe dyspnea, shortness of breath, chest tightness, or burning and wheezing sound

The principal goals of treatment of Asthma include correction of significant hypoxemia

and rapid reversal of airflow obstruction by using pharmacological and non pharmacological therapy

Evaluation

What

is Asthma?

What is the pathophysiology of

Asthma?

What are the signs and symptoms of Asthma?

How is the treatment of asthma?

References

Wells

BG,

DiPiro

J,

Schwinghammer

T (2013),

Pharmacotherapy Handbook

(6

th

Ed). New York, NY: McGraw-Hill.

DiPiro

JT, Talbert RL, Yee GC, Matzke GR, Wells BG, Posey ML, (2008):

Pharmacotherapy: A Pathophysiologic Approach

(7

th

ed

): New York, NY: McGraw-Hill.

Katz M D., Matthias KR., Chisholm-Burns M A., Pharmacotherapy(2011)

Principles & Practice Study Guide: A Case-Based Care Plan Approach

: New York, NY: McGraw-Hill.

Schwinghammer

TL, Koehler JM (2009)

Pharmacotherapy Casebook: A Patient-Focused Approach

(7

th

ed

): New York, NY: McGraw-Hill.

PST 06106

Basic Pharmacotherapy

Session 22: Pharmacotherapy of Diabetes Mellitus

Learning Objectives

By the end of this session students are expected to be able to:

Define diabetes mellitus

Explain pathophysiology of diabetes mellitus

Explain the clinical presentation of diabetes mellitus

Outline diagnosis of diabetes mellitus

Describe pharmacological treatment of diabetes mellitus

Describe the monitoring of diabetes mellitus therapy

Activity: Buzzing

What is Diabetes

Mellitus ?

Definition of Diabetes Mellitus

Diabetes mellitus (DM) is a group of metabolic disorders of fat, carbohydrate, and protein metabolism characterized by hyperglycemia

that results from defects in insulin secretion, insulin action (sensitivity), or both.

Or

Diabetes mellitus is a chronic disease caused by inherited and/or acquired deficiency in production of insulin by the pancreas, or by the ineffectiveness of the insulin produced which results in increased concentrations of glucose in the blood, which in turn damage many of the body's systems, in particular the blood vessels and nerves.

Definition of Diabetes Mellitus

Cont.…..

There are two types of DM

Type 1

diabetes (formerly known as insulin-dependent) in which the pancreas fails to produce the insulin which is essential for survival. This form develops most frequently in children and adolescents, but is being increasingly noted later in life.

Type 2

diabetes (formerly named non-insulin-dependent) which results from the body's inability to respond properly to the action of insulin produced by the pancreas.

Definition of Diabetes Mellitus Cont.…..

Type 2 diabetes is much more common and accounts for around 90% of all diabetes cases worldwide.

It occurs most frequently in adults, but is being noted increasingly in adolescents as well.

Certain genetic markers have been shown to increase the risk of developing Type 1 diabetes.

Type 2 diabetes is strongly familial, but it is only recently that some genes have been consistently associated with increased risk for Type 2 diabetes in certain populations.

Definition of Diabetes Mellitus Cont.…..

Both types of diabetes are complex diseases caused by mutations in more than one gene, as well as by environmental factors.

DM if not well managed can result into complications including;

Microvascular complications such as retinopathy, neuropathy, and nephropathy

Macrovascular

complications such as coronary heart disease, stroke, and peripheral vascular disease.

Definition of Diabetes Mellitus Cont.…..

Gestational Diabetes

It is a condition in which a woman without

diabetes

develops

high

blood sugar

levels

during

pregnancy

Diabetes in pregnancy may give rise to several adverse outcomes, including congenital malformations, increased birth weight and an elevated risk of perinatal mortality.

Strict metabolic control may reduce these risks to the level of those of non-diabetic expectant mothers

Pathophysiology Of Diabetes Mellitus

Type 1 DM

Type 1 DM is the result of a combination of genetic and environmental influences.

Type 1 DM is characterized by an absolute deficiency of pancreatic

β

-cell function.

Most often this is the result of an

immune mediated

destruction of pancreatic

β

cells, but rare unknown or idiopathic processes may contribute.

It most commonly results from autoimmune destruction of insulin-producing β-cells in the pancreas.

Pathophysiology Of Diabetes Mellitus Cont.….

One or more environmental factors, such as enteroviruses, dietary factors or toxins, might trigger the development of T-cell dependent autoimmunity in genetically susceptible individuals

Autoimmunity is manifested by detectable antibodies to ICA512/IA-2, insulin autoantibody (IAA) and glutamic acid decarboxylase (GAD).

Insulitis with gradual β-cell destruction leads to pre-diabetes and finally to overt DM.

Pathophysiology Of Diabetes Mellitus Cont.….

Type 2 DM

Type 2 diabetic individuals are characterized by

defects in insulin secretion; and

Insulin resistance involving muscle, liver, and the adipocyte.

Impaired insulin secretion

Impaired insulin secretion is a decrease in glucose responsiveness, which is observed before the clinical onset of disease.

More specifically, impaired glucose tolerance (IGT) is induced by a decrease in glucose-responsive early-phase insulin secretion, and a decrease in additional insulin secretion after meals causes postprandial

hyperglycaemia

Pathophysiology Of Diabetes Mellitus Cont.….

In the type 2 diabetic patient, decreased postprandial insulin secretion is due to both impaired pancreatic beta cell function and a reduced stimulus for insulin secretion from gut

hormones

Normally

there is an increased insulin secretion in response to an oral glucose stimulus and which is referred to as “the incretin effect”

The incretin effect is the result that gut-derived hormones (,glucagon-like peptide 1 (GLP-1) and glucose-dependent

insulinotropic

polypeptide (GIP)) when stimulated by glucose.

In type 2 diabetic patients, this “incretin effect” is very minimal

Pathophysiology Of Diabetes Mellitus Cont.….

The two gut hormones, glucagon-like peptide 1 (GLP-1) and glucose-dependent insulin tropic polypeptide (GIP), are responsible for over 90% of the increased insulin secretion seen in response to an oral glucose load.

Patients with type 2 diabetes remain sensitive to GLP-1 while they are often resistant to GIP.

Pathophysiology Of Diabetes Mellitus Cont.….

Insulin resistance

Insulin resistance is a condition in which insulin in the body does not exert sufficient action proportional to its blood concentration.

The impairment of insulin action in major target organs such as liver and muscles is a common pathophysiological feature of type 2 diabetes.

Insulin resistance develops and expands prior to disease onset.

Pathophysiology Of Diabetes Mellitus Cont.….

Insulin resistance is related to genetic factors and environmental factors (hyperglycaemia, free fatty acids, inflammatory mechanism, etc.).

Known genetic factors, such as change in the shape of insulin receptors that directly affect insulin signalling mechanisms is associated with visceral obesity and promote insulin resistance.

Glucolipotoxicity and inflammatory mediators are also important as the mechanisms for impaired insulin secretion and insulin signalling impairment

Clinical Presentation Of Diabetes Mellitus

The clinical presentations of type 1 DM and type 2 DM are very different.

Autoimmune type 1 DM can occur at any age.

Individuals with type 1 DM are often thin and are prone to develop diabetic ketoacidosis if insulin is withheld, or under conditions of severe

stress;-

P

olyuria,(Excessive urination)

P

olydipsia

,

(Excessive thirst)

P

olyphagia (Excessive eating)

Weight loss.

Blurred vision

Slow-healing sores

Frequent infections

Clinical Presentation Of Diabetes Mellitus

Signs And Symptoms Of Type 2

Diabetes

Patients

with type 2 DM often present without symptoms,

Even though complications tell us that they may have been hyperglycemic

For several years.

Often these patients are diagnosed secondary to unrelated blood testing.

Lethargy,

polyuria,

nocturnal,

and

polydipsia

Blurred vision

Slow-healing sores

Frequent infections

Patients can have normal to grossly abnormal insulin

sensitivity.

Clinical Presentation of DM

Diagnosis Of Diabetes Mellitus

DM is diagnosed by both

clinical using

signs and symptoms together with blood tests

The following are blood test for diagnosis of

DM

Glycated hemoglobin (A1C) test.

This blood test, which doesn't require fasting, indicates your average blood sugar level for the past two to three months.

It measures the percentage of blood sugar attached to hemoglobin, the oxygen-carrying protein in red blood cells.

An A1C level of 6.5 percent or higher on two separate tests indicates DM.

An A1C between 5.7 and 6.4 percent indicates prediabetes.

Below 5.7 is considered normal

.

Diagnosis Of Diabetes

Mellitus

Cont

….

Random blood glucose test.

A blood sample will be taken at a random time.

Normal blood glucose is 11

millimoles

/L

Reading of 11.1

millimoles

per liter (

mmol

/L) — or higher suggests diabetes

.

Fasting blood glucose test.

A blood sample will be taken after an overnight fast.

A fasting blood glucose level less than 5.6

mmol

/L is normal.

A fasting blood glucose level from 5.6 to 6.9

mmol

/L is considered prediabetes.

A fasting blood glucose of 7

mmol

/L) or higher on two separate tests, you have diabetes.

Diagnosis Of Diabetes

Mellitus

Cont

….

Oral glucose tolerance test.

For this test, fasting blood glucose level is measured after overnight fast.

Then a patient drink sugary liquid and blood glucose levels are measured periodically for the next two hours.

A blood sugar level less

than

7.8

mmol

/L is normal.

More than 11.1

mmol

/L after two hours indicates diabetes.

A reading between 7.8

mmol

/L and 11.0

mmol

/L indicates prediabetes

.

Urinalysis

If type

1 diabetes

is suspected, Urinalysis will be done to investigate for the presence of ketones bodies

Diagnostic criteria for DM

Activity

: Small Group Discussion

What

is the treatment of Diabetes

Mellitus

?

Pharmacological Treatment Of Diabetes Mellitus

The primary goals of DM management are to;

reduce the risk for microvascular and macrovascular disease complications,

ameliorate symptoms,

reduce mortality,

Improve quality of life.

Near-normal

glycaemia

will reduce the risk for development of microvascular disease complications,

Pharmacological Treatment Of Diabetes

Mellitus

Cont

Aggressive management of traditional cardiovascular risk factors (i.e., smoking cessation, treatment of dyslipidemia, intensive blood pressure control, and antiplatelet therapy) are needed to reduce the likelihood of development of

macrovascular

disease.

Pharmacological treatment of DM depends on the type and the severity of the disease

Insulin are the mainstay for treatment of type 1 DM

Pharmacological Treatment Of Diabetes Mellitus

Cont

Treatment of Type 2

DM

Oral

Antihyperglycemic Drugs

Biguanide

:

Metformin

Metformin is considered the agent of first line for treatment of T2DM, in the absence of contraindications

It decreases fasting blood glucose by approximately 20% and HbA1c by 1.5%.

Pharmacological Treatment Of Diabetes Mellitus

Cont

Treatment of Type 2 DM

Oral Antihyperglycemic

Drugs…..

It

can be given in combination with sulfonylureas,

Glinides

, alpha-glucosidase inhibitors, insulin, thiazolidinedione (TZD), glucagon-like peptide-1 receptor agonist (RA-GLP1), dipeptidyl peptidase 4 inhibitors (iDPP4), and sodium-glucose co-transporter 2 inhibitors (iSGLT2).

Metformin

is contraindicated in patients with factors that predispose to lactic acidosis.

The predisposing factors are: A renal function damaged, concomitant liver disease or excessive alcohol intake, unstable or acute heart failure and personal history of lactic

acidosis

Pharmacological Treatment Of Diabetes Mellitus

Cont

Antihyperglycemic

drugs

Pharmacological Treatment Of Diabetes Mellitus

Cont

Antihyperglycemic drugs

Pharmacological Treatment Of Diabetes Mellitus

Cont

Antihyperglycemic drugs

Pharmacological Treatment Of Diabetes Mellitus

Cont

Antihyperglycemic drugs

Monitoring of Diabetes Mellitus Therapy

A comprehensive pharmaceutical care plan for the patient with DM is needed in order to reach treatment goals

Parameters

to monitor include

Glycemic control (tested minimally yearly; HbA

lc

<8% is good control and

HbA

lc

>9% is poor control),

Minimally, HbA

lc

should be measured twice a year in patients meeting treatment goals on a stable therapeutic regimen.

Quarterly assessments are recommended for those whose therapy has changed or who are not meeting glycemic goals.

Glycemic control requires frequent assessment and adjustment in diet, exercise, and pharmacologic

therapies

Monitoring of Diabetes Mellitus

Therapy Cont.….

L

ipid (percentage of patients with LDL <100 mg/

dL

)

Fasting lipid profiles should be obtained as part of an initial assessment and thereafter at each

Follow-up visit, annually, or every 2 years if the lipid profile suggests low risk.

Documenting

regular frequency of foot exams (each visit), urine albumin assessment

(annually), dilated ophthalmologic exams (yearly or more frequently with identified abnormalities), and office visits for follow-up are also important.

Management of other cardiovascular risks (e.g., smoking and antiplatelet therapy) are components of preventive medicine strategies

Key

Points

Diabetes

mellitus (DM) is a group of metabolic disorders of fat, carbohydrate, and protein metabolism

characterized by hyperglycemia

that results from defects in insulin secretion, insulin action (sensitivity), or both

Symptoms of Diabetes Mellitus are variable and depends on the type of the disease

wheather

is type 1 or 2 DM.

Insulin is the mainstay pharmacological treatment for type 1 DM while Metformin is first line pharmacological treatment for type 2 DM obese patient

Evaluation

What

is Diabetes Mellitus?

What is the pathophysiology of Diabetes Mellitus?

What are the signs and symptoms of Diabetes Mellitus?

How is the treatment of Diabetes Mellitus?

References

Wells

BG,

DiPiro

J,

Schwinghammer

T (2013),

Pharmacotherapy Handbook

(6

th

Ed). New York, NY: McGraw-Hill.

DiPiro

JT, Talbert RL, Yee GC, Matzke GR, Wells BG, Posey ML, (2008):

Pharmacotherapy: A Pathophysiologic Approach

(7

th

ed

): New York, NY: McGraw-Hill.

Katz M D., Matthias KR., Chisholm-Burns M A., Pharmacotherapy(2011)

Principles & Practice Study Guide: A Case-Based Care Plan Approach

: New York, NY: McGraw-Hill.

Schwinghammer

TL, Koehler JM (2009)

Pharmacotherapy Casebook: A Patient-Focused Approach

(7

th

ed

): New York, NY: McGraw-Hill.

PST 06106

Basic Pharmacotherapy

Session 23: Pharmacotherapy of Peptic Ulcers Disease

Learning Objective

By the end of this session students are expected to be able to:

Define peptic ulcers disease

Explain pathophysiology of peptic ulcers disease

Explain the clinical presentation of peptic ulcers disease

Outline diagnosis of peptic ulcers disease

Describe pharmacological treatment of peptic ulcers disease

Describe the monitoring of peptic ulcers disease

therapy

Activity: Buzzing

What is Peptic ulcer Disease?

Definition of Peptic Ulcers Disease

Peptic

ulcer disease refers to painful sores or ulcers in the lining of the stomach or first part of the small intestine, called the duodenum.

Peptic ulcer disease (PUD), also known as a peptic ulcer or stomach ulcer, is a break in the lining of the stomach, first part of the small intestine, or occasionally the lower

oesophagus

An ulcer in the stomach is known as a

gastric ulcer

while that in the first part of the intestines is known as a

duodenal ulcer

.

Most ulcers are caused by an infection with a type of bacteria called

Helicobacter pylori

(H. pylori).

Definition of Peptic Ulcers

Disease Cont..

Factors that can increase your risk for ulcers include:

Use of nonsteroidal anti-inflammatory drugs (NSAIDs), such as;

Aspirin, even safety-coated aspirin and aspirin in powered form can frequently cause ulcers.

naproxen,

ibuprofen

Definition of Peptic Ulcers Disease Cont..

Many other prescription drugs such;

Concomitant use of oral bisphosphonates (e.g., alendronate)

Concomitant use of corticosteroids

Concomitant use of anticoagulant or coagulopathy

Concomitant use of antiplatelet drugs (e.g.,

clopidogrel

)

Concomitant use of selective serotonin reuptake inhibitor

Definition of Peptic Ulcers Disease Cont..

Excess

acid production from

Zollinger

-Ellison syndrome, (ZES)

gastrinomas

,

tumors

of the acid producing cells of the stomach that increases acid output

Excessive drinking of alcohol

Smoking or chewing tobacco

Peptic ulcers are also associated with radiation, chemotherapy, vascular insufficiency, and other chronic

diseases

Pathophysiology of Peptic Ulcers Disease

A physiologic imbalance between aggressive (gastric acid and pepsin) and protective factors (mucosal defense and repair) remain important issues in the pathophysiology of gastric and

duodenal ulcers.

Gastric acid is secreted by the parietal cells, which contain receptors for histamine, gastrin, and acetylcholine.

Acid (as well as

H. pylori

infection and NSAID use) is an independent factor that contributes to the disruption of mucosal integrity.

Increased acid secretion has been observed for patients with duodenal with Zollinger-Ellison syndrome (ZES) (described in the

section

Pathophysiology of Peptic Ulcers

Disease Cont..

Zollinger-Ellison Syndrome) have profound gastric acid hypersecretion resulting from a gastrin-producing tumor

H. pylori

produce large amounts of urease, which hydrolyzes urea in the gastric juice and converts it to ammonia and carbon dioxide.

The local buffering effect of ammonia creates a neutral microenvironment within and surrounding the bacterium, which protects it from the lethal effect of gastric acid

.

H. pylori

also produces acid inhibitory proteins, which allows it to adapt to the low-pH environment of the stomach

Pathophysiology of Peptic Ulcers Disease Cont..

Mucosal

injury is produced by

elaborating bacterial enzymes (urease, lipases, and proteases),

Lipases and proteases degrade gastric mucus, ammonia produced by urease may be toxic to gastric epithelial cells,

Adherence

bacterial adherence enhances the uptake of toxins into gastric epithelial cells

H. pylori virulence factors.

H. pylori

induces gastric inflammation by altering the host inflammatory response and damaging epithelial cells directly by cell-mediated immune mechanisms or indirectly by activated neutrophils or macrophages attempting to phagocytose bacteria or bacterial products

Clinical presentation and Diagnosis of Peptic ulcers disease

The clinical presentation of PUD varies depending on the severity of epigastric pain and the presence of complications

Ulcer-related pain in duodenal ulcer often occurs 1 to 3 hours after meals and is usually relieved by food, but this is

variable

General

Mild epigastric pain or acute life-threatening upper gastrointestinal

complications

Clinical presentation and Diagnosis of Peptic ulcers

disease

Cont

….

Symptoms

Abdominal

pain that is often epigastric and described as burning but may present as vague discomfort, abdominal fullness, or cramping

A typical nocturnal pain that awakens the patient from sleep (especially between 12 AM and 3 AM)

The severity of ulcer pain varies from patient to patient and may be seasonal,

episodes of discomfort usually occur in clusters, lasting up to a few weeks and followed by a pain-free period or remission lasting from weeks to years

Clinical presentation and Diagnosis of Peptic ulcers disease

Cont

….

Symptoms…..

Changes

in the character of the pain may suggest the presence of complications

Heartburn, belching, and bloating often accompany the pain

Nausea, vomiting, and anorexia are more common for patients with gastric ulcer than with duodenal ulcer but may also be signs of an ulcer-related complication

Clinical presentation and Diagnosis of Peptic ulcers disease

Cont

….

Signs

Weight loss associated with nausea, vomiting, and anorexia

Complications including ulcer bleeding, perforation, penetration, or

obstruction

Laboratory tests

Gastric acid secretory studies

The

hematocrit

and

hemoglobin

are low with bleeding, and stool

hemoccult

tests are positive.

Tests for

Helicobacter pylori

.

Clinical presentation and Diagnosis of Peptic ulcers disease

Cont

….

Diagnostic tests

Fiberoptic

upper endoscopy (esophagogastroduodenoscopy) detects more than 90% of peptic ulcers and permits direct inspection, biopsy, visualization of superficial erosions, and sites of active bleeding.

Upper gastrointestinal radiography with barium and upper endoscopy are also the diagnostic procedures for suspected peptic ulcer.

Tests for Detection of Helicobacter

Pyroli

Activity

: Small Group Discussion

What is the treatment of Peptic Ulcers Disease

?

Pharmacological Treatment of Peptic Disease

The treatment of chronic PUD varies depending on the etiology of the ulcer (

H. pylori

or NSAID), whether the ulcer is initial or recurrent, and whether complications have occurred

Overall treatment is aimed at relieving ulcer pain, healing the ulcer, preventing ulcer recurrence, and reducing ulcer-related complications.

The goal of therapy for

H. pylori

positive patients with an active ulcer, a previously documented ulcer, or a history of an ulcer-related complication, is to eradicate

H. pylori,

heal the ulcer, and cure the disease.

Successful eradication heals ulcers and reduces the risk of recurrence for most patients

.

Drug Regimens Used to Eradicate Helicobacter pylori

Pharmacological Treatment of Peptic

Disease Cont..

Other options for Triple therapy for eradication of the H. pylori include;

Omeprazole (PO) 20mg twice daily Plus

Amoxycillin

(PO) 1000mg twice daily

AND

Metronidazole

(PO) 400mg twice daily for 10–14 days

OR

Lansoprazole (PO) 30mg twice daily

AND

Clarithromycin

(PO) 500mg twice

AND

Tinidazole (PO) 500mg twice daily for 10–14 days

OR

Any combination of PPI + 2 antibiotics active for

H. pylori

Other

drugs as indicated in the table below can also be used in the treatment of peptic ulcer

disease

Oral Drug Regimen Used To Heal Peptic Ulcer And Maintain Ulcer Healing

Monitoring of Peptic Ulcers Disease Therapy

Treatment of

Helicobacter pylori

-associated ulcer

Assess patient allergies to determine if allergic to penicillin (or other antibiotics) so that drug regimens that contain penicillin (or other antibiotics) can be avoided.

Assess patient use of alcohol or alcohol-containing products with metronidazole and oral birth control medications with antibiotics and counsel appropriately.

Assess likelihood of nonadherence to the drug regimen as a cause of treatment failure.

Recommend a different antibiotic combination if

H . pylori

eradication fails

.

Monitoring of Peptic Ulcers Disease

Therapy Cont.…

Inform the patient of change in stool color when bismuth salicylate is included in an

H. pylori

eradication regimen.

Assess and monitor patients for potential adverse effects, especially those associated with metronidazole, clarithromycin, and amoxicillin.

Assess and monitor patients for potential drug interactions, especially those receiving metronidazole, clarithromycin, or cimetidine.

Monitor patients for persistent or recurrent symptoms within 14 days after completion of a course of

H. pylori

eradication therapy.

Monitoring of Peptic Ulcers Disease

Therapy Cont.….

Provide

patient education to patients who are receiving

H . pylori

eradication therapy and include why antibiotic and antiulcer combinations are used;

when and how to take medications;

adverse effects;

alarm symptoms;

the importance of adherence to the entire course of drug treatment; and

Contact their healthcare provider if alarm symptoms develop (e.g., blood in the stools, black tarry stools, vomiting, severe abdominal pain), or if symptoms persist or return after H. pylori eradication

.

Monitoring of Peptic Ulcers Disease Therapy

Treatment of NSAIDS induced ulcers

Monitor

patients for signs and symptoms of NSAID-related upper GI complications.

Assess and monitor patients for potential drug interactions and adverse effects (especially misoprostol).

Provide patient education to patients who are at risk of NSAID-induced ulcers or GI-related complications and include why

co-therapy

is used with nonselective NSAIDs;

when and how to take medications;

adverse effects;

alarm symptoms;

when to contact their healthcare provider; and

The importance of adherence to drug treatment

.

Key

Points

Peptic

ulcer disease refers to painful sores or ulcers in the lining of the stomach or first part of the small intestine, called the duodenum

A physiologic imbalance between aggressive (gastric acid and pepsin) and protective factors (mucosal defense and repair) and

H. pylori

infection remain important issues in the pathophysiology of gastric and duodenal ulcers.

Symptoms of PUD include abdominal pain that is often epigastric and described as burning but may present as vague discomfort, abdominal fullness, or cramping

The treatment of chronic PUD varies depending on the etiology of the ulcer (

H. pylori

or NSAID), whether the ulcer is initial or recurrent, and whether complications have occurred

Evaluation

What

is Peptic Ulcers Disease?

What is the pathophysiology of

Peptic Ulcers Disease

?

What are the signs and symptoms of Peptic Ulcers Disease?

How is the treatment of Peptic Ulcers Disease?

References

Wells

BG,

DiPiro

J,

Schwinghammer

T (2013),

Pharmacotherapy Handbook

(6

th

Ed). New York, NY: McGraw-Hill.

DiPiro

JT, Talbert RL, Yee GC, Matzke GR, Wells BG, Posey ML, (2008):

Pharmacotherapy: A Pathophysiologic Approach

(7

th

ed

): New York, NY: McGraw-Hill.

Katz M D.,

Matthias KR.,

Chisholm-Burns M A.,

Pharmacotherapy(2011)

Principles & Practice Study Guide: A Case-Based Care Plan Approach

:

New York, NY: McGraw-Hill.

Schwinghammer

TL, Koehler JM (2009)

Pharmacotherapy Casebook: A Patient-Focused Approach

(7

th

ed

): New York, NY: McGraw-Hill.

PST 06106

Basic Pharmacotherapy

Session 24: Pharmacotherapy of Hypertension

Learning Objective

By the end of this session students are expected to be able to:

Define hypertension

Explain pathophysiology of hypertension

Explain the clinical presentation of hypertension

Outline diagnosis of hypertension

Describe pharmacological treatment of hypertension

Describe the monitoring of hypertension therapy

Activity: Buzzing

What is

Hypertension

?

Definition of Hypertension

Hypertension is defined as a systolic blood pressure (SBP) of higher than 140mmHg or a diastolic blood pressure (DPB) higher than 90mmHg

The classification of BP is as been follows

:

Normal: Systolic lower than 120 mm Hg, diastolic lower than 80 mm Hg

Prehypertension: Systolic 120-139 mm Hg, diastolic 80-89 mm Hg

Stage 1: Systolic 140-159 mm Hg, diastolic 90-99 mm Hg

Stage 2: Systolic 160 mm

Hg or greater, diastolic 100 mm Hg or

greater

Definition of Hypertension

Cont.…..

Hypertension may be;

Primary, which may develop as a result of environmental or genetic causes, or

Secondary, which has multiple etiologies, including renal, vascular, and endocrine causes.

Primary or essential hypertension accounts for 90-95% of adult cases, and secondary hypertension accounts for 2-10% of cases.

Pathophysiology

of Hypertension

Multiple factors that control BP are potential contributing components in the development of essential hypertension.

These include;

Malfunctions in either humoral [i.e., the renin-angiotensin- aldosterone system (RAAS)] or vasodepressor mechanisms,

Abnormal neuronal mechanisms,

Defects in peripheral autoregulation, and

Disturbances in sodium, calcium, and natriuretic hormone.

Pathophysiology of Hypertension

Cont

Many of these factors are cumulatively affected by the multifaceted RAAS, which ultimately regulates arterial BP.

It is probable that no one factor is solely responsible for essential hypertension

.

Clinical

Presentation and Diagnosis of Hypertension

General:

The patient may appear healthy or may have the presence of additional CV risk factors:

Age (greater than or equal to 55 for men, greater than or equal to 65 for women)

Diabetes mellitus

Dyslipidemia

(elevated cholesterol or fats in the blood)

Microalbuminuria

Family history of premature CV disease

Obesity (body mass index greater than or equal to 30 kg/m2)

Physical inactivity

Tobacco

use

Clinical Presentation and Diagnosis of Hypertension

Cont

….

Symptoms:

Usually none related to elevated BP.

Signs:

Previous BP values in either the prehypertension or the hypertension category.

Laboratory Tests:

BUN/serum creatinine,

fasting lipid panel,

fasting blood glucose

,

Clinical Presentation and Diagnosis of Hypertension

Cont

….

Laboratory Tests….

serum

electrolytes (sodium, potassium),

Spot urine albumin-to-creatinine ratio.

The patient may have normal values and still have hypertension.

However, some may have abnormal values that are consistent with either additional CV risk factors or hypertension-related damage.

Other Diagnostic Tests:

12-lead electrocardiogram,

Estimated glomerular filtration rate [using modification of diet in renal disease (MDRD) equation].

Clinical Presentation and Diagnosis of Hypertension

Cont

….

Hypertension-Related

Target-Organ Damage:

The patient may have a previous medical history or diagnostic findings that indicate

the presence of hypertension-related target-organ damage:

Brain (stroke, transient ischemic attack, dementia)

Eyes (retinopathy)

Heart (left ventricular hypertrophy, angina, prior MI, prior coronary revascularization, heart failure)

Kidney (chronic kidney disease)

Peripheral vasculature (peripheral arterial disease)

Activity

: Small Group Discussion

What is the treatment of

Hypertension

?

Pharmacological Treatment Of Hypertension

The overall goal of treating hypertension is to reduce hypertension- associated morbidity and mortality.

This morbidity and mortality is related to hypertension-associated target-organ damage (e.g

. CV

events, cerebrovascular events, heart failure, and kidney disease).

Reducing CV risk remains the primary purpose of hypertension therapy and the specific choice of drug therapy is significantly influenced by evidence demonstrating such CV risk reduction.

Treating patients with hypertension to achieve a desired target BP value is simply a surrogate goal of therapy

Pharmacological Treatment Of

Hypertension

Cont

….

In most cases the target BP should be: systolic below 140 mmHg and diastolic below 90 mmHg.

In diabetic patients and patients with cardiac or renal impairment, target BP should be below 130/80mmHg;

The

choice of initial drug therapy depends on the degree of BP elevation and presence of compelling indications (

e.g

coexisting conditions such as diabetes and other cardiovascular conditions)

Most patients with stage 1 hypertension should be initially treated with a first-line antihypertensive drug, or the combination of two agents.

Combination drug therapy is recommended for patients with more severe BP elevation (stage 2 hypertension), using preferably two first-line antihypertensive drugs

.

Pharmacological Treatment Of Hypertension

Cont

….

Recommended Initial Medication Doses For Hypertension Treatment

Thiazide

diuretics

Hydrochlothiazide

12.5mg/daily

OR

Bendroflumethiazide

5mg/daily

OR

Indapamide

5mg/daily preferred for patient with previous stroke/TIA

Pharmacological Treatment Of Hypertension

Cont

….

Recommended Initial Medication Doses For Hypertension

Treatment…..

Loop

diuretics

Furosemide initial dose 40mg twice a day

OR

Torsemide

5mg/daily

Dose can be up scaled depending on congestive status to maximum dose

Pharmacological Treatment Of Hypertension

Cont

….

Recommended Initial Medication Doses For Hypertension

Treatment……

Mineralocorticoid

(Aldosterone) Receptor antagonist

Spironolactone 25mg/daily

OR

Eplerenone

25mg/daily

Angiotensin-Converting Enzyme Inhibitor (ACEI)

Captopril 6.125mg, 12.5mg or 25mg three times daily

OR

Enalapril

10mg twice a day

OR

Perindopril 8mg/daily orally

Pharmacological Treatment Of Hypertension

Cont

….

Angiotensin Receptor Blocker–ARB

(*Don’t combine with ACEI contraindications, indicated in patient sensitive to ACEIs)

Losartan 50mg/daily*

Beta–blocker

Atenolol 50mg/daily

OR

Metoprolol 50mg/daily

Pharmacological Treatment Of Hypertension

Cont

….

Calcium

Channel Blocker (

Dihydropyridines

):

Nifedipine

(Slow Release/Long Acting) 20mg/30mg/ 60mg/90mg/daily

OR

Amlodipine 5mg or 10mg/daily

Non–

dihydropyridine

Verapamil 30mg twice–three times a daily

OR

Diltiazem 30mg twice–three times a day

Monitoring of Hypertension Therapy

Routine ongoing monitoring to assess disease progression, the desired effects of antihypertensive

therapy

The

monitoring parameters include;

Signs

and symptoms of Disease Progression

Efficacy

of

antihypertensive

and BP goal attainment, and

Undesired

adverse side effects (toxicity)

Monitoring of Hypertension

Therapy

Cont

Disease Progression

Patients should be monitored for signs and symptoms of progressive hypertension-associated target-organ disease.

A careful history for ischemic chest pain (or pressure), palpitations, dizziness, dyspnea, orthopnea, headache, sudden change in vision, one-sided weakness, slurred speech, and loss of balance should be taken to assess the presence of CV and cerebrovascular hypertensive complications

Monitoring of Hypertension

Therapy

Cont

E

fficacy

The most important strategy to prevent CV morbidity and mortality in hypertension is BP control to goal values

Clinic-based BP monitoring remains the standard for managing hypertension.

BP response should be evaluated 2 to 4 weeks after initiating or making changes in therapy.

Once goal BP values are attained, assuming no signs or symptoms of acute target-organ

disease are present, BP monitoring can be done every 3 to 6 months.

More frequent evaluations are required for patients with a history of poor control, nonadherence, progressive target-organ damage, or symptoms of adverse drug effects.

Self-measurements of BP or automated ambulatory BP monitoring can be useful clinically to establish effective 24-hour

control

Monitoring of Hypertension

Therapy

Cont

Toxicity

Patients should be monitored routinely for symptoms of adverse drug reactions.

Laboratory monitoring should typically occur 2 to 4 weeks after starting a new agent or dose increase, and then every 6 to 12 months in stable patients.

Key

Points

Hypertension

is defined as a systolic blood pressure (SBP) of higher than 140mmHg or a diastolic blood pressure (DPB) higher than 90mmHg

The overall goal of treating hypertension is to reduce hypertension- associated morbidity and mortality.

This morbidity and mortality is related to hypertension-associated target-organ damage

The choice of initial drug therapy depends on the degree of BP elevation and presence of compelling indications (

e.g

coexisting conditions such as diabetes and other cardiovascular conditions)

Evaluation

What

is Hypertension?

What is the pathophysiology of

Hypertension?

What are the signs and symptoms of Hypertension?

How is the treatment of Hypertension?

References

Wells

BG,

DiPiro

J,

Schwinghammer

T (2013),

Pharmacotherapy Handbook

(6

th

Ed). New York, NY: McGraw-Hill.

DiPiro

JT, Talbert RL, Yee GC, Matzke GR, Wells BG, Posey ML, (2008):

Pharmacotherapy: A Pathophysiologic Approach

(7

th

ed

): New York, NY: McGraw-Hill.

Katz M D.,

Matthias KR.,

Chisholm-Burns M A.,

Pharmacotherapy(2011)

Principles & Practice Study Guide: A Case-Based Care Plan Approach

:

New York, NY: McGraw-Hill.

Schwinghammer

TL, Koehler JM (2009)

Pharmacotherapy Casebook: A Patient-Focused Approach

(7

th

ed

): New York, NY: McGraw-Hill.

PST 06106

Basic Pharmacotherapy

Session 25: Pharmacotherapy of Heart Failure

Learning Objectives

By the end of this session students are expected to be able to:

Define heart failure

Explain pathophysiology of heart failure

Explain the clinical presentation of heart failure

Outline diagnosis of heart failure

Describe pharmacological treatment of heart failure

Describe the monitoring of heart failure therapy

Activity: Buzzing

What is Heart Failure?

Definition of Heart Failure

Heart failure is a progressive clinical syndrome that can result from any abnormality in cardiac structure or function that impairs the ability of the ventricle to fill with or eject blood, thus rendering the heart unable to pump blood at a rate sufficient to meet the metabolic demands of the body.

It is the final common pathway for numerous cardiac disorders, including those affecting the pericardium, heart valves, and myocardium.

Diseases that adversely affect ventricular diastole (filling), ventricular systol(Contraction), or both can lead to heart failure

Heart Failure is characterized by typical symptoms (e.g. breathlessness, ankle swelling and fatigue) that may be accompanied by signs (e.g. elevated jugular venous pressure, pulmonary crackles and peripheral oedema) caused by a structural and/or functional cardiac abnormality, resulting in a reduced cardiac output and/or elevated intracardiac pressures at rest or during stress

Definition of Heart Failure Cont…

Heart Failure is characterized by typical symptoms (e.g. breathlessness, ankle swelling and fatigue) that may be accompanied by signs (e.g. elevated jugular venous pressure, pulmonary crackles and peripheral oedema) caused by a structural and/or functional cardiac abnormality, resulting in a reduced cardiac output and/or elevated intracardiac pressures at rest or during stress

Heart failure can result from any disorder that affects the ability of the heart to contract (systolic function) and/or relax (diastolic dysfunction)

Therefore, Heart Failure can be;

Systolic Heart Failure or/and

Diastolic Heart Failure

Definition of Heart Failure Cont…

Heart failure with impaired systolic function (i.e., reduced LVEF) is the classic, more familiar form of the disorder

LVEF (Left ventricular ejection fraction

Common Cause Of Heart Failure

Pathophysiology of Heart Failure

Key components of the pathophysiology of cardiac remodeling are.

Myocardial injury (e.g., myocardial infarction) results in the activation of a number of hemodynamic and neurohormonal compensatory responses in an attempt to maintain circulatory homeostasis.

Chronic activation of the neurohormonal systems results in a cascade of events that affect the myocardium at the molecular and cellular levels.

These events lead to the changes in ventricular size, shape, structure, and function known as ventricular remodeling.

The alterations in ventricular function result in further deterioration in cardiac systolic and diastolic function, which further promotes the remodeling process. (LV left ventricular)

Pathophysiology of Heart Failure Cont….

Clinical presentation and diagnosis of HF

General

Patient presentation may range from asymptomatic to cardiogenic shock.

Symptoms

Dyspnea, (Shortness of breath)

Orthopnea (Discomfort when breathed)

Paroxysmal nocturnal dyspnea (an attack of severe shortness of breath and coughing that generally occur at night)

Exercise intolerance

Tachypnea (Fast breathing)

Clinical presentation and diagnosis of HF Cont…..

Symptoms…..

Cough

Fatigue (feeling overtired)

Nocturia (Frequent urination)

Hemoptysis (Coughing up blood)

Abdominal pain

Anorexia

Nausea

Bloating (Build up of gas in the stomach and intestine)

Poor appetite, early satiety

Ascites (Abnominal swelling)

Mental status changes

Clinical presentation and diagnosis of HF Cont…..

Signs

Pulmonary rales (Abnormal lung sound)

Pulmonary edema

Cool extremities

Pleural effusion (build up of fluids between the tissue that line the lungs and the chest)

Tachycardia (Fast heart rate)

Narrow pulse pressure

Clinical presentation and diagnosis of HF Cont…..

Signs…….

Cardiomegaly

Peripheral edema

Hepatojugular reflux (test for measuring jugular venous pressure through the distention of the internal jugular vein)

Hepatomegaly

Clinical presentation and diagnosis of HF Cont…..

Laboratory Tests

Electrocardiogram may be normal, or it could show numerous abnormalities, including acute ST-T wave changes from myocardial ischemia, atrial fibrillation, bradycardia, and left ventricular hypertrophy.

Serum creatinine may be increased due to hypo perfusion.

Preexisting renal dysfunction can contribute to volume overload.

Complete blood count (CBC) can be useful in determining if heart failure is due to a reduced oxygen-carrying capacity.

Clinical presentation and diagnosis of HF Cont…..

Laboratory Tests

Chest x-ray: useful for detecting cardiac enlargement, pulmonary edema, and pleural effusions

Echocardiogram: used to assess the size of the left ventricle, valve function, pericardial effusion, wall motion abnormalities, and ejection fraction

Hyponatremia: serum sodium <130 mEq/L is associated with reduced survival and may indicate worsening volume overload and/or disease progression

Activity: Small Group Discussion

What is the treatment of Heart Failure??

Pharmacological Treatment of Heart Failure

Treatment of Heart Failure of depends on the stage of the Disease

There are four identified stages of heart failure, and their treatment recommendations

Unless contraindicated, all patients with HF-REF(reduced ejection fraction) should be started on an ACE inhibitor and a beta blocker (and a diuretic, in most cases).

No patient should receive three drugs which block the renin-angiotensin-aldosterone system as hyperkalaemia and renal dysfunction will be common.

The safety and efficacy of combining an ACE inhibitor, an ARB and MRA is uncertain and the use of these three drugs together is not recommended

Functional Classification of Heart Failure

Treatment allogarism of Heart failure according to functional stage of Heart Failure

Pharmacological Treatment of Heart Failure Cont….

Beta Blockers

A meta-analysis confirms that beta blockers also reduce mortality in patients with diabetes and HF

All patients with heart failure with reduced ejection fraction,class II-IV, should be started on beta blocker therapy as soon as their condition is stable.

Bisoprolol, carvedilol or nebivolol should be the first choice of beta blocker for the treatment of patients with heart failure with reduced ejection fraction.

If beta blockers are contraindicated consider using ivabradine

Pharmacological Treatment of Heart Failure Cont….

Angiotensin-Converting Enzyme Inhibitors

Patients with heart failure with reduced ejection fraction of all NYHA functional classes, should be given angiotensin-converting enzyme inhibitors.

Important adverse effects are cough, hypotension, renal impairment and hyperkalaemia.

A key but rare adverse effect, which can be life threatening (due to laryngeal involvement), is angioedema.

Any patient who experiences angioedema should have the ACE inhibitor withdrawn immediately and be prescribed an alternative agent.

Pharmacological Treatment of Heart Failure Cont.

….

Angiotensin Receptor Blockers

Angiotensin II type 1 receptor blockers (ARBs) block the biological effect of angiotensin II.

Unlike ACE inhibitors they do not produce cough as a side effect and should be used in patients who cannot tolerate an ACE inhibitor due to cough.

Patients with heart failure with reduced ejection fraction, NYHA class II-IV, who are intolerant of angiotensin-converting enzyme inhibitors should be given an angiotensin receptor blocker.

An angiotensin receptor blocker in addition to an angiotensin-converting enzyme inhibitor should be considered in patients with heart failure with reduced ejection fraction NYHA class II-IV, who are unable to tolerate a mineralocorticoid receptor antagonist.

Pharmacological Treatment of Heart Failure Cont.….

Mineralocorticoid Receptor Antagonists

Patients with heart failure with reduced ejection fraction who have ongoing symptoms of heart failure, NYHA class II-IV, LVEF ≤35%, despite optimal treatment, should be given mineralocorticoid receptor anatgonists unless contraindicated by the presence of renal impairment (chronic kidney disease stage ≥4–5) and/or elevated serum potassium concentration (K+ >5.0 mmol/l).

Eplerenone can be substituted for spironolactone in patients who develop gynaecomastia.

Pharmacological Treatment of Heart Failure Cont.….

Angiotensin Receptor/Neprilysin Inhibitors

Patients with heart failure with reduced ejection fraction who have ongoing symptoms of heart failure, NYHA class II-III, LVEF ≤40% despite optimal treatment should be given sacubitril/valsartan instead of their ACE inhibitor or ARB, unless contraindicated.

It may be considered in patients with NYHA class IV symptoms.

If the patient is already on an ACE inhibitor, the ACE inhibitor should be stopped for 36 hours before initiating sacubitril/valsartan to minimise the risk of angioedema.

Patients should be seen by a heart failure specialist with access to a multidisciplinary heart failure team before starting treatment with sacubitril/valsartan

Pharmacological Treatment of Heart Failure Cont.….

Diuretics/ Loop Diuretics

In the majority of patients with heart failure fluid retention occurs, causing ankle oedema, pulmonary oedema or both, contributing to the symptom of dyspnoea.

Diuretic treatment relieves oedema and dyspnoea.

Patients with heart failure and clinical signs or symptoms of fluid overload or congestion should be considered for diuretic therapy.

The tendency of loop diuretics to cause hypokalaemia is offset by ACE inhibitors, ARBs and spironolactone.

Pharmacological Treatment of Heart Failure Cont.….

Diuretics/ Loop Diuretics …

Care should be taken to select the dose of the loop diuretic on an individual basis, so that the dose chosen or reached should eliminate ankle or pulmonary oedema without dehydrating the patient and placing them at risk of renal dysfunction or hypotension.

Serum potassium should be monitored to maintain its concentration in the range 4–5 mmol/l and adjustments in therapy should be made to prevent both hypokalaemia and hyperkalaemia.

The dose of diuretic should be individualised to reduce fluid retention without overtreating which may cause dehydration or renal dysfunction.

Pharmacological Treatment of Heart Failure Cont.….

Digoxin

Digoxin is usually only reserved for patients with severe HF who have not responded to other treatment

In patients with HF and sinus rhythm, digoxin may reduce symptoms and hospital admission

Digoxin should be considered as an add-on therapy for patients with heart failure in sinus rhythm who are still symptomatic after optimum therapy.

If excessive bradycardia occurs with concurrent beta blockade and digoxin therapy, digoxin should be stopped.

Pharmacological Treatment of Heart Failure Cont.….

Hydralazine and Isosorbide Dinitrate

The combination of hydralazine and isosorbide dinitrate (H-ISDN) was shown to reduce mortality in patients with HF before ACE inhibitors were introduced

Patients who are intolerant of an angiotensin-converting enzyme inhibitor and an angiotensin II receptor blocker due to renal dysfunction or hyperkalaemia should be considered for treatment with a combination of hydralazine and isosorbide dinitrate.

Patients with heart failure with reduced ejection fraction, NYHA class III or IV, should be given hydralazine and isosorbide dinitrate in addition to standard therapy

Monitoring of Heart failure Therapy

Monitoring parameters for patients with Heart Failure focuses on three general areas:

evaluation of functional capacity,

evaluation of volume status, and

Laboratory evaluation.

Assessment of volume status is a vital component of the ongoing care of patients with heart failure.

This evaluation provides the clinician important information about the adequacy of diuretic therapy.

Monitoring of Heart failure Therapy Cont…

Because the cardinal signs and symptoms of heart failure are caused by excess fluid retention, the efficacy of diuretic treatment is readily evaluated by the disappearance of these signs and symptoms.

The physical examination is the primary method for the evaluation of fluid retention, and specific attention should be focused on;

the patient’s body weight,

extent of jugular vein distention (JVD),

presence and severity of pulmonary congestion and,

Peripheral edema.

Monitoring of Heart failure Therapy Cont…

Specifically, in a patient with pulmonary congestion, monitoring is indicated for resolution of; rales and pulmonary edema and improvement or resolution of dyspnea on exertion, orthopnea, and Paroxysmal Nocturnal Dyspnea (PND).

Other therapeutic outcomes include an improvement in exercise tolerance and fatigue and a decrease in nocturia and heart rate.

It should be noted that, particularly with

β

-blocker therapy, symptoms may worsen initially and that it may take weeks to months of treatment before patients notice improvement in symptoms.

Routine monitoring of serum electrolytes and renal function is required in patients with heart failure.

Monitoring of Heart failure Therapy Cont…

Assessment of serum potassium is especially important because hypokalemia is a common adverse effect of diuretic therapy and is associated with an increased risk of arrhythmias and digoxin toxicity.

Serum potassium monitoring is also required because of the risk of hyperkalemia associated with ACE inhibitors, ARBs, and aldosterone antagonists.

A serum potassium ≥4 mEq/L should be maintained, with some evidence suggesting it should be ≥4.5 mEq/L.

Assessment of renal function (BUN and serum creatinine) is also an important end point for monitoring diuretic and ACE inhibitor therapy

Key Points

Heart Failure is characterized by typical symptoms (e.g. breathlessness, ankle swelling and fatigue)

Other signs of Heat Failure include elevated jugular venous pressure, pulmonary crackles and peripheral oedema which are caused by a structural and/or functional cardiac abnormality, resulting in a reduced cardiac output and/or elevated intracardiac pressures at rest or during stress

Treatment of Heart Failure of depends on the stage of the Disease

Monitoring parameters for patients with Heart Failure focuses on three general areas which are evaluation of functional capacity, evaluation of volume status, and Laboratory evaluation

Evaluation

What is Heart Failure?

What is the pathophysiology of

Heart Failure?

What are the signs and symptoms of Heart Failure?

How is the treatment of Heart Failure

References

Wells BG, DiPiro J, Schwinghammer T (2013),

Pharmacotherapy Handbook

(6

th

Ed). New York, NY: McGraw-Hill.

DiPiro JT, Talbert RL, Yee GC, Matzke GR, Wells BG, Posey ML, (2008):

Pharmacotherapy: A Pathophysiologic Approach

(7

th

ed): New York, NY: McGraw-Hill.

Katz M D., Matthias KR., Chisholm-Burns M A., Pharmacotherapy(2011)

Principles & Practice Study Guide: A Case-Based Care Plan Approach

: New York, NY: McGraw-Hill.

Schwinghammer TL, Koehler JM (2009)

Pharmacotherapy Casebook: A Patient-Focused Approach

(7

th

ed): New York, NY: McGraw-Hill.

PST 06106

Basic Pharmacotherapy

Session 26: Pharmacotherapy of Schizophrenia

Learning Objectives

By the end of this session students are expected to be able to:

Define schizophrenia

Explain pathophysiology of schizophrenia

Explain the clinical presentation of schizophrenia

Outline diagnosis of schizophrenia

Describe pharmacological treatment of schizophrenia

Describe the monitoring of schizophrenia therapy

Activity: Buzzing

What is Schizophrenia

?

Definition of Schizophrenia

Schizophrenia

Schizophrenia is a chronic and severe mental disorder characterised by

disorganized and bizarre thoughts, delusions, hallucinations, inappropriate affect, and impaired psychosocial functioning

Pathophysiology of Schizophrenia

The pathophysiology of schizophrenia is complex.

A number of theories attempt to explain the link between altered brain function and schizophrenia, including;

T

he

Dopamine

hypothesis

The

Glutamate

hypothesis

Neurodevelopmental model

Pathophysiology of

Schizophrenia Cont…

The Dopamine Hypothesis

The first formulations of the dopamine hypothesis of schizophrenia came from post-mortem studies finding increased striatal availability of D

2

/D

3

receptors in the striatum, as well as studies finding elevated CSF levels of dopamine metabolites.

Psychotic symptoms are related to dopaminergic hyperactivity in the brain. Hyperactivity of dopaminergic systems during schizophrenia is result of increased sensitivity and density of dopamine D2 receptors in the different parts of the brain.

Pathophysiology of Schizophrenia Cont…

The glutamate hypothesis

In humans, NMDA receptor antagonists such as phencyclidine, ketamine and

dizocilpine

can produce both positive and negative psychotic symptoms-in contrast to amphetamine which produces only positive symptoms.

It has therefore been postulated that schizophrenia may result from disruption of glutamatergic neurotransmission, evident as a reduction in the function of NMDA receptors

Pathophysiology of Schizophrenia Cont

…..

Neurodevelopmental model

Neurodevelopmental

model supposes in schizophrenia the presence of “silent lesion” in the brain, mostly in the parts, important for the development of integration (frontal, parietal and temporal), which is caused by different factors (genetic, inborn, infection, trauma) during very early development of the brain in prenatal or early postnatal period of life.

It does not interfere too much with the basic brain functioning in early years, but expresses itself in the time, when the subject is stressed by demands of growing needs for integration, during formative years in adolescence and young

adulthood

Clinical presentation of schizophrenia

The symptoms of schizophrenia fall into three categories:

P

ositive

,

Negative,

Cognitive.

Clinical presentation of

schizophrenia Cont.…

Positive symptoms:

Positive” symptoms are psychotic behaviors not generally seen in healthy people.

People with positive symptoms may “lose touch” with some aspects of reality.

Symptoms include:

Hallucinations

Delusions

Thought disorders (unusual or dysfunctional ways of thinking)

Movement

disorders (agitated body movements)

Clinical

presentation of schizophrenia Cont.…

Negative symptoms:

Negative” symptoms are associated with disruptions to normal emotions and behaviors.

Symptoms include:

“Flat affect” (reduced expression of emotions via facial expression or voice tone)

Reduced feelings of pleasure in everyday life

Difficulty beginning and sustaining activities

Reduced

speaking

Clinical presentation of schizophrenia Cont.…

Cognitive symptoms:

For

some patients, the cognitive symptoms of schizophrenia are subtle, but for others, they are more severe and patients may notice changes in their memory or other aspects of thinking.

Symptoms include:

Poor “executive functioning” (the ability to understand information and use it to make decisions)

Trouble focusing or paying attention

Problems with “working memory” (the ability to use information immediately after learning it)

Diagnosis of Schizophrenia

The Diagnostic and Statistical Manual of the American Psychiatric Association, text revision (DSM-IV-TR), is the guide for diagnosing and classifying schizophrenia and other psychiatric disorders

Diagnosis of

Schizophrenia Cont…

Many patients demonstrate both positive and negative symptoms.

Patients with negative symptoms frequently have more antecedent cognitive dysfunction, poor premorbid adjustment, low level of educational achievement, and a poorer overall prognosis.

Differential diagnosis has to be made in order to exclude other psychiatric conditions that resembles schizophrenia as indicated in the table below

;

Differential Diagnosis Of Schizophrenia

Activity

: Small Group Discussion

What

is the treatment of

Schizophrenia

?

Pharmacological Treatment Of Schizophrenia

The treatment falls under Acute Phase and

Maintenance Phase

Acute Phase

Haloperidol 5 mg (IM) repeat in 30–60 minutes, if required. (Max dose: 20 mg within 24 hours)

AND

Diazepam 10 mg (IV), stat. Repeat after 30–60 minutes if needed.

OR

Promethazine 25–50 mg (deep IM). Repeat after 30–60 minutes if

needed.

OR

Lorazepam 4 mg (IM), stat. Repeat after 30–60 minutes if

needed

Pharmacological Treatment Of

Schizophrenia Cont….

If haloperidol is unavailable give;

Chlorpromazine 25–50 mg (deep IM). May be repeated as necessary 4 times in 24 hours.

If patient is known to suffer from schizophrenia and is not neuroleptic naïve give:

Zuclopenthixol acetate 50–150 mg (IM) Repeat after 2–3 days, if necessary

If patient develops acute dystonia give:

Promethazine deep IM 25–50 mg. In the elderly 25 mg.

OR

Anticholinergic agent, e.g

.

Biperiden

, IM/IV, 2 mg. Repeat as necessary

.

Pharmacological

Treatment Of Schizophrenia Cont….

For maintenance:

Haloperidol

3-4.5 mg (PO) 12hourly

OR

Chlorpromazine 100–600 mg (PO) daily in divided doses

OR

Olanzepine 5–10mg (PO). Maximum dose 25mg/day

OR

Risperidone 1mg (PO) 12 hourly then increase by 1mg every 2–3 days to 2–3mg 12 hourly. Maximum dose 16mg/day 7

Monitoring of Schizophrenia Therapy

Monitoring parameters for patients with Schizophrenia focuses on three general areas:

Improvement of four positive symptoms which are suspiciousness, hallucinations, unusual thought contents and conceptual disorganization

Improvement of negative symptoms such as prolonged time to respond, emotion including unchanging facial expression, blank, expressionless face, reduced social drive, poor grooming and hygiene

Cognition

Monitoring of Schizophrenia

Therapy Cont..

Pharmacotherapeutic plan should include specific monitoring parameters for side effects.

Given the risk of weight gain, diabetes, and lipid abnormalities associated with many of the

Antipsychotics, baseline

parameters should be taken before beginning antipsychotics:

F

amily

history,

W

eight

,

H

eight

,

B

ody

mass index

,

Monitoring of Schizophrenia Therapy Cont..

Waist circumference,

Blood pressure,

Fasting plasma glucose, and

Fasting lipid profile.

Then follow-up monitoring of these parameters should be done after beginning or changing antipsychotics

.

Key Points

Schizophrenia

is a chronic and severe mental disorder characterised by

disorganized and bizarre thoughts, delusions, hallucinations, inappropriate affect, and impaired psychosocial functioning

The symptoms of schizophrenia fall into three categories which are positive, negative, and cognitive

The treatment of Schizophrenia falls under Acute Phase and

Maintainance

Phase of the disease using typical or atypical antipsychotics.

Evaluation

What

is Schizophrenia?

What is the pathophysiology of

Schizophrenia?

What are the signs and symptoms of Schizophrenia?

How is the treatment of Schizophrenia?

References

Wells

BG,

DiPiro

J,

Schwinghammer

T (2013),

Pharmacotherapy Handbook

(6

th

Ed). New York, NY: McGraw-Hill.

DiPiro

JT, Talbert RL, Yee GC, Matzke GR, Wells BG, Posey ML, (2008):

Pharmacotherapy: A Pathophysiologic Approach

(7

th

ed

): New York, NY: McGraw-Hill.

Katz M D., Matthias KR., Chisholm-Burns M A., Pharmacotherapy(2011)

Principles & Practice Study Guide: A Case-Based Care Plan Approach

: New York, NY: McGraw-Hill.

Schwinghammer

TL, Koehler JM (2009)

Pharmacotherapy Casebook: A Patient-Focused Approach

(7

th

ed

): New York, NY: McGraw-Hill.

PST 06106

Basic Pharmacotherapy

Session 27: Pharmacotherapy of Epilepsy

Learning Tasks

By

the end of this session students are expected to be able to:

Define epilepsy

Explain pathophysiology of epilepsy

Explain the clinical presentation of epilepsy

Outline diagnosis of epilepsy

Describe pharmacological treatment of epilepsy

Describe the monitoring of epilepsy therapy

Activity: Buzzing

What is

Epilepsy ?

Definition of Epilepsy

The term 'epilepsy' is used to define a group of neurological disorders all of which exhibit periodic seizures.

Seizures are associated with episodic high-frequency discharge of impulses by a group

of neurons (sometimes referred to as the

focus

) in the brain.

Epilepsy implies a periodic recurrence of seizures with or without convulsions.

A seizure results from an excessive discharge of cortical neurons and is characterized by changes in electrical activity as measured by the electroencephalogram (EEG).

Definition of Epilepsy

Cont.….

A convulsion implies violent, involuntary contraction(s) of the voluntary muscles

The site of the primary discharge and the extent of its spread determine the symptoms that are produced, which range from a brief lapse of attention to a full convulsive fit lasting for several minutes, as well as odd sensations or behaviours

Table

27.1 Classification of Epilepsy

Pathophysiology of Epilepsy

Seizures result from excessive excitation, or in the case of absence seizures, from disordered inhibition of a large population of cortical neurons.

Initially, a small number of neurons fire abnormally.

Normal membrane

conductance

and inhibitory synaptic currents break down, and excess excitability spreads, either locally to produce a focal seizure or more widely to produce a generalized seizure.

This onset propagates by physiologic pathways to involve adjacent or remote areas.

The clinical manifestations depend on the site of the focus, the degree of irritability of the surrounding area of the brain, and the intensity of the impulse.

Pathophysiology of

Epilepsy Cont…

There

are multiple mechanisms that might contribute to synchronous

hyper excitability,

including:

A

lterations

in the distribution, number, type, and biophysical properties of ion channels in the neuronal membranes;

B

iochemical

modifications of receptors;

M

odulation

of second messaging systems and gene expression;

C

hanges in extracellular ion concentrations;

A

lterations in neurotransmitter uptake and metabolism in glial cells

Pathophysiology of Epilepsy Cont…

Modifications in the ratio and function of inhibitory circuits.

Local neurotransmitter imbalances between the main neurotransmitters, glutamate (excitatory) and γ -aminobutyric-acid (GABA) (inhibitory), and neuromodulators (e.g., acetylcholine, norepinephrine, and serotonin) might play a role in precipitating seizures in susceptible patients.

Clinical Presentation and Diagnosis of Epilepsy

General

In most cases, the healthcare provider will not be in a position to witness a seizure.

Many patients (particularly those with complex partial (CP) or generalized tonic

clonic

(GTC) seizures are amnestic to the actual seizure event.

Obtaining an adequate history and description of the actual event (including time course) from a witness is critically important.

Clinical Presentation and Diagnosis of Epilepsy

Cont….

Symptoms

Symptoms

of a specific seizure will depend on seizure type.

Although seizures can vary between patients, they tend to be stereotyped within an individual.

Cerebral palsy (CP) seizures

can include somatosensory or focal motor

features(jerking, loss of muscle tone or repeated movement).

CP seizures are associated with altered consciousness

.

Clinical Presentation and Diagnosis of Epilepsy Cont….

Symptoms…

Absence

seizures can be almost non-detectable with only very brief (seconds) periods of altered consciousness.

GTC (Grand mal seizures )are major convulsive episodes and are always associated with a loss of consciousness.

Cerebral palsy is a congenital disorder of movement, muscle tone or posture, it is due to abnormal brain development often before birth

Clinical Presentation and Diagnosis of Epilepsy Cont….

Signs

Interictally

(between seizure episodes), there are typically no objective or pathognomonic signs

.

Laboratory Tests

There are currently no diagnostic laboratory tests for epilepsy.

Laboratory tests can be done to rule out treatable causes of seizures (e.g., hypoglycemia, altered electrolyte concentrations, infections, etc.) that do not represent epilepsy

.

Clinical Presentation and Diagnosis of Epilepsy Cont….

Other

Diagnostic Tests

EEG(electroencephalogram) is very useful in the diagnosis of various seizure disorders.

A prolactin serum level obtained within 10 to 20 minutes of a tonic-

clonic

seizure can be useful in differentiating seizure activity from pseudo-seizure ( are seizures that occurs as a result of psychological cause such as severe mental stress) activity but not from syncope(loss of consciousness)

Magnetic resonance imaging (MRI) is very useful especially imaging of the temporal lobes

Activity

: Small Group Discussion

What

is the treatment of Epilepsy?

Pharmacological Treatment Of Epilepsy

The general approach to treatment involves assessment of seizure type and frequency, identification of treatment goals, development of a care plan, and a plan for follow-up evaluation.

During the assessment phase, it is critical to establish an accurate diagnosis of the seizure type and classification in order to select the appropriate initial AEDs

.

Pharmacological Treatment Of

Epilepsy Cont….

Pharmacological Treatment Of Epilepsy Cont….

Pharmacological Treatment Of Epilepsy Cont….

Monitoring of epilepsy Therapy

Patients should be monitored long term for seizure control, comorbid conditions, social adjustment, drug interactions, compliance, and adverse effects.

Periodic screening for comorbid neuropsychiatric disorders such as depression and anxiety is also important.

Clinical monitoring involves identifying the number and type of seizures.

Patients should record the severity and the frequency of seizures in a seizure diary. ‘

There should be a decrease in the number and/or severity of seizures.

Patients and family should be questioned regularly to determine whether they are truly seizure free

.

Key Points

The

term 'epilepsy' is used to define a group of neurological disorders all of which exhibit periodic seizures.

Seizures are associated with episodic high-frequency discharge of impulses by a group

of neurons (sometimes referred to as the

focus

) in the brain.

Seizures result from excessive excitation, or in the case of absence seizures, from disordered inhibition of a large population of cortical neurons

The general approach to treatment involves assessment of seizure type and frequency, identification of treatment goals, development of a care plan, and a plan for follow-up evaluation

Evaluation

What

is Epilepsy?

What is the pathophysiology of

Epilepsy?

What are the signs and symptoms of Epilepsy?

How is the treatment of Epilepsy

References

Wells

BG,

DiPiro

J,

Schwinghammer

T (2013),

Pharmacotherapy Handbook

(6

th

Ed). New York, NY: McGraw-Hill.

DiPiro

JT, Talbert RL, Yee GC, Matzke GR, Wells BG, Posey ML, (2008):

Pharmacotherapy: A Pathophysiologic Approach

(7

th

ed

): New York, NY: McGraw-Hill.

Katz M D.,

Matthias KR.,

Chisholm-Burns M A.,

Pharmacotherapy(2011)

Principles & Practice Study Guide: A Case-Based Care Plan Approach

:

New York, NY: McGraw-Hill.

Schwinghammer

TL, Koehler JM (2009)

Pharmacotherapy Casebook: A Patient-Focused Approach

(7

th

ed

): New York, NY: McGraw-Hill.

PST 06106

Basic Pharmacotherapy

Session 28: Pharmacotherapy of Hepatitis B

Learning Objectives

By the end of this session students are expected to be able to:

Define hepatitis B

Explain pathophysiology of hepatitis B

Explain the clinical presentation of hepatitis B

Outline diagnosis of hepatitis B

Describe pharmacological treatment of hepatitis B

Describe the monitoring of hepatitis b therapy

Activity: Buzzing

What is Hepatitis

B ?

Definition of

Hepatitis B

Hepatitis

B is a potentially life-threatening liver infection caused by the hepatitis B virus (HBV).

It can cause chronic infection and puts people at high risk of death from cirrhosis and liver cancer.

HBV is transmitted sexually, parenterally, and

perinataly

.

In areas of high HBV prevalence, perinatal transmission from mother to infant is most common, whereas in areas of intermediate prevalence, horizontal transmission from child to child is most common.

Sexual contact, both homosexual and heterosexual, and injection drug use are the predominant forms of transmission in low-endemic countries

Pathophysiology of Hepatitis B

The life cycle of HBV is complex but, essentially, it acts as a stealth virus by evading the immune system.

During the first stage of infection, the HBV

virion

(virus particle) attaches to a liver cell (hepatocyte) then penetrates the hepatocyte’s cytoplasm

The HBV

virion

is uncoated, which means that

nucleocapsids

can move into the hepatocyte’s nucleus and convert the DNA to covalently closed circular DNA (

cccDNA

) – a double-stranded DNA structure

The

cccDNA

is very stable and can stay in the host nucleus for many months in chronic disease

Pathophysiology of Hepatitis

B Cont…

The virus makes copies of itself in a process that lacks “proof reading ability”, which allows the virus to mutate

The newly formed HBV

virions

are released into the bloodstream, from where they invade other hepatocytes and repeat the replication process.

It is thought that HBV causes inflammation and progressive fibrosis in the infected liver by triggering the immune system to attack the hepatocytes

Clinical Presentation And Diagnosis Of Hepatitis B

The majority of acute HBV infections are also asymptomatic but around 30% of adults will present with the following symptoms;

Signs and symptoms

Easy fatigability, anxiety, anorexia, and malaise

Ascites, jaundice, variceal bleeding, and hepatic encephalopathy can manifest with liver

decompensation(loss of brain function when a damaged liver doesn't remove toxins from blood

)

Clinical Presentation And Diagnosis Of Hepatitis

B Cont…

Signs and

symptoms….

Hepatic

encephalopathy is associated with hyper excitability, impaired mentation, confusion,

obtundation

(loss of consciousness), and eventually coma(a period of prolonged unconsciousness)

Vomiting and seizures

Clinical Presentation And Diagnosis Of Hepatitis B Cont…

Laboratory tests

Presence of hepatitis B surface antigen >6

mo

Intermittent elevations of hepatic transaminase (alanine transaminase

and aspartate transaminase) and hepatitis B virus DNA >20,000 IU/mL (105 copies/mL)

Liver biopsies for pathologic classification as chronic persistent hepatitis, chronic active hepatitis, or cirrhosis

Activity

: Brainstorming

What

is the treatment of Hepatitis B infection??

Pharmacological Treatment Of Hepatitis B

HBV infections are not curable; rather, the goals of therapy are to increase the chances for

seroclearance

, prevent disease progression to cirrhosis and HCC, and to minimize further injury in patients with ongoing liver damage

.

Pharmacological treatment includes

;

Tenofovir

(PO) 300mg once daily for life

OR

Entecavir

(PO) 0.5mg–1mg once daily for life

OR

Lamuvidine

(PO) 100mg once daily for life

Pharmacological Treatment Of Hepatitis

B Cont….

Prophylaxis against HBV can be achieved by vaccination or by passive immunity in

postexposure

cases with hepatitis B immunoglobulin.

Vaccination is the most effective strategy to prevent infection

Monitoring Of Hepatitis B Therapy

Response to therapy is monitored by;

Biochemical (normalization of ALT levels),

Histologic examination of liver cells from biopsy (a minimum 2-point decrease in histology activity compared with baseline biopsy), and

Virologic

response (undetectable serum HBV DNA levels and loss of HBeAg in HBeAg-positive patients).

Maintenance of viral suppression is defined as durability of response.

In HBeAg-positive patients, successful therapy includes loss of HBeAg status and seroconversion to anti-HBeAg.

Key Points

Hepatitis

B is a potentially life-threatening liver infection caused by the hepatitis B virus (HBV).

It can cause chronic infection and puts people at high risk of death from cirrhosis and liver cancer

HBV infections are not curable; rather, the goals of therapy are to increase the chances for

seroclearance

, prevent disease progression to cirrhosis and HCC, and to minimize further

Evaluation

What

is Hepatitis B?

What is the pathophysiology of

Hepatitis B?

What are the signs and symptoms of Hepatitis B?

How is the treatment of

Hepatitis B?

References

Wells

BG,

DiPiro

J,

Schwinghammer

T (2013),

Pharmacotherapy Handbook

(6

th

Ed). New York, NY: McGraw-Hill.

DiPiro

JT, Talbert RL, Yee GC, Matzke GR, Wells BG, Posey ML, (2008):

Pharmacotherapy: A Pathophysiologic Approach

(7

th

ed

): New York, NY: McGraw-Hill.

Katz M D., Matthias KR., Chisholm-Burns M A., Pharmacotherapy(2011)

Principles & Practice Study Guide: A Case-Based Care Plan Approach

: New York, NY: McGraw-Hill.

Schwinghammer

TL, Koehler JM (2009)

Pharmacotherapy Casebook: A Patient-Focused Approach

(7

th

ed

): New York, NY: McGraw-Hill.

PST 06106

Basic Pharmacotherapy

Session 29: Pharmacotherapy of Cholera

Learning Objectives

By the end of this session students are expected to be able to:

Define cholera

Explain pathophysiology of cholera

Explain the clinical presentation of cholera

Outline diagnosis of cholera

Describe pharmacological treatment of cholera

Describe the monitoring of cholera therapy

Activity: Buzzing

What is Cholera?

Definition

of Cholera

Cholera

is an acute gastrointestinal infection caused by

Vibrio

cholerae

.

Infection occurs through ingestion of contaminated water or food by human faeces leading to severe diarrhoea and emesis associated with body fluid and electrolyte depletion

.

Pathophysiology of Cholera

V.

cholerae

is a gram-negative bacillus sharing similar characteristics with the family

Enterobacteriaceae

.

Most pathology of cholera results from an enterotoxin (cholera toxin) produced by the bacteria.

Conditions that reduce gastric acidity, such as the use of antacids, histamine receptor blockers, or proton pump inhibitors, or infections with

Helicobacter pylori,

increase

the

risk

for clinical disease.

Cholera toxin stimulates adenylate

cyclase,which

increases intracellular cyclic adenosine monophosphate (

cAMP

) and results in inhibition of sodium and chloride

absorption

by

microvilli and promotes the secretion of chloride and water by crypt cells.

Pathophysiology of

Cholera Cont…

The toxin likely acts along the entire intestinal tract, but most fluid loss occur in the duodenum.

The net effect of the cholera toxin is isotonic fluid secretion (primarily in the small intestine) that exceeds the absorptive capacity of the intestinal tract (primarily the colon).

This results in the production of watery diarrhea with electrolyte concentrations similar to that of plasma

Clinical presentation and diagnosis of Cholera

A sudden onset of painless watery diarrhoea that may quickly become severe with profuse watery stools, vomiting, severe dehydration and muscular cramps, leading to hypovolemic shock and death

The stool has a characteristic “rice water” appearance (non-bilious, grey, slightly cloudy fluid with flecks of mucus, no blood and inoffensive odour)

Laboratory evidence of dark field microscopic isolation of motile curved bacillus on a wet mount of fresh stool specimen OR

Isolation of bacteria through stool culture on TCBS agar.

Activity

: Brainstorming

What is the treatment of cholera

?

Pharmacological Treatment of Cholera

Treat according to Plan as indicated in the Standard Treatment Guideline (Tanzania)

Plan A: No dehydration,

Plan B: Moderate dehydration and

Plan C: Severe dehydration.

When a case of cholera is suspected at home, advise to rehydrate the patient using ORS if available while preparing to take a patient to the nearest health facility or Cholera Treatment Centre

Pharmacological Treatment of

Cholera Cont..

Manage a suspected cholera case in an isolation ward or in an established Cholera Treatment Centre

Assess the patient's level of dehydration as per National Guidelines for Prevention and Control of Cholera. It is of paramount importance to make correct diagnosis and administer the right treatment according to the Treatment

Pharmacological Treatment of Cholera Cont..

For severe Rehydration

Administer intravenous (IV) fluid immediately to replace fluid deficit; Use Ringer Lactate solution or, if that is not available, 0.9% sodium chloride solution. Give 100 ml/kg IV in 3 hours, 30 ml/kg as rapidly as possible (within 30 min) then 70 ml/kg in the next 2.5 hours

After the initial 30 ml/kg has been administered, the radial pulse should be strong and blood pressure should be normal. If the pulse is not yet strong, continue to give IV fluid rapidly. Administer ORS solution (about 5 ml/kg/hour) as soon as the patient can drink, in addition to IV fluid

If the patient can drink, begin giving A: oral rehydration salt solution (ORS) by mouth while the drip is being set up; ORS can provide the potassium, bicarbonate, and glucose that saline solution lacks.

Pharmacological Treatment of Cholera Cont..

Give an oral antibiotic to patients with severe dehydration as follows:

Adults

(Not for pregnant women) :

Doxycycline (PO) 300 mg as a single dose or 5mg/kg single dose OR
Ciprofloxacin (PO) 1g stat or 15mg/kg 12 hourly for 3 days AND

Folic acid (PO) 5mg once daily for the duration of the treatment.

Expectant mothers: Erythromycin (PO) 500mg 8 hourly for 5 days

Children: A: Erythromycin syrup (PO) 12.5mg/kg 6 hourly for 3 days OR

A: Co-

trimoxazole

48mg/kg once a day for 3 days AND

Pharmacological Treatment of Cholera Cont..

Folic acid AND Zinc.

For adolescents: Ciprofloxacin (PO) 12mg/kg 2 times for 3 days OR
Doxycycline (PO) 300mg as single dose or 5mg/kg single dose AND

Folic acid AND

Zinc

Start feeding 3-4 hours after oral rehydration begins. Preferably, give antibiotics with food to minimize vomiting

Give

ORS for rehydration; they have to be taken frequently

Pharmacological Treatment of Cholera Cont..

For moderate Dehydration

Give oral rehydration, approximately 75-100ml/kg in the first four hours

Reassess after four hours; if improved, continue giving WHO based ORS, in quantity corresponding to losses (

eg

. after each stool) or 10 to 20ml/kg.

If not improved, treat as severe If no signs of dehydration

Pharmacological Treatment of Cholera Cont..

For moderate Dehydration

….

Patients

who have no signs of dehydration when first observed can be treated at home

Give these patients ORS packets to take home, enough for 2 days

Demonstrate how to prepare and give the solution

Instruct the patient or the caretaker to return if any of the following signs develop; increased number of watery stools repeated vomiting or any signs indicating other problems (

eg

, fever, blood in stool)

Monitoring of Cholera therapy

It is important to monitor for resolution of the

symptoms,

adherence to medicines and adverse drug reactions and severe side effects; in case of any they should be reported and addressed

accordingly

Key

Points

Cholera

is an

infection of

the small

intestine by

some strains of the bacterium Vibrio

cholerae

.

Symptoms may range from none, to mild, to severe and the classic symptom is large amounts of watery

diarrhea

that lasts a few days.

Diarrhea

can be so severe that it leads within hours to severe dehydration and electrolyte imbalance

It is spread mostly by unsafe water and unsafe food that has been contaminated with human

feces

containing

the bacteria

Cholera can be successfully treated with oral rehydration therapy (ORT) and chemotherapy

Evaluation

What

is Cholera?

What is the pathophysiology of

Cholera?

What are the signs and symptoms of Cholera?

How is the treatment of Cholera?

References

Wells

BG,

DiPiro

J,

Schwinghammer

T (2013),

Pharmacotherapy Handbook

(6

th

Ed). New York, NY: McGraw-Hill.

DiPiro

JT, Talbert RL, Yee GC, Matzke GR, Wells BG, Posey ML, (2008):

Pharmacotherapy: A Pathophysiologic Approach

(7

th

ed

): New York, NY: McGraw-Hill.

Katz M D.,

Matthias KR.,

Chisholm-Burns M A.,

Pharmacotherapy(2011)

Principles & Practice Study Guide: A Case-Based Care Plan Approach

:

New York, NY: McGraw-Hill.

Schwinghammer

TL, Koehler JM (2009)

Pharmacotherapy Casebook: A Patient-Focused Approach

(7

th

ed

): New York, NY: McGraw-Hill.

PST 06106

Basic Pharmacotherapy

Session 30: Pharmacotherapy of Shigellosis

Learning objectives

By the end of this session students are expected to be able to:

Define shigellosis

Explain pathophysiology of shigellosis

Explain the clinical presentation of shigellosis

Outline diagnosis of shigellosis

Describe pharmacological treatment of shigellosis

Describe the monitoring of shigellosis therapy

Activity: Buzzing

What is Shigellosis?

Definition of Shigellosis

Shigellosis

Shigellosis is spread by means of fecal-oral, by ingestion of contaminated food and water and it leads to bacillary dysentery.

Pathophysiology of shigellosis

The source of infection is the feces of infected people or convalescent carriers; humans are the only natural reservoir for

Shigella

.

Direct spread is by the fecal-oral route. Indirect spread is by contaminated food and fomites.

Flies serve as vectors.

Because

Shigella

is relatively resistant to gastric acid, ingestion of as few as 10 to 100 organisms can cause disease.

Pathophysiology of shigellosis Cont….

Shigella

organisms penetrate the mucosa of the colon, causing mucus secretion, hyperemia, leukocytic infiltration, edema, and often superficial mucosal ulcerations.

Shigella dysenteriae

type 1 (commonly present in travelers returning from endemic areas) produces Shiga toxin, which causes marked watery diarrhea and sometimes hemolytic-uremic syndrome(HUS)

Clinical Presentation and Diagnosis of Shigellosis

Signs and Symptoms

Acute abdominal cramping, high-grade fever, emesis and large-volume watery diarrhea,

Tenesmus, urgency, fecal incontinence, mucoid bloody diarrhea,

Severe headache, lethargy, meningismus, delirium and convulsions,

Hemolytic uremic syndrome (HUS),

microangiopathic hemolytic anemia, thrombocytopenia, and renal failure,

Profound dehydration and hypoglycemia

Clinical Presentation and Diagnosis of Shigellosis Cont…

Diagnosis

Laboratory evidence of microscopic isolation of the bacteria from stool or rectal swabs specimens OR

Stool culture for suspected cases in early course of infection OR

An enzyme immunoassay (ELISA) for shiga toxin detection in stool for S. dysenteriae type-1.

Activity: Small Group Discussion

What is the treatment of Shigellosis?

Pharmacological treatment of Shigellosis

Treatment

Ciprofloxacin (PO) 500mg 12 hourly for 5 days OR

Nalidixic acid (PO) 1000mg 6 hourly for 7 days OR

Erythromycin (PO) 250mg 6 hourly for 5 days

Monitoring of Shigellosis Therapy

It is important to monitor for resolution of the symtoms, adherence to medicines and adverse drug reactions and severe side effects; in case of any they should be reported and addressed accordingly

Key Points

Shigella infection (shigellosis) is an intestinal disease caused by a family of bacteria known as shigella.

The main sign of shigella infection is diarrhea, which often is bloody.

Shigella can be passed through direct contact with the bacteria in the stool.

Shigella infection usually clears up without complications, although chemotherapy may be needed to some patients

It may take weeks or months before the bowel habits return to normal

.

Evaluation

What is Shigellosis?

What is the pathophysiology of

Shigellosis?

What are the sACigns and symptoms of Shigellosis?

How is the treatment of Shigellosis?

References

Wells BG, DiPiro J, Schwinghammer T (2013),

Pharmacotherapy Handbook

(6

th

Ed). New York, NY: McGraw-Hill.

DiPiro JT, Talbert RL, Yee GC, Matzke GR, Wells BG, Posey ML, (2008):

Pharmacotherapy: A Pathophysiologic Approach

(7

th

ed): New York, NY: McGraw-Hill.

Katz M D., Matthias KR., Chisholm-Burns M A., Pharmacotherapy(2011)

Principles & Practice Study Guide: A Case-Based Care Plan Approach

: New York, NY: McGraw-Hill.

Schwinghammer TL, Koehler JM (2009)

Pharmacotherapy Casebook: A Patient-Focused Approach

(7

th

ed): New York, NY: McGraw-Hill.

END

PST 06106

Basic Pharmacotherapy

Session 31: Pharmacotherapy of Breast

Cancer

Learning Objectives

By the end of this session students are expected to be able to:

Define breast cancer

Explain pathophysiology of breast cancer

Explain the clinical presentation of breast cancer

Outline diagnosis of breast cancer

Describe pharmacological treatment of breast cancer

Describe the monitoring of breast cancer

therapy

Definition of Breast Cancer

Breast cancer is a malignancy originating from breast tissue.

Disease confined to a localized breast lesion is referred to as early, primary, localized, or curable

Disease detected clinically or radiologically in sites distant from the breast is referred to as advanced or metastatic breast cancer (MBC), which is usually incurable.

Breast cancer cells often spread undetected by

contiguity(bordering/being in contact with something),

lymph channels, and through the blood early in the course of the disease, resulting in metastatic disease after local therapy.

The most common metastatic sites are lymph nodes, skin, bone, liver, lungs, and brain

.

Activity: Buzzing

What is the pathophysiology of breast cancer?

Pathophysiology of Breast Cancer

Breast cancer is a malignant tumor that starts in the cells of the

breast

,

Like

other cancers, there are several factors that can raise the risk of getting breast cancer:

Female gender

Age

Previous breast cancer

Benign breast disease

Hereditary factors (family history of breast cancer)

Pathophysiology of Breast

Cancer

Cont

Early age at menarche

Late age at menopause

Late age at first full-term pregnancy

Obesity (postmenopausal)

Low physical activity

High-dose exposure to ionizing radiation early in life

Pathophysiology of Breast Cancer

Cont.…

Damage to the DNA and genetic mutations can lead to breast cancer; have been experimentally linked to estrogen exposure.

Some

individuals inherit defects in the DNA and genes like the BRCA1, BRCA2 and P53 among others.

Those

with a family history of ovarian or breast cancer thus are at an increased risk of breast cancer

.

BRCA1

and

BRCA2

are human genes that produce tumor suppressor proteins.

These

proteins help repair damaged DNA and, therefore, play a role in ensuring the stability of each cell’s genetic material.

When

either of these genes is mutated, or altered, such that its protein product is not made or does not function correctly, DNA damage may not be repaired properly

..

Pathophysiology of Breast Cancer

Cont

The immune system normally seeks out cancer cells and cells with damaged DNA and destroys them.

Breast

cancer may be a result of failure of such an effective immune defense and surveillance.

These are several signalling systems of growth factors and other mediators that interact between stromal cells and epithelial cells. Disrupting these may lead to breast cancer as well.

Clinical Presentation and Diagnosis of Breast Cancer

The patient may not have any symptoms, as breast cancer may be detected in asymptomatic patients though routine screening mammography.

The initial sign in more than 90% of women with breast cancer is a painless lump that is typically solitary, unilateral, solid, hard, irregular, and

non mobile

.

Less common initial signs are pain and nipple changes.

More advanced cases present with prominent skin

oedema,

redness, warmth, and induration.

Symptoms of MBC depend on the site of metastases, but may include bone pain, difficulty breathing, abdominal pain or enlargement, jaundice, and mental status changes.

Many women first detect some breast abnormalities themselves, but it is increasingly common for breast cancer to be detected during routine screening mammography in asymptomatic women

.

Clinical Presentation and Diagnosis of Breast

Cancer Cont.….

Staging

Stage

is based on the size of the primary tumor, presence and extent of lymph node involvement, and presence or absence of distant metastases. Simplistically stated, these stages may be represented as

follows:

Early Breast Cancer

Stage 0: Carcinoma in situ or disease that has not invaded the basement

membrane.(is

a group of abnormal cells that are found only in the place where they first formed in the body

)

Stage I: Small primary

tumour

without lymph node involvement.

Stage II: Involvement of regional lymph nodes.

Clinical Presentation and Diagnosis of Breast Cancer Cont.….

Locally Advanced Breast Cancer

Stage III: Usually a large tumor with extensive nodal involvement in which node or tumor is fixed to the chest wall; also includes inflammatory breast cancer, which is rapidly progressive.

Advanced or Metastatic Breast Cancer

Stage IV: Metastases in organs distant from the primary

tumour.

Clinical Presentation and Diagnosis of Breast Cancer Cont.….

Clinical Presentation

Local

Signs and Symptoms

A painless, palpable lump is most common.

Less common: pain; nipple discharge, retraction or dimpling;

Skin edema, redness or warmth.

Palpable local–regional lymph nodes may also be

present

Signs and Symptoms of Systemic Metastases

Depends on the site of metastases, but may include bone pain, difficulty breathing, abdominal pain or enlargement, jaundice, mental status

changes

Clinical Presentation and Diagnosis of Breast Cancer Cont.….

Diagnosis

Initial workup for a woman presenting with a localized lesion or suggestive symptoms should include a careful history, physical examination of the breast, three-dimensional mammography, and, possibly, other breast imaging techniques such as ultrasound.

Breast biopsy is indicated for a mammographic abnormality that suggests malignancy or a mass that is palpable on physical examination.

Clinical Presentation and Diagnosis of Breast Cancer Cont.….

Laboratory Tests

Tumor markers such as cancer antigen (CA) or carcinoembryonic antigen (CEA) may be elevated.

Alkaline phosphatase or liver function tests may be elevated in metastatic disease.

Clinical Presentation and Diagnosis of Breast Cancer Cont.….

Other Diagnostic Tests

Mammogram

(with or without ultrasound, breast MRI, or both)

Biopsy for pathology review and determination of tumor estrogen/progesterone receptor (ER/PR) status and

HER2

status.

Systemic staging tests may include: chest x-ray, chest CT, bone scan, abdominal CT or ultrasound, or MRI

.

Activity

: Small Group Discussion

What

is the pharmacological treatment of breast cancer?

Pharmacological Treatment of Breast Cancer

Chemotherapy is indicated for almost all patients as neo-adjuvant, adjuvant or palliative. Patients, who are planned for surgery and have ≥ T3 tumors, should receive neo-adjuvant chemotherapy before

operation

Several

regimens are available. Few of them include

:

Dosing schedules for combinations for HER 2 negative disease:

Pharmacological Treatment of Breast

Cancer

Cont

Describes cancer cells that do not have a large amount of a protein called HER2 on their surface. In normal cells, HER2 helps to control cell growth. Cancer cells that are HER2 negative may grow more slowly and are less likely to recur (come back) or spread to other parts of the body than cancer cells that have a large amount of HER2 on their surface

Doxorubicin 60 mg/m2 IV day 1 + Cyclophosphamide 600 mg/m2 IV day 1 given every 2 weeks for 4 cycles THEN Paclitaxel 175 mg/m2 by 3hr IV infusion day 1, given every 14 days for 4 cycles.

Pharmacological Treatment of Breast Cancer

Cont

Doxorubicin 60 mg/m2 IV day 1 + Cyclophosphamide 600 mg/m2 IV day 1 given every 14 days for 4 cycles followed by Paclitaxel 80 mg/m2 by 1 h IV infusion weekly for 12

weeks.

Doxorubicin

60 mg/m2 IV on day1 + Cyclophosphamide 600 mg/m2 IV day 1 given every 21 days for 4 cycles then followed by Paclitaxel 175 mg/m2 by 3 h IV infusion day 1, given every 21 days for 4 cycles OR Docetaxel 100 mg/m2 IV day 1 Cycled every 21 days for 4 cycles.

NOTE:

FBC(Full blood count), RFT(Renal function test), LFT( Liver function test)

before each cycle

Pharmacological Treatment of Breast Cancer

Cont

Dosing schedule for combinations for HER2-Positive disease:

Doxorubicin 60 mg/m2 IV day1 AND Cyclophosphamide 600 mg/m2 IV day 1 given every 21 days for 4 cycles followed by Paclitaxel 80 mg/m2 by 1 h IV weekly for 12

wks

AND

Trastuzumab 4 mg/kg IV with first dose of paclitaxel followed by Trastuzumab 2 mg/kg IV weekly to complete 1 y of treatment

Pharmacological Treatment of Breast Cancer

Cont

As an alternative, Trastuzumab 6 mg/kg IV every 21 days may be used following the completion of Paclitaxel, and given to complete 1 year of Trastuzumab treatment

Endocrine

therapy

Premenopausal ER/PR Positive: Tamoxifen 20 mg (PO) daily for 5 years
Post-menopausal ER/ PR Positive: Anastrazole 1 mg daily for 5 years OR Tamoxifen 20 mg daily for 2 years followed Anastrazole 1 mg daily for 3 years.

Monitoring

of Breast Cancer Therapy

Monitoring response to treatment is a key element in the management of breast cancer that involves several different viewpoints from surgery, radiology, and medical oncology

After completion of adjuvant therapy, follow up care focuses on detecting recurrent disease with the intention of improving long term survival

Monitor patient adherence to the treatment as maintaining dose intensity has been demonstrated to be important in the cure of disease

Tumor response to a particular treatment regimen may be measured by clinical chemistry such as liver enzyme elevation in a patient with hepatic metastases or tumor markers, or imaging techniques such as bone scans or chest radiographs.

Monitoring

of Breast Cancer

Therapy

Cont

However, assessment of the patient’s clinical status and symptom control is often adequate to evaluate response to the therapy administered.

In the patient with metastatic breast cancer, it is common to initiate hormonal therapy or chemotherapy and continue administration until signs and symptoms of disease progression or new signs and symptoms present

Monitor the adverse effects of drugs and manage them accordingly

Key Points

Breast

cancer is a malignancy originating from breast tissue. Disease confined to a localized breast lesion is referred to as early, primary, localized, or curable

Disease detected clinically or radiologically in sites distant from the breast is referred to as advanced or metastatic breast cancer (MBC), which is usually incurable

Key

Points Cont.….

Damage to the DNA and genetic mutations can lead to breast cancer; have been experimentally linked to estrogen exposure. Some individuals inherit defects in the DNA and genes like the BRCA1, BRCA2 and P53 among others. Those with a family history of ovarian or breast cancer thus are at an increased risk of breast cancer.

Chemotherapy is indicated for almost all patients as neo-adjuvant, adjuvant or palliative. Patients, who are planned for surgery and have ≥ T3 tumors, should receive neo-adjuvant chemotherapy before operation

Evaluation

What

is Breast Cancer?

What is the pathophysiology of Breast Cancer?

How is Breast Cancer diagnosed?

How is monitoring of Breast Cancer therapy done?

References

Wells

BG,

DiPiro

J,

Schwinghammer

T (2013),

Pharmacotherapy Handbook

(6

th

Ed). New York, NY: McGraw-Hill.

DiPiro

JT, Talbert RL, Yee GC, Matzke GR, Wells BG, Posey ML, (2008):

Pharmacotherapy: A Pathophysiologic Approach

(7

th

ed

): New York, NY: McGraw-Hill.

Katz M D.,

Matthias KR.,

Chisholm-Burns M A.,

Pharmacotherapy (2011)

Principles & Practice Study Guide: A Case-Based Care Plan Approach

:

New York, NY: McGraw-Hill.

Schwinghammer

TL, Koehler JM (2009)

Pharmacotherapy Casebook: A Patient-Focused Approach

(7

th

ed

): New York, NY: McGraw-Hill.

PST 06106

Basic Pharmacotherapy

Session 32: Pharmacotherapy of Prostate Cancer

Learning Tasks

By the end of this session students are expected to be able to:

Define prostate cancer

Explain pathophysiology of prostate cancer

Explain the clinical presentation of prostate cancer

Outline diagnosis of prostate cancer

Describe pharmacological treatment of prostate cancer

Describe the monitoring of prostate cancer therapy

Definition of Prostate Cancer

Prostate cancer is a malignant neoplasm that arises from the prostate gland.

Prostate cancer has an indolent course; localized prostate cancer is curable by surgery

or

radiation

therapy, but advanced prostate cancer is not yet curable.

The most common type of prostate cancer is adenocarcinoma (95 %)

Tumors

are stratified by T stage, Gleason score (GS), and PSA into three prognostic groups of low, intermediate and high risk.

Definition of Prostate Cancer

Cont

Low risk: T1–T2a and PSA < 10 ng/ml and GS ≤ 6
Intermediate risk: T2b or PSA 10 – 20 ng/ml or GS 7
High risk: T2c–T4 or PSA > 20ng/ml or GS 8–10

Patient can be offered appropriate treatment options according to stage of disease, prognostic risk group and estimated survival taking into account performance status and comorbidity.

Activity: Buzzing

What is the pathophysiology of prostate cancer?

Pathophysiology of Prostate Cancer

The prostate gland is a part of the male reproductive system that helps to make and store seminal fluid.

Because of its location, prostate disease often affects urination, ejaculation, and rarely defecation.

Prostate cancer begins when normal

semen screening

prostate gland cells mutate into cancer cells.

The region of prostate gland where the adenocarcinoma is most common is the peripheral zone.

Pathophysiology of Prostate

Cancer

Cont

Initially, small clumps of cancer cells remain confined to otherwise normal prostate glands, a condition known as carcinoma in situ or prostate intraepithelial neoplasia(PIN).

Overtime, these cancer cells begin to multiply and spread to the surrounding prostate tissue (the stroma) forming a tumor.

Eventually

, the tumor may grow large enough to invade nearby organs such as the seminal vesicles, or the rectum, or the tumor cells may develop the ability to travel in the blood stream and lymphatic system.

The invasion of other organs is called metastasis.

Prostate cancer most commonly metastasizes to the bones, lymph nodes, and may invade rectum, bladder and lower ureters after local progression.

Clinical presentation and Diagnosis of Prostate Cancer

Localized Disease

Asymptomatic

Locally Invasive Disease

Impotence

Prostatic symptoms are associated with advanced stages of the disease, which include: reduced potency, urinary frequency and nocturnal, poor stream, hesitancy and terminal

dribbling

Clinical presentation and Diagnosis of Prostate

Cancer Cont.….

Advanced Disease

Back pain

Cord compression

Lower extremity edema

Anemia

Weight loss

Very often patients may present with bone pain including backache or pathological

fracture

Diagnostic and Staging Workup for prostate Cancer

Activity

: Small Group Discussion

What are the drugs treatments for prostate cancer?

Pharmacological Treatment of Prostate Cancer

Luteinizing Hormone–Releasing Hormone Agonists

LHRH agonists are a reversible method of androgen ablation and are as effective

as orchiectomy

.

Leuprolide acetate, leuprolide depot, leuprolide implant,

triptorelin

depot,

triptorelin

implant, and

goserelin

acetate implant are currently available.

Dosing intervals range from once monthly to every 16 weeks.

Leuprolide implant is a

miniosmotic

pump that delivers daily doses for 1 year.

The most common adverse effects of LHRH agonists include disease flare-up during the first week of therapy (

eg

, increased bone pain or urinary symptoms), hot flashes, erectile impotence, decreased libido, and injection-site reactions.

Pharmacological Treatment of Prostate

Cancer

Cont

….

Luteinizing Hormone–Releasing Hormone Agonists…..

Use

of an antiandrogen (

eg

,

flutamide

,

bicalutamide

, or

nilutamide

) prior to initiation of LHRH therapy and for 2 to 4 weeks after is a strategy to minimize initial tumor flare.

Decreases in bone mineral density complicate androgen deprivation therapy (ADT), resulting in increased risk of osteoporosis, osteopenia, and skeletal fractures.

Calcium and vitamin D supplements and a baseline bone mineral density are recommended.

Pharmacological Treatment of Prostate Cancer

Cont

….

Gonadotropin-Releasing Hormone Antagonists

Degarelix binds reversibly to GnRH receptors in the pituitary gland, reducing the production of testosterone to castrate levels in 7 days or less

A major advantage of

degarelix

over LHRH agonists the lack of tumor flares.

Degarelix is administered as a subcutaneous injection every 28 days

Injection site reactions are the most frequently reported adverse effects and include pain, erythema, swelling, induration, and nodules

.

Pharmacological Treatment of Prostate Cancer

Cont

….

Antiandrogens

Monotherapy with

flutamide

,

bicalutamide

, and

nilutamide

is no longer

recommended

due

to decreased efficacy as compared with patients treated with LHRH agonist therapy

Antiandrogens are indicated for advanced prostate cancer only when

combined with an LHRH agonist (

flutamide

and

bicalutamide

]) or

orchiectomy

(

nilutamide

). In combination, antiandrogens can reduce the LHRH

agonist–

inducedflare

.

Enzalutamide is approved as a single agent in metastatic hormone-resistant

prostate

cancer

patients who have previously received docetaxel

.

Pharmacological Treatment of Prostate Cancer

Cont

….

Chemotherapy

Docetaxel, 75 mg/m2 every 3 weeks up to 6 cycles, combined with prednisone, 5 mg twice daily, improves survival in castrate-refractory prostate cancer.

It is mainly reserved for hormonal-refractory prostate cancer. The most common adverse events include nausea, alopecia, and myelosuppression.

Cabazitaxel

25 mg/m2 every 3 weeks with prednisone 10 mg daily significantly improves progression-free and overall survival.

Neutropenia, febrile neutropenia, neuropathy, and diarrhea are the most significant toxicities.

For Bone metastases/osteolytic/

tumour

induced hypercalcemia:

Zolendronic

acid IV 4mg over 15min given 4 Weekly

Monitoring Of Prostate Cancer Therapy

Monitor primary tumor size, involved lymph nodes, and tumor marker response such as PSA with definitive, curative therapy

PSA level is checked every 6 months for the first 5 years, then annually.

With metastatic disease, clinical benefit can be documented by evaluating performance status, weight, quality of life, analgesic requirements, and PSA or DRE at 3-month intervals

.

Monitoring of Prostate Cancer Therapy

Monitor

primary tumor size, involved lymph nodes, and tumor marker response such as PSA with definitive, curative therapy

PSA level is checked every 6 months for the first 5 years, then annually.

With metastatic disease, clinical benefit can be documented by evaluating performance status, weight, quality of life, analgesic requirements, and PSA or DRE at 3-month intervals.

Key Points

Prostate

cancer is a malignant neoplasm that arises from the prostate gland. Prostate

cancer has an indolent course; localized prostate cancer is curable by surgery or

radiation therapy, but advanced prostate cancer is not yet curable

There are different stages of Prostate Cancer according to

Glearson

score

Metastatic spread can occur by local extension, lymphatic drainage, or

hematogenous

dissemination

Key

Points

Cont

The diagnosis is based on various diagnostic criteria and various diagnostic tests such as

abdominal and pelvic USS and or CT Scan, Pelvic MRI in early stage

disease , Bone

scan

etc

The

common drugs used for the treatment of Prostate Cancer are LHRH agonists and

GnRH

antagonists

Monitoring therapy should be done by checking primary tumor size, involved lymph nodes, and tumor marker response such as PSA with definitive, curative therapy. PSA level should checked every 6 months for the first 5 years, then annually.

Evaluation

What

is Prostate Cancer?

What is the pathophysiology of Prostate Cancer?

How is Prostate Cancer diagnosed?

What is the first line treatment of Prostate Cancer

References

Wells

BG,

DiPiro

J,

Schwinghammer

T (2013),

Pharmacotherapy Handbook

(6

th

Ed). New York, NY: McGraw-Hill.

DiPiro

JT, Talbert RL, Yee GC, Matzke GR, Wells BG, Posey ML, (2008):

Pharmacotherapy: A Pathophysiologic Approach

(7

th

ed

): New York, NY: McGraw-Hill.

Katz M D.,

Matthias KR.,

Chisholm-Burns M A.,

Pharmacotherapy(2011)

Principles & Practice Study Guide: A Case-Based Care Plan Approach

:

New York, NY: McGraw-Hill.

Schwinghammer

TL, Koehler JM (2009)

Pharmacotherapy Casebook: A Patient-Focused Approach

(7

th

ed

): New York, NY: McGraw-Hill.

PST 06106

Basic Pharmacotherapy

Session 33: Pharmacotherapy of Oropharyngeal Candidiasis

Learning Tasks

By

the end of this session students are expected to be able to:

Define oropharyngeal candidiasis

Explain pathophysiology of oropharyngeal candidiasis

Explain the clinical presentation of oropharyngeal candidiasis

Outline diagnosis of oropharyngeal candidiasis

Describe pharmacological treatment of oropharyngeal candidiasis

Describe the monitoring of oropharyngeal candidiasis therapy

Definition of Oropharyngeal Candidiasis

Oropharyngeal candidiasis

(OPC), or

thrush,

refers to an infection of the oral mucosa.

Candida

is responsible for the majority of

oralfungal

infections, and

C.

albicans

is the principal species causing the infection, commonly referred to as

candidiasis

The infection may extend into the esophagus, causing esophageal candidiasis.

Activity: Buzzing

What

is the pathophysiology of oropharyngeal candidiasis?

Pathophysiology of Oropharyngeal Candidiasis

The pathogenesis of OPC is most clearly elucidated in the setting of HIV infection.

There appear to be several levels of immune defense against the development of OPC in HIV-infected persons, and they involve both systemic and local immunity.

The primary line of host defense against

C.

albicans

is cell-mediated immunity (CMI) at the mucosal surfaces, which is mediated by CD4 T cells.

The efficacy of the CD4 T cells is reduced when the number of cells drops below a protective threshold, and protection against infection becomes dependent on secondary or local immune mechanisms

Pathophysiology of Oropharyngeal

Candidiasis

Cont

….

When the number of CD4 T cells drops too low, recruitment of these cells to the oral cavity is impaired.

The CD4 T-cell count has been considered as the hallmark predictor for development of OPC.

The changeover of the role of

Candida

species from commensal to pathogenic in the human host usually occurs when breakdown in these host defenses occurs.

Other virulence factors are the adhesive ability of

C.

albicans

to epithelial cells and proteins and its ability to invade host cells

by means of phospholipase and proteinase enzymes.

Pathophysiology of Oropharyngeal Candidiasis

Cont

….

This may be one

of the factors leading to OPC in non-HIV-infected individuals.

Other

components of the pathogenesis in the absence of HIV that have been

postulated are the ability of the

Candida

species to adhere to buccal

epithelial cells including those patients receiving broad-spectrum antimicrobial therapy.

Clinical Presentation and Diagnosis of Oropharyngeal Candidiasis

General

The clinical features can be quite diverse

Symptoms

Symptoms are diverse and range from none to sore, painful mouth, burning tongue, metallic taste, and dysphagia and odynophagia with involvement of the hypopharynx

Signs

Signs are variable and can include diffuse erythema and white patches on the surfaces of the buccal mucosa, throat, tongue, or gums; constitutional signs are absent

Clinical Presentation and Diagnosis of Oropharyngeal Candidiasis

Cont

….

Laboratory tests

Scraping of an active lesion for microscopic examination can help confirm the diagnosis (presence of

pseudohyphae

and budding yeast) but is usually not necessary

Cultures are not necessary because isolation of

Candida

species does not distinguish between colonization and true infection; cultures can be taken in patients responding poorly to therapy to determine the infecting species and to predict likely drug resistance

Activity

: Small Group Discussion

What are the drugs treatments for oropharyngeal candidiasis

?

Pharmacological Treatment of Prostate Cancer

The management of OPC should be individualized for each patient, taking into consideration the underlying immune status, other concurrent mucosal and medical diseases, concomitant medications, and exogenous infectious sources.

In HIV-infected patients with inadequately controlled disease, antifungal treatment produces only a transient clinical response, and the relapse rates are higher than in other patient populations.

Topical therapies should be the first choice for milder forms of infections

Therapeutic Options for Mucosal Candidiasis

Monitoring of Oropharyngeal Candidiasis Therapy

Efficacy end points for oropharyngeal and esophageal candidiasis include rapid relief of symptoms and prevention of complications without early relapse after completion of the course of therapy.

Symptomatic relief of presenting signs and symptoms generally occurs within 48 to 72 hours of starting therapy, with complete resolution by 7 to 10 days.

Patients should be advised about the time course and told to return for reassessment when signs and symptoms recur.

It is usually unnecessary for the patient to be reassessed soon after finishing the treatment course.

Monitoring of Oropharyngeal Candidiasis Therapy

Cont

However, HIV patients should be questioned and examined for the occurrence of

mucosal

candidiasis

as part of their regular follow-up.

The frequency of monitoring can be more often in neutropenic patients

because

of

concern for dissemination of candidiasis.

During the period of neutropenia, temperature should be monitored daily, as well

as

signs

of dissemination.

Efficacy of the antifungal agent is partly influenced by patient adherence to the medication regimen.

Patients must be counseled on proper administration and dosing, in particular for

topical

agents

Monitoring of Oropharyngeal Candidiasis Therapy

Cont

Safety end points include monitoring for occurrence of the relevant drug side effects and drug interactions

Hepatotoxicity can occur when azole therapy is prolonged beyond 7 to 10 days or high doses are used.

Periodic monitoring of liver enzymes (alanine transaminase and aspartate amino-transferase) should be considered, especially if prolonged therapy (longer than 21 days) is anticipated.

Key Points

Oropharyngeal

candidiasis

(OPC), or

thrush,

refers to an infection of the oral mucosa.

Symptoms are diverse and range from none to sore, painful mouth, burning tongue, metallic taste, and dysphagia and odynophagia with involvement of the hypopharynx

The management of OPC should be individualized for each patient, taking into consideration the underlying immune status, other concurrent mucosal and medical diseases, concomitant medications, and exogenous infectious sources

Evaluation

What

is Oropharyngeal Candidiasis?

What is the pathophysiology of Oropharyngeal Candidiasis?

How is Oropharyngeal Candidiasis?

What is the first line treatment of Oropharyngeal Candidiasis?

REFER

Students to Handout 33.1: Risk Factors for the Development of Oropharyngeal and/or Esophageal Candidiasis

References

Wells

BG,

DiPiro

J,

Schwinghammer

T (2013),

Pharmacotherapy Handbook

(6

th

Ed). New York, NY: McGraw-Hill.

DiPiro

JT, Talbert RL, Yee GC, Matzke GR, Wells BG, Posey ML, (2008):

Pharmacotherapy: A Pathophysiologic Approach

(7

th

ed

): New York, NY: McGraw-Hill.

Katz M D., Matthias KR., Chisholm-Burns M A., Pharmacotherapy(2011)

Principles & Practice Study Guide: A Case-Based Care Plan Approach

: New York, NY: McGraw-Hill.

Schwinghammer

TL, Koehler JM (2009)

Pharmacotherapy Casebook: A Patient-Focused Approach

(7

th

ed

): New York, NY: McGraw-Hill.

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