Antihypertensive Agents
Thomas G. Wells
Mohammad Ilyas
Russell W. Chesney
Deborah P. Jones
Until 1997, few antihypertensive agents were studied systematically in children, and very few were labeled for use in patients younger than 18 years (1). As new drugs were introduced into the market, pediatricians had to choose between the use of promising new agents without the benefit of controlled studies in a pediatric population and continued use of older but familiar agents. The First and Second Task Force Reports on Blood Pressure Control in Children offered treatment schemes based on strategies that were used in adults at the time (2,3). These schemes tacitly recognized the need to use drugs that were not labeled for use in children. Off-label use, with all of its implied risks, was often the only viable option available to physicians who treated children with hypertension (1). Newer drugs promised not only new approaches to the treatment of hypertension but also, in many cases, fewer adverse effects.
Recognizing the need to address this inequity, several federal initiatives designed to include children in the drug development process were proposed. In 1994, the Food and Drug Administration (FDA) promulgated the Pediatric Rule, which was expanded in 1998 and required manufacturers to perform limited studies in children if a new drug offered any potential health benefits in the pediatric population (4,5). With the passage of the FDA Modernization Act (FDAMA) in 1997 and later the Best Pharmaceuticals for Children Act (BPCA) in 2002, pharmaceutical firms were granted meaningful incentives in exchange for conducting appropriate pediatric studies (6,7).
The enabling legislation and regulatory requirements led to a dramatic increase in the number of pediatric trials. As a result, the number of anti-hypertensive medications with pediatric labeling has increased (8,9) (Table 49.1). In addition, several extemporaneously compounded liquid solutions were developed and tested for short-term stability and bioequivalence (10,11,12). Because very few drugs used to treat hypertension in children are manufactured as commercially available solutions or suspensions, these extemporaneous formulations represented a significant advance in treating younger children who are unable to swallow tablets or capsules.
Hypertension in Children
As many as 10% to 13% of children will have elevated blood pressure (BP) on a single measurement (13,14), but persistent hypertension is observed in only 1% to 2.5% of the pediatric population (15,16,17,18). More recent data estimates that the prevalence of pre-hypertension is nearly 10% and established hypertension 4%, with greater burden on minority children (19). Despite the availability of widely accepted normative BP data (20), the accurate diagnosis of persistent hypertension can be difficult. Errors in cuff selection and technique are still common despite publication of accepted methods for performing casual BP measurement in children (18). Labile BP and the “white coat” effect complicate the diagnosis in children with high normal BP or borderline to moderate hypertension (21,22). The use of ambulatory blood pressure monitoring (ABPM) in these children has helped to separate those who require evaluation and treatment from those who need only longitudinal observation (20,23,24). Accurate diagnosis is extremely important because failure to diagnose and adequately control clinically significant hypertension may result in the development of target organ damage (25,26,27,28,29,30). Conversely, improper diagnosis and subsequent treatment of normotensive children may risk unnecessary exposure to adverse events.
Selection of appropriate therapy often depends on the suspected cause of hypertension. Secondary causes of hypertension, particularly renal and renovascular diseases, are commonly observed among preadolescent children (Table 49.2) (20,31,32). During adolescence, secondary causes of hypertension continue to occur, but the prevalence of primary hypertension increases dramatically (20,33). It is likely that obesity, insulin resistance, and genetically determined factors contribute to the development of hypertension in some adolescents (34,35,36,37). Both primary and secondary hypertension in children and adolescents may result in significant target organ damage (25,26,27,28,29,30). It is particularly important that these children receive adequate antihypertensive therapy. The working group has recommended that pharmacologic treatment be initiated in individuals with symptomatic hypertension,
secondary hypertension, evidence of target organ damage (left ventricular hypertrophy), diabetes (type 1 and 2), and persistent hypertension after attempted life-style change (20). Unfortunately, these recommendations lack the support of clinical trials.
secondary hypertension, evidence of target organ damage (left ventricular hypertrophy), diabetes (type 1 and 2), and persistent hypertension after attempted life-style change (20). Unfortunately, these recommendations lack the support of clinical trials.
Table 49.1 Antihypertensive Medications with Pediatric Labeling (8) | ||||||||||||||||||||||
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Dietary modifications, weight reduction, and aerobic exercise are useful interventions in almost all children with hypertension (20). These nonpharmacologic therapies are often employed initially as the sole treatment in children with prehypertension (90th to 95th percentile) and stage I (95th to 99th percentile) primary hypertension who do not exhibit target organ damage and have few, if any, additional cardiovascular risk factors (38). It is important to note that nonpharmacologic therapies often augment the effectiveness of selected antihypertensive agents in both primary and secondary hypertension in children [e.g., sodium chloride restriction and angiotensin-converting enzyme (ACE) inhibitor therapy].
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Table 49.3 Individualization of Antihypertensive Therapy in Children: Factors to Consider | |||||||||||||||||
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In children, as in adults, many physicians have abandoned the traditional stepped-care approach to therapy. Individualized selection of therapeutic agents in children depends on many factors (Table 49.3).
Classification of Antihypertensive Agents
A scheme for classifying antihypertensive agents is presented in Table 49.4. Diuretics, although quite useful in the treatment of hypertension in children, are considered elsewhere (Chapter 43). Angiotensin-II-receptor antagonists (ARBs),
ACE inhibitors, calcium channel blockers (CCBs), adrenergic inhibitors, and direct vasodilators represent the main focus of this chapter.
ACE inhibitors, calcium channel blockers (CCBs), adrenergic inhibitors, and direct vasodilators represent the main focus of this chapter.
Table 49.4 Classification of Available Antihypertensive Agentsa | |||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
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Although initial data concerning the pharmacokinetics, effectiveness, and safety of antihypertensives in children are becoming available, the large-scale comparative trials conducted in adults that show superiority of one drug or one therapeutic approach over another have not been conducted in children. For a variety of reasons, it is unlikely that studies similar to the widely publicized Antihypertensive and Lipid-Lowering Treatment to Prevent Heart Attack Trial (ALLHAT) (39), which compared representative drugs from four different therapeutic classes in a population of 33,357 subjects, will be conducted in children in the foreseeable future. Many similar studies are ongoing in the adult population (40). Hence, in treating children with hypertension, choices among available drug classes rely less on specific comparative data collected from pediatric patients and more on the suspected cause of the elevated BP, previous clinical experience, extrapolation from studies conducted in adults, and availability of pediatric formulations. Recommended dosing for antihypertensive agents for children and adolescents (Table 49.5) and neonates (Table 49.6) is based on currently available information and may be subject to change depending on the outcome of ongoing studies. Antihypertensive agents used in the treatment of hypertensive emergencies and urgencies are presented in Table 49.7.
Adrenergic Agents
The sympathetic division of the autonomic nervous system plays a key role in the regulation of BP. At the postganglionic synapse, norepinephrine is released from vesicles in the presynaptic membrane in response to sympathetic stimulation and binds to receptors on postganglionic effector organs. Stimulation of sympathetic nerves terminating in the adrenal medulla results in release of epinephrine and, to a lesser extent, other catecholamines into circulating blood.
The effects of the adrenergic nervous system are mediated through α and β receptors, each of which has subtypes. The α1 adrenoceptors are located in the heart and smooth muscle in blood vessels, the intestinal tract, and the genitourinary tract. The cardiovascular effects of α1 stimulation include vasoconstriction, increased systemic vascular resistance, and increased BP. Stimulation of α2 receptors, which are located primarily at the postganglionic presynaptic membrane, inhibits further release of norepinephrine. Distinct subtypes of both α1 and α2 receptors have been identified. β1 – and β2 -adrenergic receptors are segregated based on their response to norepinephrine and epinephrine. The β1 receptors, located primarily in the heart, adipose tissue, and juxtaglomerular cells, respond equivalently to epinephrine and norepinephrine. Stimulation of β1 receptors results in tachycardia, increased myocardial contractility, increased conduction velocity in the atrioventricular node, and lipolysis. At β2 receptors, response to norepinephrine is much less than that seen after stimulation with epinephrine. The β2 receptors are found in many organs including the liver, skeletal muscle, and smooth muscle located in the vasculature and the gastrointestinal, respiratory, and genitourinary tracts. Stimulation of β2 receptors results in smooth muscle relaxation and bronchodilation, vasodilation, and increased glucose release. As with α receptors, distinct subtypes of both β1 and β2 receptors have been identified.
Table 49.5 Drug Therapy for Children and Adolescents with Chronic Hypertensiona | |||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
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Table 49.6 Drug Therapy for Hypertension in Neonatesa | |||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
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β-Adrenergic-receptor antagonists are distinguished by selectivity for the β1 -adrenergic receptor (Table 49.8), the presence of intrinsic sympathomimetic activity, unique pharmacologic properties (Table 49.9), and α-adrenergic blocking activity. Cardioselective drugs have greater affinity for β1 -adrenergic receptors, and nonselective agents have approximately equal affinity for both β1 – and β2 -adrenergic receptors. At higher doses, cardioselective agents may demonstrate not only β1 -antagonist activity but also some degree of β2 antagonism. Some β-adrenergic antagonists, including acebutolol and pindolol, have small but significant β-agonist effect, known as intrinsic sympathomimetic activity. Because the agonist effect is significantly less than the antagonist effect, the antihypertensive properties of these agents are not compromised. Intrinsic sympathomimetic activity of β-adrenergic blockers helps to reduce selected adverse effects resulting from β1 antagonism (e.g., bradycardia).
Adrenergic antagonists reversibly or irreversibly bind to α and β receptors. Receptor blockade antagonizes the effects of norepinephrine at the postganglionic synaptic membrane as well as circulating catecholamines. The resultant effects are complex and depend on the type of receptors that are blocked and the unique properties possessed by individual agents (41).
α-Adrenergic Antagonists
Chronic administration of peripheral α-adrenergic-receptor antagonists is uncommon in children. The prazosin arm of ALLHAT was stopped early because it was found to be inferior to other antihypertensive drugs (39). Clonidine, which stimulates central α2 receptors, resulting in inhibition of sympathetic outflow from the vasomotor center in the brain, is occasionally used when centrally mediated hypertension is suspected or selected comorbid conditions occur. Clonidine can be administered orally or transdermally. Transdermal clonidine has been useful in patients who are not compliant with oral dosing regimens. Some patients are unable to tolerate the adverse effects frequently associated with chronic oral administration of clonidine, including somnolence and xerostomia. Clonidine should be withdrawn slowly, as rebound hypertension may occur after abrupt cessation of therapy. Other central sympatholytics are rarely used to treat hypertension in ambulatory children.
Phentolamine and phenoxybenzamine are used to treat acute, severe BP elevation, which occurs in conditions associated with excess circulating catecholamines. Phentolamine is a competitive inhibitor of α1 and α2 receptors useful for short-term treatment of hypertension secondary to
pheochromocytoma. Phenoxybenzamine irreversibly blocks α1 and α2 receptors but, unlike phentolamine, can be administered orally. Blockade of α receptors decreases systemic vascular resistance and lowers the BP. Hypotension may occur at higher doses.
pheochromocytoma. Phenoxybenzamine irreversibly blocks α1 and α2 receptors but, unlike phentolamine, can be administered orally. Blockade of α receptors decreases systemic vascular resistance and lowers the BP. Hypotension may occur at higher doses.
Table 49.7 Drug Therapy for Hypertensive Urgencies and Emergencies in Pediatric Patients (Excluding Neonates) | ||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
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Table 49.8 Classification of β-Adrenergic-Receptor Antagonists | |||||||||||||||||||||||||||||||||||||||||||||||||||
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β-Adrenergic Antagonists
The β-adrenergic antagonists have been used to treat hypertension in children for more than 25 years. These agents attenuate sympathetic stimulation through competitive antagonism of epinephrine and norepinephrine at β-adrenergic receptors. Reversible blockade of β-adrenergic receptors lowers the BP by several means. Depending on the underlying pathology present in individual patients and the properties of individual drugs, the initial and long-term physiologic effects may differ (41). Proposed mechanisms for the antihypertensive effect of β-adrenergic antagonism include inhibition of β1 -adrenergic receptors of juxtaglomerular cells, thus inhibiting renin release (42,43); presynaptic facilitatory β2 -adrenergic receptors at the vascular wall; norepinephrine release from sympathetic nerve endings (44); and sympathetic outflow from the central nervous system (CNS) (45). The antihypertensive effect of β-adrenergic antagonists usually results from a combination of these factors.
The immediate systemic hemodynamic effects of β-adrenergic antagonists in hypertensive subjects are reduction in myocardial contractility, cardiac output, and heart rate. In the absence of β2 -adrenergic-induced vasodilation, peripheral vascular resistance increases due to unopposed α-adrenergic activity (46,47). With long-term use of β-adrenergic antagonist therapy, heart rate and cardiac output are reduced. Unexpectedly, long-term administration of β-adrenergic antagonists has been associated with a
gradual reduction in total peripheral resistance. Patients treated with β-adrenergic antagonists that possess intrinsic sympathomimetic ability are less likely to experience a drop in heart rate and cardiac output and generally manifest a lesser degree of reflex vasoconstriction (48).
gradual reduction in total peripheral resistance. Patients treated with β-adrenergic antagonists that possess intrinsic sympathomimetic ability are less likely to experience a drop in heart rate and cardiac output and generally manifest a lesser degree of reflex vasoconstriction (48).
Table 49.9 Pharmacology of Adrenergic Antagonists Commonly used in Children | ||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||||
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β-Adrenergic antagonists generally are well absorbed after oral administration (41). Bioavailability is variable due to variation in the extent of the first-pass effect. The oral bioavailability of β-adrenergic antagonists, commonly used in children, varies widely (Table 49.9). In adults, plasma concentrations of these drugs correlate poorly with pharmacologic effects (49,50). Genetic polymorphisms for the cytochrome P450 (CYP) 2D6 isozyme may explain the exaggerated effect observed in poor metabolizers following administration of agents that are inactivated by this pathway (41).
Clinical Use in Children
The β-adrenergic antagonists have been used to treat a wide variety of conditions in children. However, few studies have focused on the use of β-adrenergic antagonists to treat pediatric hypertension (51,52,53,54,55,56,57,58,59,60,61,62,63,64). With the advent of newer and safer drugs, β-adrenergic antagonists are used less often for the treatment of hypertension in children, but still play an important role in the management of hypertension associated with several conditions and in those children who have severe hypertension requiring multiple drugs.