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Hyperbolic functions
Hyperbolic functions
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In mathematics, hyperbolic functions are analogues of the ordinary trigonometric functions, but defined using the hyperbola rather than the circle. Just as the points (cos t, sin t) form a circle with a unit radius, the points (cosh t, sinh t) form the right half of the unit hyperbola. Also, similarly to how the derivatives of sin(t) and cos(t) are cos(t) and –sin(t) respectively, the derivatives of sinh(t) and cosh(t) are cosh(t) and sinh(t) respectively.

Hyperbolic functions are used to express the angle of parallelism in hyperbolic geometry. They are used to express Lorentz boosts as hyperbolic rotations in special relativity. They also occur in the solutions of many linear differential equations (such as the equation defining a catenary), cubic equations, and Laplace's equation in Cartesian coordinates. Laplace's equations are important in many areas of physics, including electromagnetic theory, heat transfer, and fluid dynamics.

The basic hyperbolic functions are:[1]

from which are derived:[4]

corresponding to the derived trigonometric functions.

The inverse hyperbolic functions are:

  • inverse hyperbolic sine "arsinh" (also denoted "sinh−1", "asinh" or sometimes "arcsinh")[9][10][11]
  • inverse hyperbolic cosine "arcosh" (also denoted "cosh−1", "acosh" or sometimes "arccosh")
  • inverse hyperbolic tangent "artanh" (also denoted "tanh−1", "atanh" or sometimes "arctanh")
  • inverse hyperbolic cotangent "arcoth" (also denoted "coth−1", "acoth" or sometimes "arccoth")
  • inverse hyperbolic secant "arsech" (also denoted "sech−1", "asech" or sometimes "arcsech")
  • inverse hyperbolic cosecant "arcsch" (also denoted "arcosech", "csch−1", "cosech−1","acsch", "acosech", or sometimes "arccsch" or "arccosech")
A ray through the unit hyperbola x2y2 = 1 at the point (cosh a, sinh a), where a is twice the area between the ray, the hyperbola, and the x-axis. For points on the hyperbola below the x-axis, the area is considered negative (see animated version with comparison with the trigonometric (circular) functions).

The hyperbolic functions take a real argument called a hyperbolic angle. The magnitude of a hyperbolic angle is the area of its hyperbolic sector to xy = 1. The hyperbolic functions may be defined in terms of the legs of a right triangle covering this sector.

In complex analysis, the hyperbolic functions arise when applying the ordinary sine and cosine functions to an imaginary angle. The hyperbolic sine and the hyperbolic cosine are entire functions. As a result, the other hyperbolic functions are meromorphic in the whole complex plane.

By Lindemann–Weierstrass theorem, the hyperbolic functions have a transcendental value for every non-zero algebraic value of the argument.[12]

History

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The first known calculation of a hyperbolic trigonometry problem is attributed to Gerardus Mercator when issuing the Mercator map projection circa 1566. It requires tabulating solutions to a transcendental equation involving hyperbolic functions.[13]

The first to suggest a similarity between the sector of the circle and that of the hyperbola was Isaac Newton in his 1687 Principia Mathematica.[14]

Roger Cotes suggested to modify the trigonometric functions using the imaginary unit to obtain an oblate spheroid from a prolate one.[14]

Hyperbolic functions were formally introduced in 1757 by Vincenzo Riccati.[14][13][15] Riccati used Sc. and Cc. (sinus/cosinus circulare) to refer to circular functions and Sh. and Ch. (sinus/cosinus hyperbolico) to refer to hyperbolic functions.[14] As early as 1759, Daviet de Foncenex showed the interchangeability of the trigonometric and hyperbolic functions using the imaginary unit and extended de Moivre's formula to hyperbolic functions.[15][14]

During the 1760s, Johann Heinrich Lambert systematized the use functions and provided exponential expressions in various publications.[14][15] Lambert credited Riccati for the terminology and names of the functions, but altered the abbreviations to those used today.[15][16]

Notation

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Definitions

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Right triangles with legs proportional to sinh and cosh

With hyperbolic angle u, the hyperbolic functions sinh and cosh can be defined with the exponential function eu.[1][4] In the figure .

Exponential definitions

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sinh x is half the difference of ex and ex
cosh x is the average of ex and ex
  • Hyperbolic sine: the odd part of the exponential function, that is,
  • Hyperbolic cosine: the even part of the exponential function, that is,
sinh, cosh and tanh
csch, sech and coth
  • Hyperbolic tangent:
  • Hyperbolic cotangent: for x ≠ 0,
  • Hyperbolic secant:
  • Hyperbolic cosecant: for x ≠ 0,

Differential equation definitions

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The hyperbolic functions may be defined as solutions of differential equations: The hyperbolic sine and cosine are the solution (s, c) of the system with the initial conditions The initial conditions make the solution unique; without them any pair of functions would be a solution.

sinh(x) and cosh(x) are also the unique solution of the equation f ″(x) = f (x), such that f (0) = 1, f ′(0) = 0 for the hyperbolic cosine, and f (0) = 0, f ′(0) = 1 for the hyperbolic sine.

Complex trigonometric definitions

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Hyperbolic functions may also be deduced from trigonometric functions with complex arguments:

  • Hyperbolic sine:[1]
  • Hyperbolic cosine:[1]
  • Hyperbolic tangent:
  • Hyperbolic cotangent:
  • Hyperbolic secant:
  • Hyperbolic cosecant:

where i is the imaginary unit with i2 = −1.

The above definitions are related to the exponential definitions via Euler's formula (See § Hyperbolic functions for complex numbers below).

Characterizing properties

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Hyperbolic cosine

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It can be shown that the area under the curve of the hyperbolic cosine (over a finite interval) is always equal to the arc length corresponding to that interval:[17]

Hyperbolic tangent

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The hyperbolic tangent is the (unique) solution to the differential equation f ′ = 1 − f2, with f (0) = 0.[18][19]

Useful relations

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The hyperbolic functions satisfy many identities, all of them similar in form to the trigonometric identities. In fact, Osborn's rule[20] (named after George Osborn) states that one can convert any trigonometric identity (up to but not including sinhs or implied sinhs of 4th degree) for , , or and into a hyperbolic identity, by:

  1. expanding it completely in terms of integral powers of sines and cosines,
  2. changing sine to sinh and cosine to cosh, and
  3. switching the sign of every term containing a product of two sinhs.

Odd and even functions:

Hence:

Thus, cosh x and sech x are even functions; the others are odd functions.

Hyperbolic sine and cosine satisfy:

which are analogous to Euler's formula, and

which is analogous to the Pythagorean trigonometric identity.

One also has

for the other functions.

Sums of arguments

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particularly

Also:

Product formulas

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Subtraction formulas

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Also:[21]

Half argument formulas

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where sgn is the sign function.

If x ≠ 0, then[22]

Square formulas

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Inequalities

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The following inequality is useful in statistics:[23]

It can be proved by comparing the Taylor series of the two functions term by term.

Inverse functions as logarithms

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Derivatives

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Second derivatives

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Each of the functions sinh and cosh is equal to its second derivative, that is:

All functions with this property are linear combinations of sinh and cosh, in particular the exponential functions and .[24]

Standard integrals

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The following integrals can be proved using hyperbolic substitution:

where C is the constant of integration.

Taylor series expressions

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It is possible to express explicitly the Taylor series at zero (or the Laurent series, if the function is not defined at zero) of the above functions.

This series is convergent for every complex value of x. Since the function sinh x is odd, only odd exponents for x occur in its Taylor series.

This series is convergent for every complex value of x. Since the function cosh x is even, only even exponents for x occur in its Taylor series.

The sum of the sinh and cosh series is the infinite series expression of the exponential function.

The following series are followed by a description of a subset of their domain of convergence, where the series is convergent and its sum equals the function.

where:

Infinite products and continued fractions

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The following expansions are valid in the whole complex plane:

Comparison with circular functions

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Circle and hyperbola tangent at (1, 1) display geometry of circular functions in terms of circular sector area u and hyperbolic functions depending on hyperbolic sector area u.

The hyperbolic functions represent an expansion of trigonometry beyond the circular functions. Both types depend on an argument, either circular angle or hyperbolic angle.

Since the area of a circular sector with radius r and angle u (in radians) is r2u/2, it will be equal to u when r = 2. In the diagram, such a circle is tangent to the hyperbola xy = 1 at (1, 1). The yellow sector depicts an area and angle magnitude. Similarly, the yellow and red regions together depict a hyperbolic sector with area corresponding to hyperbolic angle magnitude.

The legs of the two right triangles with hypotenuse on the ray defining the angles are of length 2 times the circular and hyperbolic functions.

The hyperbolic angle is an invariant measure with respect to the squeeze mapping, just as the circular angle is invariant under rotation.[25]

The Gudermannian function gives a direct relationship between the circular functions and the hyperbolic functions that does not involve complex numbers.

The graph of the function is the catenary, the curve formed by a uniform flexible chain, hanging freely between two fixed points under uniform gravity.

Relationship to the exponential function

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The decomposition of the exponential function in its even and odd parts gives the identities and Combined with Euler's formula this gives for the general complex exponential function.

Additionally,

Hyperbolic functions for complex numbers

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Hyperbolic functions in the complex plane

Since the exponential function can be defined for any complex argument, we can also extend the definitions of the hyperbolic functions to complex arguments. The functions sinh z and cosh z are then holomorphic.

Relationships to ordinary trigonometric functions are given by Euler's formula for complex numbers: so:

Thus, hyperbolic functions are periodic with respect to the imaginary component, with period ( for hyperbolic tangent and cotangent).

See also

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References

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Revisions and contributorsEdit on WikipediaRead on Wikipedia
from Grokipedia
Hyperbolic functions are a class of mathematical functions analogous to the , but defined using the and associated with the geometry of the rather than the circle. The primary hyperbolic functions are the hyperbolic sine (sinh x), hyperbolic cosine (cosh x), and hyperbolic tangent (tanh x), with additional functions including hyperbolic secant (sech x), cosecant (csch x), and cotangent (coth x). These functions satisfy identities similar to those of trigonometric functions, such as cosh²x - sinh²x = 1, but they model and decay rather than periodic behavior. The hyperbolic functions were first developed in the 18th century, with Italian mathematician Vincenzo Riccati (1707–1775) introducing them through the geometry of the unit x² - y² = 1 to solve differential equations arising from physical problems. Shortly thereafter, (1728–1777) formalized their trigonometric-like properties and applications, linking them explicitly to exponential expressions. Their definitions are given by sinh x = (ex - e-x)/2 and cosh x = (ex + e-x)/2, from which tanh x = sinh x / cosh x follows, along with the reciprocal functions. Key properties include the even nature of cosh x (where cosh(-x) = cosh x) and the odd nature of sinh x (where sinh(-x) = -sinh x), with tanh x also odd and approaching ±1 asymptotically as x → ±∞. Derivatives follow simple rules, such as d/dx [cosh x] = sinh x and d/dx [sinh x] = cosh x, enabling their use in integration techniques. Addition formulas mirror trigonometric ones, for example, sinh(x + y) = sinh x cosh y + cosh x sinh y. Inverse hyperbolic functions, like arsinh x = ln(x + √(x² + 1)), are defined for appropriate domains and have logarithmic expressions. Hyperbolic functions have wide applications in physics and , including modeling the shape of hanging chains (catenaries, described by cosh x), satellite orbits, and wave propagation. In , they parameterize Lorentz transformations and describe in velocity addition. Their exponential foundations make them essential for solving differential equations in areas like and electrical circuits.

History and Notation

Historical Development

The study of hyperbolas dates back to , where they were first recognized as one of the conic sections. Around 350 BC, Menaechmus discovered the hyperbola while attempting to solve the Delian problem of duplicating the , describing it as the of a with a plane. Later, in the , provided a systematic treatment in his work Conics, naming the curve "" (meaning "excess") and developing its properties, including parametric representations that related points on the curve to parameters, laying foundational geometric insights that would later inspire hyperbolic functions. A key milestone in the evolution toward hyperbolic functions occurred in the late with the problem, which describes the shape of a hanging chain under gravity. In 1690, Jakob Bernoulli posed this challenge in Acta Eruditorum, and his brother solved it in 1691, deriving the curve's equation through differential methods, though without explicit hyperbolic terminology; the solution's form was later recognized as involving what became the hyperbolic cosine. This application highlighted the utility of such functions in solving differential equations related to physical curves. The formal introduction of hyperbolic functions emerged in the 18th century. In 1757, Italian mathematician Vincenzo Riccati pioneered their definition in the first volume of Opusculorum ad res physicas et mathematicas pertinentium, expressing sinh and cosh via integrals and linking them to the geometry of the unit , complete with addition formulas and derivatives; he denoted them as Sh and Ch. Building on this, provided the first systematic development in his 1761 memoir Mémoire sur les suites, published in 1768, where he defined them logarithmically as "sinus hyperbolicus" and "cosinus hyperbolicus," establishing their trigonometric analogies without complex numbers and popularizing their use in . Leonhard Euler advanced their exponential expressions, such as relating cosh x to (e^x + e^{-x})/2, in works like his 1748 , refining earlier integral forms into more accessible analytic tools. In the , a significant milestone came in 1908, when incorporated hyperbolic functions into , interpreting Lorentz transformations as hyperbolic rotations in , thus extending their role in physics.

Standard Notation

The standard notation for hyperbolic functions employs abbreviations that parallel those of , with an added "h" to denote the hyperbolic variant. The primary functions are denoted as follows: hyperbolic sine by sinhx\sinh x, hyperbolic cosine by coshx\cosh x, hyperbolic tangent by tanhx\tanh x, hyperbolic cotangent by cothx\coth x, hyperbolic secant by \sechx\sech x, and hyperbolic cosecant by \cschx\csch x. These symbols, introduced in the , facilitate consistency with trigonometric notation, where sinx\sin x corresponds to sinhx\sinh x and cosx\cos x to coshx\cosh x. Historical alternatives include \smx\sm x and \cmx\cm x for hyperbolic sine and cosine, respectively, as seen in early 20th-century mathematical tables. In physics and older , abbreviated forms such as shx\sh x and chx\ch x are common for hyperbolic sine and cosine. For , the notations sinh1x\sinh^{-1} x, cosh1x\cosh^{-1} x, tanh1x\tanh^{-1} x, coth1x\coth^{-1} x, \sech1x\sech^{-1} x, and \csch1x\csch^{-1} x are standard, with alternative arc notations like \arcsinhx\arcsinh x, \arccoshx\arccosh x, \artanhx\artanh x, and so on also widely used. Typographical guidelines recommend rendering these in italicized lowercase letters within mathematical expressions, with the full terms "hyperbolic sine" or "hyperbolic cosine" used in for clarity. Pronunciation typically follows "shine" for sinhx\sinh x, "cosh" for coshx\cosh x, and "thanch" for tanhx\tanh x, though regional variations exist, such as "sinch" or "cynsh" for sinhx\sinh x.

Definitions

Exponential Definitions

The hyperbolic sine and cosine functions are fundamentally defined in terms of the for real arguments xRx \in \mathbb{R}. The hyperbolic sine is given by sinhx=exex2,\sinh x = \frac{e^x - e^{-x}}{2}, while the hyperbolic cosine is coshx=ex+ex2.\cosh x = \frac{e^x + e^{-x}}{2}. These definitions provide a direct means for and reveal the functions' close ties to and decay. The remaining hyperbolic functions are derived from sinhx\sinh x and coshx\cosh x. The hyperbolic tangent is the ratio tanhx=sinhxcoshx\tanh x = \frac{\sinh x}{\cosh x}, the hyperbolic cotangent is cothx=coshxsinhx\coth x = \frac{\cosh x}{\sinh x}, the hyperbolic secant is \sechx=1coshx\sech x = \frac{1}{\cosh x}, and the hyperbolic cosecant is \cschx=1sinhx\csch x = \frac{1}{\sinh x}. These expressions maintain the real domain and inherit properties from their foundational components. A key behavioral aspect stems from the exponential forms: coshx\cosh x is an even function, satisfying cosh(x)=coshx\cosh(-x) = \cosh x, whereas sinhx\sinh x is odd, with sinh(x)=sinhx\sinh(-x) = -\sinh x. The derived functions follow suit, with tanhx\tanh x, cothx\coth x, and \cschx\csch x being odd, and \sechx\sech x even. As xx \to \infty, sinhx\sinh x \to \infty and coshx\cosh x \to \infty, while tanhx1\tanh x \to 1; symmetrically, as xx \to -\infty, sinhx\sinh x \to -\infty, coshx\cosh x \to \infty, and tanhx1\tanh x \to -1. These limits highlight the non-periodic, monotonic nature of the functions for large x|x|. The exponential definitions provide a real analog to the trigonometric functions, which are defined via the complex exponential in Euler's formula.

Differential Equation Definitions

Hyperbolic functions can be characterized as solutions to specific linear ordinary differential equations (ODEs). In particular, both the hyperbolic cosine and hyperbolic sine functions serve as fundamental solutions to the second-order linear homogeneous ODE d2ydx2y=0.\frac{d^2 y}{dx^2} - y = 0. The general solution to this equation is given by y(x)=Acoshx+Bsinhx,y(x) = A \cosh x + B \sinh x, where AA and BB are arbitrary constants determined by initial conditions. This form arises because the characteristic equation r21=0r^2 - 1 = 0 has roots r=±1r = \pm 1, leading to the linear combination of exe^x and exe^{-x}, though the hyperbolic basis emphasizes the even and odd components. The individual functions are uniquely specified by their initial conditions at x=0x = 0: cosh0=1\cosh 0 = 1 and sinh0=0\sinh 0 = 0, with derivatives satisfying ddxcoshx=sinhx\frac{d}{dx} \cosh x = \sinh x and ddxsinhx=coshx\frac{d}{dx} \sinh x = \cosh x. These conditions ensure that coshx\cosh x and sinhx\sinh x form a basis for the solution space, guaranteeing uniqueness for the . Additionally, the hyperbolic sine can be defined as the unique solution to the first-order nonlinear ODE dydx=1+y2,\frac{dy}{dx} = \sqrt{1 + y^2},
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