Hyperbolic functions


In mathematics, hyperbolic functions are analogues of the ordinary trigonometric functions, but defined using the hyperbola rather than the circle. Just as the points form a circle with a unit radius, the points form the right half of the unit hyperbola. Also, similarly to how the derivatives of and are and respectively, the derivatives of and are and 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, 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:
  • hyperbolic sine "",
  • hyperbolic cosine "",
from which are derived:
  • hyperbolic tangent "",
  • hyperbolic cotangent "",
  • hyperbolic secant "",
  • hyperbolic cosecant "" or ""
corresponding to the derived trigonometric functions.
The inverse hyperbolic functions are:
  • inverse hyperbolic sine ""
  • inverse hyperbolic cosine ""
  • inverse hyperbolic tangent ""
  • inverse hyperbolic cotangent ""
  • inverse hyperbolic secant ""
  • inverse hyperbolic cosecant ""
File:Hyperbolic functions-2.svg|thumb|upright=1.4|A ray through the unit hyperbola at the point, where is twice the area between the ray, the hyperbola, and the -axis. For points on the hyperbola below the -axis, the area is considered negative.
The hyperbolic functions take an argument called a hyperbolic angle. The magnitude of a hyperbolic angle is the area of its hyperbolic sector to. 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.

History

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.
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.
Roger Cotes suggested to modify the trigonometric functions using the imaginary unit to obtain an oblate spheroid from a prolate one.
Hyperbolic functions were formally introduced in 1757 by Vincenzo Riccati. Riccati used and to refer to circular functions and and to refer to hyperbolic functions. 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.
During the 1760s, Johann Heinrich Lambert systematized the use functions and provided exponential expressions in various publications. Lambert credited Riccati for the terminology and names of the functions, but altered the abbreviations to those used today.

Notation

Definitions

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

Exponential definitions

  • Hyperbolic sine: the odd part of the exponential function, that is,
  • Hyperbolic cosine: the even part of the exponential function, that is,
  • Hyperbolic tangent:
  • Hyperbolic cotangent: for,
  • Hyperbolic secant:
  • Hyperbolic cosecant: for,

    Differential equation definitions

The hyperbolic functions may be defined as solutions of differential equations: The hyperbolic sine and cosine are the solution of the system
with the initial conditions The initial conditions make the solution unique; without them any pair of functions would be a solution.
and are also the unique solution of the equation,
such that, for the hyperbolic cosine, and, for the hyperbolic sine.

Complex trigonometric definitions

Hyperbolic functions may also be deduced from trigonometric functions with complex arguments:
  • Hyperbolic sine:
  • Hyperbolic cosine:
  • Hyperbolic tangent:
  • Hyperbolic cotangent:
  • Hyperbolic secant:
  • Hyperbolic cosecant:
where is the imaginary unit with.
The above definitions are related to the exponential definitions via Euler's formula.

Characterizing properties

Hyperbolic cosine

It can be shown that the area under the curve of the hyperbolic cosine is always equal to the arc length corresponding to that interval:

Hyperbolic tangent

The hyperbolic tangent is the solution to the differential equation, with.

Useful relations

The hyperbolic functions satisfy many identities, all of them similar in form to the trigonometric identities. In fact, Osborn's rule states that one can convert any trigonometric identity 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:
Reciprocals:
Analogous to Euler's formula:
Analogous to the Pythagorean trigonometric identity:

Sums and differences of arguments

particularly

Addition and subtraction formulas

Product formulas

Half argument formulas

where is the sign function.
If then

Tangent half argument formulas

When,

Square formulas

Inequalities

The following inequality is useful in statistics:
It can be proved by comparing the Taylor series of the two functions term by term.

Inverse functions as logarithms

Derivatives

Second derivatives

Each of the functions and is equal to its second derivative, that is:
All functions with this property are linear combinations of and, in particular the exponential functions and.

Standard integrals

The following integrals can be proved using hyperbolic substitution:
where C is the constant of integration.

Taylor series expressions

It is possible to express explicitly the Taylor series at zero of the above functions.
This series is convergent for every complex value of. Since the function is odd, only odd exponents for occur in its Taylor series.
This series is convergent for every complex value of. Since the function is even, only even exponents for 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:
The following expansions are valid in the whole complex plane:

Comparison with circular functions

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 and angle is, it will be equal to when. In the diagram, such a circle is tangent to the hyperbola at. 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 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.
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

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

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 and 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 .