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[[Image:Gudermannian.svg|thumb|270px|right|Gudermannian function with its [[asymptote]]s ''y''&nbsp;=&nbsp;±π/2 marked in blue]]
The '''Gudermannian function''', named after [[Christoph Gudermann]] (1798–1852), relates the [[circular function]]s and [[hyperbolic function]]s without using [[complex numbers]].
 
It is defined by
 
:<math>\begin{align}{\rm{gd}}\,x&=\int_0^x\frac{\mathrm{d}t}{\cosh t} \\[8pt]
&=\arcsin\left(\tanh x \right)
 
=\mathrm{arctan}\left(\sinh x \right) \\[8pt]
&=2\arctan\left[\tanh\left(\tfrac12x\right)\right]
 
=2\arctan(e^x)-\tfrac12\pi.
\end{align}\,\!</math>
 
Some related formulas don't quite work as definitions. For example, for real ''x'', <math>\arccos\mathrm{sech}\,x = \vert\mathrm{gd}\,x\vert = \arcsec(\cosh x)</math>. (See [[inverse trigonometric function]]s.)
 
The following identities hold:
 
:<math>\begin{align}{\color{white}\dot{{\color{black}
\sin\mathrm{gd}\,x}}}&=\tanh x ;\quad
\csc\mathrm{gd}\,x=\coth x ;\\
\cos\mathrm{gd}\,x&=\mathrm{sech}\, x ;\quad\,
\sec\mathrm{gd}\,x=\cosh x ;\\
\tan\mathrm{gd}\,x&=\sinh x ;\quad\,
\cot\mathrm{gd}\,x=\mathrm{csch}\, x ;\\
{}_{\color{white}.}\tan\tfrac{1}{2}\mathrm{gd}\,x&=\tanh\tfrac{1}{2}x.
\end{align}\,\!</math>
 
[[Image:GudermannianInverse.svg|thumb|270px|right|The inverse Gudermannian function]]
 
The [[inverse function|inverse]] Gudermannian function, which is defined on the interval &minus;''π''/2&nbsp;<&nbsp;''x''&nbsp;<&nbsp;''π''/2, is given by
 
:<math>
\begin{align}
\operatorname{gd}^{-1}\,x & = \int_0^x\frac{\mathrm{d}t}{\cos t} \\[8pt]
& = \ln\left| \frac{1 + \sin x}{\cos x} \right| = \tfrac12\ln \left| \frac{1 + \sin x}{1 - \sin x} \right| \\[8pt]
& = \ln\left| \tan x +\sec x \right| = \ln \left| \tan\left(\tfrac14\pi + \tfrac12x\right) \right| \\[8pt]
& = \mathrm{artanh}\,(\sin x) = \mathrm{arsinh}\,(\tan x).
\end{align}
</math>
 
(See [[inverse hyperbolic function]]s.)
 
The [[derivative]]s of the Gudermannian and its inverse are
 
:<math>\frac{\mathrm{d}}{\mathrm{d}x}\;\mathrm{gd}\,x=\mathrm{sech}\, x;
\quad \frac{\mathrm{d}}{\mathrm{d}x}\;\operatorname{gd}^{-1}\,x=\sec x.</math>
 
The expression
 
:<math>\tfrac{1}{2}\pi - \mathrm{gd}\,x</math>
 
defines the [[angle of parallelism]] function in [[hyperbolic geometry]].
 
==History==
The function was introduced by [[Johann Heinrich Lambert]] in the 1760s at the same time as the [[hyperbolic functions]]. He called it the "transcendent angle," and it went by various names until 1862 when [[Arthur Cayley]] suggested it be given its current name as a tribute to Gudermann's work in the 1830s on the theory of special functions.<ref>George F. Becker, C. E. Van Orstrand. ''Hyperbolic functions.'' Read Books, 1931. Page xlix.</ref> Gudermann had published articles in ''[[Crelle's Journal]]'' that were collected in ''Theorie der potenzial- oder cyklisch-hyperbolischen functionen'' (1833), a book which expounded ''sinh'' and ''cosh'' to a wide audience (under the guises of <math>\mathfrak{Sin}</math> and <math>\mathfrak{Cos}</math>).
 
The notation ''gd'' first appears on page 19 of the ''[[Philosophical Magazine]]'', vol. XXIV, where Cayley starts by calling ''gd. u'' the inverse of the [[integral of the secant function]]:
 
:<math>u = \int_0^\phi \sec t \,\mathrm{d}t = \ln\tan\left(\tfrac14\pi+\tfrac12\phi\right)</math>
 
and then derives "the definition" of the transcendent:
 
:<math>\operatorname{gd} \,u = i^{-1}\ln\tan\left(\tfrac14\pi+\tfrac12ui\right)</math>
 
observing immediately that it is a real function of ''u''.
 
==Applications==
 
The Gudermannian of the [[latitude|latitudinal]] (due North/South) distance from the [[equator]] on a [[Mercator projection]] is the [[meridian arc]] length, i.e. actual latitude on the globe.
 
The Gudermannian appears in a non-periodic solution of the [[inverted pendulum]].<ref>John S. Robertson, "Gudermann and the Simple Pendulum", ''The College Mathematics Journal'' '''28''':4:271–276 (September 1997) [http://www.jstor.org/stable/2687148 at JSTOR]</ref>
 
==See also==
*[[Hyperbolic secant distribution]]
*[[Mercator projection]]
*[[Tangent half-angle formula]]
*[[Tractrix]]
*[[Trigonometric identity]]
 
==Notes==
{{reflist}}
 
==References==
* CRC ''Handbook of Mathematical Sciences'' 5th&nbsp;ed. pp. 323–325.
* {{mathworld|urlname=Gudermannian|title=Gudermannian}}
 
[[Category:Trigonometry]]
[[Category:Elementary special functions]]
[[Category:Exponentials]]

Revision as of 12:39, 24 December 2013

File:Gudermannian.svg
Gudermannian function with its asymptotes y = ±π/2 marked in blue

The Gudermannian function, named after Christoph Gudermann (1798–1852), relates the circular functions and hyperbolic functions without using complex numbers.

It is defined by

gdx=0xdtcosht=arcsin(tanhx)=arctan(sinhx)=2arctan[tanh(12x)]=2arctan(ex)12π.

Some related formulas don't quite work as definitions. For example, for real x, arccossechx=|gdx|=arcsec(coshx). (See inverse trigonometric functions.)

The following identities hold:

singdx˙=tanhx;cscgdx=cothx;cosgdx=sechx;secgdx=coshx;tangdx=sinhx;cotgdx=cschx;.tan12gdx=tanh12x.
File:GudermannianInverse.svg
The inverse Gudermannian function

The inverse Gudermannian function, which is defined on the interval −π/2 < x < π/2, is given by

gd1x=0xdtcost=ln|1+sinxcosx|=12ln|1+sinx1sinx|=ln|tanx+secx|=ln|tan(14π+12x)|=artanh(sinx)=arsinh(tanx).

(See inverse hyperbolic functions.)

The derivatives of the Gudermannian and its inverse are

ddxgdx=sechx;ddxgd1x=secx.

The expression

12πgdx

defines the angle of parallelism function in hyperbolic geometry.

History

The function was introduced by Johann Heinrich Lambert in the 1760s at the same time as the hyperbolic functions. He called it the "transcendent angle," and it went by various names until 1862 when Arthur Cayley suggested it be given its current name as a tribute to Gudermann's work in the 1830s on the theory of special functions.[1] Gudermann had published articles in Crelle's Journal that were collected in Theorie der potenzial- oder cyklisch-hyperbolischen functionen (1833), a book which expounded sinh and cosh to a wide audience (under the guises of Sin and Cos).

The notation gd first appears on page 19 of the Philosophical Magazine, vol. XXIV, where Cayley starts by calling gd. u the inverse of the integral of the secant function:

u=0ϕsectdt=lntan(14π+12ϕ)

and then derives "the definition" of the transcendent:

gdu=i1lntan(14π+12ui)

observing immediately that it is a real function of u.

Applications

The Gudermannian of the latitudinal (due North/South) distance from the equator on a Mercator projection is the meridian arc length, i.e. actual latitude on the globe.

The Gudermannian appears in a non-periodic solution of the inverted pendulum.[2]

See also

Notes

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References

  • CRC Handbook of Mathematical Sciences 5th ed. pp. 323–325.
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  1. George F. Becker, C. E. Van Orstrand. Hyperbolic functions. Read Books, 1931. Page xlix.
  2. John S. Robertson, "Gudermann and the Simple Pendulum", The College Mathematics Journal 28:4:271–276 (September 1997) at JSTOR