Whipple's Transformation Of Legendre Functions
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In the theory of
special functions Special functions are particular mathematical functions that have more or less established names and notations due to their importance in mathematical analysis, functional analysis, geometry, physics, or other applications. The term is defined by ...
, Whipple's transformation for
Legendre functions In physical science and mathematics, the Legendre functions , and associated Legendre functions , , and Legendre functions of the second kind, , are all solutions of Legendre's differential equation. The Legendre polynomials and the associated ...
, named after
Francis John Welsh Whipple Francis John Welsh Whipple ScD FInstP (17 March 1876 – 25 September 1943) was an English mathematician, meteorologist and seismologist. From 1925 to 1939, he was superintendent of the Kew Observatory. Biography Whipple was the son of Kew Obse ...
, arise from a general expression, concerning associated Legendre functions. These formulae have been presented previously in terms of a viewpoint aimed at
spherical harmonic In mathematics and physical science, spherical harmonics are special functions defined on the surface of a sphere. They are often employed in solving partial differential equations in many scientific fields. Since the spherical harmonics form a ...
s, now that we view the equations in terms of
toroidal coordinates Toroidal coordinates are a three-dimensional orthogonal coordinate system that results from rotating the two-dimensional bipolar coordinate system about the axis that separates its two foci. Thus, the two foci F_1 and F_2 in bipolar coordina ...
, whole new symmetries of Legendre functions arise. For associated Legendre functions of the first and second kind, :P_^\biggl(\frac\biggr)= \frac and :Q_^\biggl(\frac\biggr)= -i(\pi/2)^\Gamma(-\nu-\mu)(z^2-1)^e^ P_\nu^\mu(z). These expressions are valid for all parameters \nu, \mu, and z. By shifting the complex degree and order in an appropriate fashion, we obtain Whipple formulae for general complex index interchange of general associated Legendre functions of the first and second kind. These are given by : P_^\mu(z)=\frac\biggl \pi\sin\mu\pi P_^\nu\biggl(\frac\biggr)+\cos\pi(\nu+\mu)e^Q_^\nu\biggl(\frac\biggr)\biggr and : Q_^\mu(z)=\frac\biggl P_^\nu\biggl(\frac\biggr)-\frace^\sin\nu\pi Q_^\nu\biggl(\frac\biggr)\biggr Note that these formulae are well-behaved for all values of the degree and order, except for those with integer values. However, if we examine these formulae for toroidal harmonics, i.e. where the degree is half-integer, the order is integer, and the argument is positive and greater than unity one obtains : P_^n(\cosh\eta)=\frac\sqrtQ_^m(\coth\eta) and : Q_^n(\cosh\eta)=\frac\sqrtP_^m(\coth\eta) . These are the Whipple formulae for toroidal harmonics. They show an important property of toroidal harmonics under index (the integers associated with the order and the degree) interchange.


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References

* {{cite journal , last=Cohl , first=Howard S. , author2=J.E. Tohline , author3=A.R.P. Rau , author4=H.M. Srivastava , title=Developments in determining the gravitational potential using toroidal functions , year=2000 , journal=
Astronomische Nachrichten ''Astronomische Nachrichten'' (''Astronomical Notes''), one of the first international journals in the field of astronomy, was established in 1821 by the German astronomer Heinrich Christian Schumacher. It claims to be the oldest astronomical jour ...
, volume=321 , issue=5/6 , pages=363–372 , doi=10.1002/1521-3994(200012)321:5/6<363::AID-ASNA363>3.0.CO;2-X, bibcode = 2000AN....321..363C Special functions