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28 Mathieu Functions and Hill’s EquationApplications

§28.32 Mathematical Applications

Contents

§28.32(i) Elliptical Coordinates and an Integral Relationship

If the boundary conditions in a physical problem relate to the perimeter of an ellipse, then elliptical coordinates are convenient. These are given by

The two-dimensional wave equation

then becomes

The separated solutions V(\xi,\eta)=v(\xi)w(\eta) can be obtained from the modified Mathieu’s equation (28.20.1) for v and from Mathieu’s equation (28.2.1) for w, where a is the separation constant and q=\tfrac{1}{4}c^{2}k^{2}.

This leads to integral equations and an integral relation between the solutions of Mathieu’s equation (setting \zeta=i\xi, z=\eta in (28.32.3)).

Let u(\zeta) be a solution of Mathieu’s equation (28.2.1) and K(z,\zeta) be a solution of

Also let \mathcal{L} be a curve (possibly improper) such that the quantity

approaches the same value when \zeta tends to the endpoints of \mathcal{L}. Then

defines a solution of Mathieu’s equation, provided that (in the case of an improper curve) the integral converges with respect to z uniformly on compact subsets of \Complex.

Kernels K can be found, for example, by separating solutions of the wave equation in other systems of orthogonal coordinates. See Schmidt and Wolf (1979).

§28.32(ii) Paraboloidal Coordinates

The general paraboloidal coordinate system is linked with Cartesian coordinates via

where c is a parameter, 0\leq\alpha<\infty, -\pi<\beta\leq\pi, and 0\leq\gamma<\infty. When the Helmholtz equation

28.32.8\nabla^{2}V+k^{2}V=0

is separated in this system, each of the separated equations can be reduced to the Whittaker–Hill equation (28.31.1), in which A,B are separation constants. Two conditions are used to determine A,B. The first is the 2\pi-periodicity of the solutions; the second can be their asymptotic form. For further information see Arscott (1967) for k^{2}<0, and Urwin and Arscott (1970) for k^{2}>0.