Prolate spheroidal coordinates are a three-dimensional orthogonal coordinate system that results from rotating the two-dimensional elliptic coordinate system about the focal axis of the ellipse, i.e., the symmetry axis on which the foci are located. Rotation about the other axis produces oblate spheroidal coordinates. Prolate spheroidal coordinates can also be considered as a limiting case of ellipsoidal coordinates in which the two smallest principal axes are equal in length.
Prolate spheroidal coordinates can be used to solve various partial differential equations in which the boundary conditions match its symmetry and shape, such as solving for a field produced by two centers, which are taken as the foci on the z-axis. One example is solving for the wavefunction of an electron moving in the electromagnetic field of two positively charged nuclei, as in the hydrogen molecular ion, H2+. Another example is solving for the electric field generated by two small electrode tips. Other limiting cases include areas generated by a line segment (μ = 0) or a line with a missing segment (ν=0). The electronic structure of general diatomic molecules with many electrons can also be solved to excellent precision in the prolate spheroidal coordinate system.[1]
The most common definition of prolate spheroidal coordinates
(\mu,\nu,\varphi)
x=a\sinh\mu\sin\nu\cos\varphi
y=a\sinh\mu\sin\nu\sin\varphi
z=a\cosh\mu\cos\nu
where
\mu
\nu\in[0,\pi]
\varphi
[0,2\pi]
The trigonometric identity
z2 | |
a2\cosh2\mu |
+
x2+y2 | |
a2\sinh2\mu |
=\cos2\nu+\sin2\nu=1
shows that surfaces of constant
\mu
z2 | |
a2\cos2\nu |
-
x2+y2 | |
a2\sin2\nu |
=\cosh2\mu-\sinh2\mu=1
shows that surfaces of constant
\nu
The distances from the foci located at
(x,y,z)=(0,0,\pma)
r\pm=\sqrt{x2+y2+(z\mpa)2}=a(\cosh\mu\mp\cos\nu).
The scale factors for the elliptic coordinates
(\mu,\nu)
h\mu=h\nu=a\sqrt{\sinh2\mu+\sin2\nu}
whereas the azimuthal scale factor is
h\varphi=a\sinh\mu\sin\nu,
resulting in a metric of
\begin{align} ds2&=
2 | |
h | |
\mu |
d\mu2+
2 | |
h | |
\nu |
d\nu2+
2 | |
h | |
\varphi |
d\varphi2\\ &=a2\left[(\sinh2\mu+\sin2\nu)d\mu2+(\sinh2\mu+\sin2\nu)d\nu2+(\sinh2\mu\sin2\nu)d\varphi2\right]. \end{align}
Consequently, an infinitesimal volume element equals
dV=a3\sinh\mu\sin\nu(\sinh2\mu+\sin2\nu)d\mud\nud\varphi
and the Laplacian can be written
\begin{align} \nabla2\Phi={}&
1 | |
a2(\sinh2\mu+\sin2\nu) |
\left[
\partial2\Phi | |
\partial\mu2 |
+
\partial2\Phi | |
\partial\nu2 |
+\coth\mu
\partial\Phi | |
\partial\mu |
+\cot\nu
\partial\Phi | |
\partial\nu |
\right]\\[6pt] &{}+
1 | |
a2\sinh2\mu\sin2\nu |
\partial2\Phi | |
\partial\varphi2 |
\end{align}
Other differential operators such as
\nabla ⋅ F
\nabla x F
(\mu,\nu,\varphi)
An alternative and geometrically intuitive set of prolate spheroidal coordinates
(\sigma,\tau,\phi)
\sigma=\cosh\mu
\tau=\cos\nu
\sigma
\tau
\tau
\sigma
\sigma
\tau
F1
F2
d1+d2
2a\sigma
d1-d2
2a\tau
F1
a(\sigma+\tau)
F2
a(\sigma-\tau)
F1
F2
z=-a
z=+a
\sigma
\tau
\varphi
\sigma=
1 | |
2a |
\left(\sqrt{x2+y2+(z+a)2}+\sqrt{x2+y2+(z-a)2}\right)
\tau=
1 | |
2a |
\left(\sqrt{x2+y2+(z+a)2}-\sqrt{x2+y2+(z-a)2}\right)
\varphi=\arctan\left(
y | |
x |
\right)
Unlike the analogous oblate spheroidal coordinates, the prolate spheroid coordinates (σ, τ, φ) are not degenerate; in other words, there is a unique, reversible correspondence between them and the Cartesian coordinates
x=a\sqrt{(\sigma2-1)(1-\tau2)}\cos\varphi
y=a\sqrt{(\sigma2-1)(1-\tau2)}\sin\varphi
z=a \sigma \tau
The scale factors for the alternative elliptic coordinates
(\sigma,\tau,\varphi)
h\sigma=a\sqrt{
\sigma2-\tau2 | |
\sigma2-1 |
h\tau=a\sqrt{
\sigma2-\tau2 | |
1-\tau2 |
while the azimuthal scale factor is now
h\varphi=a\sqrt{\left(\sigma2-1\right)\left(1-\tau2\right)}
Hence, the infinitesimal volume element becomes
dV=a3(\sigma2-\tau2)d\sigmad\taud\varphi
and the Laplacian equals
\begin{align} \nabla2\Phi={}&
1 | |
a2(\sigma2-\tau2) |
\left\{
\partial | |
\partial\sigma |
\left[ \left(\sigma2-1\right)
\partial\Phi | |
\partial\sigma |
\right]+
\partial | |
\partial\tau |
\left[(1-\tau2)
\partial\Phi | |
\partial\tau |
\right] \right\}\\ &{}+
1 | |
a2(\sigma2-1)(1-\tau2) |
\partial2\Phi | |
\partial\varphi2 |
\end{align}
Other differential operators such as
\nabla ⋅ F
\nabla x F
(\sigma,\tau)
As is the case with spherical coordinates, Laplace's equation may be solved by the method of separation of variables to yield solutions in the form of prolate spheroidal harmonics, which are convenient to use when boundary conditions are defined on a surface with a constant prolate spheroidal coordinate (See Smythe, 1968).