In mathematics, a Lamé function, or ellipsoidal harmonic function, is a solution of Lamé's equation, a second-order ordinary differential equation. It was introduced in the paper . Lamé's equation appears in the method of separation of variables applied to the Laplace equation in elliptic coordinates. In some special cases solutions can be expressed in terms of polynomials called Lamé polynomials.
Lamé's equation is
d2y | |
dx2 |
+(A+B\weierp(x))y=0,
where A and B are constants, and
\wp
B\weierp(x)=-\kappa2\operatorname{sn}2x
\operatorname{sn}
\kappa2=n(n+1)k2
k
By changing the independent variable to
t
t=\operatorname{sn}x
d2y | + | |
dt2 |
1 | \left( | |
2 |
1 | + | |
t-e1 |
1 | + | |
t-e2 |
1 | |
t-e3 |
\right)
dy | |
dt |
-
A+Bt | |
4(t-e1)(t-e2)(t-e3) |
y=0,
which after a change of variable becomes a special case of Heun's equation.
A more general form of Lamé's equation is the ellipsoidal equation or ellipsoidal wave equation which can be written (observe we now write
Λ
A
d2y | |
dx2 |
+(Λ-\kappa2\operatorname{sn}2x-\Omega2k4\operatorname{sn}4x)y=0,
where
k
\kappa
\Omega
\Omega=0
Λ=A
\Omega=0,k=0,\kappa=2h,Λ-2h2=λ,x=z\pm
\pi | |
2 |
d2y | |
dz2 |
+(λ-2h2\cos2z)y=0.
The Weierstrassian form of Lamé's equation is quite unsuitable for calculation (as Arscott also remarks, p. 191). The most suitable form of the equation is that in Jacobian form, as above. The algebraic and trigonometric forms are also cumbersome to use. Lamé equations arise in quantum mechanics as equations of small fluctuations about classical solutions—called periodic instantons, bounces or bubbles—of Schrödinger equations for various periodic and anharmonic potentials.[1] [2]
Asymptotic expansions of periodic ellipsoidal wave functions, and therewith also of Lamé functions, for large values of
\kappa
Λ
q
\begin{align} Λ(q)={}&q\kappa-
1 | |
23 |
(1+k2)(q2+1)-
q | |
26\kappa |
\{(1+k2)2(q2+3)-4k2(q2+5)\}\\[6pt] &{}-
1 | |
210\kappa2 |
\{(1+k2)3(5q4+34q2+9)-4k2(1+k2)(5q4+34q2+9)\\[6pt] &{}-384\Omega2k4(q2+1)\}- … , \end{align}
(another (fifth) term not given here has been calculated by Müller, the first three terms have also been obtained by Ince[6]). Observe terms are alternately even and odd in
q
\kappa
K(k)
\operatorname{Ec}(2K)=\operatorname{Ec}(0)=0, \operatorname{Es}(2K)=\operatorname{Es}(0)=0,
as well as (the prime meaning derivative)
' | |
(\operatorname{Ec}) | |
2K |
=
' | |
(\operatorname{Ec}) | |
0 |
=0,
' | |
(\operatorname{Es}) | |
2K |
=
' | |
(\operatorname{Es}) | |
0 |
=0,
defining respectively the ellipsoidal wave functions
q0 | |
\operatorname{Ec} | |
n, |
q0+1 | |
\operatorname{Es} | |
n, |
q0-1 | |
\operatorname{Ec} | |
n, |
q0 | |
\operatorname{Es} | |
n |
of periods
4K,2K,2K,4K,
q0=1,3,5,\ldots
q-q0=\mp2\sqrt{
2 | |
\pi |
Here the upper sign refers to the solutions
\operatorname{Ec}
\operatorname{Es}
Λ(q)
q0,
\begin{align} Λ\pm(q)\simeq{}&Λ(q0)+
(q-q | ||||
|
\right) | |
q0 |
+ … \\[6pt] ={}&Λ(q0)+(q-q0)\kappa\left[1-
| |||||||
22\kappa |
-
1 | |
26\kappa2 |
\{3(1+k2)2(q
2(q | |
0+1)-4k |
2 | |
0+2q |
0+5)\}+ … \right]\\[6pt] \simeq{}&Λ(q0)\mp2\kappa\sqrt{
2 | |
\pi |
In the limit of the Mathieu equation (to which the Lamé equation can be reduced) these expressions reduce to the corresponding expressions of the Mathieu case (as shown by Müller).