释义 |
Helmholtz Differential Equation--Spherical CoordinatesIn Spherical Coordinates, the Scale Factors are , , , andthe separation functions are , , , giving a StäckelDeterminant of . The Laplacian is
 | (1) |
To solve the Helmholtz Differential Equation in SphericalCoordinates, attempt Separation of Variables by writing
 | (2) |
Then the Helmholtz Differential Equation becomes
 | (3) |
Now divide by ,
 | (5) |
The solution to the second part of (5) must be sinusoidal, so the differential equation is
 | (6) |
which has solutions which may be defined either as a Complex function with , ..., 
 | (7) |
or as a sum of Real sine and cosine functions with , ..., 
 | (8) |
Plugging (6) back into (7),
 | (9) |
The radial part must be equal to a constant
 | (10) |
 | (11) |
But this is the Euler Differential Equation, so we try a series solution of the form
 | (12) |
Then | |  | (13) |
 | |  | (14) |
 | (15) |
This must hold true for all Powers of . For the term (with ),
 | (16) |
which is true only if and all other terms vanish. So for , . Therefore, thesolution of the component is given by
 | (17) |
Plugging (17) back into (9),
 | (18) |
 | (19) |
which is the associated Legendre Differential Equation for and , ..., . The generalComplex solution is therefore | |  | (20) | where
 | (21) |
are the (Complex) Spherical Harmonics. The general Real solution is
 | (22) |
Some of the normalization constants of can be absorbed by and , so this equation may appear in theform | |  | (23) | where
 | (24) |
 | (25) |
are the Even and Odd (real) Spherical Harmonics. If azimuthal symmetry is present, then is constant and the solution of the component is a Legendre Polynomial . Thegeneral solution is then
 | (26) |
Actually, the equation is separable under the more general condition that is of the form
 | (27) |
References
Morse, P. M. and Feshbach, H. Methods of Theoretical Physics, Part I. New York: McGraw-Hill, p. 514 and 658, 1953. |