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Date: 18-7-2018
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Date: 13-7-2018
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Date: 18-7-2018
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In spherical coordinates, the scale factors are ,
,
, and the separation functions are
,
,
, giving a Stäckel determinant of
.
The Laplacian is
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(1) |
To solve Laplace's equation in spherical coordinates, attempt separation of variables by writing
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(2) |
Then the Helmholtz differential equation becomes
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(3) |
Now divide by ,
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(4) |
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(5) |
The solution to the second part of (5) must be sinusoidal, so the differential equation is
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(6) |
which has solutions which may be defined either as a complex function with , ...,
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(7) |
or as a sum of real sine and cosine functions with , ...,
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(8) |
Plugging (6) back into (7),
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(9) |
The radial part must be equal to a constant
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(10) |
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(11) |
But this is the Euler differential equation, so we try a series solution of the form
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(12) |
Then
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(13) |
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(14) |
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(15) |
This must hold true for all powers of . For the
term (with
),
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(16) |
which is true only if and all other terms vanish. So
for
,
. Therefore, the solution of the
component is given by
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(17) |
Plugging (17) back into (◇),
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(18) |
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(19) |
which is the associated Legendre differential equation for and
, ...,
. The general complex solution is therefore
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(20) |
where
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(21) |
are the (complex) spherical harmonics. The general real solution is
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(22) |
Some of the normalization constants of can be absorbed by
and
, so this equation may appear in the form
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(23) |
where
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(24) |
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(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
. The general solution is then
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(26) |
REFERENCES:
Byerly, W. E. An Elementary Treatise on Fourier's Series, and Spherical, Cylindrical, and Ellipsoidal Harmonics, with Applications to Problems in Mathematical Physics. New York: Dover, p. 244, 1959.
Moon, P. and Spencer, D. E. Field Theory Handbook, Including Coordinate Systems, Differential Equations, and Their Solutions, 2nd ed. New York: Springer-Verlag, p. 27, 1988.
Morse, P. M. and Feshbach, H. Methods of Theoretical Physics, Part I. New York: McGraw-Hill, p. 514 and 658, 1953.
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