A second-order Ordinary Differential Equation arising in the study of stellar interiors. It is given by
|
(1) |
|
(2) |
It has the Boundary Conditions
Solutions for , 1, 2, 3, and 4 are shown above. The cases , 1, and 5 can be solved analytically
(Chandrasekhar 1967, p. 91); the others must be obtained numerically.
For (
), the Lane-Emden Differential Equation is
|
(5) |
(Chandrasekhar 1967, pp. 91-92). Directly solving gives
|
(6) |
|
(7) |
|
(8) |
|
(9) |
|
(10) |
|
(11) |
The Boundary Condition then gives and , so
|
(12) |
and is Parabolic.
For (), the differential equation becomes
|
(13) |
|
(14) |
which is the Spherical Bessel Differential Equation
|
(15) |
with and , so the solution is
|
(16) |
Applying the Boundary Condition gives
|
(17) |
where is a Spherical Bessel Function of the First Kind (Chandrasekhar 1967, pp. 92).
For , make Emden's transformation
which reduces the Lane-Emden equation to
|
(20) |
(Chandrasekhar 1967, p. 90). After further manipulation (not reproduced here), the equation becomes
|
(21) |
and then, finally,
|
(22) |
References
Chandrasekhar, S. An Introduction to the Study of Stellar Structure. New York: Dover, pp. 84-182, 1967.
© 1996-9 Eric W. Weisstein
1999-05-26