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 
![\begin{displaymath}
{d\over dr}\left({r^2{dR\over dr}}\right)+[k^2r^2-n(n+1)]R=0
\end{displaymath}](l1_567.gif)  | 
(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