A second-order ordinary differential equation arising in the study of stellar interiors, also called the polytropic differential equations. It is given by
(1)
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(2)
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(Zwillinger 1997, pp. 124 and 126). It has the boundary conditions
(3)
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(4)
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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)
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(Chandrasekhar 1967, pp. 91-92). Directly solving gives
(6)
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(7)
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(8)
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(9)
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(10)
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(11)
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The boundary condition then gives and , so
(12)
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and is parabolic.
For (), the differential equation becomes
(13)
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(14)
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which is the spherical Bessel differential equation
(15)
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with and , so the solution is
(16)
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Applying the boundary condition gives
(17)
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where is a spherical Bessel function of the first kind (Chandrasekhar 1967, p. 92).
For , make Emden's transformation
(18)
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(19)
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which reduces the Lane-Emden equation to
(20)
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(Chandrasekhar 1967, p. 90). After further manipulation (not reproduced here), the equation becomes
(21)
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and then, finally,
(22)
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