Appendix/Mathematics/Hypergeometric: Difference between revisions
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Revision as of 22:16, 26 October 2022
Hypergeometric Differential Equation
According to §9.151 (p. 1045) of Gradshteyn & Ryzhik (1965), "… a hypergeometric series is one of the solutions of the differential equation,
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which is called the hypergeometric equation. And, according to §9.10 (p. 1039) of Gradshteyn & Ryzhik (1965), "A hypergeometric series is a series of the form,
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Among other attributes, Gradshteyn & Ryzhik (1965) note that this, "… series terminates if or is equal to a negative integer or to zero."
LAWE
Drawing from an accompanying discussion, we have the,
where,
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Multiplying through by , and making the variable substitutions,
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the LAWE may be rewritten as,
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If we furthermore adopt the variable definition,
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we obtain equation (1) of R. Van der Borght (1970), namely,
Borght's LAWE
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Example Density- and Pressure-Profiles
| Properties of Analytically Defined, Spherically Symmetric, Equilibrium Structures | |||||
|---|---|---|---|---|---|
| Model | |||||
| Uniform-density | |||||
| Linear | |||||
| Parabolic | |||||
| Polytrope | |||||
Uniform Density
In the case of a uniform-density, incompressible configuration, Borght's LAWE becomes,
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Given that, in the equilibrium state,
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we obtain the LAWE derived by 📚 T. E. Sterne (1937, MNRAS, Vol. 97, pp. 582 - 593) — see his equation (1.91) on p. 585 — namely,
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where,
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This also matches equations (8) and (9) of Kopal (1948), aside from what, we presume, is a type-setting error that appears in the numerator of the second term on the RHS of his equation (8) — appears, whereas it should be .
See Also
- 📚 T. E. Sterne (1937, MNRAS, Vol. 97, pp. 582 - 593): Models of Radial Oscillation
- 📚 C. Prasad (1948, MNRAS, Vol. 108, pp. 414 - 416): Radial Oscillations of a Particular Stellar Model
- Z. Kopal (1948, Proceedings of the National Academy of Sciences, Vol. 34, pp. 377 - 384, Radial Oscillations of the Limiting Models of Polytropic Gas Spheres.
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In an article titled, "Radial Oscillations of a Stellar Model," C. Prasad (1949, MNRAS, 109, 103) investigated the properties of an equilibrium configuration with a prescribed density distribution given by the expression,
where, is the central density and, is the radius of the star.
- R. Van der Borght (1970, Proceedings of the Astronomical Society of Australia, Vol. 1, Issue 7, pp. 325 - 326), Adiabatic Oscillations of Stars.
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MathProjects/EigenvalueProblemN1: In the most general context, the LAWE takes the form,
Properties of Analytically Defined Astrophysical Structures Model Uniform-density Linear Parabolic Polytrope
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