Appendix/Mathematics/Hypergeometric

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,

$0$

$=$

$z(1-z)\frac{d^{2}u}{d{z}^2}+[\gamma -(\alpha +\beta +1)z]\frac{du}{dz}-\alpha \beta u,$

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,

$F(\alpha ,\beta ;\gamma ;z)$

$=$

$1+\left[\frac{\alpha \cdot \beta }{\gamma \cdot 1}\right]z+\left[\frac{\alpha (\alpha +1)\beta (\beta +1)}{\gamma (\gamma +1)\cdot 1\cdot 2}\right]z^2+\left[\frac{\alpha (\alpha +1)(\alpha +2)\beta (\beta +1)(\beta +2)}{\gamma (\gamma +1)(\gamma +2)\cdot 1\cdot 2\cdot 3}\right]z^3+\dots$

Among other attributes, Gradshteyn & Ryzhik (1965) note that this, "… series terminates if $\alpha$ or $\beta$ is equal to a negative integer or to zero."

LAWE

Drawing from an accompanying discussion, we have the,

LAWE:   Linear Adiabatic Wave (or Radial Pulsation) Equation

$\frac{d^{2}x}{d{r}_0^2}+[\frac{4}{r_0}-(\frac{g_0{\rho }_0}{P_0}\left)\right]\frac{dx}{d{r}_0}+\left(\frac{{\rho }_0}{{\gamma }_{\mathrm{g}}{P}_0}\right)[{\omega }^2+(4-3{\gamma }_{\mathrm{g}})\frac{g_0}{r_0}]x=0$

where,

$g_0$

$=$

$-\frac{1}{{\rho }_0}\frac{d{P}_0}{d{r}_0}.$

Multiplying through by $R^2$, and making the variable substitutions,

$x$	$\to$	$\xi ,$
$\frac{r_0}{R}$	$\to$	$x,$
$(4-3{\gamma }_g)$	$\to$	$-\alpha {\gamma }_g,$

the LAWE may be rewritten as,

$0$	$=$	$\frac{d^2\xi }{d{x}^2}+[\frac{4}{x}-(\frac{g_0{\rho }_{0}R}{P_0}\left)\right]\frac{d\xi }{dx}+\left(\frac{{\rho }_0{R}^2}{{\gamma }_{\mathrm{g}}{P}_0}\right)[{\omega }^2-\frac{\alpha {\gamma }_g{g}_0}{Rx}]\xi$
	$=$	$\frac{d^2\xi }{d{x}^2}+\frac{1}{x}[4-(\frac{g_0{\rho }_0{r}_0}{P_0}\left)\right]\frac{d\xi }{dx}+\left[\right(\frac{{\omega }^2{\rho }_0{R}^2}{{\gamma }_{\mathrm{g}}{P}_0})-\frac{\alpha }{x^2}(\frac{g_0{\rho }_0{r}_0}{P_0}\left)\right]\xi .$

If we furthermore adopt the variable definition,

$\mu$

$\equiv$

$\left(\frac{g_0{\rho }_0{r}_0}{P_0}\right)=-\frac{d\ln P_0}{d\ln r_0},$

we obtain equation (1) of R. Van der Borght (1970), namely,

Borght's LAWE

$0$

$=$

$\frac{d^2\xi }{d{x}^2}+\frac{(4-\mu )}{x}\cdot \frac{d\xi }{dx}+\left[\right(\frac{{\omega }^2{\rho }_0{R}^2}{{\gamma }_{\mathrm{g}}{P}_0})-\frac{\alpha \mu }{x^2}]\xi .$

Example Density- and Pressure-Profiles

Properties of Analytically Defined, Spherically Symmetric, Equilibrium Structures
Model	$\rho (x)$	$P(x)$	$P^{\text{'}}(x)$	$\mu (x)$	$\frac{\rho (x)}{P(x)}$
Uniform-density	$1$	$1-x^2$	$-2x$	$\frac{2x^2}{(1-x^2)}$	$\frac{1}{(1-x^2)}$
Linear	$1-x$	$(1-x{)}^2(1+2x-\frac{9}{5}{x}^2)$	$-\frac{12}{5}x(1-x)(4-3x)$	$\frac{\frac{12}{5}{x}^2(4-3x)}{(1-x)(1+2x-\frac{9}{5}{x}^2)}$	$\frac{1}{(1-x)(1+2x-\frac{9}{5}{x}^2)}$
Parabolic	$1-x^2$	$(1-x^2{)}^2(1-\frac{1}{2}{x}^2)$	$-x(1-x^2)(5-3x^2)$	$\frac{x^2(5-3x^2)}{(1-x^2)(1-\frac{1}{2}{x}^2)}$	$\frac{1}{(1-x^2)(1-\frac{1}{2}{x}^2)}$
$n=1$ Polytrope	$\frac{\sin x}{x}$	$(\frac{\sin x}{x}{)}^2$	$\frac{2}{x}[\cos x-\frac{\sin x}{x}]\frac{\sin x}{x}$	$2(1-x\cot x)$	$\frac{x}{\sin x}$

Uniform Density

In the case of a uniform-density, incompressible configuration, Borght's LAWE becomes,

$0$

$=$

$\frac{d^2\xi }{d{x}^2}+\frac{(4-\mu )}{x}\cdot \frac{d\xi }{dx}+\left[\right(\frac{{\omega }^2{\rho }_0{R}^2}{{\gamma }_{\mathrm{g}}{P}_0})-\frac{\alpha \mu }{x^2}]\xi .$

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.
• 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,

  $\rho (r)={\rho }_c[1-(\frac{r}{R}{)}^2],$

  where, ${\rho }_c$ is the central density and, $R$ 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.
• MathProjects/EigenvalueProblemN1:   In the most general context, the LAWE takes the form,

  $\left[P\right]\frac{d^2{{𝒢}}_{\sigma }}{d{x}^2}+[\frac{4P}{x}+P^{\text{'}}]\frac{d{{𝒢}}_{\sigma }}{dx}+[{\sigma }^2\rho +\frac{\alpha P^{\text{'}}}{x}]{{𝒢}}_{\sigma }$

  $=$

  $0.$

  Properties of Analytically Defined Astrophysical Structures
  Model	$\rho (x)$	$P(x)$	$P^{\text{'}}(x)$
  Uniform-density	$1$	$1-x^2$	$-2x$
  Linear	$1-x$	$(1-x{)}^2(1+2x-\frac{9}{5}{x}^2)$	$-\frac{12}{5}x(1-x)(4-3x)$
  Parabolic	$1-x^2$	$(1-x^2{)}^2(1-\frac{1}{2}{x}^2)$	$-x(1-x^2)(5-3x^2)$
  $n=1$ Polytrope	$\frac{\sin x}{x}$	$[\frac{\sin x}{x}{]}^2$	$\frac{2}{x}[\cos x-\frac{\sin x}{x}]\frac{\sin x}{x}$