Appendix/Mathematics/Hypergeometric: Difference between revisions

From jetwiki
Jump to navigation Jump to search
Line 261: Line 261:
   <td align="left">
   <td align="left">
<math>
<math>
\frac{d^2\xi}{dx^2} + \frac{(4-\mu)}{x} \cdot \frac{d\xi}{dx}  
\frac{d^2 f}{dx^2} + \frac{(4-\mu)}{x} \cdot \frac{d f}{dx}  
+ \biggl[\biggl(\frac{\omega^2\rho_0 R^2}{\gamma_\mathrm{g} P_0} \biggr)  
+ \biggl[\biggl(\frac{\omega^2\rho_0 R^2}{\gamma_\mathrm{g} P_0} \biggr)  
- \frac{\alpha \mu}{x^2} \biggr]\xi
- \frac{\alpha \mu}{x^2} \biggr] f
</math>
</math>
   </td>
   </td>
Line 277: Line 277:
   <td align="left">
   <td align="left">
<math>
<math>
\frac{d^2\xi}{dx^2} + \frac{1}{x}\biggl[ 4 - \frac{2x^2}{(1-x^2)} \biggr] \frac{d\xi}{dx}  
\frac{d^2 f}{dx^2} + \frac{1}{x}\biggl[ 4 - \frac{2x^2}{(1-x^2)} \biggr] \frac{d f}{dx}  
+ \biggl[\biggl(\frac{\omega^2\rho_c R^2}{\gamma_\mathrm{g} P_c} \biggr) \frac{1}{(1-x^2)}
+ \biggl[\biggl(\frac{\omega^2\rho_c R^2}{\gamma_\mathrm{g} P_c} \biggr) \frac{1}{(1-x^2)}
- \biggl(\frac{2\alpha }{1-x^2}\biggr) \biggr]\xi
- \biggl(\frac{2\alpha }{1-x^2}\biggr) \biggr] f
</math>
</math>
   </td>
   </td>
Line 293: Line 293:
   <td align="left">
   <td align="left">
<math>
<math>
(1-x^2) \cdot \frac{d^2\xi}{dx^2} + \frac{1}{x}\biggl[ 4 - 6x^2 \biggr] \frac{d\xi}{dx}  
(1-x^2) \cdot \frac{d^2 f}{dx^2} + \frac{1}{x}\biggl[ 4 - 6x^2 \biggr] \frac{d f}{dx}  
+ \biggl[\biggl(\frac{\omega^2\rho_c R^2}{\gamma_\mathrm{g} P_c} \biggr)  
+ \biggl[\biggl(\frac{\omega^2\rho_c R^2}{\gamma_\mathrm{g} P_c} \biggr)  
- 2\alpha \biggr]\xi \, .
- 2\alpha \biggr] f \, .
</math>
</math>
   </td>
   </td>
Line 317: Line 317:
</tr>
</tr>
</table>
</table>
we obtain the LAWE derived by [[SSC/Stability/UniformDensity#Setup_as_Presented_by_Sterne_(1937)|Sterne37]], namely,
<table border=0 cellpadding=2 align="center">
<tr>
  <td align="right">
<math>0</math>
  </td>
  <td align="center">
<math>=</math>
  </td>
  <td align="left">
<math>
(1-x^2) \cdot \frac{d^2 f}{dx^2} + \frac{1}{x}\biggl[ 4 - 6x^2 \biggr] \frac{d f}{dx}
+ \biggl[6\biggl(\frac{\omega^2}{4\pi \gamma_\mathrm{g} G \rho_c} \biggr)
- 2\alpha \biggr] f
</math>
  </td>
</tr>
<tr>
  <td align="right">
&nbsp;
  </td>
  <td align="center">
<math>=</math>
  </td>
  <td align="left">
<math>
(1-x^2) \cdot \frac{d^2 f}{dx^2} + \frac{1}{x}\biggl[ 4 - 6x^2 \biggr] \frac{d f}{dx}
+ \mathfrak{F} f \, ,
</math>
  </td>
</tr>
</table>
where,
<table border=0 cellpadding=2 align="center">
<tr>
  <td align="right">
<math>\mathfrak{F}</math>
  </td>
  <td align="center">
<math>\equiv</math>
  </td>
  <td align="left">
<math>
\biggl[6\biggl(\frac{\omega^2}{4\pi \gamma_\mathrm{g} G \rho_c} \biggr)
- 2\alpha \biggr] \, .
</math>
  </td>
</tr>
</table>
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) &#8212;<math>(4 - x^2)</math> appears, whereas it should be <math>(4 - 6x^2)</math>.


=See Also=
=See Also=

Revision as of 22:11, 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,

0

=

z(1z)d2udz2+[γ(α+β+1)z]dudzαβu,

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(α,β;γ;z)

=

1+[αβγ1]z+[α(α+1)β(β+1)γ(γ+1)12]z2+[α(α+1)(α+2)β(β+1)(β+2)γ(γ+1)(γ+2)123]z3+

Among other attributes, Gradshteyn & Ryzhik (1965) note that this, "… series terminates if α or β 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

d2xdr02+[4r0(g0ρ0P0)]dxdr0+(ρ0γgP0)[ω2+(43γg)g0r0]x=0

where,

g0

=

1ρ0dP0dr0.

Multiplying through by R2, and making the variable substitutions,

x

f,

r0R

x,

(43γg)

αγg,

the LAWE may be rewritten as,

0

=

d2fdx2+[4x(g0ρ0RP0)]dfdx+(ρ0R2γgP0)[ω2αγgg0r0]f

 

=

d2fdx2+1x[4(g0ρ0r0P0)]dfdx+[(ω2ρ0R2γgP0)αγgg0r0(ρ0R2γgP0)]f

 

=

d2fdx2+1x[4(g0ρ0r0P0)]dfdx+[(ω2ρ0R2γgP0)αx2(g0r0ρ0P0)]f.

If we furthermore adopt the variable definition,

μ

(g0ρ0r0P0)=dlnP0dlnr0,

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

Borght's LAWE

0

=

d2fdx2+(4μ)xdfdx+[(ω2ρ0R2γgP0)αμx2]f.

Example Density- and Pressure-Profiles

Properties of Analytically Defined, Spherically Symmetric, Equilibrium Structures
Model ρ(x) P(x) P'(x) μ(x) ρ(x)P(x)
Uniform-density 1 1x2 2x 2x2(1x2) 1(1x2)
Linear 1x (1x)2(1+2x95x2) 125x(1x)(43x) 125x2(43x)(1x)(1+2x95x2) 1(1x)(1+2x95x2)
Parabolic 1x2 (1x2)2(112x2) x(1x2)(53x2) x2(53x2)(1x2)(112x2) 1(1x2)(112x2)
n=1 Polytrope sinxx (sinxx)2 2x[cosxsinxx]sinxx 2(1xcotx) xsinx

Uniform Density

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

0

=

d2fdx2+(4μ)xdfdx+[(ω2ρ0R2γgP0)αμx2]f

 

=

d2fdx2+1x[42x2(1x2)]dfdx+[(ω2ρcR2γgPc)1(1x2)(2α1x2)]f

 

=

(1x2)d2fdx2+1x[46x2]dfdx+[(ω2ρcR2γgPc)2α]f.

Given that, in the equilibrium state,

ρcR2Pc

=

64πGρc

we obtain the LAWE derived by Sterne37, namely,

0

=

(1x2)d2fdx2+1x[46x2]dfdx+[6(ω24πγgGρc)2α]f

 

=

(1x2)d2fdx2+1x[46x2]dfdx+𝔉f,

where,

𝔉

[6(ω24πγgGρc)2α].

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) —(4x2) appears, whereas it should be (46x2).

See Also


Tiled Menu

Appendices: | VisTrailsEquations | VisTrailsVariables | References | Ramblings | VisTrailsImages | myphys.lsu | ADS |