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=Radial Pulsation | =LAWE= | ||
==Most General Form== | |||
In an [[SSC/Perturbations#2ndOrderODE|accompanying discussion]], we derived the so-called, | |||
<div align="center" id="2ndOrderODE"> | |||
<font color="#770000">'''Adiabatic Wave''' (or ''Radial Pulsation'') '''Equation'''</font><br /> | |||
{{Math/EQ_RadialPulsation01}} | |||
</div> | |||
<!-- | |||
<div align="center" id="2ndOrderODE"> | |||
<font color="#770000">'''Adiabatic Wave Equation'''</font><br /> | |||
<math> | |||
\frac{d^2x}{dr_0^2} + \biggl[\frac{4}{r_0} - \biggl(\frac{g_0 \rho_0}{P_0}\biggr) \biggr] \frac{dx}{dr_0} + \biggl(\frac{\rho_0}{\gamma_\mathrm{g} P_0} \biggr)\biggl[\omega^2 + (4 - 3\gamma_\mathrm{g})\frac{g_0}{r_0} \biggr] x = 0 \, , | |||
</math> | |||
</div> | |||
--> | |||
where the [[SSC/Perturbations#g0|gravitational acceleration]], | |||
<table border="0" align="center" cellpadding="8"> | |||
<tr> | |||
<td align="right"><math>g_0</math></td> | |||
<td align="center"><math>\equiv</math></td> | |||
<td align="left"> | |||
<math> | |||
\frac{GM_r}{r_0^2} = - \frac{1}{\rho_0} \frac{dP_0}{dr_0} | |||
~~~\Rightarrow ~~~ | |||
\frac{g_0\rho_0 r_0}{P_0} = - \frac{d\ln P_0}{d\ln r_0} | |||
\, . | |||
</math> | |||
</td> | |||
</tr> | |||
</table> | |||
The solution to this equation gives eigenfunctions that describe various radial modes of oscillation in spherically symmetric, self-gravitating fluid configurations. The boundary condition conventionally used in connection with the adiabatic wave equation is, | |||
<table border="0" cellpadding="5" align="center"> | |||
<tr> | |||
<td align="right"> | |||
<math>r_0 \frac{d\ln x}{dr_0}</math> | |||
</td> | |||
<td align="center"> | |||
<math>=</math> | |||
</td> | |||
<td align="left"> | |||
<math>\frac{1}{\gamma_g} \biggl( 4 - 3\gamma_g + \frac{\omega^2 R^3}{GM_\mathrm{tot}}\biggr) </math> at <math>r_0 = R \, .</math> | |||
</td> | |||
</tr> | |||
</table> | |||
==Polytropic Configurations== | |||
===Part 1=== | |||
If the initial, unperturbed equilibrium configuration is a [[SSC/Structure/Polytropes#Polytropic_Spheres|polytropic sphere]] whose internal structure is defined by the function, <math>\theta(\xi)</math>, that provides a solution to the, | |||
<div align="center"> | |||
<span id="LaneEmdenEquation"><font color="#770000">'''Lane-Emden Equation'''</font></span> | |||
<br /> | |||
{{Math/EQ_SSLaneEmden01}} | |||
</div> | |||
then, | |||
<div align="center"> | |||
<table border="0" cellpadding="5" align="center"> | |||
<tr> | |||
<td align="right"> | |||
<math>r_0</math> | |||
</td> | |||
<td align="center"> | |||
<math>=</math> | |||
</td> | |||
<td align="left"> | |||
<math>a_n \xi \, ,</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> | |||
<math>\rho_0</math> | |||
</td> | |||
<td align="center"> | |||
<math>=</math> | |||
</td> | |||
<td align="left"> | |||
<math>\rho_c \theta^{n} \, ,</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> | |||
<math>P_0</math> | |||
</td> | |||
<td align="center"> | |||
<math>=</math> | |||
</td> | |||
<td align="left"> | |||
<math>K\rho_0^{(n+1)/n} = K\rho_c^{(n+1)/n} \theta^{n+1} \, ,</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> | |||
<math>g_0</math> | |||
</td> | |||
<td align="center"> | |||
<math>=</math> | |||
</td> | |||
<td align="left"> | |||
<math>\frac{GM(r_0)}{r_0^2} = \frac{G}{r_0^2} \biggl[ 4\pi a_n^3 \rho_c \biggl(-\xi^2 \frac{d\theta}{d\xi}\biggr) \biggr] | |||
\, ,</math> | |||
</td> | |||
</tr> | |||
</table> | |||
</div> | |||
where, | |||
<div align="center"> | |||
<table border="0" cellpadding="5" align="center"> | |||
<tr> | |||
<td align="right"> | |||
<math>a_n</math> | |||
</td> | |||
<td align="center"> | |||
<math>=</math> | |||
</td> | |||
<td align="left"> | |||
<math>\biggl[\frac{(n+1)K}{4\pi G} \cdot \rho_c^{(1-n)/n} \biggr]^{1/2} \, .</math> | |||
</td> | |||
</tr> | |||
</table> | |||
</div> | |||
Hence, after multiplying through by <math>~a_n^2</math>, the above adiabatic wave equation can be rewritten in the form, | |||
<div align="center"> | |||
<table border="0" cellpadding="5" align="center"> | |||
<tr> | |||
<td align="right"> | |||
<math>~\frac{d^2x}{d\xi^2} + \biggl[\frac{4}{\xi} - \frac{g_0}{a_n}\biggl(\frac{a_n^2 \rho_0}{P_0}\biggr) \biggr] \frac{dx}{d\xi} + \biggl(\frac{a_n^2\rho_0}{\gamma_\mathrm{g} P_0} \biggr)\biggl[\omega^2 + (4 - 3\gamma_\mathrm{g})\frac{g_0}{a_n\xi} \biggr] x </math> | |||
</td> | |||
<td align="center"> | |||
<math>~=</math> | |||
</td> | |||
<td align="left"> | |||
<math>~0 \, .</math> | |||
</td> | |||
</tr> | |||
</table> | |||
</div> | |||
In addition, given that, | |||
<div align="center"> | |||
<table border="0" cellpadding="5" align="center"> | |||
<tr> | |||
<td align="right"> | |||
<math>~\frac{g_0}{a_n}</math> | |||
</td> | |||
<td align="center"> | |||
<math>~=</math> | |||
</td> | |||
<td align="left"> | |||
<math>~4\pi G \rho_c \biggl(-\frac{d \theta}{d\xi} \biggr) \, ,</math> | |||
</td> | |||
</tr> | |||
</table> | |||
</div> | |||
and, | |||
<div align="center"> | |||
<table border="0" cellpadding="5" align="center"> | |||
<tr> | |||
<td align="right"> | |||
<math>~\frac{a_n^2 \rho_0}{P_0}</math> | |||
</td> | |||
<td align="center"> | |||
<math>~=</math> | |||
</td> | |||
<td align="left"> | |||
<math>~\frac{(n+1)}{(4\pi G\rho_c)\theta} = \frac{a_n^2 \rho_c}{P_c} \cdot \frac{\theta_c}{\theta}\, ,</math> | |||
</td> | |||
</tr> | |||
</table> | |||
</div> | |||
we can write, | |||
<table border="0" cellpadding="5" align="center"> | |||
<tr> | |||
<td align="right"> | |||
<math>0 </math> | |||
</td> | |||
<td align="center"> | |||
<math>~=</math> | |||
</td> | |||
<td align="left"> | |||
<math>\frac{d^2x}{d\xi^2} + \biggl[\frac{4 - (n+1)V(\xi)}{\xi} \biggr] \frac{dx}{d\xi} + | |||
\biggl[\omega^2 \biggl(\frac{a_n^2 \rho_c }{\gamma_g P_c} \biggr) \frac{\theta_c}{\theta} - | |||
\biggl(3-\frac{4}{\gamma_g}\biggr) \cdot \frac{(n+1)V(x)}{\xi^2} \biggr] x </math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> | |||
| |||
</td> | |||
<td align="center"> | |||
<math>~=</math> | |||
</td> | |||
<td align="left"> | |||
<math>\frac{d^2x}{d\xi^2} + \biggl[\frac{4 - (n+1)V(\xi)}{\xi} \biggr] \frac{dx}{d\xi} + | |||
(n+1)\biggl[\omega^2 \biggl(\frac{a_n^2 \rho_c }{\gamma_g P_c} \biggr) \frac{\xi^2 \theta_c}{(n+1)\theta} - | |||
\biggl(3-\frac{4}{\gamma_g}\biggr) \cdot V(x) \biggr] \frac{x}{\xi^2} </math> | |||
</td> | |||
</tr> | |||
</table> | |||
where we have adopted the function notation, | |||
<div align="center"> | |||
<table border="0" cellpadding="5" align="center"> | |||
<tr> | |||
<td align="right"> | |||
<math>V(\xi)</math> | |||
</td> | |||
<td align="center"> | |||
<math>\equiv</math> | |||
</td> | |||
<td align="left"> | |||
<math>- \frac{\xi}{\theta} \frac{d \theta}{d\xi} \, .</math> | |||
</td> | |||
</tr> | |||
</table> | |||
</div> | |||
===Part 2=== | |||
Drawing from an [[SSC/Stability/InstabilityOnsetOverview#Polytropic_Stability|accompanying discussion]], we have the following: | Drawing from an [[SSC/Stability/InstabilityOnsetOverview#Polytropic_Stability|accompanying discussion]], we have the following: | ||
| Line 8: | Line 240: | ||
{{ Math/EQ_RadialPulsation02 }} | {{ Math/EQ_RadialPulsation02 }} | ||
</div> | </div> | ||
<table border="1" align="center" width="80%" cellpadding="8"><tr><td align="left"> | |||
In order to reconcile with the "Part 1" expression, we note first that <math>V(\xi) \leftrightarrow Q(\xi)</math>. We note as well that since, | |||
<table border="0" cellpadding="5" align="center"> | |||
<tr> | |||
<td align="right"> | |||
<math>\biggl(\frac{a_n^2 \rho_c }{P_c} \biggr)\theta_c</math> | |||
</td> | |||
<td align="center"> | |||
<math>=</math> | |||
</td> | |||
<td align="left"> | |||
<math>\frac{(n+1)}{4\pi G\rho_c}\, , </math> | |||
</td> | |||
</tr> | |||
</table> | |||
we have, | |||
<table border="0" cellpadding="5" align="center"> | |||
<tr> | |||
<td align="right"> | |||
<math>\omega^2 \biggl(\frac{a_n^2 \rho_c }{\gamma_g P_c} \biggr) \frac{\xi^2 \theta_c}{(n+1)\theta}</math> | |||
</td> | |||
<td align="center"> | |||
<math>\leftrightarrow</math> | |||
</td> | |||
<td align="left"> | |||
<math> | |||
\frac{\omega^2}{\gamma_g} \biggl[\frac{(n+1)}{4\pi G\rho_c} \biggr] \frac{\xi^2 }{(n+1)\theta} | |||
= | |||
\frac{1}{6\gamma_g} \biggl[\frac{3\omega^2}{2\pi G\rho_c} \biggr] \frac{\xi^2 }{\theta} | |||
= | |||
\biggl( \frac{\sigma_c^2}{6\gamma_g}\biggr) \frac{\xi^2 }{\theta} | |||
\, . | |||
</math> | |||
</td> | |||
</tr> | |||
</table> | |||
</td></tr></table> | |||
All physically reasonable solutions are subject to the inner boundary condition, | All physically reasonable solutions are subject to the inner boundary condition, | ||
<div align="center"> | <div align="center"> | ||
| Line 16: | Line 288: | ||
<math>-\frac{d\ln x}{d\ln\xi} = 3</math> at <math>\xi = \tilde\xi \, .</math> | <math>-\frac{d\ln x}{d\ln\xi} = 3</math> at <math>\xi = \tilde\xi \, .</math> | ||
</div> | </div> | ||
But, for ''isolated'' polytropes | But, for ''isolated'' polytropes, the sought-after solution is subject to the more conventional boundary condition, | ||
<div align="center"> | <div align="center"> | ||
<math>- \frac{d\ln x}{d\ln \xi} = \biggl(\frac{3-n}{n+1}\biggr) + \frac{n\sigma_c^2}{6(n+1)} \biggl[\frac{\xi}{\theta^'}\biggr] </math> at <math>\xi = \xi_\mathrm{surf} \, .</math><br /> | <math>- \frac{d\ln x}{d\ln \xi} = \biggl(\frac{3-n}{n+1}\biggr) + \frac{n\sigma_c^2}{6(n+1)} \biggl[\frac{\xi}{\theta^'}\biggr] </math> at <math>\xi = \xi_\mathrm{surf} \, .</math><br /> | ||
</div> | </div> | ||
=Radial Pulsation Neutral Mode= | |||
==Background== | |||
The integro-differential version of the statement of hydrostatic balance is | |||
<div align="center"> | |||
{{Math/EQ_SShydrostaticBalance01}} | |||
</div> | |||
[[SSC/Stability/InstabilityOnsetOverview#Analyses_of_Radial_Oscillations|From our separate discussion]], we have found that, | |||
<div align="center"> | |||
<table border="0" cellpadding="5" align="center"> | |||
<tr> | |||
<td align="center" colspan="3"><font color="maroon"><b>Exact Solution to the <math>~(3 \le n < \infty)</math> Polytropic LAWE</b></font></td> | |||
</tr> | |||
<tr> | |||
<td align="right"> | |||
<math>~\sigma_c^2 = 0</math> | |||
</td> | |||
<td align="center"> | |||
and | |||
</td> | |||
<td align="left"> | |||
<math>~x_P \equiv \frac{3(n-1)}{2n}\biggl[1 + \biggl(\frac{n-3}{n-1}\biggr) \biggl( \frac{1}{\xi \theta^{n}}\biggr) \frac{d\theta}{d\xi}\biggr] \, .</math> | |||
</td> | |||
</tr> | |||
</table> | |||
</div> | |||
Let's rewrite the significant functional term in this expressions in terms of basic variables. That is, | |||
<table border="0" cellpadding="5" align="center"> | |||
<tr> | |||
<td align="right"> | |||
<math>\biggl( \frac{1}{\xi \theta^n}\biggr)\frac{d\theta}{d\xi}</math> | |||
</td> | |||
<td align="center"> | |||
<math>=</math> | |||
</td> | |||
<td align="left"> | |||
<math> | |||
-\biggl(\frac{a_n \rho_c}{r_0 \rho_0}\biggr)\frac{g_0}{4\pi G \rho_c a_n} | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> | |||
| |||
</td> | |||
<td align="center"> | |||
<math>=</math> | |||
</td> | |||
<td align="left"> | |||
<math> | |||
-\frac{M(r_0)}{4\pi r_0^3 \rho_0 } | |||
\, . | |||
</math> | |||
</td> | |||
</tr> | |||
</table> | |||
==Trial Eigenfunction & Its Derivatives== | |||
Let's adopt the following ''trial'' solution: | |||
<table border="0" cellpadding="5" align="center"> | |||
<tr> | |||
<td align="right"> | |||
<math>x_t</math> | |||
</td> | |||
<td align="center"> | |||
<math>=</math> | |||
</td> | |||
<td align="left"> | |||
<math> | |||
a -\frac{bM_r}{4\pi r_0^3 \rho_0 } = a - \frac{bg_0}{4\pi G r_0 \rho_0 } | |||
\, . | |||
</math> | |||
</td> | |||
</tr> | |||
</table> | |||
Then we have, | |||
<table border="0" cellpadding="5" align="center"> | |||
<tr> | |||
<td align="right"> | |||
<math>-\biggl(\frac{1}{b}\biggr)\frac{dx_t}{dr_0}</math> | |||
</td> | |||
<td align="center"> | |||
<math>=</math> | |||
</td> | |||
<td align="left"> | |||
<math> | |||
\frac{d}{dr_0} \biggl[\frac{M_r}{4\pi r_0^3 \rho_0 }\biggr] | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> | |||
| |||
</td> | |||
<td align="center"> | |||
<math>=</math> | |||
</td> | |||
<td align="left"> | |||
<math> | |||
\biggl[\frac{1}{4\pi r_0^3 \rho_0 }\biggr]\frac{dM_r}{dr_0} | |||
- | |||
\biggl[\frac{M_r}{4\pi r_0^3 \rho_0^2 }\biggr] | |||
\frac{d\rho_0 }{dr_0} | |||
- | |||
\biggl[\frac{3M_r}{4\pi r_0^4 \rho_0 }\biggr] | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> | |||
| |||
</td> | |||
<td align="center"> | |||
<math>=</math> | |||
</td> | |||
<td align="left"> | |||
<math> | |||
\frac{1}{r_0 } | |||
- | |||
\biggl[\frac{3M_r}{4\pi r_0^4 \rho_0 }\biggr] | |||
- | |||
\biggl[\frac{M_r}{4\pi r_0^3 \rho_0^2 }\biggr] | |||
\frac{d\rho_0 }{dr_0} | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> | |||
<math>-\biggl(\frac{1}{b}\biggr)\frac{d^2 x_t}{dr_0^2}</math> | |||
</td> | |||
<td align="center"> | |||
<math>=</math> | |||
</td> | |||
<td align="left"> | |||
<math> | |||
\frac{d}{dr_0}\biggl\{ | |||
\frac{1}{r_0 } | |||
- | |||
\biggl[\frac{3M_r}{4\pi r_0^4 \rho_0 }\biggr] | |||
- | |||
\biggl[\frac{M_r}{4\pi r_0^3 \rho_0^2 }\biggr] | |||
\frac{d\rho_0 }{dr_0} | |||
\biggr\} | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> | |||
| |||
</td> | |||
<td align="center"> | |||
<math>=</math> | |||
</td> | |||
<td align="left"> | |||
<math> | |||
-\frac{1}{r_0^2 } | |||
- | |||
\biggl[\frac{3}{4\pi r_0^4 \rho_0 }\biggr]\frac{dM_r}{dr_0} | |||
+ | |||
\biggl[\frac{3M_r}{4\pi r_0^4 \rho_0^2 }\biggr]\frac{d\rho_0}{dr_0} | |||
+4 | |||
\biggl[\frac{3M_r}{4\pi r_0^5 \rho_0 }\biggr] | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> | |||
| |||
</td> | |||
<td align="center"> | |||
| |||
</td> | |||
<td align="left"> | |||
<math> | |||
- | |||
\biggl[\frac{M_r}{4\pi r_0^3 \rho_0^2 }\biggr]\frac{d^2\rho_0 }{dr_0^2} | |||
- | |||
\biggl[\frac{1}{4\pi r_0^3 \rho_0^2 }\biggr]\frac{d\rho_0 }{dr_0} \cdot \frac{dM_r}{dr_0} | |||
+ | |||
\biggl[\frac{3M_r}{4\pi r_0^4 \rho_0^2 }\biggr]\frac{d\rho_0 }{dr_0} | |||
+ | |||
\biggl[\frac{2M_r}{4\pi r_0^3 \rho_0^3 }\biggr]\biggl(\frac{d\rho_0 }{dr_0}\biggr)^2 | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> | |||
| |||
</td> | |||
<td align="center"> | |||
<math>=</math> | |||
</td> | |||
<td align="left"> | |||
<math> | |||
-\frac{4}{r_0^2 } | |||
+ | |||
\frac{3M_r}{4\pi r_0^5 \rho_0 }\biggl[4 | |||
+ | |||
\frac{d\ln \rho_0}{d \ln r_0}\biggr] | |||
+ | |||
\frac{1}{r_0^2 }\biggl[ \frac{3M_r}{4\pi r_0^3 \rho_0 } | |||
- | |||
1 \biggr] \frac{d \ln \rho_0 }{d\ln r_0} | |||
- | |||
\biggl[\frac{M_r}{4\pi r_0^3 \rho_0^2 }\biggr]\frac{d^2\rho_0 }{dr_0^2} | |||
+ | |||
\biggl[\frac{2M_r}{4\pi r_0^5 \rho_0 }\biggr]\biggl(\frac{d\ln \rho_0 }{d \ln r_0}\biggr)^2 \, . | |||
</math> | |||
</td> | |||
</tr> | |||
</table> | |||
Given that, | |||
<table border="0" cellpadding="5" align="center"> | |||
<tr> | |||
<td align="right"> | |||
<math>\Delta \equiv \frac{M_r}{4\pi r_0^3\rho_0}</math> | |||
</td> | |||
<td align="center"> | |||
<math>=</math> | |||
</td> | |||
<td align="left"> | |||
<math> | |||
\frac{1}{4\pi G} \biggl( \frac{g_0}{r_0\rho_0}\biggr) | |||
= | |||
- \biggl[\frac{P_0}{4\pi G r_0^2 \rho_0^2} \cdot \frac{d\ln P_0}{d \ln r_0} \biggr] | |||
\, , | |||
</math> | |||
</td> | |||
</tr> | |||
</table> | |||
these expression can be rewritten as, | |||
<table border="0" cellpadding="5" align="center"> | |||
<tr> | |||
<td align="right"> | |||
<math>-\biggl(\frac{r_0^2}{b}\biggr)\frac{dx_t}{dr_0}</math> | |||
</td> | |||
<td align="center"> | |||
<math>=</math> | |||
</td> | |||
<td align="left"> | |||
<math>r_0 \biggl\{ | |||
1 - 3\Delta - \Delta \cdot \frac{d\ln \rho_0 }{d\ln r_0} | |||
\biggr\} \, , | |||
</math> | |||
</td> | |||
</tr> | |||
</table> | |||
and, | |||
<table border="0" cellpadding="5" align="center"> | |||
<tr> | |||
<td align="right"> | |||
<math>-\biggl(\frac{r_0^2}{b}\biggr)\frac{d^2 x_t}{dr_0^2}</math> | |||
</td> | |||
<td align="center"> | |||
<math>=</math> | |||
</td> | |||
<td align="left"> | |||
<math> | |||
- 4 + 3\Delta \biggl[4 + \frac{d\ln \rho_0}{d \ln r_0}\biggr] | |||
+ \biggl[ 3\Delta - 1 \biggr] \frac{d \ln \rho_0 }{d\ln r_0} | |||
- \Delta \biggl( \frac{r_0^2}{\rho_0}\biggr)\frac{d^2\rho_0 }{dr_0^2} | |||
+ 2\Delta \biggl(\frac{d\ln \rho_0 }{d \ln r_0}\biggr)^2 | |||
\, . | |||
</math> | |||
</td> | |||
</tr> | |||
</table> | |||
==Plug Trial Eigenfunction Into LAWE== | |||
<br /> | |||
<table border="1" width="60%" align="center" cellpadding="8"><tr><td align="center"> | |||
<div align="center">'''LAWE'''</div> | |||
{{Math/EQ_RadialPulsation01}} | |||
</td></tr></table> | |||
Plugging our ''trial'' radial displacement function, <math>x_t</math>, into the LAWE gives, | |||
<table border="0" cellpadding="5" align="center"> | |||
<tr> | |||
<td align="right"> | |||
LAWE | |||
</td> | |||
<td align="center"> | |||
<math>=</math> | |||
</td> | |||
<td align="left"> | |||
<math> | |||
-\biggl(\frac{r_0^2}{b}\biggr)\frac{d^2 x_t}{dr_0^2} | |||
-\biggl(\frac{r_0}{b}\biggr)\biggl[ 4 + \frac{d\ln P_0}{d\ln r_0}\biggr]\frac{dx_t}{dr_0} | |||
- \biggl(\frac{r_0^2}{b}\biggr) \biggl( \frac{\rho_0}{\gamma_g P_0}\biggr) | |||
\biggl[ (4-3\gamma_g)\frac{g_0}{r_0} + \sigma_c^2\biggl(\frac{2\pi G\rho_c}{3}\biggr)\biggr]x_t | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> | |||
| |||
</td> | |||
<td align="center"> | |||
<math>=</math> | |||
</td> | |||
<td align="left"> | |||
<math> | |||
-\biggl(\frac{r_0^2}{b}\biggr)\frac{d^2 x_t}{dr_0^2} | |||
-\biggl(\frac{r_0}{b}\biggr)\biggl[ 4 + \frac{d\ln P_0}{d\ln r_0}\biggr]\frac{dx_t}{dr_0} | |||
+ \biggl(\frac{1}{b}\biggr) \frac{1}{\gamma_g} \biggl( \frac{d\ln P_0}{d \ln r_0}\biggr) | |||
(4-3\gamma_g)x_t | |||
- \biggl(\frac{r_0^2}{b}\biggr) \biggl( \frac{\rho_0}{\gamma_g P_0}\biggr) | |||
\biggl[ \sigma_c^2\biggl(\frac{2\pi G\rho_c}{3}\biggr)\biggr]x_t | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> | |||
| |||
</td> | |||
<td align="center"> | |||
<math>=</math> | |||
</td> | |||
<td align="left"> | |||
<math> | |||
- 4 + 3\Delta \biggl[4 + \frac{d\ln \rho_0}{d \ln r_0}\biggr] | |||
+ \biggl[ 3\Delta - 1 \biggr] \frac{d \ln \rho_0 }{d\ln r_0} | |||
- \Delta \biggl( \frac{r_0^2}{\rho_0}\biggr)\frac{d^2\rho_0 }{dr_0^2} | |||
+ 2\Delta \biggl(\frac{d\ln \rho_0 }{d \ln r_0}\biggr)^2 | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> | |||
| |||
</td> | |||
<td align="center"> | |||
| |||
</td> | |||
<td align="left"> | |||
<math> | |||
+\biggl[ 4 + \frac{d\ln P_0}{d\ln r_0}\biggr]\biggl\{ | |||
1 - 3\Delta - \Delta \cdot \frac{d\ln \rho_0 }{d\ln r_0} | |||
\biggr\} | |||
+ \biggl(\frac{1}{b}\biggr) \frac{1}{\gamma_g} \biggl( \frac{d\ln P_0}{d \ln r_0}\biggr) | |||
(4-3\gamma_g)(a - b\Delta) | |||
- \biggl(\frac{1}{b}\biggr) \biggl( \frac{\rho_0r_0^2}{\gamma_g P_0}\biggr) | |||
\biggl[ \sigma_c^2\biggl(\frac{2\pi G\rho_c}{3}\biggr)\biggr](a - b\Delta) | |||
\, . | |||
</math> | |||
</td> | |||
</tr> | |||
</table> | |||
Now, if we set <math>\sigma_c^2 = 0</math> and <math> d\ln P_0/d\ln r_0 = \gamma_g(d\ln \rho_0/d\ln r_0)</math>, this expression becomes, | |||
<table border="0" cellpadding="5" align="center"> | |||
<tr> | |||
<td align="right"> | |||
LAWE | |||
</td> | |||
<td align="center"> | |||
<math>=</math> | |||
</td> | |||
<td align="left"> | |||
<math> | |||
- 4 + 3\Delta \biggl[4 + \frac{d\ln \rho_0}{d \ln r_0}\biggr] | |||
+ \biggl[ 3\Delta - 1 \biggr] \frac{d \ln \rho_0 }{d\ln r_0} | |||
- \Delta \biggl( \frac{r_0^2}{\rho_0}\biggr)\frac{d^2\rho_0 }{dr_0^2} | |||
+ 2\Delta \biggl(\frac{d\ln \rho_0 }{d \ln r_0}\biggr)^2 | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> | |||
| |||
</td> | |||
<td align="center"> | |||
| |||
</td> | |||
<td align="left"> | |||
<math> | |||
+\biggl[ 4 + \frac{d\ln P_0}{d\ln r_0}\biggr]\biggl\{ | |||
1 - 3\Delta - \Delta \cdot \frac{d\ln \rho_0 }{d\ln r_0} | |||
\biggr\} | |||
+ \biggl(\frac{1}{b}\biggr) \frac{1}{\gamma_g} \biggl( \frac{d\ln P_0}{d \ln r_0}\biggr) | |||
(4-3\gamma_g)(a - b\Delta) | |||
- \biggl(\frac{1}{b}\biggr) \biggl( \frac{\rho_0r_0^2}{\gamma_g P_0}\biggr) | |||
\biggl[ \sigma_c^2\biggl(\frac{2\pi G\rho_c}{3}\biggr)\biggr](a - b\Delta) | |||
\, . | |||
</math> | |||
</td> | |||
</tr> | |||
</table> | |||
Notice that the key components of this last term may be rewritten as, | |||
<table border="0" cellpadding="5" align="center"> | |||
<tr> | |||
<td align="right"> | |||
<math> | |||
\biggl( \frac{\rho_0r_0^2}{\gamma_g P_0}\biggr) | |||
\biggl[ \sigma_c^2\biggl(\frac{2\pi G\rho_c}{3}\biggr)\biggr] | |||
</math> | |||
</td> | |||
<td align="center"> | |||
<math>=</math> | |||
</td> | |||
<td align="left"> | |||
<math> | |||
\biggl( \frac{4\pi G \rho_0^2r_0^2}{P_0}\biggr) | |||
\biggl[ \frac{\sigma_c^2}{6\gamma_g} \biggl(\frac{\rho_c}{\rho_0}\biggr)\biggr] | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> | |||
| |||
</td> | |||
<td align="center"> | |||
<math>=</math> | |||
</td> | |||
<td align="left"> | |||
<math> | |||
- | |||
\biggl( \frac{1}{\Delta}\biggr) \frac{d\ln P_0}{d\ln r_0}\biggl[ \frac{\sigma_c^2}{6\gamma_g} \biggl(\frac{\rho_c}{\rho_0}\biggr)\biggr] | |||
\, . | |||
</math> | |||
</td> | |||
</tr> | |||
</table> | |||
So, for our ''trial'' eigenfunction, we have … | |||
<table border="0" cellpadding="5" align="center"> | |||
<tr> | |||
<td align="right"> | |||
LAWE | |||
</td> | |||
<td align="center"> | |||
<math>=</math> | |||
</td> | |||
<td align="left"> | |||
<math> | |||
\biggl[ 2\Delta - 1 \biggr] \frac{d \ln \rho_0 }{d\ln r_0} | |||
- \Delta \biggl( \frac{r_0^2}{\rho_0}\biggr)\frac{d^2\rho_0 }{dr_0^2} | |||
+ 2\Delta \biggl(\frac{d\ln \rho_0 }{d \ln r_0}\biggr)^2 | |||
+ \frac{d\ln P_0}{d\ln r_0} \cdot \biggl\{\biggl[ | |||
1 - 3\Delta - \Delta \cdot \frac{d\ln \rho_0 }{d\ln r_0} | |||
\biggr] | |||
+ \frac{(4-3\gamma_g)}{\gamma_g} | |||
\biggl[ \frac{a}{b} - \Delta \biggr] | |||
+ | |||
\frac{\sigma_c^2}{6\gamma_g} \biggl(\frac{\rho_c}{\rho_0}\biggr) | |||
\biggl[ \frac{a}{b\Delta} - 1\biggr] | |||
\biggr\} | |||
\, . | |||
</math> | |||
</td> | |||
</tr> | |||
</table> | |||
==Consider Polytropic Structures== | |||
Referring back to, for example, [[SSC/Stability/Polytropes#Groundwork|a separate review of polytropic structures]], we recognize that, | |||
<table border="0" cellpadding="5" align="center"> | |||
<tr> | |||
<td align="right"> | |||
<math>\Delta = \frac{1}{4\pi G} \biggl( \frac{g_0}{r_0\rho_0}\biggr)</math> | |||
</td> | |||
<td align="center"> | |||
<math>=</math> | |||
</td> | |||
<td align="left"> | |||
<math> | |||
\frac{1}{\xi^3} \biggl[ \biggl(-\xi^2 \frac{d\theta}{d\xi}\biggr) \biggr]\theta^{-n} | |||
= | |||
\frac{1}{\xi} \biggl(- \frac{d\theta}{d\xi}\biggr) \theta^{-n} | |||
= | |||
-\frac{\theta^'}{\xi \theta^n} | |||
\, , | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> | |||
<math>\frac{d\ln \rho_0}{d\ln r_0}</math> | |||
</td> | |||
<td align="center"> | |||
<math>=</math> | |||
</td> | |||
<td align="left"> | |||
<math> | |||
n\, , | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> | |||
<math>\frac{d\ln P_0}{d\ln r_0}</math> | |||
</td> | |||
<td align="center"> | |||
<math>=</math> | |||
</td> | |||
<td align="left"> | |||
<math> | |||
(n+1) \, . | |||
</math> | |||
</td> | |||
</tr> | |||
</table> | |||
Also, | |||
<table border="0" cellpadding="5" align="center"> | |||
<tr> | |||
<td align="right"> | |||
<math>\biggl(\frac{r_0^2}{\rho_0}\biggr) \frac{d^2\rho_0}{dr_0^2}</math> | |||
</td> | |||
<td align="center"> | |||
<math>=</math> | |||
</td> | |||
<td align="left"> | |||
<math> | |||
\biggl(\frac{\xi^2}{\rho_c \theta^n}\biggr) \frac{d}{d\xi}\biggl[n\rho_c \theta^{n-1} \theta^'\biggr] | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> | |||
| |||
</td> | |||
<td align="center"> | |||
<math>=</math> | |||
</td> | |||
<td align="left"> | |||
<math> | |||
\biggl(\frac{n\xi^2}{\theta^n}\biggr) \biggl[ | |||
(n-1)\theta^{n-2} (\theta^')^2 + \theta^{n-1} \theta^{''} | |||
\biggr] | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> | |||
| |||
</td> | |||
<td align="center"> | |||
<math>=</math> | |||
</td> | |||
<td align="left"> | |||
<math> | |||
\biggl( \frac{n\xi^2}{\theta^2}\biggr) \biggl[ | |||
(n-1)(\theta^')^2 + \theta \cdot \theta^{''} | |||
\biggr] | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> | |||
| |||
</td> | |||
<td align="center"> | |||
<math>=</math> | |||
</td> | |||
<td align="left"> | |||
<math> | |||
\biggl( \frac{n\xi^2}{\theta^2}\biggr) \biggl[ | |||
(n-1)(\theta^')^2 - \biggl( \theta^{n+1} + \frac{2\theta ~\theta^'}{\xi} \biggr) | |||
\biggr] | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> | |||
| |||
</td> | |||
<td align="center"> | |||
<math>=</math> | |||
</td> | |||
<td align="left"> | |||
<math> | |||
\biggl( \frac{n\xi^2}{\theta^2}\biggr) \biggl[ | |||
(n-1)(\xi \theta^n \Delta)^2 + \theta^{n+1} | |||
\biggr] | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> | |||
| |||
</td> | |||
<td align="center"> | |||
<math>=</math> | |||
</td> | |||
<td align="left"> | |||
<math> | |||
n(n-1)(\xi^{n+1} \theta^{n-1} \Delta)^2 + n\xi^2 \theta^{n-1}\, . | |||
</math> | |||
</td> | |||
</tr> | |||
</table> | |||
Hence, | |||
<table border="0" cellpadding="5" align="center"> | |||
<tr> | |||
<td align="right"> | |||
LAWE | |||
</td> | |||
<td align="center"> | |||
<math>=</math> | |||
</td> | |||
<td align="left"> | |||
<math> | |||
n( 2\Delta - 1 ) | |||
- \Delta \biggl( \frac{r_0^2}{\rho_0}\biggr)\frac{d^2\rho_0 }{dr_0^2} | |||
+ 2n^2 \Delta | |||
+ (n+1) \biggl[ | |||
1 - 3\Delta - n\Delta | |||
\biggr] | |||
+ (n+1) \biggl\{\frac{(4-3\gamma_g)}{\gamma_g} | |||
\biggl[ \frac{a}{b} - \Delta \biggr] | |||
+ | |||
\frac{\sigma_c^2}{6\gamma_g} \biggl(\frac{\rho_c}{\rho_0}\biggr) | |||
\biggl[ \frac{a}{b\Delta} - 1\biggr] | |||
\biggr\} | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> | |||
| |||
</td> | |||
<td align="center"> | |||
<math>=</math> | |||
</td> | |||
<td align="left"> | |||
<math> | |||
2n\Delta - n | |||
+ 2n^2 \Delta | |||
+ n - 3n\Delta - n^2\Delta | |||
+ 1 - 3\Delta - n\Delta | |||
- \Delta \biggl( \frac{r_0^2}{\rho_0}\biggr)\frac{d^2\rho_0 }{dr_0^2} | |||
+ (n+1) \biggl\{\frac{(4-3\gamma_g)}{\gamma_g} | |||
\biggl[ \frac{a}{b} - \Delta \biggr] | |||
+ | |||
\frac{\sigma_c^2}{6\gamma_g} \biggl(\frac{\rho_c}{\rho_0}\biggr) | |||
\biggl[ \frac{a}{b\Delta} - 1\biggr] | |||
\biggr\} | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> | |||
| |||
</td> | |||
<td align="center"> | |||
<math>=</math> | |||
</td> | |||
<td align="left"> | |||
<math> | |||
1 + n^2 \Delta | |||
- (2n+3)\Delta | |||
- \Delta \biggl( \frac{r_0^2}{\rho_0}\biggr)\frac{d^2\rho_0 }{dr_0^2} | |||
+ (n+1) \biggl[ \frac{4}{\gamma_g} -3\biggr] | |||
\biggl[ \frac{a}{b} - \Delta \biggr] | |||
+ | |||
(n+1) \biggl\{\frac{\sigma_c^2}{6\gamma_g} \biggl(\frac{\rho_c}{\rho_0}\biggr) | |||
\biggl[ \frac{a}{b\Delta} - 1\biggr] | |||
\biggr\} \, . | |||
</math> | |||
</td> | |||
</tr> | |||
</table> | |||
If, <math>\gamma_g = (n+1)/n</math>, we can further simplify and obtain, | |||
<table border="0" cellpadding="5" align="center"> | |||
<tr> | |||
<td align="right"> | |||
LAWE | |||
</td> | |||
<td align="center"> | |||
<math>=</math> | |||
</td> | |||
<td align="left"> | |||
<math> | |||
1 + n^2 \Delta | |||
- (2n+3)\Delta | |||
- \Delta \biggl( \frac{r_0^2}{\rho_0}\biggr)\frac{d^2\rho_0 }{dr_0^2} | |||
+ \biggl[ n-3\biggr] | |||
\biggl[ \frac{a}{b} - \Delta \biggr] | |||
+ | |||
(n+1) \biggl\{\frac{\sigma_c^2}{6\gamma_g} \biggl(\frac{\rho_c}{\rho_0}\biggr) | |||
\biggl[ \frac{a}{b\Delta} - 1\biggr] | |||
\biggr\} | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> | |||
| |||
</td> | |||
<td align="center"> | |||
<math>=</math> | |||
</td> | |||
<td align="left"> | |||
<math> | |||
1 + (n-3)\frac{a}{b} + n^2 \Delta | |||
+ (3-n)\Delta - (2n+3)\Delta | |||
- \Delta \biggl( \frac{r_0^2}{\rho_0}\biggr)\frac{d^2\rho_0 }{dr_0^2} | |||
+ | |||
(n+1) \biggl\{\frac{\sigma_c^2}{6\gamma_g} \biggl(\frac{\rho_c}{\rho_0}\biggr) | |||
\biggl[ \frac{a}{b\Delta} - 1\biggr] | |||
\biggr\} | |||
</math> | |||
</td> | |||
</tr> | |||
</table> | |||
=Try Again= | |||
==General Form of Wave Equation== | |||
<br /> | |||
<table border="1" width="60%" align="center" cellpadding="8"><tr><td align="center"> | |||
<div align="center">'''LAWE'''</div> | |||
{{Math/EQ_RadialPulsation01}} | |||
</td></tr></table> | |||
Employing the substitutions, | |||
<table border="0" align="center" cellpadding="5"> | |||
<tr> | |||
<td align="right"><math>\sigma_c^2</math></td> | |||
<td align="center"><math>\equiv</math></td> | |||
<td align="left"> | |||
<math> | |||
\frac{3\omega^2}{2\pi G \rho_c} | |||
\, , | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"><math>\alpha</math></td> | |||
<td align="center"><math>\equiv</math></td> | |||
<td align="left"> | |||
<math> | |||
3 - \frac{4}{\gamma_g} = \frac{3-n}{n+1} | |||
\, , | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"><math>g_0</math></td> | |||
<td align="center"><math>\equiv</math></td> | |||
<td align="left"> | |||
<math> | |||
\frac{GM_r}{r_0^2} = - \frac{1}{\rho_0} \frac{dP_0}{dr_0} | |||
~~~\Rightarrow ~~~ | |||
\frac{g_0\rho_0 r_0}{P_0} = - \frac{d\ln P_0}{d\ln r_0} | |||
\, , | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> | |||
<math>\Delta </math> | |||
</td> | |||
<td align="center"> | |||
<math>\equiv</math> | |||
</td> | |||
<td align="left"> | |||
<math> | |||
\frac{M_r}{4\pi r_0^3\rho_0} | |||
= | |||
\frac{1}{4\pi G} \biggl( \frac{g_0}{r_0\rho_0}\biggr) | |||
= | |||
- \biggl[\frac{P_0}{4\pi G r_0^2 \rho_0^2} \cdot \frac{d\ln P_0}{d \ln r_0} \biggr] | |||
\, , | |||
</math> | |||
</td> | |||
</tr> | |||
</table> | |||
we have, | |||
<table border="0" cellpadding="5" align="center"> | |||
<tr> | |||
<td align="right">LAWE</td> | |||
<td align="center"><math>=</math></td> | |||
<td align="left"> | |||
<math> | |||
\frac{d^2x}{dr_0^2} + \frac{1}{r_0}\biggl[4 - \frac{g_0 \rho_0 r_0}{P_0} \biggr] \frac{dx}{dr_0} | |||
+ \biggl[ \biggl(\frac{4}{\gamma_g} - 3 \biggr)\frac{g_0 \rho_0 r_0}{ P_0} \biggr] \frac{x}{r_0^2} | |||
+ \biggl(\frac{\rho_0}{ P_0} \biggr)\biggl[ 4\pi G \rho_c \biggl( \frac{\sigma_c^2}{6\gamma_g}\biggr) \biggr] x | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> </td> | |||
<td align="center"><math>=</math></td> | |||
<td align="left"> | |||
<math> | |||
\frac{d^2x}{dr_0^2} + \frac{1}{r_0}\biggl[4 + \frac{d\ln P_0}{d\ln r_0} \biggr] \frac{dx}{dr_0} | |||
+ \biggl[ \alpha \cdot \frac{d\ln P_0}{d\ln r_0} \biggr] \frac{x}{r_0^2} | |||
- \frac{1}{\Delta} \biggl[\frac{d\ln P_0}{d\ln r_0}\cdot \frac{\rho_c}{\rho_0} \biggl( \frac{\sigma_c^2}{6\gamma_g}\biggr)\biggr] \frac{x}{r_0^2} | |||
\, . | |||
</math> | |||
</td> | |||
</tr> | |||
</table> | |||
<table border="1" width="80%" align="center" cellpadding="8"><tr><td align="left"> | |||
In the context of polytropic configurations (see more [[#Assume_Polytropic_Relations|below]]), we appreciate that, | |||
<table border="0" cellpadding="5" align="center"> | |||
<tr> | |||
<td align="right"><math>\frac{\rho_0}{\rho_c} </math></td> | |||
<td align="center"><math>=</math></td> | |||
<td align="left"> | |||
<math> | |||
\theta^n \, , | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"><math>\frac{d \ln P_0}{d\ln r_0}</math></td> | |||
<td align="center"><math>=</math></td> | |||
<td align="left"> | |||
<math> | |||
(n+1) \frac{d\ln \theta}{d\ln\xi} = - (n+1)Q \, , | |||
</math> and, | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"><math>\frac{1}{\Delta} \cdot \frac{d \ln P_0}{d\ln r_0}</math></td> | |||
<td align="center"><math>=</math></td> | |||
<td align="left"> | |||
<math> | |||
- (n+1) \xi^2 \theta^{n-1} \, . | |||
</math> | |||
</td> | |||
</tr> | |||
</table> | |||
Inserting these into the LAWE expression and multiplying through by the square of the polytropic length scale, <math>a_n^2</math>, we obtain, | |||
<table border="0" cellpadding="5" align="center"> | |||
<tr> | |||
<td align="right">LAWE</td> | |||
<td align="center"><math>=</math></td> | |||
<td align="left"> | |||
<math> | |||
\frac{d^2x}{d\xi^2} + \frac{1}{\xi}\biggl[4 -(n+1)Q \biggr] \frac{dx}{d\xi} | |||
- \biggl[ \alpha (n+1)Q \biggr] \frac{x}{\xi^2} | |||
+ \biggl[(n+1)\frac{\xi^2}{\theta} \biggl( \frac{\sigma_c^2}{6\gamma_g}\biggr)\biggr] \frac{x}{\xi^2} | |||
\, . | |||
</math> | |||
</td> | |||
</tr> | |||
</table> | |||
This is identical to what has been referred to in [[SSC/Stability/InstabilityOnsetOverview#Polytropic_Stability|a separate discussion]], as the | |||
<div align="center">'''Polytropic LAWE'''<br /> | |||
{{Math/EQ_RadialPulsation02}} | |||
</div> | |||
</td></tr></table> | |||
==Derivatives of Δ== | |||
Here we evaluate the first derivative of <math>\Delta</math> with respect to <math>r_0</math>, | |||
<table border="0" cellpadding="5" align="center"> | |||
<tr> | |||
<td align="right"><math>\frac{d\Delta}{dr_0}</math></td> | |||
<td align="center"><math>=</math></td> | |||
<td align="left"> | |||
<math> | |||
\frac{d}{dr_0} | |||
\biggl\{ | |||
\frac{M_r}{4\pi r_0^3\rho_0} | |||
\biggr\} | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> </td> | |||
<td align="center"><math>=</math></td> | |||
<td align="left"> | |||
<math> | |||
\frac{1}{4\pi r_0^3 \rho_0} \cdot \frac{dM_r}{dr_0} | |||
- \frac{3M_r}{4\pi r_0^4 \rho_0} | |||
- \frac{M_r}{4\pi r_0^3 \rho_0^2}\cdot \frac{d\rho_0}{dr_0} | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> </td> | |||
<td align="center"><math>=</math></td> | |||
<td align="left"> | |||
<math> | |||
\frac{1}{r_0} | |||
- \frac{3M_r}{4\pi r_0^4 \rho_0} | |||
- \frac{M_r}{4\pi r_0^3 \rho_0^2}\cdot \frac{d\rho_0}{dr_0} | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> </td> | |||
<td align="center"><math>=</math></td> | |||
<td align="left"> | |||
<math> | |||
\frac{1}{r_0} \biggl\{ 1 | |||
- \Delta\biggl[3 + \frac{d\ln \rho_0}{d\ln r_0} \biggr]\biggr\} | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"><math>\Rightarrow ~~~ r_0 \cdot \frac{d\Delta}{dr_0}</math></td> | |||
<td align="center"><math>=</math></td> | |||
<td align="left"> | |||
<math> | |||
\biggl[ 1 - 3\Delta - \Delta \cdot \frac{d\ln \rho_0}{d\ln r_0} \biggr] | |||
\, ; | |||
</math> | |||
</td> | |||
</tr> | |||
</table> | |||
and the second derivative of <math>\Delta</math> with respect to <math>r_0</math>, | |||
<table border="0" cellpadding="5" align="center"> | |||
<tr> | |||
<td align="right"><math>\frac{d^2\Delta}{dr_0^2}</math></td> | |||
<td align="center"><math>=</math></td> | |||
<td align="left"> | |||
<math> | |||
\frac{d}{dr_0} | |||
\biggl\{ | |||
\frac{1}{r_0} | |||
\biggr\} | |||
- | |||
\frac{d}{dr_0} | |||
\biggl\{ | |||
\frac{3M_r}{4\pi r_0^4 \rho_0} | |||
\biggr\} | |||
- | |||
\frac{d}{dr_0} | |||
\biggl\{ | |||
\frac{M_r}{4\pi r_0^3 \rho_0^2}\cdot \frac{d\rho_0}{dr_0} | |||
\biggr\} | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> </td> | |||
<td align="center"><math>=</math></td> | |||
<td align="left"> | |||
<math> | |||
-\frac{1}{r_0^2} | |||
- | |||
\frac{3}{4\pi} | |||
\biggl\{ | |||
\frac{1}{r_0^4 \rho_0}\cdot \frac{dM_r}{dr_0} | |||
- | |||
\frac{4M_r}{ r_0^5 \rho_0} | |||
- | |||
\frac{M_r}{ r_0^4 \rho_0^2} \cdot \frac{d\rho_0}{dr_0} | |||
\biggr\} | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> </td> | |||
<td align="center"> </td> | |||
<td align="left"> | |||
<math> | |||
- | |||
\frac{1}{4\pi} | |||
\biggl\{ | |||
\frac{1}{r_0^3 \rho_0^2}\cdot \frac{d\rho_0}{dr_0} \cdot \frac{dM_r}{dr_0} | |||
- | |||
\frac{3M_r}{r_0^4 \rho_0^2}\cdot \frac{d\rho_0}{dr_0} | |||
- | |||
\frac{2M_r}{r_0^3 \rho_0^3}\cdot \biggl[\frac{d\rho_0}{dr_0}\biggr]^2 | |||
+ | |||
\frac{M_r}{r_0^3 \rho_0^2}\cdot \frac{d^2\rho_0}{dr_0^2} | |||
\biggr\} | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> </td> | |||
<td align="center"><math>=</math></td> | |||
<td align="left"> | |||
<math> | |||
-\frac{1}{r_0^2} | |||
- | |||
\frac{3}{r_0^2} | |||
\biggl\{ | |||
1 | |||
- | |||
\Delta \biggl[4 + \frac{d\ln \rho_0}{d\ln r_0}\biggr] | |||
\biggr\} | |||
- \frac{1}{r_0^2} | |||
\biggl\{ | |||
\biggl[ 1 | |||
- | |||
3\Delta \biggr] \frac{d\ln \rho_0}{d\ln r_0} | |||
- | |||
2\Delta\cdot \biggl[\frac{d\ln \rho_0}{d\ln r_0}\biggr]^2 | |||
+ | |||
\Delta \biggl( \frac{r_0^2}{\rho_0}\biggr) \frac{d^2\rho_0}{dr_0^2} | |||
\biggr\} | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"><math>\Rightarrow ~~~ - r_0^2 \cdot \frac{d^2\Delta}{dr_0^2}</math></td> | |||
<td align="center"><math>=</math></td> | |||
<td align="left"> | |||
<math> | |||
1 | |||
+ | |||
3 | |||
- | |||
3\Delta \biggl[4 + \frac{d\ln \rho_0}{d\ln r_0}\biggr] | |||
+ | |||
\biggl[ 1 | |||
- | |||
3\Delta \biggr] \frac{d\ln \rho_0}{d\ln r_0} | |||
- | |||
2\Delta\cdot \biggl[\frac{d\ln \rho_0}{d\ln r_0}\biggr]^2 | |||
+ | |||
\Delta \biggl( \frac{r_0^2}{\rho_0}\biggr) \frac{d^2\rho_0}{dr_0^2} | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> </td> | |||
<td align="center"><math>=</math></td> | |||
<td align="left"> | |||
<math> | |||
4 | |||
- | |||
12\Delta | |||
+ | |||
\biggl[ 1 | |||
- | |||
6\Delta \biggr] \frac{d\ln \rho_0}{d\ln r_0} | |||
- | |||
2\Delta\cdot \biggl[\frac{d\ln \rho_0}{d\ln r_0}\biggr]^2 | |||
+ | |||
\Delta \biggl( \frac{r_0^2}{\rho_0}\biggr) \frac{d^2\rho_0}{dr_0^2} | |||
\, . | |||
</math> | |||
</td> | |||
</tr> | |||
</table> | |||
==Trial Eigenfunction== | |||
As [[#Trial_Eigenfunction_.26_Its_Derivatives|above]], let's adopt a ''trial'' eigenfunction of the form, | |||
<table border="0" cellpadding="5" align="center"> | |||
<tr> | |||
<td align="right"> | |||
<math>x_t</math> | |||
</td> | |||
<td align="center"> | |||
<math>=</math> | |||
</td> | |||
<td align="left"> | |||
<math> | |||
a -\frac{bM_r}{4\pi r_0^3 \rho_0 } = a - b\Delta | |||
\, . | |||
</math> | |||
</td> | |||
</tr> | |||
</table> | |||
Then we have, | |||
<table border="0" cellpadding="5" align="center"> | |||
<tr> | |||
<td align="right"><math>\frac{1}{b} \biggl[ r_0^2 ~\times~ \mathrm{LAWE}~\biggr]_\mathrm{trial}</math></td> | |||
<td align="center"><math>=</math></td> | |||
<td align="left"> | |||
<math> | |||
- r_0^2 \cdot \frac{d^2\Delta}{dr_0^2} | |||
- \biggl[4 + \frac{d\ln P_0}{d\ln r_0} \biggr]r_0\cdot \frac{d\Delta}{dr_0} | |||
+ \biggl[ \alpha \cdot \frac{d\ln P_0}{d\ln r_0} \biggr] \biggl(\frac{a}{b} - \Delta \biggr) | |||
- \frac{1}{\Delta} \biggl[\frac{d\ln P_0}{d\ln r_0}\cdot \frac{\rho_c}{\rho_0} \biggl( \frac{\sigma_c^2}{6\gamma_g}\biggr)\biggr] \biggl(\frac{a}{b} - \Delta \biggr) | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> </td> | |||
<td align="center"><math>=</math></td> | |||
<td align="left"> | |||
<math> | |||
\biggl\{ | |||
4 | |||
- | |||
12\Delta | |||
+ | |||
\biggl[ 1 | |||
- | |||
6\Delta \biggr] \frac{d\ln \rho_0}{d\ln r_0} | |||
- | |||
2\Delta\cdot \biggl[\frac{d\ln \rho_0}{d\ln r_0}\biggr]^2 | |||
+ | |||
\Delta \biggl( \frac{r_0^2}{\rho_0}\biggr) \frac{d^2\rho_0}{dr_0^2} | |||
\biggr\} | |||
- ~ \biggl[4 + \frac{d\ln P_0}{d\ln r_0} \biggr] | |||
\biggl[ 1 - 3\Delta - \Delta \cdot \frac{d\ln \rho_0}{d\ln r_0} \biggr] | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> </td> | |||
<td align="center"> </td> | |||
<td align="left"> | |||
<math> | |||
+ ~\biggl[ \alpha \cdot \frac{d\ln P_0}{d\ln r_0} \biggr] \biggl(\frac{a}{b} - \Delta \biggr) | |||
- \frac{1}{\Delta} \biggl[\frac{d\ln P_0}{d\ln r_0}\cdot \frac{\rho_c}{\rho_0} \biggl( \frac{\sigma_c^2}{6\gamma_g}\biggr)\biggr] \biggl(\frac{a}{b} - \Delta \biggr) | |||
\, . | |||
</math> | |||
</td> | |||
</tr> | |||
</table> | |||
===Assume Polytropic Relations=== | |||
If we assume that the equilibrium models are polytropes, then we know that, | |||
<table border="0" cellpadding="5" align="center"> | |||
<tr> | |||
<td align="right"> | |||
<math>\rho_0 \propto \theta^n</math> | |||
</td> | |||
<td align="center"> | |||
<math>\Rightarrow</math> | |||
</td> | |||
<td align="left"> | |||
<math> | |||
\frac{d\ln \rho_0}{d\ln r_0} = n \cdot \frac{d\ln\theta}{d\ln\xi} | |||
\, ; | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> | |||
<math>P_0 \propto \theta^{n+1}</math> | |||
</td> | |||
<td align="center"> | |||
<math>\Rightarrow</math> | |||
</td> | |||
<td align="left"> | |||
<math> | |||
\frac{d\ln P_0}{d\ln r_0} = (n+1)\cdot \frac{d\ln\theta}{d\ln\xi} | |||
\, . | |||
</math> | |||
</td> | |||
</tr> | |||
</table> | |||
We also deduce that, | |||
<table border="0" cellpadding="5" align="center"> | |||
<tr> | |||
<td align="right"> | |||
<math>\biggl( \frac{r_0^2}{\rho_0}\biggr) \frac{d^2\rho_0}{dr_0^2}</math> | |||
</td> | |||
<td align="center"> | |||
<math>=</math> | |||
</td> | |||
<td align="left"> | |||
<math> | |||
\biggl( \frac{\xi^2}{\theta^n}\biggr) \frac{d}{d\xi}\biggl[ \frac{d\theta^n}{d\xi}\biggr] | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> | |||
| |||
</td> | |||
<td align="center"> | |||
<math>=</math> | |||
</td> | |||
<td align="left"> | |||
<math> | |||
\biggl( \frac{\xi^2}{\theta^n}\biggr) \frac{d}{d\xi}\biggl[ n\theta^{n-1} \theta^'\biggr] | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> | |||
| |||
</td> | |||
<td align="center"> | |||
<math>=</math> | |||
</td> | |||
<td align="left"> | |||
<math> | |||
\biggl( \frac{n\xi^2}{\theta^n}\biggr) \biggl[ | |||
(n-1)\theta^{n-2} (\theta^' )^2 | |||
+ \theta^{n-1} \theta^{''} | |||
\biggr] | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> | |||
| |||
</td> | |||
<td align="center"> | |||
<math>=</math> | |||
</td> | |||
<td align="left"> | |||
<math> | |||
\biggl[ \frac{n(n-1)\xi^2}{\theta^2}\biggr] (\theta^' )^2 | |||
- \biggl( \frac{n\xi^2}{\theta}\biggr) \biggl[ | |||
\theta^n + \frac{2}{\xi} \theta^' | |||
\biggr] | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> | |||
| |||
</td> | |||
<td align="center"> | |||
<math>=</math> | |||
</td> | |||
<td align="left"> | |||
<math> | |||
n(n-1) \cdot \biggl[ \frac{d\ln\theta}{d\ln\xi}\biggr]^2 | |||
- n \xi^2\theta^{n-1} | |||
- 2n \cdot \frac{d\ln \theta}{d\ln \xi} | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> | |||
| |||
</td> | |||
<td align="center"> | |||
<math>=</math> | |||
</td> | |||
<td align="left"> | |||
<math> | |||
n(n-1) \cdot \Xi^2- n \xi^2\theta^{n-1} - 2n \cdot \Xi | |||
\, , | |||
</math> | |||
</td> | |||
</tr> | |||
</table> | |||
where we have introduced the shorthand notation, | |||
<table border="0" cellpadding="5" align="center"> | |||
<tr> | |||
<td align="right"> | |||
<math>\Xi</math> | |||
</td> | |||
<td align="center"> | |||
<math>\equiv</math> | |||
</td> | |||
<td align="left"> | |||
<math> | |||
\frac{d\ln\theta}{d\ln \xi}\, . | |||
</math> | |||
</td> | |||
</tr> | |||
</table> | |||
Drawing from our [[SSC/Stability/Polytropes#Groundwork|accompanying discussion]], for example, we note as well that, | |||
<table border="0" align="center" cellpadding="5"> | |||
<tr> | |||
<td align="right"> | |||
<math>\Delta </math> | |||
</td> | |||
<td align="center"> | |||
<math>=</math> | |||
</td> | |||
<td align="left"> | |||
<math> | |||
- \biggl[\frac{P_0}{4\pi G r_0^2 \rho_0^2} \cdot \frac{d\ln P_0}{d \ln r_0} \biggr] | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> | |||
<math>\Rightarrow ~~~ - \frac{1}{\Delta} \cdot \frac{d\ln P_0}{d \ln r_0} </math> | |||
</td> | |||
<td align="center"> | |||
<math>=</math> | |||
</td> | |||
<td align="left"> | |||
<math> | |||
\frac{4\pi G r_0^2 \rho_0^2}{P_0} | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> | |||
| |||
</td> | |||
<td align="center"> | |||
<math>=</math> | |||
</td> | |||
<td align="left"> | |||
<math> | |||
4\pi G (a_n^2 \xi^2) (\rho_c \theta^n)^2 [K^{-1} \rho_c^{-(n+1)/n} \theta^{-(n+1)}] | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> | |||
| |||
</td> | |||
<td align="center"> | |||
<math>=</math> | |||
</td> | |||
<td align="left"> | |||
<math> | |||
4\pi G \biggl[ \frac{(n+1)K}{4\pi G} \cdot \rho_c^{(1-n)/n} \biggr] (\rho_c )^2 \biggl[K^{-1} \rho_c^{-(n+1)/n} \biggr] \xi^2 \theta^{ (n-1)} | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> | |||
| |||
</td> | |||
<td align="center"> | |||
<math>=</math> | |||
</td> | |||
<td align="left"> | |||
<math> | |||
(n+1)\xi^2 \theta^{ (n-1)} | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> | |||
<math>\Rightarrow ~~~ \Delta \cdot \xi^2 \theta^{n-1} | |||
</math> | |||
</td> | |||
<td align="center"> | |||
<math>=</math> | |||
</td> | |||
<td align="left"> | |||
<math> | |||
- \frac{1}{(n+1)} \cdot \frac{d\ln P_0}{d \ln r_0} | |||
= | |||
- \Xi | |||
\, . | |||
</math> | |||
</td> | |||
</tr> | |||
</table> | |||
Hence, | |||
<table border="0" cellpadding="5" align="center"> | |||
<tr> | |||
<td align="right"><math>\frac{1}{b} \biggl[ r_0^2 ~\times~ \mathrm{LAWE}~\biggr]_\mathrm{trial}</math></td> | |||
<td align="center"><math>=</math></td> | |||
<td align="left"> | |||
<math> | |||
4 | |||
- | |||
12\Delta | |||
+ | |||
\biggl[ 1 | |||
- | |||
6\Delta \biggr] n\Xi | |||
- | |||
2\Delta\cdot \biggl[n\Xi\biggr]^2 | |||
+ | |||
\Delta \biggl[ n(n-1) \cdot \Xi^2- n \xi^2\theta^{n-1} - 2n \cdot \Xi \biggr] | |||
- ~ \biggl[4 + (n+1)\Xi \biggr] | |||
\biggl[ 1 - 3\Delta - \Delta \cdot n\Xi \biggr] | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> </td> | |||
<td align="center"> </td> | |||
<td align="left"> | |||
<math> | |||
+ ~\biggl[ \alpha \cdot (n+1)\Xi \biggr] \biggl(\frac{a}{b} - \Delta \biggr) | |||
- \frac{1}{\Delta} \biggl[(n+1)\Xi \cdot \frac{\rho_c}{\rho_0} \biggl( \frac{\sigma_c^2}{6\gamma_g}\biggr)\biggr] \biggl(\frac{a}{b} - \Delta \biggr) | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> </td> | |||
<td align="center"><math>=</math></td> | |||
<td align="left"> | |||
<math> | |||
n\Xi | |||
- 6\Delta n\Xi | |||
- 2\Delta\cdot \biggl[n\Xi\biggr]^2 | |||
+ | |||
\Delta \biggl[ n(n-1) \cdot \Xi^2- n \xi^2\theta^{n-1} + 2n \cdot \Xi \biggr] | |||
+ ~ 2(n+1)\Xi | |||
+ ~ n(n+1)\Xi^2 \cdot \Delta | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> </td> | |||
<td align="center"> </td> | |||
<td align="left"> | |||
<math> | |||
+ ~\biggl[ \alpha \cdot (n+1)\Xi \biggr] \biggl(\frac{a}{b} \biggr) | |||
- ~\biggl[ \alpha \cdot (n+1)\Xi \biggr] \Delta | |||
- \frac{1}{\Delta} \biggl[(n+1)\Xi \cdot \frac{\rho_c}{\rho_0} \biggl( \frac{\sigma_c^2}{6\gamma_g}\biggr)\biggr] \biggl(\frac{a}{b} - \Delta \biggr) | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> </td> | |||
<td align="center"><math>=</math></td> | |||
<td align="left"> | |||
<math>\Xi \biggl[ | |||
1 + n | |||
+ ~ 2(n+1) | |||
+ \alpha \cdot (n+1) \biggl(\frac{a}{b} \biggr) | |||
\biggr] | |||
+ | |||
\Delta \biggl[ - [4n + \alpha \cdot (n+1)]\Xi + n(n-1) \cdot \Xi^2 + n(n+1)\Xi^2 - 2n^2 \Xi^2 \biggr] | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> </td> | |||
<td align="center"> </td> | |||
<td align="left"> | |||
<math> | |||
- \frac{1}{\Delta} \biggl[(n+1)\Xi \cdot \frac{\rho_c}{\rho_0} \biggl( \frac{\sigma_c^2}{6\gamma_g}\biggr)\biggr] \biggl(\frac{a}{b} - \Delta \biggr) | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> </td> | |||
<td align="center"><math>=</math></td> | |||
<td align="left"> | |||
<math>\Xi \biggl[ | |||
3(n+1) | |||
+ \alpha \cdot (n+1) \biggl(\frac{a}{b} \biggr) | |||
\biggr] | |||
- \Delta [4n + \alpha \cdot (n+1)]\Xi | |||
- \frac{1}{\Delta} \biggl[(n+1)\Xi \cdot \frac{\rho_c}{\rho_0} \biggl( \frac{\sigma_c^2}{6\gamma_g}\biggr)\biggr] \biggl(\frac{a}{b} - \Delta \biggr) | |||
</math> | |||
</td> | |||
</tr> | |||
</table> | |||
=Third Time= | |||
==General Relations== | |||
Various ''general'' relations taken from above derivations: | |||
<table border="0" cellpadding="5" align="center"> | |||
<tr> | |||
<td align="right">LAWE</td> | |||
<td align="center"><math>=</math></td> | |||
<td align="left"> | |||
<math> | |||
\frac{d^2x}{dr_0^2} + \frac{1}{r_0}\biggl[4 + \frac{d\ln P_0}{d\ln r_0} \biggr] \frac{dx}{dr_0} | |||
+ \biggl[ \alpha \cdot \frac{d\ln P_0}{d\ln r_0} \biggr] \frac{x}{r_0^2} | |||
- \frac{1}{\Delta} \biggl[\frac{d\ln P_0}{d\ln r_0}\cdot \frac{\rho_c}{\rho_0} \biggl( \frac{\sigma_c^2}{6\gamma_g}\biggr)\biggr] \frac{x}{r_0^2} | |||
\, , | |||
</math> | |||
</td> | |||
</tr> | |||
</table> | |||
where, | |||
<table border="0" cellpadding="5" align="center"> | |||
<tr> | |||
<td align="right"><math>\Delta</math></td> | |||
<td align="center"><math>\equiv</math></td> | |||
<td align="left"> | |||
<math> | |||
\frac{M_r}{4\pi r_0^3 \rho_0} | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"><math>\Rightarrow ~~~ \frac{1}{\Delta} \cdot \frac{d\ln P_0}{d\ln r_0}</math></td> | |||
<td align="center"><math>=</math></td> | |||
<td align="left"> | |||
<math> | |||
-~\frac{4\pi G r_0^2 \rho_0^2}{P_0} | |||
\, ; | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"><math>r_0 \cdot \frac{d\Delta}{dr_0}</math></td> | |||
<td align="center"><math>=</math></td> | |||
<td align="left"> | |||
<math> | |||
\biggl[ 1 - 3\Delta - \Delta \cdot \frac{d\ln \rho_0}{d\ln r_0} \biggr] | |||
\, ; | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"><math>- r_0^2 \cdot \frac{d^2\Delta}{dr_0^2}</math></td> | |||
<td align="center"><math>=</math></td> | |||
<td align="left"> | |||
<math> | |||
4 | |||
- | |||
12\Delta | |||
+ | |||
\biggl[ 1 | |||
- | |||
6\Delta \biggr] \frac{d\ln \rho_0}{d\ln r_0} | |||
- | |||
2\Delta\cdot \biggl[\frac{d\ln \rho_0}{d\ln r_0}\biggr]^2 | |||
+ | |||
\Delta \biggl( \frac{r_0^2}{\rho_0}\biggr) \frac{d^2\rho_0}{dr_0^2} | |||
\, . | |||
</math> | |||
</td> | |||
</tr> | |||
</table> | |||
==Polytropes== | |||
If polytropic relations are adopted: | |||
<table border="0" cellpadding="5" align="center"> | |||
<tr> | |||
<td align="right"><math>\Delta</math></td> | |||
<td align="center"><math>=</math></td> | |||
<td align="left"> | |||
<math> | |||
\frac{Q}{\xi^2 \theta^{n-1}} | |||
\, ; | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"><math>\frac{1}{\Delta} \cdot \frac{d\ln P_0}{d\ln r_0}</math></td> | |||
<td align="center"><math>=</math></td> | |||
<td align="left"> | |||
<math> | |||
-(n+1) \xi^2 \theta^{n-1} | |||
\, ; | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"><math>r_0^2 \times~ \mathrm{LAWE}</math></td> | |||
<td align="center"><math>=</math></td> | |||
<td align="left"> | |||
<math> | |||
r_0^2 \frac{d^2x}{dr_0^2} + \biggl[4 -(n+1)Q \biggr] r_0 \cdot \frac{dx}{dr_0} | |||
+ \biggl[ (n-3)Q \biggr] x | |||
+ \frac{1}{\Delta} \biggl[(n+1) Q \cdot \frac{1}{\theta^n} \biggl( \frac{\sigma_c^2}{6\gamma_g}\biggr)\biggr] x | |||
\, ; | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"><math>r_0 \cdot \frac{d\Delta}{dr_0}</math></td> | |||
<td align="center"><math>=</math></td> | |||
<td align="left"> | |||
<math> | |||
\biggl[ 1 - 3\Delta + n \Delta Q \biggr] | |||
=1 + (nQ - 3)\Delta | |||
\, ; | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"><math>- r_0^2 \cdot \frac{d^2\Delta}{dr_0^2}</math></td> | |||
<td align="center"><math>=</math></td> | |||
<td align="left"> | |||
<math> | |||
4 - 12\Delta | |||
- n\biggl[ 1 - 6\Delta \biggr] Q | |||
- | |||
2n^2 \Delta Q^2 | |||
+ | |||
\Delta \biggl( \frac{r_0^2}{\rho_0}\biggr) \frac{d^2\rho_0}{dr_0^2} | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> </td> | |||
<td align="center"><math>=</math></td> | |||
<td align="left"> | |||
<math> | |||
4 - 12\Delta | |||
- n\biggl[ 1 - 6\Delta \biggr] Q | |||
- | |||
2n^2 \Delta Q^2 | |||
+ \Delta \biggl[ | |||
n(n-1)Q^2 +2nQ-\frac{nQ}{\Delta} | |||
\biggr] | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> </td> | |||
<td align="center"><math>=</math></td> | |||
<td align="left"> | |||
<math> | |||
4 -nQ - 12\Delta | |||
+ 6nQ\Delta | |||
- | |||
2n^2 \Delta Q^2 | |||
+ \Delta \biggl[ | |||
n(n-1)Q^2 +2nQ | |||
\biggr] - nQ | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> </td> | |||
<td align="center"><math>=</math></td> | |||
<td align="left"> | |||
<math> | |||
4 - 2nQ | |||
+ \Delta \biggl[6nQ -2n^2Q^2 | |||
+ n(n-1)Q^2 +2nQ - 12 | |||
\biggr] | |||
\, . | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> </td> | |||
<td align="center"><math>=</math></td> | |||
<td align="left"> | |||
<math> | |||
4 - 2nQ + \Delta \biggl[8nQ - n^2Q^2 - nQ^2 - 12 | |||
\biggr] | |||
\, . | |||
</math> | |||
</td> | |||
</tr> | |||
</table> | |||
==Eigenfunction Choice== | |||
Again, let's try the ''trial'' eigenfunction, | |||
<table border="0" cellpadding="5" align="center"> | |||
<tr> | |||
<td align="right"><math>x_t</math></td> | |||
<td align="center"><math>=</math></td> | |||
<td align="left"> | |||
<math> | |||
a - b\Delta | |||
\, , | |||
</math> | |||
</td> | |||
</tr> | |||
</table> | |||
in which case, | |||
<table border="0" cellpadding="5" align="center"> | |||
<tr> | |||
<td align="right"><math>\frac{1}{b}\biggl[ r_0^2 \times~ \mathrm{LAWE} \biggr]</math></td> | |||
<td align="center"><math>=</math></td> | |||
<td align="left"> | |||
<math> | |||
- r_0^2 \frac{d^2\Delta}{dr_0^2} - \biggl[4 -(n+1)Q \biggr] r_0 \cdot \frac{d\Delta}{dr_0} | |||
+ \biggl[ (n-3)Q \biggr] \biggl( \frac{a}{b} - \Delta\biggr) | |||
+ \frac{1}{\Delta} \biggl[(n+1) Q \cdot \frac{1}{\theta^n} \biggl( \frac{\sigma_c^2}{6\gamma_g}\biggr)\biggr] \biggl( \frac{a}{b} - \Delta\biggr) | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> </td> | |||
<td align="center"><math>=</math></td> | |||
<td align="left"> | |||
<math> | |||
4 - 2nQ + \Delta \biggl[8nQ - n^2Q^2 - nQ^2 - 12\biggr] | |||
- \biggl[4 -(n+1)Q \biggr] \biggl[1 + (nQ - 3)\Delta \biggr] | |||
+ \biggl[ (n-3)Q \biggr] \biggl( \frac{a}{b} - \Delta\biggr) | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> </td> | |||
<td align="center"> </td> | |||
<td align="left"> | |||
<math> | |||
+ \frac{1}{\Delta} \biggl[(n+1) Q \cdot \frac{1}{\theta^n} \biggl( \frac{\sigma_c^2}{6\gamma_g}\biggr)\biggr] \biggl( \frac{a}{b} - \Delta\biggr) | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> </td> | |||
<td align="center"><math>=</math></td> | |||
<td align="left"> | |||
<math> | |||
4 - 2nQ + \Delta \biggl[8nQ - n^2Q^2 - nQ^2 - 12\biggr] | |||
- 4 - (4nQ - 12)\Delta | |||
+ (n+1)Q | |||
+ (n+1) (nQ^2 - 3Q)\Delta | |||
+ (n-3)Q \biggl( \frac{a}{b} \biggr) | |||
- (n-3)Q \Delta | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> </td> | |||
<td align="center"> </td> | |||
<td align="left"> | |||
<math> | |||
+ \frac{1}{\Delta} \biggl[(n+1) Q \cdot \frac{1}{\theta^n} \biggl( \frac{\sigma_c^2}{6\gamma_g}\biggr)\biggr] \biggl( \frac{a}{b} - \Delta\biggr) | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> </td> | |||
<td align="center"><math>=</math></td> | |||
<td align="left"> | |||
<math> | |||
\biggl[(n+1) | |||
- 2n | |||
+ (n-3) \biggl( \frac{a}{b} \biggr)\biggr]Q | |||
+ \Delta \biggl[8nQ - n^2Q^2 - nQ^2 - 12 | |||
- 4nQ + 12 | |||
+ (n+1) (nQ^2 ) | |||
-3Q (n+1) | |||
+ (3-n)Q | |||
\biggr] | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> </td> | |||
<td align="center"> </td> | |||
<td align="left"> | |||
<math> | |||
+ \frac{1}{\Delta} \biggl[(n+1) Q \cdot \frac{1}{\theta^n} \biggl( \frac{\sigma_c^2}{6\gamma_g}\biggr)\biggr] \biggl( \frac{a}{b} - \Delta\biggr) | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> </td> | |||
<td align="center"><math>=</math></td> | |||
<td align="left"> | |||
<math> | |||
\biggl[(1-n) + (n-3) \biggl( \frac{a}{b} \biggr)\biggr]Q | |||
+ \Delta \biggl[ 0 \biggr] | |||
+ \frac{1}{\Delta} \biggl[(n+1) Q \cdot \frac{1}{\theta^n} \biggl( \frac{\sigma_c^2}{6\gamma_g}\biggr)\biggr] \biggl( \frac{a}{b} - \Delta\biggr) | |||
\, . | |||
</math> | |||
</td> | |||
</tr> | |||
</table> | |||
Hence, we are left with only the <math>\sigma_c^2</math> term if we set, | |||
<table border="0" cellpadding="5" align="center"> | |||
<tr> | |||
<td align="right"><math>0</math></td> | |||
<td align="center"><math>=</math></td> | |||
<td align="left"> | |||
<math> | |||
(1-n) + (n-3) \biggl( \frac{a}{b} \biggr)</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"><math>\Rightarrow ~~~ \biggl( \frac{a}{b} \biggr)</math></td> | |||
<td align="center"><math>=</math></td> | |||
<td align="left"> | |||
<math> | |||
\frac{n-1}{n-3} \, . | |||
</math> | |||
</td> | |||
</tr> | |||
</table> | |||
We conclude, therefore, that the radial displacement function (''i.e.,'' the eigenfunction) for the neutral <math>(\sigma_c^2 = 0)</math> mode of all polytropic configurations is, | |||
<table border="0" cellpadding="5" align="center"> | |||
<tr> | |||
<td align="right"><math>x_\mathrm{neutral}</math></td> | |||
<td align="center"><math>=</math></td> | |||
<td align="left"> | |||
<math> | |||
\frac{1}{b} \biggl[ \frac{n-1}{n-3} - \Delta \biggr] | |||
= | |||
\frac{1}{b} \biggl[ \frac{n-1}{n-3} - \frac{Q}{\xi^2 \theta^{n-1}} \biggr] | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> </td> | |||
<td align="center"><math>=</math></td> | |||
<td align="left"> | |||
<math> | |||
\frac{1}{b} \biggl( \frac{n-1}{n-3} \biggr) | |||
\biggl[1 + \biggl(\frac{n-3}{n-1}\biggr)\frac{1}{\xi^2 \theta^{n-1}} \cdot \frac{d\ln \theta}{d\ln \xi} \biggr] | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> </td> | |||
<td align="center"><math>=</math></td> | |||
<td align="left"> | |||
<math> | |||
\frac{1}{b} \biggl( \frac{n-1}{n-3} \biggr) | |||
\biggl[1 + \biggl(\frac{n-3}{n-1}\biggr)\frac{1}{\xi \theta^{n}} \cdot \frac{d \theta}{d \xi} \biggr] | |||
\, . | |||
</math> | |||
</td> | |||
</tr> | |||
</table> | |||
This last expression exactly matches [[SSC/Stability/InstabilityOnsetOverview#NeutralMode|our earlier result found for polytropic configurations]] if we choose an overall amplitude coefficient of the form, | |||
<table border="0" cellpadding="5" align="center"> | |||
<tr> | |||
<td align="right"><math>b</math></td> | |||
<td align="center"><math>=</math></td> | |||
<td align="left"> | |||
<math> | |||
\frac{2n}{3(n-3)} \, . | |||
</math> | |||
</td> | |||
</tr> | |||
</table> | |||
'''<font color="red">Hooray!</font>''' | |||
=Summary= | |||
==Setup== | |||
We begin with the traditional, | |||
<div align="center" id="2ndOrderODE"> | |||
<font color="#770000">'''Adiabatic Wave''' (or ''Radial Pulsation'') '''Equation'''</font><br /> | |||
{{Math/EQ_RadialPulsation01}} | |||
</div> | |||
This linear, adiabatic wave equation (LAWE) can straightforwardly be rewritten in the form we will refer to as the, | |||
<div align="center" id="Delta_Highlighted"> | |||
<font color="#770000">'''Δ-Highlighted LAWE'''</font><br /> | |||
{{Math/EQ_RadialPulsation04}} | |||
</div> | |||
Multiplying this ''Δ-Highlighted LAWE'' through by <math>a_n^2 = (r_0/\xi)^2</math> and recognizing that, for polytropic configurations, | |||
<table border="0" cellpadding="5" align="center"> | |||
<tr> | |||
<td align="right"><math>\Delta</math></td> | |||
<td align="center"><math>=</math></td> | |||
<td align="left"> | |||
<math> | |||
-~\frac{1}{\xi^2 \theta^{n-1}} \frac{d\ln \theta}{d\ln \xi} | |||
\, , | |||
</math> | |||
</td> | |||
<td align="center"> </td> | |||
<td align="right"><math>\frac{d\ln P_0}{d\ln r_0}</math></td> | |||
<td align="center"><math>=</math></td> | |||
<td align="left"> | |||
<math> | |||
~(n+1)\frac{d\ln \theta}{d\ln \xi} | |||
\, , | |||
</math> | |||
</td> | |||
<td align="center"> <math>\Rightarrow</math> </td> | |||
<td align="right"><math>\frac{1}{\Delta} \cdot \frac{d\ln P_0}{d\ln r_0}</math></td> | |||
<td align="center"><math>=</math></td> | |||
<td align="left"> | |||
<math> | |||
-(n+1) \xi^2 \theta^{n-1} | |||
\, , | |||
</math> | |||
</td> | |||
</tr> | |||
</table> | |||
we immediately obtain what we have frequently referred to as the, | |||
<div align="center" id="PolytropicLAWE"> | |||
<font color="#770000">'''Polytropic LAWE'''</font><br /> | |||
{{Math/EQ_RadialPulsation02}} | |||
</div> | |||
==Neutral-Mode Eigenfunction== | |||
In the preceding subsections of this chapter, we have demonstrated that if | |||
<table border="0" cellpadding="5" align="center"> | |||
<tr> | |||
<td align="right"><math>\gamma_g = \frac{n+1}{n}</math></td> | |||
<td align="center"><math>~~~\Rightarrow ~~~</math></td> | |||
<td align="left"> | |||
<math> | |||
\alpha = \frac{3-n}{n+1} | |||
\, , | |||
</math> | |||
</td> | |||
</tr> | |||
</table> | |||
the radial displacement function (''i.e.,'' the eigenfunction) for the neutral <math>(\sigma_c^2 = 0)</math> mode of all polytropic configurations is, | |||
<table border="0" cellpadding="5" align="center"> | |||
<tr> | |||
<td align="right"><math>x_\mathrm{neutral}</math></td> | |||
<td align="center"><math>=</math></td> | |||
<td align="left"> | |||
<math> | |||
\frac{3(n-3)}{2n} \biggl[ \frac{n-1}{n-3} - \Delta \biggr] | |||
\, , | |||
</math> | |||
</td> | |||
</tr> | |||
</table> | |||
to within an arbitrarily chosen leading scaling coefficient. More completely, if we let "LAWE" stand for the RHS of our Δ-Highlighted LAWE, then setting <math>x = x_\mathrm{neutral}</math> results in the expression, | |||
<table border="0" cellpadding="5" align="center"> | |||
<tr> | |||
<td align="right"><math>\frac{1}{b}\biggl[ r_0^2 \times~ \mathrm{LAWE} \biggr]</math></td> | |||
<td align="center"><math>=</math></td> | |||
<td align="left"> | |||
<math> | |||
(n+1) Q \cdot \frac{1}{\theta^n} \biggl( \frac{\sigma_c^2}{6\gamma_g}\biggr) | |||
\biggl[ \frac{1}{\Delta} \biggl( \frac{n-1}{n-3}\biggr) - 1 \biggr] | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> </td> | |||
<td align="center"><math>=</math></td> | |||
<td align="left"> | |||
<math> | |||
-(n+1) \biggl( \frac{\sigma_c^2}{6\gamma_g}\biggr) | |||
\biggl[ \frac{\xi^2}{ \theta} \biggl( \frac{n-1}{n-3}\biggr) - \frac{1}{\theta^n} \cdot \frac{d\ln\theta}{d\ln\xi} \biggr] \, , | |||
</math> | |||
</td> | |||
</tr> | |||
</table> | |||
which goes to zero if <math>\sigma_c^2 = 0</math>. | |||
=Parabolic Density Distribution= | |||
Here, we build upon our [[SSC/Structure/OtherAnalyticModels#Parabolic_Density_Distribution|separate discussion]] of equilibrium configurations with a parabolic density distribution. | |||
==Equilibrium Structure== | |||
In an article titled, "Radial Oscillations of a Stellar Model," [http://adsabs.harvard.edu/abs/1949MNRAS.109..103P C. Prasad (1949, MNRAS, 109, 103)] investigated the properties of an equilibrium configuration with a prescribed density distribution given by the expression, | |||
<div align="center"> | |||
<math>\rho_0 = \rho_c\biggl[ 1 - \biggl(\frac{r_0}{R} \biggr)^2 \biggr] \, ,</math> | |||
</div> | |||
where, <math>\rho_c</math> is the central density and, <math>R</math> is the radius of the star. Both the mass distribution and the pressure distribution can be obtained analytically from this specified density distribution. Specifically, | |||
<div align="center"> | |||
<table border="0" cellpadding="5" align="center"> | |||
<tr> | |||
<td align="right"> | |||
<math>M_r</math> | |||
</td> | |||
<td align="center"> | |||
<math>=</math> | |||
</td> | |||
<td align="left"> | |||
<math>\int_0^{r_0} 4\pi r_0^2 \rho_0 dr_0</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> | |||
| |||
</td> | |||
<td align="center"> | |||
<math>=</math> | |||
</td> | |||
<td align="left"> | |||
<math>\frac{4\pi\rho_c r_0^3}{3} \biggl[1 - \frac{3}{5} \biggl( \frac{r_0}{R} \biggr)^2 \biggr] \, ,</math> | |||
</td> | |||
</tr> | |||
</table> | |||
</div> | |||
in which case we can write, | |||
<div align="center"> | |||
<table border="0" cellpadding="5" align="center"> | |||
<tr> | |||
<td align="right"> | |||
<math>~g_0 \equiv \frac{G M_r }{r_0^2} </math> | |||
</td> | |||
<td align="center"> | |||
<math>~=</math> | |||
</td> | |||
<td align="left"> | |||
<math>~\frac{4\pi G \rho_c r_0}{3} | |||
\biggl[1 - \frac{3}{5} \biggl( \frac{r_0}{R} \biggr)^2\biggr] \, ,</math> | |||
</td> | |||
</tr> | |||
</table> | |||
</div> | |||
and, | |||
<table border="0" cellpadding="5" align="center"> | |||
<tr> | |||
<td align="right"> | |||
<math>\Delta \equiv \frac{M_r }{4\pi r_0^3\rho_0} </math> | |||
</td> | |||
<td align="center"> | |||
<math>~=</math> | |||
</td> | |||
<td align="left"> | |||
<math> | |||
\frac{1 }{3} \biggl[1 - \frac{3}{5} \biggl( \frac{r_0}{R} \biggr)^2 \biggr]\biggl[ 1 - \biggl(\frac{r_0}{R} \biggr)^2 \biggr]^{-1} | |||
\, .</math> | |||
</td> | |||
</tr> | |||
</table> | |||
Hence, proceeding via what we have labeled as [[SSCpt2/SolutionStrategies#Technique_1|"Technique 1"]], and enforcing the surface boundary condition, <math>~P(R) = 0</math>, [http://adsabs.harvard.edu/abs/1949MNRAS.109..103P Prasad (1949)] determines that, | |||
<div align="center"> | |||
<table border="0" cellpadding="5" align="center"> | |||
<tr> | |||
<td align="right"> | |||
<math>P_0</math> | |||
</td> | |||
<td align="center"> | |||
<math>=</math> | |||
</td> | |||
<td align="left"> | |||
<math> | |||
\frac{4\pi G\rho_c^2 R^2}{15} | |||
\biggl[1-\biggl(\frac{r_0}{R}\biggr)^2\biggr]^2 | |||
\biggl[1-\frac{1}{2}\biggl(\frac{r_0}{R}\biggr)^2\biggr] | |||
\, ,</math> | |||
</td> | |||
</tr> | |||
</table> | |||
</div> | |||
where, it can readily be deduced, as well, that the central pressure is, | |||
<div align="center"> | |||
<math>P_c = \frac{4\pi}{15} G\rho_c^2 R^2 \, .</math> | |||
</div> | |||
<table border="1" width="90%" cellpadding="8" align="center"><tr><td align="left"> | |||
<div align="center">'''Specific Entropy Distribution'''</div> | |||
For purposes of later discussion, we find from [[Appendix/Ramblings/PatrickMotl#Tying_Expressions_into_H_Book_Context|a separate examination of specific entropy distributions]], <math>s_0(r_0)</math>, that, | |||
<table border="0" cellpadding="5" align="center"> | |||
<tr> | |||
<td align="right"> | |||
<math>~\frac{s_0}{\Re/\bar{\mu}}</math> | |||
</td> | |||
<td align="center"> | |||
<math>~=</math> | |||
</td> | |||
<td align="left"> | |||
<math>~ | |||
\frac{1}{(\gamma_g-1)}\ln \biggl(\frac{\tau_0}{\rho_0}\biggr)^{\gamma_g} | |||
= | |||
\frac{1}{(\gamma_g-1)}\ln \biggl[ \frac{P_0}{(\gamma_g-1)\rho_0^{\gamma_g}} \biggr] | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> | |||
<math>\Rightarrow ~~~ \biggl[ \frac{\gamma_g - 1}{\Re/\bar{\mu}} \biggr]s_0</math> | |||
</td> | |||
<td align="center"> | |||
<math>~=</math> | |||
</td> | |||
<td align="left"> | |||
<math>~ | |||
\ln \biggl[ \frac{P_c}{(\gamma_g-1)\rho_c^{\gamma_g}} \biggr] | |||
+ | |||
\ln \biggl\{ \biggl[1-\biggl(\frac{r_0}{R}\biggr)^2\biggr]^2 | |||
\biggl[1-\frac{1}{2}\biggl(\frac{r_0}{R}\biggr)^2\biggr] | |||
\biggr\} | |||
+ | |||
\ln \biggl\{ \biggl[ 1 - \biggl(\frac{r_0}{R} \biggr)^2 \biggr]^{-\gamma_g}\biggr\} | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> | |||
| |||
</td> | |||
<td align="center"> | |||
<math>~=</math> | |||
</td> | |||
<td align="left"> | |||
<math>~ | |||
\ln \biggl[ \frac{P_c}{(\gamma_g-1)\rho_c^{\gamma_g}} \biggr] | |||
+ | |||
\ln \biggl\{ | |||
\biggl[1-\frac{1}{2}\biggl(\frac{r_0}{R}\biggr)^2\biggr] | |||
\biggr\} | |||
+ (2- \gamma_g) | |||
\ln \biggl\{ \biggl[ 1 - \biggl(\frac{r_0}{R} \biggr)^2 \biggr]\biggr\} \, . | |||
</math> | |||
</td> | |||
</tr> | |||
</table> | |||
Notice that, independent of the value of <math>\gamma_g</math>, the specific entropy varies with <math>r_0</math> throughout the structure. According to the [[2DStructure/AxisymmetricInstabilities#Schwarzschild_Criterion|Schwarzschild criterion]], spherically symmetric equilibrium configurations will be stable against convection if the specific entropy increases outward, and unstable toward convection if the specific entropy decreases outward. Let's examine the slope, <math>ds_0/dr_0</math>, throughout configurations that have a parabolic density distribution. | |||
<table border="0" cellpadding="5" align="center"> | |||
<tr> | |||
<td align="right"> | |||
<math>\biggl[ \frac{\gamma_g - 1}{\Re/\bar{\mu}} \biggr]\frac{ds_0}{dr_0}</math> | |||
</td> | |||
<td align="center"> | |||
<math>~=</math> | |||
</td> | |||
<td align="left"> | |||
<math>~ | |||
-\frac{r_0}{R^2} \biggl[1-\frac{1}{2}\biggl(\frac{r_0}{R}\biggr)^2\biggr]^{-1} | |||
- \frac{2(2- \gamma_g)r_0}{R^2} | |||
\biggl[ 1 - \biggl(\frac{r_0}{R} \biggr)^2 \biggr]^{-1} | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> | |||
<math> | |||
\Rightarrow ~~~ \frac{R^2}{r_0} | |||
\biggl[1-\frac{1}{2}\biggl(\frac{r_0}{R}\biggr)^2\biggr] | |||
\biggl[ 1 - \biggl(\frac{r_0}{R} \biggr)^2 \biggr] | |||
\biggl[ \frac{\gamma_g - 1}{\Re/\bar{\mu}} \biggr]\frac{ds_0}{dr_0} | |||
</math> | |||
</td> | |||
<td align="center"> | |||
<math>=</math> | |||
</td> | |||
<td align="left"> | |||
<math> | |||
-~\biggl[1-\biggl(\frac{r_0}{R}\biggr)^2\biggr] | |||
- 2(2- \gamma_g) | |||
\biggl[ 1 - \frac{1}{2}\biggl(\frac{r_0}{R} \biggr)^2 \biggr] | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> | |||
| |||
</td> | |||
<td align="center"> | |||
<math>~=</math> | |||
</td> | |||
<td align="left"> | |||
<math>~(2\gamma_g- 5) | |||
+ (3 - \gamma_g) | |||
\biggl[\biggl(\frac{r_0}{R} \biggr)^2 \biggr] | |||
</math> | |||
</td> | |||
</tr> | |||
</table> | |||
[[File:EntropyDistribution245.png|right|400px]] | |||
The slope is zero when, | |||
<table border="0" cellpadding="5" align="center"> | |||
<tr> | |||
<td align="right"> | |||
<math> | |||
\biggl(\frac{r_0}{R} \biggr)^2 | |||
</math> | |||
</td> | |||
<td align="center"> | |||
<math>=</math> | |||
</td> | |||
<td align="left"> | |||
<math> | |||
\frac{5 - 2\gamma_g}{3 - \gamma_g} \, . | |||
</math> | |||
</td> | |||
</tr> | |||
</table> | |||
Moving from the center of the configuration to its surface, <math>0 < (r_0/R)^2 < 1</math>, the slope will go to zero — hence, the slope of the entropy will change sign | |||
</td></tr></table> | |||
==Some Relevant Structural Derivatives== | |||
We note for later use that, | |||
<table border="0" cellpadding="5" align="center"> | |||
<tr> | |||
<td align="right"> | |||
<math>\frac{1}{P_c} \cdot \frac{dP_0}{dr_0}</math> | |||
</td> | |||
<td align="center"> | |||
<math>=</math> | |||
</td> | |||
<td align="left"> | |||
<math> | |||
\biggl[1-\biggl(\frac{r_0}{R}\biggr)^2\biggr]^2 | |||
\frac{d}{dr_0}\biggl[1-\frac{1}{2}\biggl(\frac{r_0}{R}\biggr)^2\biggr] | |||
+ | |||
\biggl[1-\frac{1}{2}\biggl(\frac{r_0}{R}\biggr)^2\biggr] | |||
\frac{d}{dr_0}\biggl[1-\biggl(\frac{r_0}{R}\biggr)^2\biggr]^2 | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> | |||
| |||
</td> | |||
<td align="center"> | |||
<math>=</math> | |||
</td> | |||
<td align="left"> | |||
<math> | |||
-\frac{1}{2R^2} \biggl[1-\biggl(\frac{r_0}{R}\biggr)^2\biggr]^2 | |||
\frac{d}{dr_0}\biggl[r_0^2\biggr] | |||
+ | |||
2\biggl[1-\biggl(\frac{r_0}{R}\biggr)^2\biggr] | |||
\biggl[1-\frac{1}{2}\biggl(\frac{r_0}{R}\biggr)^2\biggr] | |||
\frac{d}{dr_0}\biggl[1-\biggl(\frac{r_0}{R}\biggr)^2\biggr] | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> | |||
| |||
</td> | |||
<td align="center"> | |||
<math>=</math> | |||
</td> | |||
<td align="left"> | |||
<math>\biggl\{ | |||
-\frac{1}{2R^2} \biggl[1-\biggl(\frac{r_0}{R}\biggr)^2\biggr]^2 | |||
- \frac{2}{R^2}\biggl[1-\biggl(\frac{r_0}{R}\biggr)^2\biggr] | |||
\biggl[1-\frac{1}{2}\biggl(\frac{r_0}{R}\biggr)^2\biggr] | |||
\biggr\}\frac{d}{dr_0}\biggl[r_0^2\biggr] | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> | |||
| |||
</td> | |||
<td align="center"> | |||
<math>=</math> | |||
</td> | |||
<td align="left"> | |||
<math>-\frac{r_0}{R^2}\biggl\{ | |||
\biggl[1-\biggl(\frac{r_0}{R}\biggr)^2\biggr]^2 | |||
+ 4\biggl[1-\biggl(\frac{r_0}{R}\biggr)^2\biggr] | |||
\biggl[1-\frac{1}{2}\biggl(\frac{r_0}{R}\biggr)^2\biggr] | |||
\biggr\} | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> | |||
| |||
</td> | |||
<td align="center"> | |||
<math>=</math> | |||
</td> | |||
<td align="left"> | |||
<math>-\frac{r_0}{R^2}\biggl\{ | |||
\biggl[1-\biggl(\frac{r_0}{R}\biggr)^2\biggr] | |||
+ 4 | |||
\biggl[1-\frac{1}{2}\biggl(\frac{r_0}{R}\biggr)^2\biggr] | |||
\biggr\} \biggl[1-\biggl(\frac{r_0}{R}\biggr)^2\biggr] | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> | |||
| |||
</td> | |||
<td align="center"> | |||
<math>=</math> | |||
</td> | |||
<td align="left"> | |||
<math>-\frac{5r_0}{R^2} | |||
\biggl[1-\frac{3}{5}\biggl(\frac{r_0}{R}\biggr)^2\biggr] | |||
\biggl[1-\biggl(\frac{r_0}{R}\biggr)^2\biggr] \, . | |||
</math> | |||
</td> | |||
</tr> | |||
</table> | |||
<table border="1" align="center" width="80%" cellpadding="10"><tr><td align="left"> | |||
Checking for detailed force-balance, we note that, | |||
<table border="0" cellpadding="5" align="center"> | |||
<tr> | |||
<td align="right"> | |||
<math>- ~\frac{1}{\rho_0} \cdot \frac{dP_0}{dr_0}</math> | |||
</td> | |||
<td align="center"> | |||
<math>=</math> | |||
</td> | |||
<td align="left"> | |||
<math>\frac{5r_0}{R^2}\biggl[ \frac{4\pi G \rho_c^2 R^2}{15} \biggr] | |||
\biggl[1-\frac{3}{5}\biggl(\frac{r_0}{R}\biggr)^2\biggr] | |||
\biggl[1-\biggl(\frac{r_0}{R}\biggr)^2\biggr] \cdot \frac{1}{\rho_c} \biggl[1 - \biggl(\frac{r_0}{R} \biggr)^2\biggr]^{-1} | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> | |||
| |||
</td> | |||
<td align="center"> | |||
<math>=</math> | |||
</td> | |||
<td align="left"> | |||
<math>\frac{4\pi G \rho_c r_0}{3} | |||
\biggl[1-\frac{3}{5}\biggl(\frac{r_0}{R}\biggr)^2\biggr] \, , | |||
</math> | |||
</td> | |||
</tr> | |||
</table> | |||
which is exactly the expression that we have just derived for <math>g_0 = GM_r/r_0^2</math>. | |||
</td></tr></table> | |||
Hence, | |||
<table border="0" cellpadding="5" align="center"> | |||
<tr> | |||
<td align="right"> | |||
<math>\frac{d\ln P_0}{d \ln r_0} = \frac{r_0}{P_0/P_c} \biggl[ \frac{1}{P_c}\cdot \frac{dP_0}{dr_0} \biggr]</math> | |||
</td> | |||
<td align="center"> | |||
<math>=</math> | |||
</td> | |||
<td align="left"> | |||
<math>-\frac{5r_0^2}{R^2} | |||
\biggl[1-\frac{3}{5}\biggl(\frac{r_0}{R}\biggr)^2\biggr] | |||
\biggl[1-\biggl(\frac{r_0}{R}\biggr)^2\biggr] | |||
\biggl\{\biggl[1-\biggl(\frac{r_0}{R}\biggr)^2\biggr]^2 | |||
\biggl[1-\frac{1}{2}\biggl(\frac{r_0}{R}\biggr)^2\biggr]\biggr\}^{-1} | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> | |||
| |||
</td> | |||
<td align="center"> | |||
<math>=</math> | |||
</td> | |||
<td align="left"> | |||
<math> | |||
-5 \biggl(\frac{r_0}{R}\biggr)^2 | |||
\biggl[1-\frac{3}{5}\biggl(\frac{r_0}{R}\biggr)^2\biggr] | |||
\biggl[1-\biggl(\frac{r_0}{R}\biggr)^2\biggr]^{-1} | |||
\biggl[1-\frac{1}{2}\biggl(\frac{r_0}{R}\biggr)^2\biggr]^{-1} | |||
\, ; | |||
</math> | |||
</td> | |||
</tr> | |||
</table> | |||
and, given that, | |||
<table border="0" cellpadding="5" align="center"> | |||
<tr> | |||
<td align="right"> | |||
<math>\Delta^{-1} </math> | |||
</td> | |||
<td align="center"> | |||
<math>~=</math> | |||
</td> | |||
<td align="left"> | |||
<math> | |||
3 | |||
\biggl[1 - \frac{3}{5} \biggl( \frac{r_0}{R} \biggr)^2 \biggr]^{-1} | |||
\biggl[ 1 - \biggl(\frac{r_0}{R} \biggr)^2 \biggr] | |||
\, ,</math> | |||
</td> | |||
</tr> | |||
</table> | |||
we can write, | |||
<table border="0" cellpadding="5" align="center"> | |||
<tr> | |||
<td align="right"> | |||
<math>\frac{1}{\Delta}\cdot \frac{d\ln P_0}{d \ln r_0} </math> | |||
</td> | |||
<td align="center"> | |||
<math>=</math> | |||
</td> | |||
<td align="left"> | |||
<math>- 15 \biggl(\frac{r_0}{R}\biggr)^2 | |||
\biggl[1-\frac{3}{5}\biggl(\frac{r_0}{R}\biggr)^2\biggr] | |||
\biggl[1-\biggl(\frac{r_0}{R}\biggr)^2\biggr]^{-1} | |||
\biggl[1-\frac{1}{2}\biggl(\frac{r_0}{R}\biggr)^2\biggr]^{-1} | |||
\biggl[1 - \frac{3}{5} \biggl( \frac{r_0}{R} \biggr)^2 \biggr]^{-1} | |||
\biggl[ 1 - \biggl(\frac{r_0}{R} \biggr)^2 \biggr] | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> | |||
| |||
</td> | |||
<td align="center"> | |||
<math>=</math> | |||
</td> | |||
<td align="left"> | |||
<math>- 15 \biggl(\frac{r_0}{R}\biggr)^2 | |||
\biggl[1-\frac{1}{2}\biggl(\frac{r_0}{R}\biggr)^2\biggr]^{-1} \, . | |||
</math> | |||
</td> | |||
</tr> | |||
</table> | |||
Also, | |||
<table border="0" cellpadding="5" align="center"> | |||
<tr> | |||
<td align="right"> | |||
<math>3 \cdot \frac{d\Delta}{dr_0} </math> | |||
</td> | |||
<td align="center"> | |||
<math>=</math> | |||
</td> | |||
<td align="left"> | |||
<math> | |||
\frac{d}{dr_0}\biggl\{ | |||
\biggl[1 - \frac{3}{5} \biggl( \frac{r_0}{R} \biggr)^2 \biggr] | |||
\biggl[ 1 - \biggl(\frac{r_0}{R} \biggr)^2 \biggr]^{-1} | |||
\biggr\} | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> | |||
| |||
</td> | |||
<td align="center"> | |||
<math>=</math> | |||
</td> | |||
<td align="left"> | |||
<math> | |||
\biggl[1 - \frac{3}{5} \biggl( \frac{r_0}{R} \biggr)^2 \biggr]\frac{d}{dr_0} | |||
\biggl[ 1 - \biggl(\frac{r_0}{R} \biggr)^2 \biggr]^{-1} | |||
+ | |||
\biggl[ 1 - \biggl(\frac{r_0}{R} \biggr)^2 \biggr]^{-1}\frac{d}{dr_0} | |||
\biggl[1 - \frac{3}{5} \biggl( \frac{r_0}{R} \biggr)^2 \biggr] | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> | |||
| |||
</td> | |||
<td align="center"> | |||
<math>=</math> | |||
</td> | |||
<td align="left"> | |||
<math> | |||
\biggl[1 - \frac{3}{5} \biggl( \frac{r_0}{R} \biggr)^2 \biggr] | |||
\biggl[ 1 - \biggl(\frac{r_0}{R} \biggr)^2 \biggr]^{-2} | |||
\frac{2r_0}{R^2} | |||
+ | |||
\biggl[ 1 - \biggl(\frac{r_0}{R} \biggr)^2 \biggr]^{-1} | |||
\biggl[- \frac{6}{5} \cdot \frac{r_0}{R^2} \biggr] | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> | |||
| |||
</td> | |||
<td align="center"> | |||
<math>=</math> | |||
</td> | |||
<td align="left"> | |||
<math> | |||
\frac{r_0}{R^2} \biggl\{ | |||
2\biggl[1 - \frac{3}{5} \biggl( \frac{r_0}{R} \biggr)^2 \biggr] | |||
\biggl[ 1 - \biggl(\frac{r_0}{R} \biggr)^2 \biggr]^{-2} | |||
- \frac{6}{5} | |||
\biggl[ 1 - \biggl(\frac{r_0}{R} \biggr)^2 \biggr]^{-1} | |||
\biggr\} | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> | |||
| |||
</td> | |||
<td align="center"> | |||
<math>=</math> | |||
</td> | |||
<td align="left"> | |||
<math> | |||
\frac{r_0}{5R^2} \biggl[ 1 - \biggl(\frac{r_0}{R} \biggr)^2 \biggr]^{-2}\biggl\{ | |||
\biggl[10 - 6 \biggl( \frac{r_0}{R} \biggr)^2 \biggr] | |||
- | |||
\biggl[ 6 - 6\biggl(\frac{r_0}{R} \biggr)^2 \biggr] | |||
\biggr\} | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> | |||
| |||
</td> | |||
<td align="center"> | |||
<math>=</math> | |||
</td> | |||
<td align="left"> | |||
<math> | |||
\frac{4r_0}{5R^2} \biggl[ 1 - \biggl(\frac{r_0}{R} \biggr)^2 \biggr]^{-2} | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> | |||
<math>\Rightarrow ~~~ \frac{d\Delta}{dr_0}</math> | |||
</td> | |||
<td align="center"> | |||
<math>=</math> | |||
</td> | |||
<td align="left"> | |||
<math> | |||
\frac{4r_0}{15R^2} \biggl[ 1 - \biggl(\frac{r_0}{R} \biggr)^2 \biggr]^{-2} | |||
\, ; | |||
</math> | |||
</td> | |||
</tr> | |||
</table> | |||
and, | |||
<table border="0" cellpadding="5" align="center"> | |||
<tr> | |||
<td align="right"> | |||
<math>\frac{15R^2}{4} \cdot \frac{d^2\Delta}{dr_0^2}</math> | |||
</td> | |||
<td align="center"> | |||
<math>=</math> | |||
</td> | |||
<td align="left"> | |||
<math> | |||
\biggl[ 1 - \biggl(\frac{r_0}{R} \biggr)^2 \biggr]^{-2} | |||
-2r_0 | |||
\biggl[ 1 - \biggl(\frac{r_0}{R} \biggr)^2 \biggr]^{-3}\biggl[ -\frac{2r_0}{R^2} \biggr] | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> | |||
| |||
</td> | |||
<td align="center"> | |||
<math>=</math> | |||
</td> | |||
<td align="left"> | |||
<math> | |||
\biggl[ 1 - \biggl(\frac{r_0}{R} \biggr)^2 \biggr]^{-3} \biggl\{ | |||
\biggl[ 1 - \biggl(\frac{r_0}{R} \biggr)^2 \biggr] | |||
+\frac{4r_0^2}{R^2} \biggr\} | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> | |||
| |||
</td> | |||
<td align="center"> | |||
<math>=</math> | |||
</td> | |||
<td align="left"> | |||
<math> | |||
\biggl[ 1 - \biggl(\frac{r_0}{R} \biggr)^2 \biggr]^{-3} | |||
\biggl[1 + 3 \biggl(\frac{r_0}{R}\biggr)^2 \biggr] | |||
\, . | |||
</math> | |||
</td> | |||
</tr> | |||
</table> | |||
==Neutral Mode== | |||
Again, adopting the ''trial'' eigenfunction, | |||
<table border="0" cellpadding="5" align="center"> | |||
<tr> | |||
<td align="right"><math>x_t</math></td> | |||
<td align="center"><math>=</math></td> | |||
<td align="left"> | |||
<math> | |||
a - b\Delta | |||
\, , | |||
</math> | |||
</td> | |||
</tr> | |||
</table> | |||
from the, | |||
<div align="center" id="Delta_Highlighted"> | |||
<font color="#770000">'''Δ-Highlighted LAWE'''</font><br /> | |||
{{Math/EQ_RadialPulsation04}} | |||
</div> | |||
we can write, | |||
<table border="0" cellpadding="5" align="center"> | |||
<tr> | |||
<td align="right"><math>\mathrm{LAWE}</math></td> | |||
<td align="center"><math>=</math></td> | |||
<td align="left"> | |||
<math> | |||
- b \cdot \frac{d^2\Delta}{dr_0^2} - \frac{b}{r_0}\biggl[4 + \frac{d\ln P_0}{d\ln r_0} \biggr] \frac{d\Delta}{dr_0} | |||
+ \alpha\biggl[ \frac{d\ln P_0}{d\ln r_0} \biggr] \frac{(a - b\Delta)}{r_0^2} | |||
- \frac{1}{\Delta} \biggl[\frac{d\ln P_0}{d\ln r_0}\cdot \frac{\rho_c}{\rho_0} \biggl( \frac{\sigma_c^2}{6\gamma_g}\biggr)\biggr] \frac{(a - b\Delta)}{r_0^2} | |||
</math> | |||
</td> | |||
</tr> | |||
</table> | |||
===First Attempt=== | |||
<table border="0" cellpadding="5" align="center"> | |||
<tr> | |||
<td align="right"><math>\Rightarrow ~~~ \frac{1}{b} \biggl[ r_0^2 \times \mathrm{LAWE} \biggr]</math></td> | |||
<td align="center"><math>=</math></td> | |||
<td align="left"> | |||
<math> | |||
- r_0^2 \cdot \frac{d^2\Delta}{dr_0^2} - r_0\biggl[4 + \frac{d\ln P_0}{d\ln r_0} \biggr] \frac{d\Delta}{dr_0} | |||
+ \alpha\biggl[ \frac{d\ln P_0}{d\ln r_0} \biggr] \biggl( \frac{a}{b} - \Delta \biggr) | |||
- \frac{1}{\Delta} \biggl[\frac{d\ln P_0}{d\ln r_0}\cdot \frac{\rho_c}{\rho_0} \biggl( \frac{\sigma_c^2}{6\gamma_g}\biggr)\biggr] \biggl(\frac{a}{b} - \Delta \biggr) | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> </td> | |||
<td align="center"><math>=</math></td> | |||
<td align="left"> | |||
<math> | |||
- r_0^2 \cdot \frac{d^2\Delta}{dr_0^2} | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> </td> | |||
<td align="center"> </td> | |||
<td align="left"> | |||
<math> | |||
- r_0\biggl[4 + \frac{d\ln P_0}{d\ln r_0} \biggr] \frac{d\Delta}{dr_0} | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> </td> | |||
<td align="center"> </td> | |||
<td align="left"> | |||
<math> | |||
+ \alpha\biggl[ \frac{d\ln P_0}{d\ln r_0} \biggr] \biggl( \frac{a}{b} - \Delta \biggr) | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> </td> | |||
<td align="center"> </td> | |||
<td align="left"> | |||
<math> | |||
+ \frac{\rho_c}{\rho_0} \biggl( \frac{\sigma_c^2}{6\gamma_g}\biggr) \biggl\{ | |||
\biggl[\frac{d\ln P_0}{d\ln r_0}\biggr] | |||
- \frac{a}{b}\biggl[\frac{1}{\Delta} \cdot \frac{d\ln P_0}{d\ln r_0}\biggr] \biggr\} | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> </td> | |||
<td align="center"><math>=</math></td> | |||
<td align="left"> | |||
<math> | |||
- \frac{4}{15} \biggl(\frac{r_0}{R}\biggr)^2 | |||
\biggl[ 1 - \biggl(\frac{r_0}{R} \biggr)^2 \biggr]^{-3} | |||
\biggl[1 + 3 \biggl(\frac{r_0}{R}\biggr)^2 \biggr] | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> </td> | |||
<td align="center"> </td> | |||
<td align="left"> | |||
<math> | |||
- \frac{16}{15}\biggl(\frac{r_0}{R}\biggr)^2 | |||
\biggl[ 1 - \biggl(\frac{r_0}{R} \biggr)^2 \biggr]^{-2} | |||
- \frac{4}{15}\biggl(\frac{r_0}{R}\biggr)^2 | |||
\biggl\{ -5 \biggl(\frac{r_0}{R}\biggr)^2 | |||
\biggl[1-\frac{3}{5}\biggl(\frac{r_0}{R}\biggr)^2\biggr] | |||
\biggl[1-\biggl(\frac{r_0}{R}\biggr)^2\biggr]^{-1} | |||
\biggl[1-\frac{1}{2}\biggl(\frac{r_0}{R}\biggr)^2\biggr]^{-1} | |||
\biggr\} | |||
\biggl[ 1 - \biggl(\frac{r_0}{R} \biggr)^2 \biggr]^{-2} | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> </td> | |||
<td align="center"> </td> | |||
<td align="left"> | |||
<math> | |||
+ \alpha | |||
\biggl\{ -5 \biggl(\frac{r_0}{R}\biggr)^2 | |||
\biggl[1-\frac{3}{5}\biggl(\frac{r_0}{R}\biggr)^2\biggr] | |||
\biggl[1-\biggl(\frac{r_0}{R}\biggr)^2\biggr]^{-1} | |||
\biggl[1-\frac{1}{2}\biggl(\frac{r_0}{R}\biggr)^2\biggr]^{-1} | |||
\biggr\} | |||
\biggl\{ \frac{a}{b} - \Delta \biggr\} | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> </td> | |||
<td align="center"> </td> | |||
<td align="left"> | |||
<math> | |||
+ \frac{\rho_c}{\rho_0} \biggl( \frac{\sigma_c^2}{6\gamma_g}\biggr) \biggl\{ | |||
\biggl[\frac{d\ln P_0}{d\ln r_0}\biggr] | |||
- \frac{a}{b}\biggl[\frac{1}{\Delta} \cdot \frac{d\ln P_0}{d\ln r_0}\biggr] \biggr\} | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> </td> | |||
<td align="center"><math>=</math></td> | |||
<td align="left"> | |||
<math> | |||
- \frac{4}{3}\biggl(\frac{r_0}{R}\biggr)^2\biggl[ 1 - \frac{1}{5} \biggl(\frac{r_0}{R}\biggr)^2 \biggr] | |||
\biggl[ 1 - \biggl(\frac{r_0}{R} \biggr)^2 \biggr]^{-3} | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> </td> | |||
<td align="center"> </td> | |||
<td align="left"> | |||
<math> | |||
+~ \frac{4}{3}\biggl(\frac{r_0}{R}\biggr)^4 | |||
\biggl[1-\frac{3}{5}\biggl(\frac{r_0}{R}\biggr)^2\biggr] | |||
\biggl[1-\frac{1}{2}\biggl(\frac{r_0}{R}\biggr)^2\biggr]^{-1} | |||
\biggl[ 1 - \biggl(\frac{r_0}{R} \biggr)^2 \biggr]^{-3} | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> </td> | |||
<td align="center"> </td> | |||
<td align="left"> | |||
<math> | |||
+ ~ \frac{5\alpha}{3} | |||
\biggl(\frac{r_0}{R}\biggr)^2 \biggl[1-\frac{3}{5}\biggl(\frac{r_0}{R}\biggr)^2\biggr] | |||
\biggl[1-\biggl(\frac{r_0}{R}\biggr)^2\biggr]^{-2} | |||
\biggl[1-\frac{1}{2}\biggl(\frac{r_0}{R}\biggr)^2\biggr]^{-1} | |||
\biggl\{ | |||
1 - \frac{3a}{b} -\frac{3}{5}\biggl(\frac{r_0}{R}\biggr)^2 | |||
\biggr\} | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> </td> | |||
<td align="center"> </td> | |||
<td align="left"> | |||
<math> | |||
+ \frac{\rho_c}{\rho_0} \biggl( \frac{\sigma_c^2}{6\gamma_g}\biggr) \biggl\{ | |||
\biggl[\frac{d\ln P_0}{d\ln r_0}\biggr] | |||
- \frac{a}{b}\biggl[\frac{1}{\Delta} \cdot \frac{d\ln P_0}{d\ln r_0}\biggr] \biggr\} | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> </td> | |||
<td align="center"><math>=</math></td> | |||
<td align="left"> | |||
<math> | |||
- \frac{4}{3}\biggl(\frac{r_0}{R}\biggr)^2\biggl[ 1 - \frac{1}{5} \biggl(\frac{r_0}{R}\biggr)^2 \biggr] | |||
\biggl[ 1 - \biggl(\frac{r_0}{R} \biggr)^2 \biggr]^{-3} | |||
+ ~ \frac{5\alpha}{3} | |||
\biggl(\frac{r_0}{R}\biggr)^2 \biggl[1-\frac{3}{5}\biggl(\frac{r_0}{R}\biggr)^2\biggr] | |||
\biggl[1-\biggl(\frac{r_0}{R}\biggr)^2\biggr]^{-2} | |||
\biggl[1-\frac{1}{2}\biggl(\frac{r_0}{R}\biggr)^2\biggr]^{-1} | |||
\biggl(1 - \frac{3a}{b} \biggr) | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> </td> | |||
<td align="center"> </td> | |||
<td align="left"> | |||
<math> | |||
+~ \frac{4}{3}\biggl(\frac{r_0}{R}\biggr)^4 | |||
\biggl[1-\frac{3}{5}\biggl(\frac{r_0}{R}\biggr)^2\biggr] | |||
\biggl[1-\frac{1}{2}\biggl(\frac{r_0}{R}\biggr)^2\biggr]^{-1} | |||
\biggl[ 1 - \biggl(\frac{r_0}{R} \biggr)^2 \biggr]^{-3} | |||
- ~ \alpha | |||
\biggl(\frac{r_0}{R}\biggr)^4 \biggl[1-\frac{3}{5}\biggl(\frac{r_0}{R}\biggr)^2\biggr] | |||
\biggl[1-\biggl(\frac{r_0}{R}\biggr)^2\biggr]^{-2} | |||
\biggl[1-\frac{1}{2}\biggl(\frac{r_0}{R}\biggr)^2\biggr]^{-1} | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> </td> | |||
<td align="center"> </td> | |||
<td align="left"> | |||
<math> | |||
+ \frac{\rho_c}{\rho_0} \biggl( \frac{\sigma_c^2}{6\gamma_g}\biggr) \biggl\{ | |||
\biggl[\frac{d\ln P_0}{d\ln r_0}\biggr] | |||
- \frac{a}{b}\biggl[\frac{1}{\Delta} \cdot \frac{d\ln P_0}{d\ln r_0}\biggr] \biggr\} | |||
</math> | |||
</td> | |||
</tr> | |||
</table> | |||
Continuing … | |||
<table border="0" cellpadding="5" align="center"> | |||
<tr> | |||
<td align="right"><math>\frac{1}{b} \biggl[ r_0^2 \times \mathrm{LAWE} \biggr]</math></td> | |||
<td align="center"><math>=</math></td> | |||
<td align="left"> | |||
<math> | |||
\biggl(\frac{r_0}{R}\biggr)^2 \biggl[ 1 - \biggl(\frac{r_0}{R} \biggr)^2 \biggr]^{-3} | |||
\biggl[1-\frac{1}{2}\biggl(\frac{r_0}{R}\biggr)^2\biggr]^{-1} | |||
\biggl\{ | |||
\frac{5\alpha}{3}\biggl(1 - \frac{3a}{b} \biggr) | |||
\biggl[1-\frac{3}{5}\biggl(\frac{r_0}{R}\biggr)^2 \biggr] | |||
\biggl[1-\biggl(\frac{r_0}{R}\biggr)^2\biggr] | |||
- \frac{4}{3}\biggl[ 1 - \frac{1}{5} \biggl(\frac{r_0}{R}\biggr)^2 \biggr]\biggl[1-\frac{1}{2}\biggl(\frac{r_0}{R}\biggr)^2\biggr] | |||
\biggr\} | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> </td> | |||
<td align="center"> </td> | |||
<td align="left"> | |||
<math> | |||
+~ \biggl(\frac{4}{3} - \alpha \biggr)\biggl(\frac{r_0}{R}\biggr)^4\biggl[1-\frac{3}{5}\biggl(\frac{r_0}{R}\biggr)^2\biggr] | |||
\biggl[1-\frac{1}{2}\biggl(\frac{r_0}{R}\biggr)^2\biggr]^{-1}\biggl[ 1 - \biggl(\frac{r_0}{R} \biggr)^2 \biggr]^{-3} | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> </td> | |||
<td align="center"> </td> | |||
<td align="left"> | |||
<math> | |||
-~ \alpha \biggl(\frac{r_0}{R}\biggr)^6\biggl[1-\frac{3}{5}\biggl(\frac{r_0}{R}\biggr)^2\biggr] | |||
\biggl[1-\frac{1}{2}\biggl(\frac{r_0}{R}\biggr)^2\biggr]^{-1}\biggl[ 1 - \biggl(\frac{r_0}{R} \biggr)^2 \biggr]^{-3} | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> </td> | |||
<td align="center"> </td> | |||
<td align="left"> | |||
<math> | |||
+ \frac{\rho_c}{\rho_0} \biggl( \frac{\sigma_c^2}{6\gamma_g}\biggr) \biggl\{ | |||
\biggl[\frac{d\ln P_0}{d\ln r_0}\biggr] | |||
- \frac{a}{b}\biggl[\frac{1}{\Delta} \cdot \frac{d\ln P_0}{d\ln r_0}\biggr] \biggr\} | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> </td> | |||
<td align="center"><math>=</math></td> | |||
<td align="left"> | |||
<math> | |||
\biggl(\frac{r_0}{R}\biggr)^2 | |||
\biggl[1-\frac{1}{2}\biggl(\frac{r_0}{R}\biggr)^2\biggr]^{-1} | |||
\biggl[ 1 - \biggl(\frac{r_0}{R} \biggr)^2 \biggr]^{-3} | |||
\biggl\{ | |||
\frac{5\alpha}{3}\biggl(1 - \frac{3a}{b} \biggr) | |||
\biggl[1-\frac{8}{5}\biggl(\frac{r_0}{R}\biggr)^2 + \frac{3}{5} \biggl( \frac{r_0}{R}\biggr)^4\biggr] | |||
- | |||
~\frac{4}{3}\biggl[ 1 - \frac{7}{5} \biggl(\frac{r_0}{R}\biggr)^2 + \frac{1}{10}\biggl(\frac{r_0}{R}\biggr)^4\biggr] | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> </td> | |||
<td align="center"> </td> | |||
<td align="left"> | |||
<math> | |||
+~ \biggl(\frac{4}{3} - \alpha \biggr)\biggl(\frac{r_0}{R}\biggr)^2 | |||
\biggl[1-\frac{3}{5}\biggl(\frac{r_0}{R}\biggr)^2\biggr] | |||
-~ \alpha \biggl(\frac{r_0}{R}\biggr)^4\biggl[1-\frac{3}{5}\biggl(\frac{r_0}{R}\biggr)^2\biggr] | |||
\biggr\} | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> </td> | |||
<td align="center"> </td> | |||
<td align="left"> | |||
<math> | |||
+ \frac{\rho_c}{\rho_0} \biggl( \frac{\sigma_c^2}{6\gamma_g}\biggr) \biggl\{ | |||
\biggl[\frac{d\ln P_0}{d\ln r_0}\biggr] | |||
- \frac{a}{b}\biggl[\frac{1}{\Delta} \cdot \frac{d\ln P_0}{d\ln r_0}\biggr] \biggr\} | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> </td> | |||
<td align="center"><math>=</math></td> | |||
<td align="left"> | |||
<math> | |||
\biggl(\frac{r_0}{R}\biggr)^2 | |||
\biggl[1-\frac{1}{2}\biggl(\frac{r_0}{R}\biggr)^2\biggr]^{-1} | |||
\biggl[ 1 - \biggl(\frac{r_0}{R} \biggr)^2 \biggr]^{-3} | |||
\biggl\{ \biggl[\frac{5\alpha}{3}\biggl(1 - \frac{3a}{b} \biggr) - \frac{4}{3} \biggr] | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> </td> | |||
<td align="center"> </td> | |||
<td align="left"> | |||
<math> | |||
+ \biggl(\frac{r_0}{R}\biggr)^2 | |||
\biggl[ | |||
-\frac{8\alpha}{3}\biggl(1 - \frac{3a}{b} \biggr) + \frac{28}{15} | |||
\biggr] | |||
+ \biggl( \frac{r_0}{R}\biggr)^4 \biggl[\alpha\biggl(1 - \frac{3a}{b} \biggr) | |||
- ~\frac{2}{15} \biggr] | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> </td> | |||
<td align="center"> </td> | |||
<td align="left"> | |||
<math> | |||
+~ \biggl(\frac{4}{3} - \alpha \biggr)\biggl(\frac{r_0}{R}\biggr)^2 | |||
\biggl[1-\frac{3}{5}\biggl(\frac{r_0}{R}\biggr)^2\biggr] | |||
-~ \alpha \biggl(\frac{r_0}{R}\biggr)^4\biggl[1-\frac{3}{5}\biggl(\frac{r_0}{R}\biggr)^2\biggr] | |||
\biggr\} | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> </td> | |||
<td align="center"> </td> | |||
<td align="left"> | |||
<math> | |||
+ \frac{\rho_c}{\rho_0} \biggl( \frac{\sigma_c^2}{6\gamma_g}\biggr) \biggl\{ | |||
\biggl[\frac{d\ln P_0}{d\ln r_0}\biggr] | |||
- \frac{a}{b}\biggl[\frac{1}{\Delta} \cdot \frac{d\ln P_0}{d\ln r_0}\biggr] \biggr\} | |||
</math> | |||
</td> | |||
</tr> | |||
</table> | |||
===Second Attempt=== | |||
<table border="0" cellpadding="5" align="center"> | |||
<tr> | |||
<td align="right"><math>\frac{1}{b} \biggl[ r_0^2 \times \mathrm{LAWE} \biggr]</math></td> | |||
<td align="center"><math>=</math></td> | |||
<td align="left"> | |||
<math> | |||
- r_0^2 \cdot \frac{d^2\Delta}{dr_0^2} | |||
- r_0\biggl[4 \biggr] \frac{d\Delta}{dr_0} | |||
+ \biggl[\frac{d\ln P_0}{d\ln r_0} \biggr]\biggl[ - r_0\cdot \frac{d\Delta}{dr_0} + \alpha \biggl( \frac{a}{b} - \Delta \biggr)\biggr] | |||
+ \biggl[\frac{d\ln P_0}{d\ln r_0}\biggr]\biggl( \frac{\sigma_c^2}{6\gamma_g}\biggr) | |||
\biggl\{1 - \frac{a}{b}\biggl[\frac{1}{\Delta} \biggr] \biggr\} \frac{\rho_c}{\rho_0} | |||
\, , | |||
</math> | |||
</td> | |||
</tr> | |||
</table> | |||
where, | |||
<table border="0" cellpadding="5" align="center"> | |||
<tr> | |||
<td align="right"><math>\frac{\rho_0}{\rho_c}</math></td> | |||
<td align="center"><math>=</math></td> | |||
<td align="left"> | |||
<math> | |||
\biggl(1 - x^2\biggr) \, , | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"><math>\Delta</math></td> | |||
<td align="center"><math>=</math></td> | |||
<td align="left"> | |||
<math> | |||
\frac{1}{3} \biggl(1 - \frac{3}{5} x^2\biggr)\biggl(1 - x^2\biggr)^{-1} \, , | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"><math>\frac{d\ln P_0}{d\ln r_0}</math></td> | |||
<td align="center"><math>=</math></td> | |||
<td align="left"> | |||
<math> | |||
-5x^2 \biggl(1 - \frac{3}{5} x^2\biggr)\biggl(1 - x^2\biggr)^{-1} \biggl(1 - \frac{1}{2}x^2\biggr)^{-1} | |||
= | |||
-15 x^2 \biggl(1 - \frac{1}{2}x^2\biggr)^{-1} \Delta \, , | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"><math>r_0 \cdot \frac{d\Delta}{dr_0}</math></td> | |||
<td align="center"><math>=</math></td> | |||
<td align="left"> | |||
<math> | |||
\frac{4}{15} x^2 \biggl(1 - x^2\biggr)^{-2} \, , | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"><math>r_0^2 \cdot \frac{d^2\Delta}{dr_0^2}</math></td> | |||
<td align="center"><math>=</math></td> | |||
<td align="left"> | |||
<math> | |||
\frac{4}{15} x^2 \biggl(1 - x^2\biggr)^{-3}\biggl( 1 + 3x^2\biggr) \, . | |||
</math> | |||
</td> | |||
</tr> | |||
</table> | |||
Hence, | |||
<table border="0" cellpadding="5" align="center"> | |||
<tr> | |||
<td align="right"><math>\frac{1}{b} \biggl[ r_0^2 \times \mathrm{LAWE} \biggr]</math></td> | |||
<td align="center"><math>=</math></td> | |||
<td align="left"> | |||
<math> | |||
- r_0^2 \cdot \frac{d^2\Delta}{dr_0^2} | |||
- r_0\biggl[4 \biggr] \frac{d\Delta}{dr_0} | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> </td> | |||
<td align="center"> </td> | |||
<td align="left"> | |||
<math> | |||
+ \biggl[\frac{d\ln P_0}{d\ln r_0} \biggr]\biggl[ - r_0\cdot \frac{d\Delta}{dr_0} + \alpha \biggl( \frac{a}{b} - \Delta \biggr)\biggr] | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> </td> | |||
<td align="center"> </td> | |||
<td align="left"> | |||
<math> | |||
+ \biggl[\frac{d\ln P_0}{d\ln r_0}\biggr]\biggl( \frac{\sigma_c^2}{6\gamma_g}\biggr) \biggl\{ | |||
1 | |||
- \frac{a}{b}\biggl[\frac{1}{\Delta} \biggr] \biggr\} \frac{\rho_c}{\rho_0} | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> </td> | |||
<td align="center"><math>=</math></td> | |||
<td align="left"> | |||
<math> | |||
- \frac{4}{15} x^2 \biggl(1 - x^2\biggr)^{-3}\biggl( 1 + 3x^2\biggr) | |||
- \frac{16}{15} x^2 \biggl(1 - x^2\biggr)^{-2} | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> </td> | |||
<td align="center"> </td> | |||
<td align="left"> | |||
<math> | |||
+ \biggl[\frac{d\ln P_0}{d\ln r_0} \biggr] | |||
\biggl[\frac{a\alpha}{b} - \frac{4}{15} x^2 \biggl(1 - x^2\biggr)^{-2} | |||
- \frac{\alpha}{3} \biggl(1 - \frac{3}{5} x^2\biggr)\biggl(1 - x^2\biggr)^{-1}\biggr] | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> </td> | |||
<td align="center"> </td> | |||
<td align="left"> | |||
<math> | |||
+ \biggl[\frac{d\ln P_0}{d\ln r_0}\biggr]\biggl( \frac{\sigma_c^2}{6\gamma_g}\biggr) \biggl\{ | |||
1 | |||
- \frac{3a}{b}\biggl(1 - \frac{3}{5}x^2\biggr)^{-1} \biggl(1-x^2\biggr)\biggr\} \biggl(1 - x^2\biggr)^{-1} \, . | |||
</math> | |||
</td> | |||
</tr> | |||
</table> | |||
<table border="0" cellpadding="5" align="center"> | |||
<tr> | |||
<td align="right"><math>\Rightarrow ~~~ \frac{1}{x^2}\biggl(1 - x^2\biggr) | |||
\frac{1}{b} \biggl[ r_0^2 \times \mathrm{LAWE} \biggr]</math></td> | |||
<td align="center"><math>=</math></td> | |||
<td align="left"> | |||
<math> | |||
- \frac{4}{15} \biggl(1 - x^2\biggr)^{-2}\biggl( 1 + 3x^2\biggr) | |||
- \frac{16}{15} \biggl(1 - x^2\biggr)^{-1} | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> </td> | |||
<td align="center"> </td> | |||
<td align="left"> | |||
<math> | |||
-5 \biggl(1 - \frac{3}{5} x^2\biggr) \biggl(1 - \frac{1}{2}x^2\biggr)^{-1} | |||
\biggl[\frac{a\alpha}{b} - \frac{4}{15} x^2 \biggl(1 - x^2\biggr)^{-2} | |||
- \frac{\alpha}{3} \biggl(1 - \frac{3}{5} x^2\biggr)\biggl(1 - x^2\biggr)^{-1}\biggr] | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> </td> | |||
<td align="center"> </td> | |||
<td align="left"> | |||
<math> | |||
-5 \biggl(1 - \frac{3}{5} x^2\biggr) \biggl(1 - \frac{1}{2}x^2\biggr)^{-1}\biggl( \frac{\sigma_c^2}{6\gamma_g}\biggr) \biggl\{ | |||
1 | |||
- \frac{3a}{b}\biggl(1 - \frac{3}{5}x^2\biggr)^{-1} \biggl(1-x^2\biggr)\biggr\} \biggl(1 - x^2\biggr)^{-1} | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"><math>\Rightarrow ~~~ \frac{1}{x^2}\biggl(1 - x^2\biggr)^3 | |||
\frac{1}{b} \biggl[ r_0^2 \times \mathrm{LAWE} \biggr]</math></td> | |||
<td align="center"><math>=</math></td> | |||
<td align="left"> | |||
<math> | |||
- \frac{4}{15} \biggl( 1 + 3x^2\biggr) | |||
- \frac{16}{15} \biggl(1 - x^2\biggr) | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> </td> | |||
<td align="center"> </td> | |||
<td align="left"> | |||
<math> | |||
-5 \biggl(1 - \frac{3}{5} x^2\biggr) \biggl(1 - \frac{1}{2}x^2\biggr)^{-1} | |||
\biggl[\frac{a\alpha}{b}\biggl(1 - x^2\biggr)^2 - \frac{4}{15} x^2 | |||
- \frac{\alpha}{3} \biggl(1 - \frac{3}{5} x^2\biggr)\biggl(1 - x^2\biggr)\biggr] | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> </td> | |||
<td align="center"> </td> | |||
<td align="left"> | |||
<math> | |||
-5 \biggl(1 - \frac{1}{2}x^2\biggr)^{-1}\biggl( \frac{\sigma_c^2}{6\gamma_g}\biggr) \biggl\{ | |||
\biggl(1 - \frac{3}{5} x^2\biggr) | |||
- \frac{3a}{b} \biggl(1-x^2\biggr)\biggr\} \biggl(1 - x^2\biggr) | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"><math>\Rightarrow ~~~ \frac{15}{x^2}\biggl(1 - x^2\biggr)^3 \biggl(1 - \frac{1}{2}x^2\biggr) | |||
\frac{1}{b} \biggl[ r_0^2 \times \mathrm{LAWE} \biggr]</math></td> | |||
<td align="center"><math>=</math></td> | |||
<td align="left"> | |||
<math>- 2 \biggl(2 - x^2\biggr)\biggl(5 - x^2\biggr) | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> </td> | |||
<td align="center"> </td> | |||
<td align="left"> | |||
<math> | |||
-~ \biggl(5 - 3 x^2\biggr) | |||
\biggl[\frac{15a\alpha}{b}\biggl(1 - 2x^2 + x^4\biggr) - 4 x^2 | |||
- \alpha \biggl(5 - 8 x^2 + 3x^4 \biggr)\biggr] | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> </td> | |||
<td align="center"> </td> | |||
<td align="left"> | |||
<math> | |||
-~ \biggl( \frac{5\sigma_c^2}{2\gamma_g}\biggr) \biggl\{ | |||
\biggl(5 - 3 x^2\biggr) | |||
- \frac{15a}{b} \biggl(1-x^2\biggr)\biggr\} \biggl(1 - x^2\biggr) | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"><math>\Rightarrow ~~~ -~\frac{15}{x^2}\biggl(1 - x^2\biggr)^3 \biggl(1 - \frac{1}{2}x^2\biggr) | |||
\frac{1}{b} \biggl[ r_0^2 \times \mathrm{LAWE} \biggr]</math></td> | |||
<td align="center"><math>=</math></td> | |||
<td align="left"> | |||
<math> | |||
20 - 14x^2 + 2x^4 | |||
+~ \biggl(5 - 3 x^2\biggr) | |||
\biggl[ | |||
\biggl(\frac{15a\alpha}{b}-5\alpha \biggr) + x^2\biggl( \frac{30 a\alpha}{b} -4 + 8\alpha \biggr) + \alpha x^4 \biggl(\frac{15a}{b} - 3 \biggr) | |||
\biggr] | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> </td> | |||
<td align="center"> </td> | |||
<td align="left"> | |||
<math> | |||
+~ \biggl( \frac{5\sigma_c^2}{2\gamma_g}\biggr) \biggl[ | |||
\biggl(5 - \frac{15a}{b}\biggr) + x^2 \biggl(-3 + \frac{15a}{b} \biggr) \biggr] \biggl(1 - x^2\biggr) | |||
\, . | |||
</math> | |||
</td> | |||
</tr> | |||
</table> | |||
Now, if we set <math>(15a/b) = 3</math>, this last expression reduces to, | |||
<table border="0" cellpadding="5" align="center"> | |||
<tr> | |||
<td align="right"><math>-~\frac{15}{x^2}\biggl(1 - x^2\biggr)^3 \biggl(1 - \frac{1}{2}x^2\biggr) | |||
\frac{1}{b} \biggl[ r_0^2 \times \mathrm{LAWE} \biggr]</math></td> | |||
<td align="center"><math>=</math></td> | |||
<td align="left"> | |||
<math> | |||
20 - 14x^2 + 2x^4 | |||
-~ 2\biggl(5 - 3 x^2\biggr) | |||
\biggl[ | |||
\alpha + x^2 (2 - 7\alpha ) | |||
\biggr] | |||
+~ \biggl( \frac{5\sigma_c^2}{\gamma_g}\biggr) \biggl(1 - x^2\biggr) | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> </td> | |||
<td align="center"><math>=</math></td> | |||
<td align="left"> | |||
<math> | |||
20 - 14x^2 + 2x^4 | |||
-~ 2 | |||
\biggl[ 5\alpha + x^2 (10-38\alpha ) + x^4(21\alpha - 6) \biggr] | |||
+~ \biggl( \frac{5\sigma_c^2}{\gamma_g}\biggr) \biggl(1 - x^2\biggr) | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> </td> | |||
<td align="center"><math>=</math></td> | |||
<td align="left"> | |||
<math>x^0 \biggl[20 - 10\alpha + \biggl( \frac{5\sigma_c^2}{\gamma_g}\biggr) \biggr] | |||
+ x^2\biggl[76\alpha -34 - \biggl( \frac{5\sigma_c^2}{\gamma_g}\biggr) \biggr] | |||
+ 14 x^4 \biggl[1 - 3\alpha \biggr] | |||
</math> | |||
</td> | |||
</tr> | |||
</table> | |||
=See Also= | =See Also= | ||
{{ SGFfooter }} | {{ SGFfooter }} | ||
Latest revision as of 17:55, 20 October 2021
LAWE
Most General Form
In an accompanying discussion, we derived the so-called,
where the gravitational acceleration,
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The solution to this equation gives eigenfunctions that describe various radial modes of oscillation in spherically symmetric, self-gravitating fluid configurations. The boundary condition conventionally used in connection with the adiabatic wave equation is,
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Polytropic Configurations
Part 1
If the initial, unperturbed equilibrium configuration is a polytropic sphere whose internal structure is defined by the function, , that provides a solution to the,
then,
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where,
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Hence, after multiplying through by , the above adiabatic wave equation can be rewritten in the form,
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In addition, given that,
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and,
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we can write,
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where we have adopted the function notation,
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Part 2
Drawing from an accompanying discussion, we have the following:
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In order to reconcile with the "Part 1" expression, we note first that . We note as well that since,
we have,
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All physically reasonable solutions are subject to the inner boundary condition,
at
but the relevant outer boundary condition depends on whether the underlying equilibrium configuration is isolated (surface pressure is zero), or whether it is a "pressure-truncated" configuration. As is the case with the pressure-truncated isothermal spheres, discussed above, if the polytropic configuration is truncated by the pressure, , of a hot, tenuous external medium, then the solution to the LAWE is subject to the outer boundary condition,
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But, for isolated polytropes, the sought-after solution is subject to the more conventional boundary condition,
at
Radial Pulsation Neutral Mode
Background
The integro-differential version of the statement of hydrostatic balance is
From our separate discussion, we have found that,
| Exact Solution to the Polytropic LAWE | ||
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Let's rewrite the significant functional term in this expressions in terms of basic variables. That is,
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Trial Eigenfunction & Its Derivatives
Let's adopt the following trial solution:
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Then we have,
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Given that,
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these expression can be rewritten as,
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and,
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Plug Trial Eigenfunction Into LAWE
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LAWE
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Plugging our trial radial displacement function, , into the LAWE gives,
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LAWE |
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Now, if we set and , this expression becomes,
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LAWE |
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Notice that the key components of this last term may be rewritten as,
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So, for our trial eigenfunction, we have …
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LAWE |
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Consider Polytropic Structures
Referring back to, for example, a separate review of polytropic structures, we recognize that,
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Also,
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Hence,
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LAWE |
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If, , we can further simplify and obtain,
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LAWE |
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Try Again
General Form of Wave Equation
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LAWE
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Employing the substitutions,
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we have,
| LAWE |
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In the context of polytropic configurations (see more below), we appreciate that,
Inserting these into the LAWE expression and multiplying through by the square of the polytropic length scale, , we obtain,
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Derivatives of Δ
Here we evaluate the first derivative of with respect to ,
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and the second derivative of with respect to ,
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Trial Eigenfunction
As above, let's adopt a trial eigenfunction of the form,
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Then we have,
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Assume Polytropic Relations
If we assume that the equilibrium models are polytropes, then we know that,
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We also deduce that,
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where we have introduced the shorthand notation,
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Drawing from our accompanying discussion, for example, we note as well that,
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Hence,
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Third Time
General Relations
Various general relations taken from above derivations:
| LAWE |
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where,
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Polytropes
If polytropic relations are adopted:
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Eigenfunction Choice
Again, let's try the trial eigenfunction,
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in which case,
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Hence, we are left with only the term if we set,
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We conclude, therefore, that the radial displacement function (i.e., the eigenfunction) for the neutral mode of all polytropic configurations is,
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This last expression exactly matches our earlier result found for polytropic configurations if we choose an overall amplitude coefficient of the form,
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Hooray!
Summary
Setup
We begin with the traditional,
This linear, adiabatic wave equation (LAWE) can straightforwardly be rewritten in the form we will refer to as the,
Multiplying this Δ-Highlighted LAWE through by and recognizing that, for polytropic configurations,
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we immediately obtain what we have frequently referred to as the,
Neutral-Mode Eigenfunction
In the preceding subsections of this chapter, we have demonstrated that if
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the radial displacement function (i.e., the eigenfunction) for the neutral mode of all polytropic configurations is,
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to within an arbitrarily chosen leading scaling coefficient. More completely, if we let "LAWE" stand for the RHS of our Δ-Highlighted LAWE, then setting results in the expression,
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which goes to zero if .
Parabolic Density Distribution
Here, we build upon our separate discussion of equilibrium configurations with a parabolic density distribution.
Equilibrium Structure
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. Both the mass distribution and the pressure distribution can be obtained analytically from this specified density distribution. Specifically,
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in which case we can write,
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and,
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Hence, proceeding via what we have labeled as "Technique 1", and enforcing the surface boundary condition, , Prasad (1949) determines that,
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where, it can readily be deduced, as well, that the central pressure is,
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Specific Entropy Distribution
Notice that, independent of the value of , the specific entropy varies with throughout the structure. According to the Schwarzschild criterion, spherically symmetric equilibrium configurations will be stable against convection if the specific entropy increases outward, and unstable toward convection if the specific entropy decreases outward. Let's examine the slope, , throughout configurations that have a parabolic density distribution.
The slope is zero when,
Moving from the center of the configuration to its surface, , the slope will go to zero — hence, the slope of the entropy will change sign |
Some Relevant Structural Derivatives
We note for later use that,
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Checking for detailed force-balance, we note that,
which is exactly the expression that we have just derived for . |
Hence,
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and, given that,
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we can write,
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Also,
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and,
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Neutral Mode
Again, adopting the trial eigenfunction,
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from the,
we can write,
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First Attempt
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Continuing …
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Second Attempt
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where,
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Hence,
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Now, if we set , this last expression reduces to,
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See Also
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Appendices: | VisTrailsEquations | VisTrailsVariables | References | Ramblings | VisTrailsImages | myphys.lsu | ADS | |
