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Created page with "=Bipolytrope Generalization (Pt 3)= <table border="1" align="center" width="100%" colspan="8"> <tr> <td align="center" bgcolor="lightblue" width="25%"><br />Part I:  Bipolytrope Generalization   </td> <td align="center" bgcolor="lightblue" width="25%"><br />Part II:  Derivations   </td> <td align="center" bgcolor="lightblue" width="25%"><br />SSC/BipolytropeGeneralizat..."
 
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</tr>
</tr>
</table>
</table>
==Examples==
===(0, 0) Bipolytropes===
====Review====
In an [[SSC/Structure/BiPolytropes/Analytic00#BiPolytrope_with_nc_.3D_0_and_ne_.3D_0|accompanying discussion]] we have derived analytic expressions describing the equilibrium structure and the stability of bipolytropes in which both the core and the envelope have uniform densities, that is, bipolytropes with <math>~(n_c, n_e) = (0, 0)</math>.  From this work, we find that integrals over the mass and pressure distributions give:
<div align="center">
<table border="0">
<tr>
  <td align="right">
<math>~ \frac{W}{R_\mathrm{eq}^3 P_i} = - \frac{A}{R_\mathrm{eq}^4 P_i} </math>
  </td>
  <td align="center">
<math>~=~</math>
  </td>
  <td align="left">
&nbsp;<math>- ~ \frac{3}{5} \biggl[ \frac{GM_\mathrm{tot}^2}{R^4P_i} \biggr] \biggl( \frac{\nu^2}{q} \biggr) f </math>
  </td>
</tr>
<tr>
  <td align="right">
&nbsp;
  </td>
  <td align="center">
<math>~=~</math>
  </td>
  <td align="left">
&nbsp;<math>- ~4\pi q^3 \Lambda f \, ,</math>
  </td>
</tr>
<tr>
  <td align="right">
<math>~\frac{S_\mathrm{core}}{R_\mathrm{eq}^3 P_i} = B_\mathrm{core}</math>
  </td>
  <td align="center">
<math>~=~</math>
  </td>
  <td align="left">
<math>
~2\pi q^3 (1 + \Lambda) \, ,</math>
  </td>
</tr>
<tr>
  <td align="right">
<math>~\frac{S_\mathrm{env}}{R_\mathrm{eq}^3 P_i} = B_\mathrm{env}</math>
  </td>
  <td align="center">
<math>~=~</math>
  </td>
  <td align="left">
<math>
2\pi \biggl[ (1-q^3) + \frac{5}{2} \Lambda \biggl( \frac{\rho_e}{\rho_0}\biggr) (-2 + 3q - q^3) +
\frac{3}{2q^2} \Lambda \biggl( \frac{\rho_e}{\rho_0}\biggr)^2 (-1 +5q^2 - 5q^3 + q^5) \biggr] \, ,</math>
  </td>
</tr>
</table>
</div>
where,
<div align="center">
<table border="0">
<tr>
  <td align="right">
<math>~\Lambda</math>
  </td>
  <td align="center">
<math>~\equiv~</math>
  </td>
  <td align="left">
<math>
\frac{3}{2^2 \cdot 5\pi} \biggl( \frac{GM_\mathrm{tot}^2}{R_\mathrm{eq}^4 P_i} \biggr) \frac{\nu^2}{q^4} \, ,</math>
  </td>
</tr>
<tr>
  <td align="right">
<math>~f(q,\rho_e/\rho_c)</math>
  </td>
  <td align="center">
<math>~\equiv~</math>
  </td>
  <td align="left">
<math>1 + \frac{5}{2} \biggl( \frac{\rho_e}{\rho_c} \biggr) \biggl(\frac{1}{q^2} - 1 \biggr)
+ \biggl( \frac{\rho_e}{\rho_c} \biggr)^2 \biggl[ \biggl(\frac{1}{q^5} - 1 \biggr) - \frac{5}{2}\biggl(\frac{1}{q^2} - 1 \biggr) \biggr] </math>
  </td>
</tr>
<tr>
  <td align="right">
&nbsp;
  </td>
  <td align="center">
<math>~=~</math>
  </td>
  <td align="left">
<math>1 + \frac{5}{2q^2} \biggl( \frac{\rho_e}{\rho_c} \biggr) (1-q^2)
+ \frac{1}{2q^5} \biggl( \frac{\rho_e}{\rho_c} \biggr)^2 (2 - 5q^3 + 3q^5) \, ,</math>
  </td>
</tr>
<tr>
  <td align="right">
<math>~g^2(q,\rho_e/\rho_c)</math>
  </td>
  <td align="center">
<math>~\equiv~</math>
  </td>
  <td align="left">
<math>1  +
\biggl(\frac{\rho_e}{\rho_0}\biggr)  \biggl[ 2 \biggl(1 - \frac{\rho_e}{\rho_0} \biggr) \biggl( 1-q \biggr) +
\frac{\rho_e}{\rho_0} \biggl(\frac{1}{q^2} - 1\biggr) \biggr] </math>
  </td>
</tr>
<tr>
  <td align="right">
&nbsp;
  </td>
  <td align="center">
<math>~\equiv~</math>
  </td>
  <td align="left">
<math>1 + \biggl[ 2\biggl( \frac{\rho_e}{\rho_c} \biggr) (1-q)
+ \frac{1}{q^2} \biggl( \frac{\rho_e}{\rho_c} \biggr)^2 (1 - 3q^2 + 2q^3 )  \biggr] \, ,
</math>
  </td>
</tr>
</table>
</div>
====Renormalize====
Let's renormalize these energy terms in order to more readily relate them to the [[#Setup|generalized expressions derived above]].
<div align="center">
<table border="0" cellpadding="5" align="center">
<tr>
  <td align="right">
<math>~R^3 P_i</math>
  </td>
  <td align="center">
<math>~=</math>
  </td>
  <td align="left">
<math>
~R^3 K_c \biggl(\frac{\rho_{ic}}{\bar\rho} \biggr)^{\gamma_c} \biggl[ \biggl( \frac{3}{4\pi}\biggr) \frac{M_\mathrm{tot}}{R^3} \biggr]^{\gamma_c}
</math>
  </td>
</tr>
<tr>
  <td align="right">
&nbsp;
  </td>
  <td align="center">
<math>~=</math>
  </td>
  <td align="left">
<math>~\biggl[ \frac{R}{R_\mathrm{norm}} \biggr]^{3-3\gamma_c} \biggl[ \biggl( \frac{3}{4\pi} \biggr) \frac{\rho_{ic}}{\bar\rho} \biggr]^{\gamma_c}
K_c M_\mathrm{tot}^{\gamma_c} R_\mathrm{norm}^{3-3\gamma_c}</math>
  </td>
</tr>
<tr>
  <td align="right">
&nbsp;
  </td>
  <td align="center">
<math>~=</math>
  </td>
  <td align="left">
<math>~\biggl[ \frac{R}{R_\mathrm{norm}} \biggr]^{3-3\gamma_c} \biggl[ \biggl( \frac{3}{4\pi} \biggr) \frac{\rho_{ic}}{\bar\rho} \biggr]^{\gamma_c}
\biggl\{ K_c^{3\gamma_c -4} M_\mathrm{tot}^{\gamma_c(3\gamma_c -4)} \biggl[ \biggl( \frac{K_c}{G} \biggr) M_\mathrm{tot}^{\gamma_c-2} \biggr]^{3-3\gamma_c} \biggr\}^{1/(3\gamma_c -4)}</math>
  </td>
</tr>
<tr>
  <td align="right">
&nbsp;
  </td>
  <td align="center">
<math>~=</math>
  </td>
  <td align="left">
<math>~\biggl[ \frac{R}{R_\mathrm{norm}} \biggr]^{3-3\gamma_c} \biggl[ \biggl( \frac{3}{4\pi} \biggr) \frac{\rho_{ic}}{\bar\rho} \biggr]^{\gamma_c}
\biggl\{ \frac{G^{3\gamma_c-3} M_\mathrm{tot}^{5\gamma_c-6} }{K_c} \biggr\}^{1/(3\gamma_c -4)}</math>
  </td>
</tr>
<tr>
  <td align="right">
&nbsp;
  </td>
  <td align="center">
<math>~=</math>
  </td>
  <td align="left">
<math>~\biggl[ \frac{R}{R_\mathrm{norm}} \biggr]^{3-3\gamma_c} \biggl[ \biggl( \frac{3}{4\pi} \biggr) \frac{\rho_{ic}}{\bar\rho} \biggr]^{\gamma_c}
E_\mathrm{norm} \, .</math>
  </td>
</tr>
</table>
</div>
Also,
<div align="center">
<table border="0" cellpadding="5" align="center">
<tr>
  <td align="right">
<math>~\biggl[ \frac{GM_\mathrm{tot}^2}{R} \biggr]^{3\gamma_c -4}</math>
  </td>
  <td align="center">
<math>~=</math>
  </td>
  <td align="left">
<math>
~\biggl( \frac{R}{R_\mathrm{norm}} \biggr)^{-(3\gamma_c-4)} G^{3\gamma_c -4} M_\mathrm{tot}^{6\gamma_c -8}
\biggl( \frac{G}{K_c} \biggr) M_\mathrm{tot}^{2-\gamma_c}
</math>
  </td>
</tr>
<tr>
  <td align="right">
&nbsp;
  </td>
  <td align="center">
<math>~=</math>
  </td>
  <td align="left">
<math>
~\biggl( \frac{R}{R_\mathrm{norm}} \biggr)^{-(3\gamma_c-4)} \biggl[ \frac{ G^{3\gamma_c -3} M_\mathrm{tot}^{5\gamma_c -6} }{K_c} \biggr]
</math>
  </td>
</tr>
<tr>
  <td align="right">
&nbsp;
  </td>
  <td align="center">
<math>~=</math>
  </td>
  <td align="left">
<math>
~\biggl( \frac{R}{R_\mathrm{norm}} \biggr)^{-(3\gamma_c-4)} E_\mathrm{norm}^{3\gamma_c-4} \, .
</math>
  </td>
</tr>
<tr>
  <td align="right">
<math>
\Rightarrow ~~~~\frac{GM_\mathrm{tot}^2}{R^4 P_i} </math>
  </td>
  <td align="center">
<math>~=</math>
  </td>
  <td align="left">
<math>
~\biggl( \frac{R}{R_\mathrm{norm}} \biggr)^{-1}
\biggl[ \frac{R}{R_\mathrm{norm}} \biggr]^{3\gamma_c - 3} \biggl[ \biggl( \frac{3}{4\pi} \biggr) \frac{\rho_{ic}}{\bar\rho} \biggr]^{-\gamma_c}
</math>
  </td>
</tr>
<tr>
  <td align="right">
&nbsp;
  </td>
  <td align="center">
<math>~=</math>
  </td>
  <td align="left">
<math>
\biggl( \frac{R}{R_\mathrm{norm}} \biggr)^{3\gamma_c - 4} \biggl[ \biggl( \frac{3}{4\pi} \biggr) \frac{\rho_{ic}}{\bar\rho} \biggr]^{-\gamma_c} \, .
</math>
  </td>
</tr>
</table>
</div>
Hence,
<div align="center">
<table border="0" cellpadding="5" align="center">
<tr>
  <td align="right">
<math>~\Lambda</math>
  </td>
  <td align="center">
<math>~\equiv~</math>
  </td>
  <td align="left">
<math>
\frac{3}{2^2 \cdot 5\pi} \frac{\nu^2}{q^4} \biggl[ \biggl( \frac{3}{4\pi} \biggr) \frac{\rho_{ic}}{\bar\rho} \biggr]^{-\gamma_c}
\biggl( \frac{R}{R_\mathrm{norm}} \biggr)^{3\gamma_c - 4}
\, .</math>
  </td>
</tr>
</table>
</div>
Given that <math>~\rho_{ic}/\bar\rho = \nu/q^3</math> for the <math>~(n_c, n_e) = (0, 0)</math> bipolytrope,  we can finally write,
<div align="center">
<table border="0" cellpadding="5" align="center">
<tr>
  <td align="right">
<math>~\frac{R^3 P_i}{E_\mathrm{norm}}</math>
  </td>
  <td align="center">
<math>~=</math>
  </td>
  <td align="left">
<math>~\biggl[ \biggl( \frac{3}{4\pi} \biggr) \frac{\nu}{q^3} \biggr]^{\gamma_c} \biggl( \frac{R}{R_\mathrm{norm}} \biggr)^{3-3\gamma_c}
\, ,</math>
  </td>
</tr>
</table>
</div>
and,
<div align="center">
<table border="0" cellpadding="5" align="center">
<tr>
  <td align="right">
<math>~\Lambda</math>
  </td>
  <td align="center">
<math>~\equiv~</math>
  </td>
  <td align="left">
<math>
\frac{3}{2^2 \cdot 5\pi} \frac{\nu^2}{q^4} \biggl[ \biggl( \frac{3}{4\pi} \biggr) \frac{\nu}{q^3} \biggr]^{-\gamma_c}
\biggl( \frac{R}{R_\mathrm{norm}} \biggr)^{3\gamma_c - 4} =
\frac{1}{5} \frac{\nu}{q} \biggl[ \biggl( \frac{3}{4\pi} \biggr) \frac{\nu}{q^3} \biggr]^{1-\gamma_c}
\biggl( \frac{R}{R_\mathrm{norm}} \biggr)^{3\gamma_c - 4}
\, .</math>
  </td>
</tr>
</table>
</div>
Hence the renormalized gravitational potential energy becomes,
<div align="center">
<table border="0" cellpadding="5" align="center">
<tr>
  <td align="right">
<math>
\frac{W_\mathrm{grav}}{E_\mathrm{norm}}
</math>
  </td>
  <td align="center">
<math>~=</math>
  </td>
  <td align="left">
<math>
- \biggl( \frac{3}{5} \biggr) \frac{\nu^2}{q} \biggl( \frac{R}{R_\mathrm{norm}} \biggr)^{-1} \cdot f
\, ;</math>
  </td>
</tr>
</table>
</div>
and the two, renormalized contributions to the thermal energy become,
<div align="center">
<table border="0" cellpadding="5" align="center">
<tr>
  <td align="right">
<math>~\frac{U_\mathrm{core}}{ E_\mathrm{norm} } = \frac{2}{3(\gamma_c-1)} \biggl[ \frac{S_\mathrm{core}}{ E_\mathrm{norm} } \biggr]</math>
  </td>
  <td align="center">
<math>~=~</math>
  </td>
  <td align="left">
<math>
\frac{4\pi q^3 (1 + \Lambda) }{3(\gamma_c-1)}
\biggl[ \biggl( \frac{3}{4\pi} \biggr) \frac{\nu}{q^3} \biggr]^{\gamma_c} \biggl( \frac{R}{R_\mathrm{norm}} \biggr)^{3-3\gamma_c}
\, ,</math>
  </td>
</tr>
<tr>
  <td align="right">
<math>~\frac{U_\mathrm{env}}{ E_\mathrm{norm} } = \frac{2}{3(\gamma_e-1)} \biggl[ \frac{S_\mathrm{env}}{ E_\mathrm{norm} } \biggr]</math>
  </td>
  <td align="center">
<math>~=~</math>
  </td>
  <td align="left">
<math>
\frac{4\pi}{3(\gamma_e-1)} \biggl[ \biggl( \frac{3}{4\pi} \biggr) \frac{(1-\nu)}{(1-q^3)} \biggr]^{\gamma_e} \biggl( \frac{K_e}{K_c} \biggr)
\biggl[ \frac{K_c^3}{G^3 M_\mathrm{tot}^2} \biggr]^{(3\gamma_c-3\gamma_e)/(3\gamma_c-4)}
\biggl( \frac{R}{R_\mathrm{norm}} \biggr)^{3-3\gamma_e}
</math>
  </td>
</tr>
<tr>
  <td align="right">
&nbsp;
  </td>
  <td align="center">
&nbsp;
  </td>
  <td align="left">
<math>
\times \biggl[ (1-q^3) + \frac{5}{2} \Lambda \biggl( \frac{\rho_e}{\rho_0}\biggr) (-2 + 3q - q^3) +
\frac{3}{2q^2} \Lambda \biggl( \frac{\rho_e}{\rho_0}\biggr)^2 (-1 +5q^2 - 5q^3 + q^5) \biggr]
\, ,</math>
  </td>
</tr>
</table>
</div>
Finally, then, we can state that,
<div align="center">
<table border="0" cellpadding="5" align="center">
<tr>
  <td align="right">
<math>~\mathfrak{f}_{WM}</math>
  </td>
  <td align="center">
<math>~\equiv</math>
  </td>
  <td align="left">
<math>~\frac{\nu^2}{q} \cdot f \, ,</math>
  </td>
</tr>
<tr>
  <td align="right">
<math>~s_\mathrm{core}</math>
  </td>
  <td align="center">
<math>~\equiv</math>
  </td>
  <td align="left">
<math>
1 + \Lambda \, ,
</math>
  </td>
</tr>
<tr>
  <td align="right">
<math>~(1-q^3) s_\mathrm{env}</math>
  </td>
  <td align="center">
<math>~\equiv</math>
  </td>
  <td align="left">
<math>
(1-q^3) + \Lambda\biggl[ \frac{5}{2} \biggl( \frac{\rho_e}{\rho_0}\biggr) (-2 + 3q - q^3) +
\frac{3}{2q^2} \biggl( \frac{\rho_e}{\rho_0}\biggr)^2 (-1 +5q^2 - 5q^3 + q^5) \biggr]
\, .</math>
  </td>
</tr>
</table>
</div>
====Virial Equilibrium and Stability Evaluation====
With these expressions in hand, we can deduce the equilibrium radius and relativity stability of <math>~(n_c, n_e) = (0, 0)</math> bipolytropes using the generalized expressions provided above.  For example, from the statement of virial equilibrium <math>~(2S_\mathrm{tot} = - W )</math> we obtain,
<div align="center">
<table border="0">
<tr>
  <td align="right">
<math>~q^3 (1 + \Lambda) + (1-q^3) + \frac{5}{2} \Lambda \biggl( \frac{\rho_e}{\rho_0}\biggr) (-2 + 3q - q^3) +
\frac{3}{2q^2} \Lambda \biggl( \frac{\rho_e}{\rho_0}\biggr)^2 (-1 +5q^2 - 5q^3 + q^5)  </math>
  </td>
  <td align="center">
<math>~=~</math>
  </td>
  <td align="left">
<math>~q^3 \Lambda \biggl[ 1 + \frac{5}{2q^2} \biggl( \frac{\rho_e}{\rho_c} \biggr) (1-q^2)
+ \frac{1}{2q^5} \biggl( \frac{\rho_e}{\rho_c} \biggr)^2 (2 - 5q^3 + 3q^5) \biggr] </math>
  </td>
</tr>
</table>
</div>
<div align="center">
<table border="0">
<tr>
  <td align="right">
<math>\Rightarrow ~~~~ \frac{1}{\Lambda}</math>
  </td>
  <td align="center">
<math>~=~</math>
  </td>
  <td align="left">
<math>\frac{5}{2} \biggl( \frac{\rho_e}{\rho_c} \biggr) (q-q^3)
+ \frac{1}{2q^2} \biggl( \frac{\rho_e}{\rho_c} \biggr)^2 (2 - 5q^3 + 3q^5)
- \biggl[ \frac{5}{2} \biggl( \frac{\rho_e}{\rho_0}\biggr) (-2 + 3q - q^3) +
\frac{3}{2q^2} \biggl( \frac{\rho_e}{\rho_0}\biggr)^2 (-1 +5q^2 - 5q^3 + q^5) \biggr]
</math>
  </td>
</tr>
<tr>
  <td align="right">
&nbsp;
  </td>
  <td align="center">
<math>~=~</math>
  </td>
  <td align="left">
<math>\frac{5}{2} \biggl( \frac{\rho_e}{\rho_c} \biggr) (q-q^3 + 2 -3q +q^3)
+ \frac{1}{2q^2} \biggl( \frac{\rho_e}{\rho_c} \biggr)^2 (2 - 5q^3 + 3q^5 +3 - 15q^2+15q^3 -3q^5) 
</math>
  </td>
</tr>
<tr>
  <td align="right">
&nbsp;
  </td>
  <td align="center">
<math>~=~</math>
  </td>
  <td align="left">
<math>\frac{5}{2}\biggl[ 2\biggl( \frac{\rho_e}{\rho_c} \biggr) (1-q)
+ \frac{1}{q^2} \biggl( \frac{\rho_e}{\rho_c} \biggr)^2 (1 - 3q^2 + 2q^3 )  \biggr]
</math>
  </td>
</tr>
<tr>
  <td align="right">
&nbsp;
  </td>
  <td align="center">
<math>~=~</math>
  </td>
  <td align="left">
<math>\frac{5}{2}(g^2-1)
</math>
  </td>
</tr>
<tr>
  <td align="right">
<math>\Rightarrow ~~~~ \biggl[ \frac{P_i}{GM_\mathrm{tot}^2} \biggr] R_\mathrm{eq}^4</math>
  </td>
  <td align="center">
<math>~=~</math>
  </td>
  <td align="left">
<math>\biggl( \frac{3}{2^3 \pi } \biggr) \frac{\nu^2}{q^4} (g^2-1) \, .
</math>
  </td>
</tr>
</table>
</div>
Or, given the above renormalization, this expression can be written as,
<div align="center">
<table border="0" cellpadding="5" align="center">
<tr>
  <td align="right">
<math>
\biggl( \frac{R}{R_\mathrm{norm}} \biggr)^{4-3\gamma_c } \biggl[ \biggl( \frac{3}{4\pi} \biggr) \frac{\rho_{ic}}{\bar\rho} \biggr]^{\gamma_c}
</math>
  </td>
  <td align="center">
<math>~=~</math>
  </td>
  <td align="left">
<math>\biggl( \frac{3}{2^3 \pi } \biggr) \frac{\nu^2}{q^4} (g^2-1)
</math>
  </td>
</tr>
<tr>
  <td align="right">
<math>
\Rightarrow ~~~~ \frac{R}{R_\mathrm{norm}}
</math>
  </td>
  <td align="center">
<math>~=~</math>
  </td>
  <td align="left">
<math>
\biggl\{ \biggl( \frac{3}{2^3 \pi } \biggr) \frac{\nu^2}{q^4} (g^2-1)
\biggl[ \biggl( \frac{3}{4\pi} \biggr) \frac{\rho_{ic}}{\bar\rho} \biggr]^{\gamma_c} \biggr\}^{1/(4-3\gamma_c)} \, .
</math>
  </td>
</tr>
</table>
</div>
And the condition for dynamical stability is,
<div align="center">
<table border="0">
<tr>
  <td align="right">
<math>-\frac{W}{2}\biggl( \gamma_e - \frac{4}{3}\biggr) -
(\gamma_e-\gamma_c) S_\mathrm{core} </math>
  </td>
  <td align="center">
&nbsp; <math>~>~</math>&nbsp;
  </td>
  <td align="left">
<math>~0 \, .</math>
  </td>
</tr>
<tr>
  <td align="right">
<math>\Rightarrow ~~~~ 2\pi q^3 \Lambda \biggl[ \biggl( \gamma_e - \frac{4}{3}\biggr) f -
(\gamma_e-\gamma_c) \biggl( 1 + \frac{1}{\Lambda}\biggr) \biggr] </math>
  </td>
  <td align="center">
&nbsp; <math>~>~</math>&nbsp;
  </td>
  <td align="left">
<math>~0 \, .</math>
  </td>
</tr>
<tr>
  <td align="right">
<math>~\biggl( \gamma_e - \frac{4}{3} \biggr)f - (\gamma_e - \gamma_c) \biggl[1 + \frac{5}{2}(g^2-1) \biggr]</math>
  </td>
  <td align="center">
&nbsp; <math>~>~</math>&nbsp;
  </td>
  <td align="left">
<math>~0 \, .</math>
  </td>
</tr>
</table>
</div>
===(5, 1) Bipolytropes===
In another [[SSC/Structure/BiPolytropes/Analytic51#BiPolytrope_with_nc_.3D_5_and_ne_.3D_1|accompanying discussion]] we have derived analytic expressions describing the equilibrium structure of bipolytropes with <math>(n_c, n_e) = (5, 1)</math>.  Can we perform a similar stability analysis of these configurations?
Work in progress!


=Related Discussions=
=Related Discussions=

Latest revision as of 00:49, 16 January 2024

Bipolytrope Generalization (Pt 3)[edit]


Part I:  Bipolytrope Generalization

 


Part II:  Derivations

 


Part III:  Examples

 


Part IV:  Best of the Best

 

Examples[edit]

(0, 0) Bipolytropes[edit]

Review[edit]

In an accompanying discussion we have derived analytic expressions describing the equilibrium structure and the stability of bipolytropes in which both the core and the envelope have uniform densities, that is, bipolytropes with (nc,ne)=(0,0). From this work, we find that integrals over the mass and pressure distributions give:

WReq3Pi=AReq4Pi

=

 35[GMtot2R4Pi](ν2q)f

 

=

 4πq3Λf,

ScoreReq3Pi=Bcore

=

2πq3(1+Λ),

SenvReq3Pi=Benv

=

2π[(1q3)+52Λ(ρeρ0)(2+3qq3)+32q2Λ(ρeρ0)2(1+5q25q3+q5)],

where,

Λ

3225π(GMtot2Req4Pi)ν2q4,

f(q,ρe/ρc)

1+52(ρeρc)(1q21)+(ρeρc)2[(1q51)52(1q21)]

 

=

1+52q2(ρeρc)(1q2)+12q5(ρeρc)2(25q3+3q5),

g2(q,ρe/ρc)

1+(ρeρ0)[2(1ρeρ0)(1q)+ρeρ0(1q21)]

 

1+[2(ρeρc)(1q)+1q2(ρeρc)2(13q2+2q3)],

Renormalize[edit]

Let's renormalize these energy terms in order to more readily relate them to the generalized expressions derived above.

R3Pi

=

R3Kc(ρicρ¯)γc[(34π)MtotR3]γc

 

=

[RRnorm]33γc[(34π)ρicρ¯]γcKcMtotγcRnorm33γc

 

=

[RRnorm]33γc[(34π)ρicρ¯]γc{Kc3γc4Mtotγc(3γc4)[(KcG)Mtotγc2]33γc}1/(3γc4)

 

=

[RRnorm]33γc[(34π)ρicρ¯]γc{G3γc3Mtot5γc6Kc}1/(3γc4)

 

=

[RRnorm]33γc[(34π)ρicρ¯]γcEnorm.

Also,

[GMtot2R]3γc4

=

(RRnorm)(3γc4)G3γc4Mtot6γc8(GKc)Mtot2γc

 

=

(RRnorm)(3γc4)[G3γc3Mtot5γc6Kc]

 

=

(RRnorm)(3γc4)Enorm3γc4.

GMtot2R4Pi

=

(RRnorm)1[RRnorm]3γc3[(34π)ρicρ¯]γc

 

=

(RRnorm)3γc4[(34π)ρicρ¯]γc.

Hence,

Λ

3225πν2q4[(34π)ρicρ¯]γc(RRnorm)3γc4.

Given that ρic/ρ¯=ν/q3 for the (nc,ne)=(0,0) bipolytrope, we can finally write,

R3PiEnorm

=

[(34π)νq3]γc(RRnorm)33γc,

and,

Λ

3225πν2q4[(34π)νq3]γc(RRnorm)3γc4=15νq[(34π)νq3]1γc(RRnorm)3γc4.

Hence the renormalized gravitational potential energy becomes,

WgravEnorm

=

(35)ν2q(RRnorm)1f;

and the two, renormalized contributions to the thermal energy become,

UcoreEnorm=23(γc1)[ScoreEnorm]

=

4πq3(1+Λ)3(γc1)[(34π)νq3]γc(RRnorm)33γc,

UenvEnorm=23(γe1)[SenvEnorm]

=

4π3(γe1)[(34π)(1ν)(1q3)]γe(KeKc)[Kc3G3Mtot2](3γc3γe)/(3γc4)(RRnorm)33γe

 

 

×[(1q3)+52Λ(ρeρ0)(2+3qq3)+32q2Λ(ρeρ0)2(1+5q25q3+q5)],

Finally, then, we can state that,

𝔣WM

ν2qf,

score

1+Λ,

(1q3)senv

(1q3)+Λ[52(ρeρ0)(2+3qq3)+32q2(ρeρ0)2(1+5q25q3+q5)].

Virial Equilibrium and Stability Evaluation[edit]

With these expressions in hand, we can deduce the equilibrium radius and relativity stability of (nc,ne)=(0,0) bipolytropes using the generalized expressions provided above. For example, from the statement of virial equilibrium (2Stot=W) we obtain,

q3(1+Λ)+(1q3)+52Λ(ρeρ0)(2+3qq3)+32q2Λ(ρeρ0)2(1+5q25q3+q5)

=

q3Λ[1+52q2(ρeρc)(1q2)+12q5(ρeρc)2(25q3+3q5)]

1Λ

=

52(ρeρc)(qq3)+12q2(ρeρc)2(25q3+3q5)[52(ρeρ0)(2+3qq3)+32q2(ρeρ0)2(1+5q25q3+q5)]

 

=

52(ρeρc)(qq3+23q+q3)+12q2(ρeρc)2(25q3+3q5+315q2+15q33q5)

 

=

52[2(ρeρc)(1q)+1q2(ρeρc)2(13q2+2q3)]

 

=

52(g21)

[PiGMtot2]Req4

=

(323π)ν2q4(g21).

Or, given the above renormalization, this expression can be written as,

(RRnorm)43γc[(34π)ρicρ¯]γc

=

(323π)ν2q4(g21)

RRnorm

=

{(323π)ν2q4(g21)[(34π)ρicρ¯]γc}1/(43γc).


And the condition for dynamical stability is,

W2(γe43)(γeγc)Score

  > 

0.

2πq3Λ[(γe43)f(γeγc)(1+1Λ)]

  > 

0.

(γe43)f(γeγc)[1+52(g21)]

  > 

0.

(5, 1) Bipolytropes[edit]

In another accompanying discussion we have derived analytic expressions describing the equilibrium structure of bipolytropes with (nc,ne)=(5,1). Can we perform a similar stability analysis of these configurations? Work in progress!

Related Discussions[edit]

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