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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=

Revision as of 00:41, 16 January 2024

Bipolytrope Generalization (Pt 3)


Part I:  Bipolytrope Generalization

 


Part II:  Derivations

 


Part III:  Examples

 


Part IV:  Best of the Best

 

Examples

(0, 0) Bipolytropes

Review

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[(1−q3)+52Λ(ρeρ0)(−2+3q−q3)+32q2Λ(ρeρ0)2(−1+5q2−5q3+q5)],

where,

Λ

≡

322⋅5π(GMtot2Req4Pi)ν2q4,

f(q,ρe/ρc)

≡

1+52(ρeρc)(1q2−1)+(ρeρc)2[(1q5−1)−52(1q2−1)]

 

=

1+52q2(ρeρc)(1−q2)+12q5(ρeρc)2(2−5q3+3q5),

g2(q,ρe/ρc)

≡

1+(ρeρ0)[2(1−ρeρ0)(1−q)+ρeρ0(1q2−1)]

 

≡

1+[2(ρeρc)(1−q)+1q2(ρeρc)2(1−3q2+2q3)],

Renormalize

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]3−3γc[(34π)ρicρ¯]γcKcMtotγcRnorm3−3γc

 

=

[RRnorm]3−3γc[(34π)ρicρ¯]γc{Kc3γc−4Mtotγc(3γc−4)[(KcG)Mtotγc−2]3−3γc}1/(3γc−4)

 

=

[RRnorm]3−3γc[(34π)ρicρ¯]γc{G3γc−3Mtot5γc−6Kc}1/(3γc−4)

 

=

[RRnorm]3−3γc[(34π)ρicρ¯]γcEnorm.

Also,

[GMtot2R]3γc−4

=

(RRnorm)−(3γc−4)G3γc−4Mtot6γc−8(GKc)Mtot2−γc

 

=

(RRnorm)−(3γc−4)[G3γc−3Mtot5γc−6Kc]

 

=

(RRnorm)−(3γc−4)Enorm3γc−4.

⇒GMtot2R4Pi

=

(RRnorm)−1[RRnorm]3γc−3[(34π)ρicρ¯]−γc

 

=

(RRnorm)3γc−4[(34π)ρicρ¯]−γc.

Hence,

Λ

≡

322⋅5πν2q4[(34π)ρicρ¯]−γc(RRnorm)3γc−4.

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

R3PiEnorm

=

[(34π)νq3]γc(RRnorm)3−3γc,

and,

Λ

≡

322⋅5πν2q4[(34π)νq3]−γc(RRnorm)3γc−4=15νq[(34π)νq3]1−γc(RRnorm)3γc−4.

Hence the renormalized gravitational potential energy becomes,

WgravEnorm

=

−(35)ν2q(RRnorm)−1⋅f;

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

UcoreEnorm=23(γc−1)[ScoreEnorm]

=

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

UenvEnorm=23(γe−1)[SenvEnorm]

=

4π3(γe−1)[(34π)(1−ν)(1−q3)]γe(KeKc)[Kc3G3Mtot2](3γc−3γe)/(3γc−4)(RRnorm)3−3γe

 

 

×[(1−q3)+52Λ(ρeρ0)(−2+3q−q3)+32q2Λ(ρeρ0)2(−1+5q2−5q3+q5)],

Finally, then, we can state that,

𝔣WM

≡

ν2q⋅f,

score

≡

1+Λ,

(1−q3)senv

≡

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

Virial Equilibrium and Stability Evaluation

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)+(1−q3)+52Λ(ρeρ0)(−2+3q−q3)+32q2Λ(ρeρ0)2(−1+5q2−5q3+q5)

=

q3Λ[1+52q2(ρeρc)(1−q2)+12q5(ρeρc)2(2−5q3+3q5)]

⇒1Λ

=

52(ρeρc)(q−q3)+12q2(ρeρc)2(2−5q3+3q5)−[52(ρeρ0)(−2+3q−q3)+32q2(ρeρ0)2(−1+5q2−5q3+q5)]

 

=

52(ρeρc)(q−q3+2−3q+q3)+12q2(ρeρc)2(2−5q3+3q5+3−15q2+15q3−3q5)

 

=

52[2(ρeρc)(1−q)+1q2(ρeρc)2(1−3q2+2q3)]

 

=

52(g2−1)

⇒[PiGMtot2]Req4

=

(323π)ν2q4(g2−1).

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

(RRnorm)4−3γc[(34π)ρicρ¯]γc

=

(323π)ν2q4(g2−1)

⇒RRnorm

=

{(323π)ν2q4(g2−1)[(34π)ρicρ¯]γc}1/(4−3γc).


And the condition for dynamical stability is,

−W2(γe−43)−(γe−γc)Score

  > 

0.

⇒2πq3Λ[(γe−43)f−(γe−γc)(1+1Λ)]

  > 

0.

(γe−43)f−(γe−γc)[1+52(g2−1)]

  > 

0.

(5, 1) Bipolytropes

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!

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