SSC/BipolytropeGeneralization/Pt3: Difference between revisions
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=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"> | |||
<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"> | |||
| |||
</td> | |||
<td align="center"> | |||
<math>~=~</math> | |||
</td> | |||
<td align="left"> | |||
<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"> | |||
| |||
</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"> | |||
| |||
</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"> | |||
| |||
</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"> | |||
| |||
</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"> | |||
| |||
</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"> | |||
| |||
</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"> | |||
| |||
</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"> | |||
| |||
</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"> | |||
| |||
</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"> | |||
| |||
</td> | |||
<td align="center"> | |||
| |||
</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"> | |||
| |||
</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"> | |||
| |||
</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"> | |||
| |||
</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"> | |||
<math>~>~</math> | |||
</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"> | |||
<math>~>~</math> | |||
</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"> | |||
<math>~>~</math> | |||
</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
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Part II: Derivations
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Part III: Examples
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Part IV: Best of the Best
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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 . From this work, we find that integrals over the mass and pressure distributions give:
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where,
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Renormalize
Let's renormalize these energy terms in order to more readily relate them to the generalized expressions derived above.
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Also,
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Hence,
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Given that for the bipolytrope, we can finally write,
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and,
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Hence the renormalized gravitational potential energy becomes,
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and the two, renormalized contributions to the thermal energy become,
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Finally, then, we can state that,
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Virial Equilibrium and Stability Evaluation
With these expressions in hand, we can deduce the equilibrium radius and relativity stability of bipolytropes using the generalized expressions provided above. For example, from the statement of virial equilibrium we obtain,
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Or, given the above renormalization, this expression can be written as,
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And the condition for dynamical stability is,
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(5, 1) Bipolytropes
In another accompanying discussion we have derived analytic expressions describing the equilibrium structure of bipolytropes with . Can we perform a similar stability analysis of these configurations? Work in progress!
Related Discussions
- Newer, Version2 of Bipolytrope Generalization derivations.
- Analytic solution with and .
- Analytic solution with and .
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Appendices: | VisTrailsEquations | VisTrailsVariables | References | Ramblings | VisTrailsImages | myphys.lsu | ADS | |