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==Free-Energy Analysis== <span id="Homologous">If we assume</span> the simplest approximation for the fundamental-mode eigenfunction, namely, <math>~\xi = \xi_0</math> = constant — that is, homologous expansion/contraction — then this last integral expression gives, <div align="center"> <table border="0" cellpadding="5" align="center"> <tr> <td align="right"> <math>~ \sigma^2 I</math> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~ (4 - 3\Gamma_1) W_\mathrm{grav} + 3^2 \Gamma_1 P_e V \, . </math> </td> </tr> </table> </div> Contrast this result with the following free-energy analysis: <div align="center"> <table border="0" cellpadding="5" align="center"> <tr> <td align="right"> <math>~\mathfrak{G}</math> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~W_\mathrm{grav} + U_\mathrm{int} + P_eV \, ,</math> </td> </tr> </table> </div> where, in terms of the configuration's (generally non-equilibrium) dimensionless radius, <math>~\chi \equiv R/R_0</math>, <div align="center"> <table border="0" cellpadding="5" align="center"> <tr> <td align="right"> <math>~W_\mathrm{grav}</math> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~-a\chi^{-1}</math> </td> </tr> <tr> <td align="right"> <math>~U_\mathrm{int}</math> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~b\chi^{3-3\Gamma_1}</math> </td> </tr> <tr> <td align="right"> <math>~V</math> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~\frac{4\pi}{3} \chi^3 \, .</math> </td> </tr> </table> </div> Then, <div align="center"> <table border="0" cellpadding="5" align="center"> <tr> <td align="right"> <math>~\frac{\partial \mathfrak{G}}{\partial \chi}</math> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~+a \chi^{-2} + 3(1-\Gamma_1) b \chi^{2-3\Gamma_1} + 4\pi P_e \chi^{2} </math> </td> </tr> <tr> <td align="right"> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~\chi^{-1} \biggl[- W_\mathrm{grav} + 3(1-\Gamma_1) U_\mathrm{int} + 3 P_e V \biggr] \, ,</math> </td> </tr> </table> </div> and, <div align="center"> <table border="0" cellpadding="5" align="center"> <tr> <td align="right"> <math>~\frac{\partial^2 \mathfrak{G}}{\partial \chi^2}</math> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~-2a \chi^{-3} + 3(1-\Gamma_1)(2-3\Gamma_1) b \chi^{1-3\Gamma_1} + 8\pi P_e \chi </math> </td> </tr> <tr> <td align="right"> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~\chi^{-2} \biggl[ 2W_\mathrm{grav} + 3(1-\Gamma_1)(2-3\Gamma_1) U_\mathrm{int}+ 6 P_e V \biggr] \, .</math> </td> </tr> </table> </div> The equilibrium condition occurs when <math>~\partial \mathfrak{G}/\partial \chi = 0</math>, that is, when, <div align="center"> <table border="0" cellpadding="5" align="center"> <tr> <td align="right"> <math>~3(1-\Gamma_1) U_\mathrm{int}</math> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~W_\mathrm{grav} - 3 P_e V \, ,</math> </td> </tr> </table> </div> in which case, <div align="center"> <table border="0" cellpadding="5" align="center"> <tr> <td align="right"> <math>~\chi^2 \cdot \frac{\partial^2 \mathfrak{G}}{\partial \chi^2}</math> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~2W_\mathrm{grav} + (2-3\Gamma_1) (W_\mathrm{grav} - 3P_eV) + 6 P_e V </math> </td> </tr> <tr> <td align="right"> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~(4-3\Gamma_1)W_\mathrm{grav} + 3^2 \Gamma_1 P_e V \, .</math> </td> </tr> </table> </div> Fantastic! The righthand-side of this "free-energy-based" expression exactly matches the righthand-side of the [[#Homologous|above expression]] that has been derived from the variational principle, assuming homologous expansion/contraction (''i.e.,'' <math>~\xi</math> = constant). In this case, we can make the direct association, <div align="center"> <math>~\sigma^2 I = \chi^2 \cdot \frac{\partial^2 \mathfrak{G}}{\partial \chi^2} \, .</math> </div> This also make sense in that the equilibrium configuration should be stable if <math>~\tfrac{\partial^2 \mathfrak{G}}{\partial \chi^2} > 0</math> — in which case, <math>~\sigma^2</math> is positive; whereas the equilibrium configuration should be ''unstable'' if <math>~\tfrac{\partial^2 \mathfrak{G}}{\partial \chi^2} < 0</math> — in which case, <math>~\sigma^2</math> is negative.
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