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===Displacement Function for Isothermal LAWE=== The [[SSC/Stability/Isothermal#Taff_and_Van_Horn_.281974.29|LAWE for isothermal spheres]] may be written as, <div align="center"> <table border="0" cellpadding="5" align="center"> <tr> <td align="right"> <math>~\frac{d^2 x}{dr^2} + \biggl[4 - r \biggl(\frac{dw }{dr}\biggr) \biggr] \frac{1}{r}\frac{dx}{dr}</math> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~ - \biggl[ \frac{\sigma_c^2}{6\gamma} - \frac{\alpha}{r} \biggl(\frac{dw }{dr}\biggr)\biggr] x \, , </math> </td> </tr> </table> </div> where, <math>~w(r)</math> is the isothermal Lane-Emden function describing the configuration's unperturbed radial density distribution, and <math>~\gamma</math>, <math>~\sigma_c^2</math>, and <math>~\alpha \equiv (3-4/\gamma)</math> are constants. Here we seek a power-series expression for the displacement function, <math>~x(r)</math>, expanded about the center of the configuration, that approximately satisfies this LAWE. First we note that, near the center, an accurate [[#Isothermal_Lane-Emden_Function|power-series expression for the isothermal Lane-Emden function]] is, <div align="center"> <table border="0" cellpadding="5" align="center"> <tr> <td align="right"> <math>~w(r) </math> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~\frac{r^2}{6} - \frac{r^4}{120} + \frac{r^6}{1890} - \frac{61 r^8}{1,632,960} + \cdots \, .</math> </td> </tr> </table> </div> Hence, <div align="center"> <table border="0" cellpadding="5" align="center"> <tr> <td align="right"> <math>~\frac{dw}{dr}</math> </td> <td align="center"> <math>~\approx</math> </td> <td align="left"> <math>~\frac{r}{3} - \frac{r^3}{30} + \frac{r^5}{315} \, .</math> </td> </tr> </table> </div> Therefore, near the center of the configuration, the LAWE may be written as, <div align="center"> <table border="0" cellpadding="5" align="center"> <tr> <td align="right"> <math>~\frac{d^2 x}{dr^2} + \biggl[4 - \biggl(\frac{r^2}{3} - \frac{r^4}{30} + \frac{r^6}{315}\biggr) \biggr] \frac{1}{r}\frac{dx}{dr}</math> </td> <td align="center"> <math>~\approx</math> </td> <td align="left"> <math>~ - \frac{1}{6} \biggl[ \frac{\sigma_c^2}{\gamma} - 2\alpha \biggl(1 - \frac{r^2}{10} + \frac{r^4}{105}\biggr) \biggr] x \, . </math> </td> </tr> </table> </div> Let's now adopt a power-series expression for the displacement function of the form, <div align="center"> <table border="0" cellpadding="5" align="center"> <tr> <td align="right"> <math>~x</math> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~ 1 + ar + br^2 + cr^3 + dr^4 + \cdots </math> </td> </tr> <tr> <td align="right"> <math>~\Rightarrow ~~~ \frac{1}{r}\frac{dx}{dr}</math> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~ \frac{a}{r} + 2b + 3 cr + 4dr^2 + \cdots </math> </td> </tr> </table> </div> and, <div align="center"> <table border="0" cellpadding="5" align="center"> <tr> <td align="right"> <math>~\frac{d^2x}{dr^2}</math> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~ 2b + 6cr + 12dr^2 + \cdots </math> </td> </tr> </table> </div> Substituting these expressions into the LAWE gives, <div align="center"> <table border="0" cellpadding="5" align="center"> <tr> <td align="right"> <math>~2b + 6cr + 12dr^2 + \biggl[4 - \biggl(\frac{r^2}{3} - \frac{r^4}{30} + \frac{r^6}{315}\biggr) \biggr] \biggl[ \frac{a}{r} + 2b + 3 cr + 4dr^2 \biggr] </math> </td> <td align="center"> <math>~\approx</math> </td> <td align="left"> <math>~ - \frac{1}{6} \biggl[ \frac{\sigma_c^2}{\gamma} - 2\alpha \biggl(1 - \frac{r^2}{10} + \frac{r^4}{105}\biggr) \biggr] \biggl( 1 + ar + br^2 + cr^3 + dr^4 \biggr) \, . </math> </td> </tr> </table> </div> Keeping terms only up through <math>~r^2</math> leads to the following simplification: <div align="center"> <table border="0" cellpadding="5" align="center"> <tr> <td align="right"> <math>~ 2b + 6cr + 12dr^2 + 4 \biggl[ \frac{a}{r} + 2b + 3 cr + 4dr^2 \biggr] - \frac{r^2}{3} \biggl[ \frac{a}{r} + 2b \biggr] </math> </td> <td align="center"> <math>~\approx</math> </td> <td align="left"> <math>~ - \frac{\mathfrak{F} }{6} \biggl( 1 + ar + br^2 \biggr) - \frac{\alpha}{3} \biggl(\frac{r^2}{10} \biggr) </math> </td> </tr> </table> </div> where, <div align="center"> <math>~\mathfrak{F} \equiv \frac{\sigma_c^2}{\gamma} - 2\alpha \, .</math> </div> Finally, balancing terms of like powers on both sides of the equation leads us to conclude the following: <div align="center"> <table border="1" cellpadding="5" align="center"> <tr> <td align="center">Term</td> <td align="center">LHS</td> <td align="center">RHS</td> <td align="center">Implication</td> </tr> <tr> <td align="right"> <math>~r^{-1}:</math> </td> <td align="center"> <math>~4a</math> </td> <td align="center"> <math>~0</math> </td> <td align="left"> <math>~\Rightarrow ~~~a = 0 </math> </td> </tr> <tr> <td align="right"> <math>~r^{0}:</math> </td> <td align="center"> <math>~2b + 8b</math> </td> <td align="center"> <math>~- \frac{\mathfrak{F}}{6}</math> </td> <td align="left"> <math>~\Rightarrow ~~~b = - \frac{\mathfrak{F}}{60}</math> </td> </tr> <tr> <td align="right"> <math>~r^{1}:</math> </td> <td align="center"> <math>~6c + 12c - \frac{a}{3}</math> </td> <td align="center"> <math>~-\frac{a\mathfrak{F}}{6}</math> </td> <td align="left"> <math>~\Rightarrow ~~~c=0</math> </td> </tr> <tr> <td align="right"> <math>~r^{2}:</math> </td> <td align="center"> <math>~12d + 16d - \frac{2b}{3}</math> </td> <td align="center"> <math>~-\frac{\mathfrak{F}b}{6} - \frac{\alpha}{30}</math> </td> <td align="left"> <math>~\Rightarrow ~~~ 28d = \frac{1}{30}\biggl[ 5b (4- \mathfrak{F} ) - \alpha \biggr] ~ \Rightarrow~ d = \frac{1}{10080}\biggl[ \mathfrak{F}(\mathfrak{F} -4) - 12\alpha \biggr] </math> </td> </tr> </table> </div> In summary, the desired, approximate power-series expression for the isothermal displacement function is: <div align="center" id="IsothermalDisplacement"> <table border="1" width="80%" cellpadding="8" align="center"><tr><td align="center"> <table border="0" cellpadding="5" align="center"> <tr> <td align="right"> <math>~x(r)</math> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~ 1 - \frac{\mathfrak{F}}{60} r^2 + \frac{1}{10080}\biggl[ \mathfrak{F}(\mathfrak{F} -4) - 12\alpha \biggr] r^4 + \cdots </math> </td> </tr> </table> </td></tr></table> </div>
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