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===Whitworth's Presentation=== In §5 of his paper, {{ Whitworth81}} — hereafter, {{ Whitworth81hereafter }} — also presents the set of parametric equations that define what the equilibrium radius, <math>R_\mathrm{eq}</math>, is of an embedded polytrope for a certain imposed external pressure, <math>P_\mathrm{e}</math>, namely, <div align="center"> <table border="0" cellpadding="3"> <tr> <td align="right"> <math> ~R_\mathrm{eq} </math> </td> <td align="center"> <math>~=~</math> </td> <td align="left"> <math> ~R_\mathrm{rf} \biggl\{ \frac{4\eta}{5|\eta-1|} \biggl(\frac{\xi}{3} \biggr)^\eta \biggl|\frac{d\theta_n}{d\xi} \biggr|^{(2-\eta)} \biggr\}_{\xi_e}^{1/(3\eta - 4)} </math> </td> </tr> <tr> <td align="right"> <math> \Rightarrow ~~~~~ \biggl( \frac{R_\mathrm{eq}}{R_\mathrm{rf}} \biggr)^{(3-n)} </math> </td> <td align="center"> <math>~=~</math> </td> <td align="left"> <math> \biggl[ \frac{4(n+1)}{5} \biggr]^{n} \biggl(\frac{\xi_e}{3} \biggr)^{(n+1)} \biggl|\frac{d\theta_n}{d\xi} \biggr|^{(n-1)}_{\xi_e} \, , </math> </td> </tr> <tr> <td align="right"> <math> ~P_\mathrm{e} </math> </td> <td align="center"> <math>~=~</math> </td> <td align="left"> <math> P_\mathrm{rf} \biggl\{ 2^{-8/\eta} \biggl(\frac{5|\eta-1|}{\eta} \biggr)^3 \biggl(\frac{3}{\xi} \biggr)^4 \biggl|\frac{d\theta_n}{d\xi} \biggr|^{-2} \biggr\}_{\xi_e}^{\eta/(3\eta - 4)} \theta_n^{\eta/(\eta-1)} </math> </td> </tr> <tr> <td align="right"> <math> \Rightarrow ~~~~~ \biggl( \frac{P_\mathrm{e}}{P_\mathrm{rf}} \biggr)^{(3-n)} </math> </td> <td align="center"> <math>~=~</math> </td> <td align="left"> <math> 2^{-8n}\biggl\{ \biggl(\frac{5}{n+1} \biggr)^3 \biggl(\frac{3}{\xi} \biggr)^4 \theta_n^{(3-n)} \biggl|\frac{d\theta_n}{d\xi} \biggr|^{-2} \biggr\}_{\xi_e}^{(n+1)} \, , </math> </td> </tr> </table> </div> where, in order to obtain the second line of the two relations we have used the substitution, <math>\eta \rightarrow (1+1/n)</math>, and, as is detailed in an [[SSC/Structure/PolytropesASIDE1|accompanying ASIDE]], {{ Whitworth81hereafter }} "referenced" <math>P_\mathrm{e}</math> and <math>R_\mathrm{eq}</math> to, respectively, <div align="center"> <table border="0" cellpadding="3"> <tr> <td align="right"> <math> P_\mathrm{rf}^{(4-3\eta)} </math> </td> <td align="center"> <math>~=~</math> </td> <td align="left"> <math> 2^{-2(4+\eta)} \biggl( \frac{3^4 \cdot 5^3}{\pi} \biggr)^\eta \biggl[ \frac{K_n^4}{G^{3\eta} M^{2\eta} } \biggr] </math> </td> </tr> <tr> <td align="right"> <math> \Rightarrow ~~~~~ P_\mathrm{rf}^{(n-3)} </math> </td> <td align="center"> <math>~=~</math> </td> <td align="left"> <math> 2^{-2(5n+1)} \biggl( \frac{3^4 \cdot 5^3}{\pi} \biggr)^{(n+1)} \biggl[ \frac{K_n^{4n}}{G^{3(n+1)} M^{2(n+1)} } \biggr] \, , </math> </td> </tr> <tr> <td align="right"> <math> ~R_\mathrm{rf}^\eta </math> </td> <td align="center"> <math>~=~</math> </td> <td align="left"> <math> \frac{2^2}{K_n} \biggl(\frac{GM}{3\cdot 5}\biggr)^\eta P_\mathrm{rf}^{(1-\eta)} </math> </td> </tr> <tr> <td align="right"> <math> \Rightarrow ~~~~~ R_\mathrm{rf}^{(n+1)} </math> </td> <td align="center"> <math>~=~</math> </td> <td align="left"> <math> \biggl( \frac{2^2}{K_n} \biggr)^{n} \biggl(\frac{GM}{3\cdot 5}\biggr)^{(n+1)} P_\mathrm{rf}^{-1} </math> </td> </tr> <tr> <td align="right"> <math> \Rightarrow ~~~~~ R_\mathrm{rf}^{(3-n)} </math> </td> <td align="center"> <math>~=~</math> </td> <td align="left"> <math> \biggl( \frac{2^2}{K_n} \biggr)^{n(3-n)/(n+1)} \biggl(\frac{GM}{3\cdot 5}\biggr)^{(3-n)} P_\mathrm{rf}^{(n-3)/(n+1)} </math> </td> </tr> <tr> <td align="right"> </td> <td align="center"> <math>~=~</math> </td> <td align="left"> <math> \biggl( \frac{2^2}{K_n} \biggr)^{n(3-n)/(n+1)} \biggl(\frac{GM}{3\cdot 5}\biggr)^{(3-n)} \biggl\{2^{-2(5n+1)} \biggl( \frac{3^4 \cdot 5^3}{\pi} \biggr)^{(n+1)} \biggl[ \frac{K_n^{4n}}{G^{3(n+1)} M^{2(n+1)} } \biggr] \biggr\}^{1/(n+1)} </math> </td> </tr> <tr> <td align="right"> </td> <td align="center"> <math>~=~</math> </td> <td align="left"> <math>K_n^{n} ( 2^2 )^{-(n+1)} \biggl(\frac{GM}{3\cdot 5}\biggr)^{(3-n)} \biggl( \frac{3^4 \cdot 5^3}{\pi} \biggr) \biggl[ \frac{1}{G^{3} M^{2} } \biggr] </math> </td> </tr> <tr> <td align="right"> </td> <td align="center"> <math>~=~</math> </td> <td align="left"> <math> 2^{-2(n+1)} \pi^{-1} 3^{n+1} \cdot 5^{n} K_n^n G^{-n} M^{1-n} </math> </td> </tr> </table> </div> Via these normalizations, {{ Whitworth81hereafter }} — as did {{ Horedt70hereafter }} — chose to express <math>R_\mathrm{eq}</math> and <math>P_\mathrm{e}</math> in terms of {{Math/MP_PolytropicConstant}} and the system's total mass, <math>M</math>. To convert from Whitworth's expressions, which use one set of normalization parameters <math>(R_\mathrm{rf},P_\mathrm{rf})</math>, to Horedt's expressions, which use a somewhat different set of normalization parameters — identified here as <math>(R_\mathrm{Horedt},P_\mathrm{Horedt})</math> — one simply needs to make use of the relations, <div align="center"> <table border="0" cellpadding="3"> <tr> <td align="right"> <math> \biggl( \frac{R_\mathrm{rf}}{R_\mathrm{Horedt}} \biggr)^{(3-n)} </math> </td> <td align="center"> <math>~=~</math> </td> <td align="left"> <math> 3^{(n+1)} \biggl[ \frac{5}{2^2 (n+1)} \biggr]^{n} \, . </math> </td> </tr> <tr> <td align="right"> <math> \biggl( \frac{P_\mathrm{rf}}{P_\mathrm{Horedt}} \biggr)^{(3-n)} </math> </td> <td align="center"> <math>~=~</math> </td> <td align="left"> <math> 2^{8n} \biggl[ \frac{(n+1)^3}{3^4 \cdot 5^3} \biggr]^{(n+1)} \, , </math> </td> </tr> </table> </div>
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