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====Fixed Mass Ratio==== Let's define the mass ratio, <table border="0" cellpadding="5" align="center"> <tr> <td align="right"> <math>~q</math> </td> <td align="center"> <math>~\equiv</math> </td> <td align="left"> <math>~ \frac{M_t}{M_c} \, , </math> </td> </tr> </table> and build a sequence along which this ratio is held constant. For the problem being considered here, the relevant expression for <math>~q</math> is, <table border="0" cellpadding="5" align="center"> <tr> <td align="right"> <math>~q</math> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~ \biggl[ 2\pi^2 R_\mathrm{eq}^3 \rho \alpha_t \beta_t^2 \biggr] \biggl[ \frac{4\pi}{3} \rho R_\mathrm{eq}^3 (1 - e^2)^{1 / 2} \biggr]^{-1} </math> </td> </tr> <tr> <td align="right"> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~ \biggl( \frac{3\pi}{2} \biggr) \alpha_t \beta_t^2 (1 - e^2)^{- 1 / 2}\, . </math> </td> </tr> </table> The sequence is constructed by choosing <math>~q</math> (held fixed), and varying the value of <math>~0 < \beta_t \le \beta_\mathrm{max}</math>; then, for each chosen parameter pair, recognize that, <table border="0" cellpadding="5" align="center"> <tr> <td align="right"> <math>~ \alpha_t (1 - e^2)^{- 1 / 2} </math> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~\biggl( \frac{2}{3\pi} \biggr) \frac{q}{ \beta_t^2 } \, ,</math> </td> </tr> </table> that is, from the [[#Surrounding_Torus|above expression for <math>~\alpha_t</math>]], <table border="0" cellpadding="5" align="center"> <tr> <td align="right"> <math>~ \biggl[\frac{1}{3\Omega^2} (1 - e^2)^{1 / 2} \biggr] (1 - e^2)^{- 3 / 2} </math> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~\biggl[ \biggl( \frac{2}{3\pi} \biggr) \frac{q}{ \beta_t^2 } \biggr]^3</math> </td> </tr> <tr> <td align="right"> <math>~\Rightarrow~~~ \Omega^2 (1 - e^2) </math> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~\frac{1}{3}\biggl[ \biggl( \frac{3\pi}{2} \biggr) \frac{ \beta_t^2 }{q} \biggr]^3 \, .</math> </td> </tr> </table> But, for central models along the MLS, we also must satisfy the relation [[#Model_Sequences|given above]], namely, <table border="0" cellpadding="5" align="center"> <tr> <td align="right"> <math>~\Omega^2 </math> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~ \frac{1}{2}(3 - 2e^2)(1 - e^2)^{1 / 2} \cdot \frac{\sin^{-1} e}{e^3} - \frac{3(1-e^2)}{2e^2} \, . </math> </td> </tr> </table> Hence, for each <math>~(q, \beta_t)</math> parameter pair, the relevant central-object eccentricity is given by the root of the relation, <table border="0" cellpadding="5" align="center"> <tr> <td align="right"> <math>~ \frac{1}{2}(3 - 2e^2)(1 - e^2)^{3 / 2} \cdot \frac{\sin^{-1} e}{e^3} - \frac{3(1-e^2)^2 }{2e^2} </math> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~\frac{1}{3}\biggl[ \biggl( \frac{3\pi}{2} \biggr) \frac{ \beta_t^2 }{q} \biggr]^3 \, .</math> </td> </tr> </table> Note that, for the limiting value, <math>~\beta_\mathrm{max} = (\alpha_t - 1)</math>, the relevant relation becomes, <table border="0" cellpadding="5" align="center"> <tr> <td align="right"> <math>~ (\alpha_t - 1)^2\alpha_t (1 - e^2)^{- 1 / 2} </math> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~\frac{2q}{3\pi} </math> </td> </tr> </table> where [[#Surrounding_Torus|again, as above]] <table border="0" cellpadding="5" align="center"> <tr> <td align="right"> <math>~\alpha_t \equiv \frac{a}{R_\mathrm{eq}} </math> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~\biggl[\frac{1}{3\Omega^2} (1 - e^2)^{1 / 2} \biggr]^{1 / 3} \, .</math> </td> </tr> </table>
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