Editing SSC/Structure/BiPolytropes/Analytic51/Pt2 (section)

=BiPolytrope with n<sub>c</sub> = 5 and n<sub>e</sub> = 1 (Pt 2)=
<table border="1" align="center" width="100%" colspan="8">
<tr>
  <td align="center" bgcolor="lightblue" width="25%"><br />[[SSC/Structure/BiPolytropes/Analytic51|Part I:&nbsp; (n<sub>c</sub>,n<sub>e</sub>) = (5,1) BiPolytrope]]
&nbsp;
  </td>
  <td align="center" bgcolor="lightblue" width="25%"><br />[[SSC/Structure/BiPolytropes/Analytic51/Pt2|Part II:&nbsp; Example Models]]
&nbsp;
  </td>
  <td align="center" bgcolor="lightblue" width="25%"><br />[[SSC/Structure/BiPolytropes/Analytic51/Pt3|Part III:&nbsp; Limiting Mass]]
&nbsp;
  </td>
  <td align="center" bgcolor="lightblue"><br />[[SSC/Structure/BiPolytropes/Analytic51/Pt4|Part IV:&nbsp; Free Energy]]
&nbsp;
  </td>
</tr>
</table>

==Examples==

===Normalization===
The dimensionless variables used in Tables 1 &amp; 2 are defined as follows:
<div align="center">
<table border="0" cellpadding="3">
<tr>
  <td align="right">
<math>\rho^*</math>
  </td>
  <td align="center">
<math>\equiv</math>
  </td>
  <td align="left">
<math>\frac{\rho}{\rho_0}</math>
  </td>

  <td align="center">; &nbsp;&nbsp;&nbsp;</td>

  <td align="right">
<math>r^*</math>
  </td>
  <td align="center">
<math>\equiv</math>
  </td>
  <td align="left">
<math>\frac{r}{[K_c^{1/2}/(G^{1/2}\rho_0^{2/5})]}</math>
  </td>
</tr>

<tr>
  <td align="right">
<math>P^*</math>
  </td>
  <td align="center">
<math>\equiv</math>
  </td>
  <td align="left">
<math>\frac{P}{K_c\rho_0^{6/5}}</math>
  </td>

  <td align="center">; &nbsp;&nbsp;&nbsp;</td>

  <td align="right">
<math>M_r^*</math>
  </td>
  <td align="center">
<math>\equiv</math>
  </td>
  <td align="left">
<math>\frac{M_r}{[K_c^{3/2}/(G^{3/2}\rho_0^{1/5})]}</math>
  </td>
</tr>

<tr>
  <td align="right">
<math>H^*</math>
  </td>
  <td align="center">
<math>\equiv</math>
  </td>
  <td align="left">
<math>\frac{H}{K_c\rho_0^{1/5}}</math>
  </td>

  <td align="center">. &nbsp;&nbsp;&nbsp;</td>

  <td align="right" colspan="3">
&nbsp;
  </td>
</tr>

</table>
</div>

===Parameter Values===

The <math>2^\mathrm{nd}</math> column of Table 1 catalogues the analytic expressions that define various parameters and physical properties (as identified, respectively, in column 1) of the <math>(n_c, n_e) = (5, 1)</math> bipolytrope.  We have evaluated these expressions for various choices of the dimensionless interface radius, <math>\xi_i</math>, and have tabulated the results in the last few columns of the table.  The tabulated values have been derived assuming <math>\mu_e/\mu_c = 1</math>, that is, assuming that the core and the envelope have the same mean molecular weights.  

<!--  BEGIN TABLE OF PARAMETERS --->
<div align="center">
<b>Table 1:  Properties of <math>(n_c, n_e) = (5, 1)</math> BiPolytrope Having Various Interface Locations, <math>\xi_i</math></b><br>
[[File:BiPolytropeParametersV01.xml|Accompanying spreadsheet with parameter values]]

<table border="1" cellpadding="5" width="80%">
<tr>
  <td align="center">
Parameter
  </td>
  <td align="center">
<math>\xi_i</math>
  </td>
  <td align="center">
0.5
  </td>
  <td align="center">
1.0
  </td>
  <td align="center">
1.66864602<sup>&dagger;</sup>
  </td>
  <td align="center">
3.0
  </td>
  <td rowspan="21">
[[File:Bipolytrope51Boundaries02.png|500px|Examples]]<br />
<table border="0" align="left" cellpadding="10"><tr><td align="left">
For bipolytropic models having <math>\mu_e/\mu_c = 1.0</math>, this figure shows how the interface location, <math>\eta_i</math> (solid purple curve), the surface radius, <math>\eta_s</math> (green circular markers), and the parameter, <math>\tan^{-1}\Lambda_i</math> (orange circular markers), vary with <math>\xi_i</math> (ordinate) over the range, <math>0 \le \xi_i \le 12</math>.  The three horizontal, red-dashed line segments identify the values of <math>\xi_i</math> for which numerical values of these (and other) parameters have been listed in the table shown here on the left.</td></tr></table>
  </td>
</tr>

<tr>
  <td align="center">
<math>\theta_i</math>
  </td>
  <td align="center">
<math>\biggl( 1+\frac{1}{3}\xi_i^2 \biggr)^{-1/2}</math>
  </td>
  <td align="center">
0.96077
  </td>

  <td align="center">
0.86603
  </td>
  <td align="center">
0.72016538
  </td>
  <td align="center">
0.50000
  </td>
</tr>

<tr>
  <td align="center">
<math>-\biggl(\frac{d\theta_i}{d\xi}\biggr)_i</math>
  </td>
  <td align="center">
<math>\frac{1}{3} \xi_i \biggl( 1+\frac{1}{3}\xi_i^2 \biggr)^{-3/2}</math>
  </td>
  <td align="center">
0.14781
  </td>

  <td align="center">
0.21651
  </td>
  <td align="center">
0.20774935
  </td>
  <td align="center">
0.12500
  </td>
</tr>

<tr>
  <td align="center">
<math>r^*_\mathrm{core} \equiv r^*_i</math>
  </td>
  <td align="center">
<math>\biggl( \frac{3}{2\pi} \biggr)^{1/2} \xi_i</math>
  </td>
  <td align="center">
0.34549
  </td>

  <td align="center">
0.69099
  </td>
  <td align="center">
1.15301487
  </td>
  <td align="center">
2.07297
  </td>
</tr>

<tr>
  <td align="center">
<math>\rho^*_i \biggr|_c = \biggl( \frac{\mu_e}{\mu_c} \biggr)^{-1} \rho^*_i \biggr|_e</math>
  </td>
  <td align="center">
<math>\biggl( 1+\frac{1}{3}\xi_i^2 \biggr)^{-5/2}</math>
  </td>
  <td align="center">
0.81864
  </td>

  <td align="center">
0.48714
  </td>
  <td align="center">
0.19371408
  </td>
  <td align="center">
0.03125
  </td>
</tr>

<tr>
  <td align="center">
<math>P^*_i</math>
  </td>
  <td align="center">
<math>\biggl( 1+\frac{1}{3}\xi_i^2 \biggr)^{-3}</math>
  </td>
  <td align="center">
0.78653
  </td>

  <td align="center">
0.42188
  </td>
  <td align="center">
0.13950617
  </td>
  <td align="center">
0.01563
  </td>
</tr>

<tr>
  <td align="center">
<math>H^*_i \biggr|_c = \frac{n_c+1}{n_e+1} \biggl( \frac{\mu_e}{\mu_c} \biggr) H^*_i \biggr|_e</math>
  </td>
  <td align="center">
<math>6 \biggl( 1+\frac{1}{3}\xi_i^2 \biggr)^{-1/2}</math>
  </td>
  <td align="center">
5.76461
  </td>

  <td align="center">
5.19615
  </td>
  <td align="center">
4.32099225
  </td>
  <td align="center">
3.00000
  </td>
</tr>

<tr>
  <td align="center">
<math>M^*_\mathrm{core}</math>
  </td>
  <td align="center">
<math>\biggl( \frac{6}{\pi}\biggr)^{1/2} (\xi_i \theta_i)^3</math>
  </td>
  <td align="center">
0.15320
  </td>

  <td align="center">
0.89762
  </td>
  <td align="center">
2.39822567
  </td>
  <td align="center">
4.66417
  </td>
</tr>

<tr>
  <td align="center">
<math>\biggl( \frac{\mu_e}{\mu_c} \biggr)^{-1}\eta_i</math>
  </td>
  <td align="center">
<math>\sqrt{3} ~\theta_i^2 \xi_i</math>
  </td>
  <td align="center">
0.79941
  </td>

  <td align="center">
1.29904
  </td>
  <td align="center">
1.49895749
  </td>
  <td align="center">
1.29904
  </td>
</tr>

<tr>
  <td align="center">
<math>-\biggl( \frac{d\phi}{d\eta} \biggr)_i</math>
  </td>
  <td align="center">
<math>\sqrt{3} ~\theta_i^{-3} \biggl( - \frac{d\theta}{d\xi} \biggr)_i = \frac{\xi_i}{\sqrt{3}}</math>
  </td>
  <td align="center">
0.28868
  </td>

  <td align="center">
0.57735
  </td>
  <td align="center">
0.96339323
  </td>
  <td align="center">
1.73205
  </td>
</tr>

<tr>
  <td align="center">
<math>\Lambda_i</math>
  </td>
  <td align="center">
<math>\frac{1}{\eta_i} + \biggl( \frac{d\phi}{d\eta} \biggr)_i</math>
  </td>
  <td align="center">
0.96225
  </td>

  <td align="center">
0.19245
  </td>
  <td align="center">
-&nbsp; 0.2962629
  </td>
  <td align="center">
-0.96225
  </td>
</tr>

<tr>
  <td align="center">
<math>A</math>
  </td>
  <td align="center">
<math>\eta_i (1 + \Lambda_i^2)^{1/2}</math>
  </td>
  <td align="center">
1.10940
  </td>

  <td align="center">
1.32288
  </td>
  <td align="center">
1.56335712
  </td>
  <td align="center">
1.80278
  </td>
</tr>

<tr>
  <td align="center">
<math>B</math>
  </td>
  <td align="center">
<math>\eta_i - \frac{\pi}{2} + \tan^{-1}( \Lambda_i)</math>
  </td>
  <td align="center">
- 0.00523
  </td>

  <td align="center">
-0.08163
  </td>
  <td align="center">
-0.359863583
  </td>
  <td align="center">
-1.03792
  </td>
</tr>

<tr>
  <td align="center">
<math>\eta_s</math>
  </td>
  <td align="center">
<math>\pi + B</math>
  </td>
  <td align="center">
3.13637
  </td>

  <td align="center">
3.05996
  </td>
  <td align="center">
2.781729071
  </td>
  <td align="center">
2.10367
  </td>
</tr>

<tr>
  <td align="center">
<math>- \biggl( \frac{d\phi}{d\eta} \biggr)_s</math>
  </td>
  <td align="center">
<math>\frac{A}{\eta_s}</math>
  </td>
  <td align="center">
0.35372
  </td>

  <td align="center">
0.43232
  </td>
  <td align="center">
0.562009126
  </td>
  <td align="center">
0.85697
  </td>
</tr>

<tr>
  <td align="center">
<math>\biggl( \frac{\mu_e}{\mu_c} \biggr) \cdot \biggl[ R^* \equiv r^*_s \biggr]</math>
  </td>
  <td align="center">
<math>\frac{\eta_s}{\sqrt{2\pi} ~\theta_i^2}</math>
  </td>
  <td align="center">
1.35550
  </td>

  <td align="center">
1.62766
  </td>
  <td align="center">
2.139737125
  </td>
  <td align="center">
3.35697
  </td>
</tr>

<tr>
  <td align="center">
<math>\biggl( \frac{\mu_e}{\mu_c} \biggr)^2 M^*_\mathrm{tot}</math>
  </td>
  <td align="center">
<math>\biggl(\frac{2}{\pi}\biggr)^{1/2} \theta_i^{-1} \biggl( -\eta^2 \frac{d\phi}{d\eta} \biggr)_s = \biggl(\frac{2}{\pi}\biggr)^{1/2} \frac{A\eta_s}{\theta_i}</math>
  </td>
  <td align="center">
2.88959
  </td>

  <td align="center">
3.72945
  </td>
  <td align="center">
4.818155932
  </td>
  <td align="center">
6.05187
  </td>
</tr>

<tr>
  <td align="center">
<math>\biggl( \frac{\mu_e}{\mu_c} \biggr) \frac{\rho_c}{\bar\rho}</math>
  </td>
  <td align="center">
<math>~\frac{\eta_s^2}{3A\theta_i^5}</math>
  </td>
  <td align="center">
3.61035
  </td>

  <td align="center">
4.84326
  </td>
  <td align="center">
8.517046605
  </td>
  <td align="center">
26.1844
  </td>
</tr>

<tr>
  <td align="center">
<math>\biggl(\frac{\mu_e}{\mu_c}\biggr)^{-2} \cdot \biggl[ \nu \equiv \frac{M_\mathrm{core}}{M_\mathrm{tot}} \biggr]</math>
  </td>
  <td align="center">
<math>\sqrt{3} ~\biggl( \frac{\xi_i^3 \theta_i^4}{A\eta_s} \biggr)</math>
  </td>
  <td align="center">
0.05302
  </td>

  <td align="center">
0.24068
  </td>
  <td align="center">
0.497747627
  </td>
  <td align="center">
0.77070
  </td>
</tr>

<tr>
  <td align="center">
<math>\biggl(\frac{\mu_e}{\mu_c}\biggr)^{-1} \cdot \biggl[ q \equiv \frac{r_\mathrm{core}}{R} \biggr]</math>
  </td>
  <td align="center">
<math>\sqrt{3}~\biggl[\frac{\xi_i \theta_i^2}{\eta_s}\biggr]</math>
  </td>
  <td align="center">
0.25488
  </td>

  <td align="center">
0.42453
  </td>
  <td align="center">
0.538858190
  </td>
  <td align="center">
0.61751
  </td>
</tr>

<tr>
  <td align="left" colspan="6">
<sup>&dagger;</sup>This choice of the value of <math>\xi_i = 1.66864602</math> is motivated by our [[SSC/Stability/BiPolytropes/Pt3#Fundamental_Modes|discussion of the fundamental mode of oscillation]] of the marginally unstable model that has <math>\mu_e/\mu_c = 1.0</math>; see especially row 1 of Table 2 in that associated chapter.
</tr>

</table>
</div>
<!--  END TABLE OF PARAMETERS --->


Alternatively, if given <math>\mu_e/\mu_c</math> and the value of the parameter, <math>\eta_i</math>, then we have,
<table border="0" cellpadding="5" align="center">

<tr>
  <td align="right">
<math>\biggl(\frac{\mu_e}{\mu_c} \biggr)^{-1}\eta_i</math>
  </td>
  <td align="center">
<math>=</math>
  </td>
  <td align="left">
<math>\frac{3^{3/2}\xi_i}{3 + \xi_i^2}</math>
  </td>
</tr>

<tr>
  <td align="right">
<math>\Rightarrow ~~~ 0</math>
  </td>
  <td align="center">
<math>=</math>
  </td>
  <td align="left">
<math>\xi_i^2 - \biggl[ \biggl(\frac{\mu_e}{\mu_c} \biggr) \frac{3^{3/2}}{\eta_i }\biggr] \xi_i + 3</math>
  </td>
</tr>

<tr>
  <td align="right">
<math>\Rightarrow ~~~\xi_i </math>
  </td>
  <td align="center">
<math>=</math>
  </td>
  <td align="left">
<math>\sqrt{3}
\biggl(\frac{\mu_e}{\mu_c} \biggr) \frac{3}{2\eta_i } \biggl\{ 1 \pm  
\sqrt{1 - \biggl[ \biggl(\frac{\mu_e}{\mu_c} \biggr)^{-1} \frac{2 \eta_i }{3}\biggr]^2  }
\biggr\} \, .
</math>
  </td>
</tr>
</table>

It must be understood, therefore, that the interface location is restricted to the range,
<table border="0" cellpadding="5" align="center">

<tr>
  <td align="right">
<math>~0</math>
  </td>
  <td align="center">
<math>~\le \eta_i \le</math>
  </td>
  <td align="left">
<math>~\frac{3}{2}\biggl(\frac{\mu_e}{\mu_c} \biggr)\, ,</math>
  </td>
</tr>
</table>

and that this upper limit on <math>\eta_i</math> is associated with a model whose core radius is, <math>\xi_i = \sqrt{3}</math>.  Also,

<table border="0" cellpadding="5" align="center">

<tr>
  <td align="right">
<math>\Lambda_i </math>
  </td>
  <td align="center">
<math>=</math>
  </td>
  <td align="left">
<math>
\frac{1}{\eta_i} -
\biggl(\frac{\mu_e}{\mu_c} \biggr) \frac{3}{2\eta_i } \biggl\{ 1 \pm  
\sqrt{1 - \biggl[ \biggl(\frac{\mu_e}{\mu_c} \biggr)^{-1} \frac{2 \eta_i }{3}\biggr]^2  }
\biggr\} \, .
</math>
  </td>
</tr>
</table>

===Profile===

Once the values of the key set of parameters have been determined as illustrated in Table 1, the radial profile of various physical variables can be determined throughout the bipolytrope as detailed in [[#Steps_2_.26_3|step &#35;4]] and [[#Step_7|step &#35;8]], above.  Table 2 summarizes the mathematical expressions that define the profile throughout the core (column 2) and throughout the envelope (column 3) of the normalized mass density, <math>\rho^*(r^*)</math>, the normalized gas pressure, <math>P^*(r^*)</math>, and the normalized mass interior to <math>r^*</math>, <math>M_r^*(r^*)</math>.  For all profiles, the relevant normalized radial coordinate is <math>r^*</math>, as defined in the <math>2^\mathrm{nd}</math> row of Table 2.  Graphical illustrations of these resulting profiles can be viewed by clicking on the thumbnail images posted in the last few columns of Table 2.  

<div align="center">
<b>Table 2:  Radial Profile of Various Physical Variables</b>
<table border="1" cellpadding="6">
<tr>
  <td align="center" rowspan="2">
Variable
  </td>
  <td align="center" rowspan="2">
Throughout the Core<br>
<math>0 \le \xi \le \xi_i</math>
  </td>
  <td align="center" rowspan="2">
Throughout the Envelope<sup>&dagger;</sup><br>
<math>\eta_i \le \eta \le \eta_s</math>
  </td>

  <td align="center" colspan="3">
Plotted Profiles
  </td>
</tr>

<tr>
  <td align="center">
<math>\xi_i = 0.5</math>
  </td>
  <td align="center">
<math>\xi_i = 1.0</math>
  </td>
  <td align="center">
<math>\xi_i = 3.0</math>
  </td>
</tr>

<tr>
  <td align="center">
<math>r^*</math>
  </td>
  <td align="center">
<math>\biggl( \frac{3}{2\pi} \biggr)^{1/2} \xi</math>
  </td>
  <td align="center">
<math>\biggl( \frac{\mu_e}{\mu_c} \biggr)^{-1} \theta^{-2}_i (2\pi)^{-1/2}\eta</math>
  </td>

  <td align="center" colspan="3">
&nbsp;
  </td>
</tr>

<tr>
  <td align="center">
<math>\rho^*</math>
  </td>
  <td align="center">
<math>\biggl( 1 + \frac{1}{3}\xi^2 \biggr)^{-5/2}</math>
  </td>
  <td align="center">
<math>\biggl( \frac{\mu_e}{\mu_c} \biggr) \theta^{5}_i \phi(\eta)</math>
  </td>

  <td align="center">
<!--  [[File:PlotDensity_xi_0.5.jpg|thumb|75px]] -->
[[Image:DenXi05.jpg|thumb|75px]]
  </td>
  <td align="center">
[[Image:DenXi10.jpg|thumb|75px]]
  </td>
  <td align="center">
[[Image:DenXi30.jpg|thumb|75px]]
  </td>
</tr>

<tr>
  <td align="center">
<math>P^*</math>
  </td>
  <td align="center">
<math>\biggl( 1 + \frac{1}{3}\xi^2 \biggr)^{-3}</math>
  </td>
  <td align="center">
<math>\theta^{6}_i [\phi(\eta)]^{2}</math>
  </td>

  <td align="center">
<!-- [[File:PlotPressure_xi_0.5.jpg|thumb|75px]] -->
[[Image:PresXi05.jpg|thumb|75px]]
  </td>
  <td align="center">
[[Image:PresXi10.jpg|thumb|75px]]
  </td>
  <td align="center">
[[Image:PresXi30.jpg|thumb|75px]]
  </td>
</tr>

<tr>
  <td align="center">
<math>M_r^*</math>
  </td>
  <td align="center">
<math>\biggl( \frac{2\cdot 3}{\pi } \biggr)^{1/2} \biggl[ \xi^3 \biggl( 1 + \frac{1}{3}\xi^2 \biggr)^{-3/2} \biggr]</math>
  </td>
  <td align="center">
<math>\biggl( \frac{\mu_e}{\mu_c} \biggr)^{-2} \theta^{-1}_i \biggl( \frac{2}{\pi} \biggr)^{1/2} \biggl(-\eta^2 \frac{d\phi}{d\eta} \biggr)</math>
  </td>

  <td align="center">
<!-- [[File:PlotPressure_xi_0.5.jpg|thumb|75px]] -->
[[Image:MassXi05.jpg|thumb|75px]]
  </td>
  <td align="center">
[[Image:MassXi10.jpg|thumb|75px]]
  </td>
  <td align="center">
[[Image:MassXi30.jpg|thumb|75px]]
  </td>
</tr>

<tr>
  <td align="left" colspan="6">
<sup>&dagger;</sup>In order to obtain the various envelope profiles, it is necessary to evaluate <math>\phi(\eta)</math> and its first derivative using the information presented in Step 6, above.
  </td>
</tr>
</table>
</div>

[As of 28 April 2013] For the interface locations <math>\xi_i = 0.5, 1.0,\mathrm{and}~3.0</math>, Table 2 provides profiles for three values of the molecular weight ratio:  <math>\mu_e/\mu_c = 1.0, 1/2,\mathrm{and}~1/4</math>.  In all nine graphs, blue diamonds trace the structure of the <math>n_c=5</math> core; the core extends to a radius, <math>r^*_\mathrm{core}</math>, that is independent of molecular weight ratio but varies in direct proportion to the choice of <math>\xi_i</math>.  Specifically, as tabulated in the fourth row of Table 1, <math>r^*_\mathrm{core} = 0.34549, ~0.69099, \mathrm{and} ~2.07297</math> for, respectively, <math>\xi_i = 0.5,~1,~\mathrm{and}~3</math>.  Notice that, while the pressure profile and mass profile are continuous at the interface for all choices of the molecular weight ratio, the density profile exhibits a discontinuous jump that is in direct proportion to the chosen value of <math>\mu_e/\mu_c</math>.  

Throughout the <math>n_e = 1</math> envelope, the profile of all physical variables varies with the choice of the molecular weight ratio.  In the Table 2 graphs, red squares trace the envelope profile for <math>\mu_e/\mu_c = 1.0</math>; green triangles trace the envelope profile for <math>\mu_e/\mu_c = 1/2</math>; and purple crosses trace the envelope profile for <math>\mu_e/\mu_c = 1/4</math>.  The surface of the bipolytropic configuration is defined by the (normalized) radius, <math>R^*</math>, at which the envelope density and pressure drop to zero; the values tabulated in row 16 of Table 1 &#8212; <math>1.35550, ~1.62766, ~\mathrm{and} ~3.35697</math> for, respectively, <math>\xi_i = 0.5,~1,~\mathrm{and}~3</math> &#8212; correspond to a molecular weight ratio of unity and, hence also, to the envelope profiles traced by red squares in the Table 2 graphs.  As the molecular weight ratio is decreased from unity to <math>1/2</math> and, then, <math>1/4</math> for a given choice of <math>\xi_i</math>, the (normalized) radius of the bipolytrope increases roughly in inverse proportion to <math>\mu_e/\mu_c</math> as suggested by the formula for <math>R^*</math> shown in Table 1.  This proportional relation is not exact, however, because the parameter <math>\eta_s</math>, which also appears in the formula for <math>R^*</math>, contains an implicit dependence on the chosen value of the molecular weight ratio through the parameter <math>\eta_i</math>.

For a given choice of the interface parameter, <math>\xi_i</math>, the (normalized) mass that is contained in the core is independent of the choice of the molecular weight ratio.  However, the (normalized) total mass, <math>M_\mathrm{tot}^*</math>, varies significantly with the choice of <math>\mu_e/\mu_c</math>; as suggested by the expression provided in row 17 of Table 1, the variation is in rough proportion to <math>(\mu_e/\mu_c)^{-2}</math> but, as with <math>R^*</math>, this proportional relation is not exact because the parameters <math>\eta_s</math> and <math>A</math> which also appear in the formula for <math>M_\mathrm{tot}^*</math> harbor an implicit dependence on the molecular weight ratio.

===Model Sequences===

For a given choice of <math>\mu_e/\mu_c</math> a physically relevant sequence of models can be constructed by steadily increasing the value of <math>\xi_i</math> from zero to infinity &#8212; or at least to some value, <math>\xi_i \gg 1</math>.  Figure 1 shows how the fractional core mass, <math>\nu \equiv M_\mathrm{core}/M_\mathrm{tot}</math>, varies with the fractional core radius, <math>q \equiv r_\mathrm{core}/R</math>, along sequences having six different values of <math>\mu_e/\mu_c</math>, as detailed in the figure caption.  The natural expectation is that an increase in <math>\xi_i</math> along a given sequence will correspond to an increase in the relative size &#8212; both the radius and the mass &#8212; of the core. This expectation is realized along the sequences marked by blue diamonds (<math>\mu_e/\mu_c = 1</math>) and by red squares (<math>\mu_e/\mu_c = </math>&frac12;).  But the behavior is different along the other four illustrated sequences.  For sufficiently large <math>\xi_i</math>, the relative radius of the core begins to decrease; then, as <math>\xi_i</math> is pushed to even larger values, eventually the relative core mass begins to decrease.  Additional properties of these equilibrium sequences are discussed in [[SSC/FreeEnergy/PolytropesEmbedded#Behavior_of_Equilibrium_Sequence|an accompanying chapter]].

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[[Image:PlotSequencesBest02.png|500px|center]]
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'''Figure 1:'''  Analytically determined plot of fractional core mass (<math>\nu</math>) versus fractional core radius (<math>q</math>) for <math>(n_c, n_e) = (5, 1)</math> bipolytrope model sequences having six different values of <math>\mu_e/\mu_c</math>: 1 (blue diamonds), &frac12; (red squares), 0.345 (dark purple crosses), &#8531; (pink triangles), 0.309 (light green dashes),  and &frac14; (purple asterisks).  Along each of the model sequences, points marked by solid-colored circles correspond to models whose interface parameter, <math>\xi_i</math>, has one of three values:  0.5 (green circles), 1 (dark blue circles), or 3 (orange circles); the images linked to Table 2 provide plots of the density, pressure and mass profiles for nine of these identified models.
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The variation of <math>\nu</math> with <math>q</math> for a seventh analytically determined model sequence &#8212; one for which <math>\mu_e/\mu_c = 1/5</math> &#8212; is mapped out by a string of blue diamond symbols in the left-hand side of Figure 2. It behaves in an analogous fashion to the <math>\mu_e/\mu_c = </math>&frac14; (purple asterisks) sequence displayed in Figure 1.  It also quantitatively, as well as qualitatively, resembles the sequence that was numerically constructed by {{ SC42full }} for models with an isothermal core (<math>n_c = \infty</math>) and an <math>n_e=3/2</math> envelope; Fig. 1 from their paper has been reproduced here on the right-hand side of Figure 2.

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Figure 2: Relationship to Sch&ouml;nberg-Chandrasekhar Mass Limit
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Analytic BiPolytrope with <math>n_c=5</math>, <math>n_e = 1</math>, and <math>\mu_e/\mu_c = 1/5</math>
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Edited excerpt from [http://adsabs.harvard.edu/abs/1942ApJ....96..161S Sch&ouml;nberg &amp; Chandrasekhar (1942)]
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Figure from [http://adsabs.harvard.edu/abs/1941ApJ....94..525H Henrich &amp; Chandraskhar (1941)]
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[[Image:SC_42Comparison.jpg|400px|center]]
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[[Image:SC42_Fig1.jpg|400px|center]]
<!-- [[Image:AAAwaiting01.png|400px|center]] -->
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[[Image:HenrichChandra41b.jpg|200px|center]]
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(''Above'') Plot of fractional core mass (<math>\nu</math>) versus fractional core radius (<math>q</math>) for the analytic bipolytrope having <math>\mu_e/\mu_c = 1/5</math>.  The behavior of this analytically defined model sequence resembles the behavior of the numerically constructed isothermal core models presented by (''center'') {{ SC42 }} and by (''far right'') {{ HC41full }}.
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