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Created page with "__FORCETOC__ <!-- __NOTOC__ will force TOC off --> =Interrelating (5, 1) and (0, 0) Bipolytropes= Here we construct a bipolytrope in which both the core and the envelope have uniform densities, that is, the structure of both the core and the envelope will be modeled using an <math>n = 0</math> polytropic index. It should be possible for the entire structure to be described by closed-form, analytic expressions. Generally, we..."
 
 
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=Interrelating (5, 1) and (0, 0) Bipolytropes=
=Interrelating (5, 1) and (0, 0) Bipolytropes=


Here we construct a [[SSC/Structure/BiPolytropes#BiPolytropes|bipolytrope]] in which both the core and the envelope have uniform densities, that is, the structure of both the core and the envelope will be modeled using an <math>n = 0</math> polytropic index. It should be possible for the entire structure to be described by closed-form, analytic expressions.  Generally, we will follow the [[SSC/Structure/BiPolytropes#Solution_Steps|general solution steps for constructing a bipolytrope]] that we have outlined elsewhere.  [On '''<font color="red">1 February 2014</font>''', J. E. Tohline wrote:  This particular system became of interest to me during discussions with Kundan Kadam about the relative stability of bipolytropes.]
==Structure of (n<sub>c</sub>, n<sub>e</sub>) = (0, 0) Bipolytropes==
Here we draw heavily from an [[SSC/Structure/BiPolytropes/Analytic00|accompanying discussion]] to construct a [[SSC/Structure/BiPolytropes#BiPolytropes|bipolytrope]] in which both the core and the envelope have uniform densities, that is, the structure of both the core and the envelope will be modeled using an <math>n = 0</math> polytropic index.


==Structure of (0, 0) Bipolytropes==
Assuming that the central density, <math>\rho_0</math>, and central pressure, <math>P_0</math>, are specified, the natural dimensionless radius is given by the expression,


<table border="0" cellpadding="5" align="center">
<tr>
  <td align="right">
<math>\chi</math>
  </td>
  <td align="center">
<math>\equiv</math>
  </td>
  <td align="left">
<math>
r \biggl[ \frac{G\rho_0^2}{P_0} \biggr]^{1 / 2}
\, .</math>
  </td>
</tr>
</table>
===Throughout the core (0 &le; &chi; &le; &chi;<sub>i</sub>)===
In equilibrium, the radial profile of the density, pressure, and integrated mass are, respectively,
<table border="0" cellpadding="5" align="center">
<tr>
  <td align="right">
<math>\rho</math>
  </td>
  <td align="center">
<math>=</math>
  </td>
  <td align="left">
<math>\rho_0</math>
  </td>
</tr>
<tr>
  <td align="right">
<math>P</math>
  </td>
  <td align="center">
<math>=</math>
  </td>
  <td align="left">
<math>P_0 \biggl( 1 - \frac{2\pi}{3}\chi^2 \biggr)</math>
  </td>
</tr>
<tr>
  <td align="right">
<math>M_r</math>
  </td>
  <td align="center">
<math>=</math>
</td>
  <td align="left">
<math>\frac{4\pi}{3} \biggl[ \frac{P_0^3}{G^3 \rho_0^4} \biggr]^{1/2} \chi^3 \, .</math>
  </td>
</tr>
</table>
===Interface Conditions===
In terms of the (as yet unspecified) total radius, <math>R</math>, we use <math>q</math> to specify the fractional radial location of the core/envelope interface, that is,
<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{r_i}{R}
</math>
  </td>
</tr>
<tr>
  <td align="right">
<math>\Rightarrow ~~~ \chi_i</math>
  </td>
  <td align="center">
<math>\equiv</math>
  </td>
  <td align="left">
<math>
q ~ \biggl[ \frac{G\rho_0^2 R^2}{P_0} \biggr]^{1 / 2} \, .
</math>
  </td>
</tr>
</table>
And whether viewed from the perspective of the core or the envelope, the pressure at the interface is given by the expression,
<table border="0" cellpadding="5" align="center">
<tr>
  <td align="right">
<math>P_i</math>
  </td>
  <td align="center">
<math>=</math>
  </td>
  <td align="left">
<math>P_0 \biggl( 1 - \frac{2\pi}{3}\chi_i^2 \biggr)</math>
  </td>
</tr>
</table>
===Envelope Solution (&chi; &ge; &chi;<sub>i</sub>)===
After specifying the envelope-to-core density ratio, <math>\rho_e/\rho_0</math>, the envelope's equilibrium radial profile of the density, pressure, and integrated mass are, respectively,
<table border="0" cellpadding="3" align="center">
<tr>
  <td align="right">
<math>~\rho</math>
  </td>
  <td align="center">
&nbsp; <math>~=</math>&nbsp;
  </td>
  <td align="left">
<math>~\rho_e</math>
  </td>
</tr>
<tr>
  <td align="right">
<math>~\frac{P}{P_0}</math>
  </td>
  <td align="center">
&nbsp; <math>~=</math>&nbsp;
  </td>
  <td align="left">
<math>1 - \frac{2\pi}{3}\chi_i^2  +
\frac{2\pi}{3} \biggl(\frac{\rho_e}{\rho_0}\biggr) \chi_i^2
\biggl[ 2 \biggl(1 - \frac{\rho_e}{\rho_0} \biggr) \biggl( \frac{\chi_i}{\chi} -
1\biggr) - \frac{\rho_e}{\rho_0} \biggl(\frac{\chi^2}{\chi_i^2} - 1 \biggr) \biggr]</math>
  </td>
</tr>
<tr>
  <td align="right">
<math>M_r</math>
  </td>
  <td align="center">
<math>=</math>
</td>
  <td align="left">
<math>\frac{4\pi}{3} \biggl[ \frac{P_0^3}{G^3 \rho_0^4} \biggr]^{1/2} \chi_i^3\biggl[1 +\frac{\rho_e}{\rho_0}
\biggl( \frac{\chi^3}{\chi_i^3} - 1\biggr) \biggr]</math>
  </td>
</tr>
</table>


=Related Discussions=
=Related Discussions=
* [[SSC/Structure/BiPolytropes/Analytic51#BiPolytrope_with_nc_.3D_5_and_ne_.3D_1|Analytic solution]] with <math>~n_c = 5</math> and <math>~n_e=1</math>.
* [[SSC/Structure/BiPolytropes/Analytic51#BiPolytrope_with_nc_.3D_5_and_ne_.3D_1|Analytic solution]] with <math>(n_c, n_e) = (5,1)</math>.




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Latest revision as of 17:12, 16 October 2022

Interrelating (5, 1) and (0, 0) Bipolytropes

Structure of (nc, ne) = (0, 0) Bipolytropes

Here we draw heavily from an accompanying discussion to construct a bipolytrope in which both the core and the envelope have uniform densities, that is, the structure of both the core and the envelope will be modeled using an n=0 polytropic index.

Assuming that the central density, ρ0, and central pressure, P0, are specified, the natural dimensionless radius is given by the expression,

χ

r[Gρ02P0]1/2.

Throughout the core (0 ≤ χ ≤ χi)

In equilibrium, the radial profile of the density, pressure, and integrated mass are, respectively,

ρ

=

ρ0

P

=

P0(12π3χ2)

Mr

=

4π3[P03G3ρ04]1/2χ3.

Interface Conditions

In terms of the (as yet unspecified) total radius, R, we use q to specify the fractional radial location of the core/envelope interface, that is,

q

riR

χi

q[Gρ02R2P0]1/2.

And whether viewed from the perspective of the core or the envelope, the pressure at the interface is given by the expression,

Pi

=

P0(12π3χi2)

Envelope Solution (χ ≥ χi)

After specifying the envelope-to-core density ratio, ρe/ρ0, the envelope's equilibrium radial profile of the density, pressure, and integrated mass are, respectively,

ρ

  = 

ρe

PP0

  = 

12π3χi2+2π3(ρeρ0)χi2[2(1ρeρ0)(χiχ1)ρeρ0(χ2χi21)]

Mr

=

4π3[P03G3ρ04]1/2χi3[1+ρeρ0(χ3χi31)]

Related Discussions


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