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&nbsp;<br /> &nbsp; <br />
=Bipolytropes=
&nbsp;<br /> &nbsp; <br />
 
&nbsp;<br /> &nbsp; <br />
If we consider only the structure and oscillations of the core, we should set the "external" pressure, <math>P_e</math>, equal to the pressure, <math>P_i</math>, at the core-envelope interface ''as viewed from the perspective of the envelope. 
&nbsp;<br /> &nbsp; <br />
 
==Extra Relations==
Keep in mind that, in hydrostatic balance,
 
<div align="center">
{{Math/EQ_SShydrostaticBalance01}}
</div>
 
Otherwise,
<div align="center">
 
<span id="PGE:Euler"><font color="#770000">'''Euler Equation'''</font></span><br />
('''Momentum Conservation''')
 
{{ Math/EQ_Euler01 }}
</div>
In equilibrium, the pressure at the core-envelope interface is,
<div align="center">
<math>P_i = K_c \rho_c^{6/5}\biggl(1 + \frac{\xi_i^2}{3} \biggr)^{-3}</math>.
</div>
 
 
<table border="0" align="center" cellpadding="8">
<tr>
  <td  align="right"><math>P</math></td>
  <td  align="center"><math>=</math></td>
  <td  align="right">
<math>K_n \rho^{1 + 1/n}</math>
  </td>
</tr>
</table>
 
==Use Surface Area==
 
According to the "piston model", it should be true that,
<table border="0" align="center" cellpadding="8">
<tr>
  <td  align="right"><math>P_e = \frac{G^*}{A}</math></td>
  <td  align="center"><math>=</math></td>
  <td  align="right">
<math>\frac{g_i M^*}{4\pi r_i^2} \, ,</math>
  </td>
</tr>
</table>
 
where (the magnitude of) the acceleration at the interface is,
<table border="0" align="center" cellpadding="8">
<tr>
  <td  align="right"><math>g_i</math></td>
  <td  align="center"><math>=</math></td>
  <td  align="right">
<math>\frac{GM_\mathrm{core}}{r_i^2} \, .</math>
  </td>
</tr>
</table>
 
This means that,
<table border="0" align="center" cellpadding="8">
<tr>
  <td  align="right"><math>M^*</math></td>
  <td  align="center"><math>=</math></td>
  <td  align="right">
<math>
\frac{4\pi r_i^2 P_e}{g_i}
=
\frac{4\pi r_i^4 P_e}{GM_\mathrm{core}}
\, .</math>
  </td>
</tr>
</table>


=See Also=
=See Also=

Revision as of 19:15, 12 March 2026

Piston Model

KW94
Piston Model

Here we draw principally from the discussion of a simple piston model as presented in §2.7 and §6.6 of [KW94].

An ideal gas of mass m* is held in a vertical container with a movable piston resting on top of — and confining — the gas; the mass of the piston is M*. A vertically directed gravitational acceleration, g, acts on the piston, in which case the weight of the piston is given by the expression,

G*=gM*.

"In the case of hydrostatic equilibrium, the gas pressure P adjusts in such a way that the weight per unit area is balanced by the pressure:"

P=G*A.

"If the forces do not compensate each other, the piston is accelerated in the vertical direction according to the equation of motion,"

M*d2hdt2=G*+PA.

Bipolytropes

If we consider only the structure and oscillations of the core, we should set the "external" pressure, Pe, equal to the pressure, Pi, at the core-envelope interface as viewed from the perspective of the envelope.

Extra Relations

Keep in mind that, in hydrostatic balance,

dPdr=GMrρr2

Otherwise,

Euler Equation
(Momentum Conservation)

dvdt=1ρPΦ

In equilibrium, the pressure at the core-envelope interface is,

Pi=Kcρc6/5(1+ξi23)3.


P =

Knρ1+1/n

Use Surface Area

According to the "piston model", it should be true that,

Pe=G*A =

giM*4πri2,

where (the magnitude of) the acceleration at the interface is,

gi =

GMcoreri2.

This means that,

M* =

4πri2Pegi=4πri4PeGMcore.

See Also

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