SR/Piston: Difference between revisions

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\biggl[ K_c \rho_c^{6/5}\biggl(1 + \frac{\xi_i^2}{3} \biggr)^{-3} \biggr]
\biggl[ K_c \rho_c^{6/5}\biggl(1 + \frac{\xi_i^2}{3} \biggr)^{-3} \biggr]
\biggl[ \frac{G^{3 / 2}\rho_c^{1 / 5}}{K_c^{3 / 2}}\biggl(\frac{\pi}{6}\biggr)^{1 / 2} ~ (\xi \theta)^{-3} \biggr]
\biggl[ \frac{G^{3 / 2}\rho_c^{1 / 5}}{K_c^{3 / 2}}\biggl(\frac{\pi}{6}\biggr)^{1 / 2} ~ (\xi \theta)^{-3} \biggr]
</math>
  </td>
</tr>
<tr>
  <td  align="right">&nbsp;</td>
  <td  align="center"><math>=</math></td>
  <td  align="left">
<math>
\frac{4\pi }{G} \biggl[ \frac{K_c^{ 2}}{G^{ 2}\rho_c^{8 / 5}}\biggr]
\biggl[ K_c \rho_c^{6/5}\biggr]
\biggl[ \frac{G^{3 / 2}\rho_c^{1 / 5}}{K_c^{3 / 2}}\biggr]
\biggl(\frac{3}{2\pi}\biggr)^{ 2} ~ \xi_i^4 \biggl(1 + \frac{\xi_i^2}{3} \biggr)^{-3} \biggl(\frac{\pi}{6}\biggr)^{1 / 2} ~ (\xi \theta)^{-3}
</math>
  </td>
</tr>
<tr>
  <td  align="right">&nbsp;</td>
  <td  align="center"><math>=</math></td>
  <td  align="left">
<math>
4\pi\biggl[ \frac{K_c^{ 3 / 2}}{G^{ 3 / 2}\rho_c^{1 / 5}}\biggr]
\biggl(\frac{3^3}{2^5\pi^3}\biggr)^{1 / 2} ~ \biggl(1 + \frac{\xi_i^2}{3} \biggr)^{-3}  ~ \xi \theta^{-3}
\, .
</math>
</math>
   </td>
   </td>

Revision as of 19:59, 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.

Insert Interface Details

Now, according to our analysis of the bipolytrope having (nc,ne)=(5,1), we have,

Pi =

Kcρc6/5(1+ξi23)3;

ri =

Kc1/2G1/2ρc2/5(32π)1/2ξi;

Mcore =

Kc3/2G3/2ρc1/5(6π)1/2(ξθ)3.

Hence, we find that,

M* =

4πG[ri4][Pi][Mcore]1

  =

4πG[Kc1/2G1/2ρc2/5(32π)1/2ξi]4[Kcρc6/5(1+ξi23)3][Kc3/2G3/2ρc1/5(6π)1/2(ξθ)3]1

  =

4πG[Kc2G2ρc8/5(32π)2ξi4][Kcρc6/5(1+ξi23)3][G3/2ρc1/5Kc3/2(π6)1/2(ξθ)3]

  =

4πG[Kc2G2ρc8/5][Kcρc6/5][G3/2ρc1/5Kc3/2](32π)2ξi4(1+ξi23)3(π6)1/2(ξθ)3

  =

4π[Kc3/2G3/2ρc1/5](3325π3)1/2(1+ξi23)3ξθ3.

See Also

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