SR/Piston: Difference between revisions

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<math>K_c\rho_c^{6/5} \biggl\{1 + 2\cdot 3^4~ \biggl[  
<math>K_c\rho_c^{6/5} \biggl\{1 + 2\cdot 3^4~ \biggl[  
\frac{1}{6(3 + \xi^2)^3}
\frac{1}{6(3 + \xi^2)^3}
\biggr]_0^{\xi_i} \biggl\}</math> &nbsp; DONE
\biggr]_0^{\xi_i} \biggl\}</math>
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   </td>
</tr>
</tr>
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  <td  align="center"><math>=</math></td>
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<math>K_c\rho_c^{6/5} \biggl\{1 - 3^3~ \biggl[
\frac{1}{(3 + \xi_{\xi_i}^2)^3} - \frac{1}{3^3}
\biggr] \biggl\}</math>
  </td>
</tr>
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  <td  align="right">&nbsp;</td>
  <td  align="center"><math>=</math></td>
  <td  align="left">
<math>K_c\rho_c^{6/5} \biggl[ 2 -
~ \biggl(1 + \frac{\xi_i^2}{3} \biggr)^{-3}\biggr]</math>
  </td>
</tr>
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<math>K_c\rho_c^{6/5} \biggl\{1 +  \biggl[  
<math>K_c\rho_c^{6/5} \biggl\{1 +  \biggl[  
\frac{3^2}{(3 + \xi_i^2)^3} - 1
\frac{3^3}{(3 + \xi_i^2)^3} - 1
\biggr] \biggl\}</math>  
\biggr] \biggl\}</math>  
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   </td>
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   <td  align="center"><math>=</math></td>
   <td  align="center"><math>=</math></td>
   <td  align="left">
   <td  align="left">
<math>K_c\rho_c^{6/5} \biggl[
<math>K_c\rho_c^{6/5} \biggl(1 + \frac{\xi_i^2}{3} \biggr)^{-3}</math>  
\frac{3^2}{(3 + \xi_i^2)^3}
\biggr]</math>  
   </td>
   </td>
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<tr>
</table>
  <td  align="right">&nbsp;</td>
  <td  align="center"><math>=</math></td>
  <td  align="left">
<math>K_c\rho_c^{6/5} 
\frac{1}{3}\biggl(1 + \frac{\xi_i^2}{3} \biggr)^{-3}</math>
  </td>
</tr>


</table>
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=See Also=
=See Also=


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Latest revision as of 19:30, 28 March 2026

Piston Model[edit]

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[edit]

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[edit]

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[edit]

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[edit]

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.

Hydrostatic Balance[edit]

Drawing principally from an accompanying discussion, we understand that hydrostatic balance throughout a self-gravitating sphere is given by the key relation,

dPdr=GMrρr2

where,

Mr=0r4πr2ρdr .


Now, according to our analysis of the bipolytrope having (nc,ne)=(5,1), we have throughout the core, θ=(1+ξ2/3)1/2 and,

r =

Kc1/2G1/2ρc2/5(32π)1/2ξ;

ρ =

ρcθ5=ρc[1+ξ23]5/2;

Mr =

Kc3/2G3/2ρc1/5(6π)1/2(ξθ)3=Kc3/2G3/2ρc1/5(6π)1/2ξ3[1+ξ23]3/2.

Therefore the RHS of the hydrostatic-balance expression is,

RHS =

G{Kc3/2G3/2ρc1/5(6π)1/2ξ3[1+ξ23]3/2}{ρc[1+ξ23]5/2}{Kc1/2G1/2ρc2/5(32π)1/2ξ}2

  =

G{Kc3/2G3/2ρc1/5(6π)1/2ξ3[1+ξ23]3/2}{ρc[1+ξ23]5/2}{Gρc4/5Kc(2π3)ξ2}

  =

G1/2Kc1/2ρc8/5(23π22π232)1/2{ξ3[1+ξ23]3/2}{[1+ξ23]5/2}{ξ2}

  =

G1/2Kc1/2ρc8/5(23π3)1/2[1+ξ23]4ξ

Integrating the hydrostatic-balance expression from the center, ξ=0, to a location, ξi, gives,

PcPidP =

0riRHSdr

PiPc =

Kc1/2G1/2ρc2/5(32π)1/20ξiRHSdξ

Pi =

PcKc1/2G1/2ρc2/5(32π)1/20ξiG1/2Kc1/2ρc8/5(23π3)1/2[1+ξ23]4ξdξ

  =

Kcρc6/52Kcρc6/50ξi[1+ξ23]4ξdξ

  =

Kcρc6/5{12340ξi(3+ξ2)4ξdξ}

  =

Kcρc6/5{1+234[16(3+ξ2)3]0ξi}

  =

Kcρc6/5{1+[2346(3+ξi2)32346(3)3]}

  =

Kcρc6/5{1+[33(3+ξi2)31]}

  =

Kcρc6/5(1+ξi23)3


See Also[edit]

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