SR/Piston

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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.

Hydrostatic Balance

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}   DONE

  =

Kcρc6/5{1+[2346(3+ξi2)32346(3)3]}

  =

Kcρc6/5{1+[32(3+ξi2)31]}

  =

Kcρc6/5[32(3+ξi2)3]

  =

Kcρc6/513(1+ξi23)3

This result should be compared with,

P =

Kcρc6/5(1+ξ23)3;

March 13, 2026:  This difference needs to be resolved!!!

See Also

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