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> | \biggr]_0^{\xi_i} \biggl\}</math> | ||
</td> | </td> | ||
</tr> | </tr> | ||
<tr> | <tr> | ||
<td align="right"> </td> | <td align="right"> </td> | ||
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<td align="left"> | <td align="left"> | ||
<math>K_c\rho_c^{6/5} \biggl\{1 + \biggl[ | <math>K_c\rho_c^{6/5} \biggl\{1 + \biggl[ | ||
\frac{3^ | \frac{3^3}{(3 + \xi_i^2)^3} - 1 | ||
\biggr] \biggl\}</math> | \biggr] \biggl\}</math> | ||
</td> | </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{ | |||
</td> | </td> | ||
</tr> | </tr> | ||
</table> | |||
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This result should be compared with, | This result should be compared with, | ||
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March 13, 2026: <font color="red">This difference needs to be resolved!!!</font> | March 13, 2026: <font color="red">This difference needs to be resolved!!!</font> | ||
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=See Also= | =See Also= | ||
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Latest revision as of 19:30, 28 March 2026
Piston Model[edit]
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 is held in a vertical container with a movable piston resting on top of — and confining — the gas; the mass of the piston is . A vertically directed gravitational acceleration, , acts on the piston, in which case the weight of the piston is given by the expression,
"In the case of hydrostatic equilibrium, the gas pressure adjusts in such a way that the weight per unit area is balanced by the pressure:"
"If the forces do not compensate each other, the piston is accelerated in the vertical direction according to the equation of motion,"
Bipolytropes[edit]
If we consider only the structure and oscillations of the core, we should set the "external" pressure, , equal to the pressure, , at the core-envelope interface as viewed from the perspective of the envelope.
Extra Relations[edit]
Keep in mind that, in hydrostatic balance,
Otherwise,
In equilibrium, the pressure at the core-envelope interface is,
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Use Surface Area[edit]
According to the "piston model," it should be true that,
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where (the magnitude of) the acceleration at the interface is,
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This means that,
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Insert Interface Details[edit]
Now, according to our analysis of the bipolytrope having we have,
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Hence, we find that,
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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,
where,
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Now, according to our analysis of the bipolytrope having we have throughout the core, and,
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Therefore the RHS of the hydrostatic-balance expression is,
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Integrating the hydrostatic-balance expression from the center, , to a location, , gives,
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See Also[edit]
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Appendices: | VisTrailsEquations | VisTrailsVariables | References | Ramblings | VisTrailsImages | myphys.lsu | ADS | |