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=Piston Model= | =Piston Model= | ||
{| class="PGEclass" style="float:left; margin-right: 20px; border-style: solid; border-width: 3px border-color: black" | |||
|- | |||
! style="height: 125px; width: 125px; background-color:white;" | | |||
<font size="-1">[[H_BookTiledMenu#Context|<b>KW94<br />Piston Model</b>]]</font> | |||
|} | |||
Here we draw principally from the discussion of a simple piston model as presented in §2.7 and §6.6 of [<b>[[Appendix/References#KW94|<font color="red">KW94</font>]]</b>]. | |||
= | An ''[[SR#Equation_of_State|ideal gas]]'' of mass <math>m^*</math> is held in a vertical container with a movable piston resting on top of — and confining — the gas; the mass of the piston is <math>M^*</math>. A vertically directed gravitational acceleration, <math>g</math>, acts on the piston, in which case the weight of the piston is given by the expression, | ||
<div align="center"><math>G^* = g M^*.</math></div> | |||
<font color="darkgreen">"In the case of hydrostatic equilibrium, the gas pressure <math>P</math> adjusts in such a way that the weight per unit area is balanced by the pressure:"</font> | |||
<div align="center"><math>P = \frac{G^*}{A}.</math></div> | |||
<font color="darkgreen">"If the forces do not compensate each other, the piston is accelerated in the vertical direction according to the equation of motion," | |||
<div align="center"> | |||
<math>M^*\frac{d^2 h}{dt^2} = -G^* + PA.</math> | |||
</div> | |||
</font> | |||
=Bipolytropes= | |||
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. | |||
==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="left"> | |||
<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="left"> | |||
<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="left"> | |||
<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="left"> | |||
<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> | |||
==Insert Interface Details== | |||
Now, according to [[SSC/Structure/BiPolytropes/Analytic51/Pt2#Examples|our analysis of the bipolytrope having <math>(n_c, n_e) = (5,1),</math>]] we have, | |||
<table border="0" align="center" cellpadding="8"> | |||
<tr> | |||
<td align="right"><math>P_i</math></td> | |||
<td align="center"><math>=</math></td> | |||
<td align="left"> | |||
<math> | |||
K_c \rho_c^{6/5}\biggl(1 + \frac{\xi_i^2}{3} \biggr)^{-3} | |||
\, ;</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"><math>r_i</math></td> | |||
<td align="center"><math>=</math></td> | |||
<td align="left"> | |||
<math> | |||
\frac{K_c^{1 / 2}}{G^{1 / 2}\rho_c^{2 / 5}}\biggl(\frac{3}{2\pi}\biggr)^{1 / 2} ~ \xi_i | |||
\, ;</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"><math>M_\mathrm{core}</math></td> | |||
<td align="center"><math>=</math></td> | |||
<td align="left"> | |||
<math> | |||
\frac{K_c^{3 / 2}}{G^{3 / 2}\rho_c^{1 / 5}}\biggl(\frac{6}{\pi}\biggr)^{1 / 2} ~ (\xi \theta)^3 | |||
\, .</math> | |||
</td> | |||
</tr> | |||
</table> | |||
Hence, we find that, | |||
<table border="0" align="center" cellpadding="8"> | |||
<tr> | |||
<td align="right"><math>M^*</math></td> | |||
<td align="center"><math>=</math></td> | |||
<td align="left"> | |||
<math> | |||
\frac{4\pi }{G} \biggl[ r_i^4 \biggr] | |||
\biggl[P_i\biggr] | |||
\biggl[ M_\mathrm{core} \biggr]^{-1} | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> </td> | |||
<td align="center"><math>=</math></td> | |||
<td align="left"> | |||
<math> | |||
\frac{4\pi }{G} \biggl[ \frac{K_c^{1 / 2}}{G^{1 / 2}\rho_c^{2 / 5}}\biggl(\frac{3}{2\pi}\biggr)^{1 / 2} ~ \xi_i \biggr]^4 | |||
\biggl[ K_c \rho_c^{6/5}\biggl(1 + \frac{\xi_i^2}{3} \biggr)^{-3} \biggr] | |||
\biggl[ \frac{K_c^{3 / 2}}{G^{3 / 2}\rho_c^{1 / 5}}\biggl(\frac{6}{\pi}\biggr)^{1 / 2} ~ (\xi \theta)^3 \biggr]^{-1} | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> </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}}\biggl(\frac{3}{2\pi}\biggr)^{ 2} ~ \xi_i^4 \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] | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> </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"> </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> | |||
</td> | |||
</tr> | |||
</table> | |||
=Hydrostatic Balance= | |||
Drawing principally from [[SSCpt2/SolutionStrategies|an accompanying discussion]], we understand that hydrostatic balance throughout a self-gravitating sphere is given by the key relation, | |||
<div align="center"> | |||
{{Math/EQ_SShydrostaticBalance01}} | |||
</div> | |||
where, | |||
<div align="center"> | |||
<math>~M_r = \int_0^r 4\pi r^2 \rho dr</math> . | |||
</div> | |||
Now, according to [[SSC/Structure/BiPolytropes/Analytic51/Pt2#Examples|our analysis of the bipolytrope having <math>(n_c, n_e) = (5,1),</math>]] we have throughout the core, <math>\theta = (1 + \xi^2/3)^{-1 / 2}</math> and, | |||
<table border="0" align="center" cellpadding="8"> | |||
<tr> | |||
<td align="right"><math>r</math></td> | |||
<td align="center"><math>=</math></td> | |||
<td align="left"> | |||
<math> | |||
\frac{K_c^{1 / 2}}{G^{1 / 2}\rho_c^{2 / 5}}\biggl(\frac{3}{2\pi}\biggr)^{1 / 2} ~ \xi | |||
\, ;</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"><math>\rho</math></td> | |||
<td align="center"><math>=</math></td> | |||
<td align="left"> | |||
<math> | |||
\rho_c \theta^5 = \rho_c \biggl[1 + \frac{\xi^2}{3}\biggr]^{-5/2} | |||
\, ;</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"><math>M_r</math></td> | |||
<td align="center"><math>=</math></td> | |||
<td align="left"> | |||
<math> | |||
\frac{K_c^{3 / 2}}{G^{3 / 2}\rho_c^{1 / 5}}\biggl(\frac{6}{\pi}\biggr)^{1 / 2} ~ (\xi \theta)^3 | |||
= | |||
\frac{K_c^{3 / 2}}{G^{3 / 2}\rho_c^{1 / 5}}\biggl(\frac{6}{\pi}\biggr)^{1 / 2} ~ \xi^3\biggl[1 + \frac{\xi^2}{3}\biggr]^{-3/2} | |||
\, .</math> | |||
</td> | |||
</tr> | |||
</table> | |||
Therefore the RHS of the hydrostatic-balance expression is, | |||
<table border="0" align="center" cellpadding="8"> | |||
<tr> | |||
<td align="right">RHS</td> | |||
<td align="center"><math>=</math></td> | |||
<td align="left"> | |||
<math> | |||
G \biggl\{ \frac{K_c^{3 / 2}}{G^{3 / 2}\rho_c^{1 / 5}}\biggl(\frac{6}{\pi}\biggr)^{1 / 2} ~ \xi^3\biggl[1 + \frac{\xi^2}{3}\biggr]^{-3/2} \biggr\} | |||
\biggl\{ \rho_c \biggl[1 + \frac{\xi^2}{3}\biggr]^{-5/2} \biggr\} | |||
\biggl\{ \frac{K_c^{1 / 2}}{G^{1 / 2}\rho_c^{2 / 5}}\biggl(\frac{3}{2\pi}\biggr)^{1 / 2} ~ \xi \biggr\}^{-2} | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> </td> | |||
<td align="center"><math>=</math></td> | |||
<td align="left"> | |||
<math> | |||
G \biggl\{ \frac{K_c^{3 / 2}}{G^{3 / 2}\rho_c^{1 / 5}}\biggl(\frac{6}{\pi}\biggr)^{1 / 2} ~ \xi^3\biggl[1 + \frac{\xi^2}{3}\biggr]^{-3/2} \biggr\} | |||
\biggl\{ \rho_c \biggl[1 + \frac{\xi^2}{3}\biggr]^{-5/2} \biggr\} | |||
\biggl\{ \frac{G\rho_c^{4 / 5}}{K_c}\biggl(\frac{2\pi}{3}\biggr) ~ \xi^{-2} \biggr\} | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> </td> | |||
<td align="center"><math>=</math></td> | |||
<td align="left"> | |||
<math> | |||
G^{1 / 2} K_c^{1 / 2} \rho_c^{8/5} \biggl(\frac{2\cdot 3}{\pi} \cdot \frac{2^2 \pi^2}{3^2}\biggr)^{1 / 2} | |||
\biggl\{ ~ \xi^3\biggl[1 + \frac{\xi^2}{3}\biggr]^{-3/2} \biggr\} | |||
\biggl\{ \biggl[1 + \frac{\xi^2}{3}\biggr]^{-5/2} \biggr\} | |||
\biggl\{ \xi^{-2} \biggr\} | |||
</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> </td> | |||
<td align="center"><math>=</math></td> | |||
<td align="left"> | |||
<math> | |||
G^{1 / 2} K_c^{1 / 2} \rho_c^{8/5} \biggl(\frac{2^3\pi}{3}\biggr)^{1 / 2} | |||
\biggl[1 + \frac{\xi^2}{3}\biggr]^{-4} ~\xi | |||
</math> | |||
</td> | |||
</tr> | |||
</table> | |||
Integrating the hydrostatic-balance expression from the center, <math>\xi=0</math>, to a location, <math>\xi_i</math>, gives, | |||
<table border="0" align="center" cellpadding="8"> | |||
<tr> | |||
<td align="right"><math>\int_{P_c}^{P_i} dP</math></td> | |||
<td align="center"><math>=</math></td> | |||
<td align="left"> | |||
<math>-~\int_0^{r_i} \mathrm{RHS} \cdot dr</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"><math>\Rightarrow ~~~ P_i - P_c</math></td> | |||
<td align="center"><math>=</math></td> | |||
<td align="left"> | |||
<math>-~\frac{K_c^{1 / 2}}{G^{1 / 2}\rho_c^{2 / 5}}\biggl(\frac{3}{2\pi}\biggr)^{1 / 2} ~ \int_0^{\xi_i} \mathrm{RHS} \cdot d\xi</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"><math>\Rightarrow ~~~ P_i </math></td> | |||
<td align="center"><math>=</math></td> | |||
<td align="left"> | |||
<math>P_c - \frac{K_c^{1 / 2}}{G^{1 / 2}\rho_c^{2 / 5}}\biggl(\frac{3}{2\pi}\biggr)^{1 / 2} ~ \int_0^{\xi_i} | |||
G^{1 / 2} K_c^{1 / 2} \rho_c^{8/5} \biggl(\frac{2^3\pi}{3}\biggr)^{1 / 2} | |||
\biggl[1 + \frac{\xi^2}{3}\biggr]^{-4} ~\xi | |||
\cdot d\xi</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> </td> | |||
<td align="center"><math>=</math></td> | |||
<td align="left"> | |||
<math>K_c\rho_c^{6/5} - 2K_c\rho_c^{6/5}~ \int_0^{\xi_i} | |||
\biggl[1 + \frac{\xi^2}{3}\biggr]^{-4} ~\xi | |||
\cdot d\xi</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> </td> | |||
<td align="center"><math>=</math></td> | |||
<td align="left"> | |||
<math>K_c\rho_c^{6/5} \biggl\{1 - 2\cdot 3^4~ \int_0^{\xi_i} | |||
(3+\xi^2)^{-4} \xi\cdot d\xi\biggr\}</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> </td> | |||
<td align="center"><math>=</math></td> | |||
<td align="left"> | |||
<math>K_c\rho_c^{6/5} \biggl\{1 + 2\cdot 3^4~ \biggl[ | |||
\frac{1}{6(3 + \xi^2)^3} | |||
\biggr]_0^{\xi_i} \biggl\}</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> </td> | |||
<td align="center"><math>=</math></td> | |||
<td align="left"> | |||
<math>K_c\rho_c^{6/5} \biggl\{1 + \biggl[ | |||
\frac{2\cdot 3^4~}{6(3 + \xi_i^2)^3} - \frac{2\cdot 3^4~}{6(3 )^3} | |||
\biggr] \biggl\}</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> </td> | |||
<td align="center"><math>=</math></td> | |||
<td align="left"> | |||
<math>K_c\rho_c^{6/5} \biggl\{1 + \biggl[ | |||
\frac{3^3}{(3 + \xi_i^2)^3} - 1 | |||
\biggr] \biggl\}</math> | |||
</td> | |||
</tr> | |||
<tr> | |||
<td align="right"> </td> | |||
<td align="center"><math>=</math></td> | |||
<td align="left"> | |||
<math>K_c\rho_c^{6/5} \biggl(1 + \frac{\xi_i^2}{3} \biggr)^{-3}</math> | |||
</td> | |||
</tr> | |||
</table> | |||
<!-- | |||
This result should be compared with, | |||
<table border="0" align="center" cellpadding="8"> | |||
<tr> | |||
<td align="right"><math>P</math></td> | |||
<td align="center"><math>=</math></td> | |||
<td align="left"> | |||
<math> | |||
K_c \rho_c^{6/5}\biggl(1 + \frac{\xi^2}{3} \biggr)^{-3} | |||
\, ;</math> | |||
</td> | |||
</tr> | |||
</table> | |||
March 13, 2026: <font color="red">This difference needs to be resolved!!!</font> | |||
--> | |||
=See Also= | |||
{{ SGFfooter }} | {{ SGFfooter }} | ||
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,
.
|
|
Use Surface Area[edit]
According to the "piston model," it should be true that,
|
|
where (the magnitude of) the acceleration at the interface is,
|
|
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,
.
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,
| RHS |
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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 | |