Difference between revisions of "User:Tohline/SSC/Structure/Polytropes/VirialSummary"

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<math>~\frac{1}{x^3} \biggl[ \biggl( \frac{3b}{n} \biggr)\biggl(\frac{n+3}{n}\biggr) x^{(n-3)/n} + 6c x^4 - 2a  \biggr] \, .</math>
<math>~\frac{1}{x^3} \biggl[\biggl(\frac{n+3}{n}\biggr) \biggl( \frac{3b}{n} \biggr) x^{(n-3)/n} + 6c x^4 - 2a  \biggr]  \, .</math>
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Virial equilibrium is obtained when <math>~d\mathfrak{G}^*/dx = 0</math>, that is, when
 
<table border="0" cellpadding="5" align="center">
 
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<math>~0</math>
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<math>~=</math>
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<math>~a  - \biggl( \frac{3b}{n} \biggr) x^{(n-3)/n} + 3c x^4</math>
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<tr>
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<math>~\Rightarrow ~~~ \biggl( \frac{3b}{n} \biggr) x_\mathrm{eq}^{(n-3)/n} </math>
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<math>~=</math>
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<math>~ a  + 3c x_\mathrm{eq}^4 \, .</math>
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And along an equilibrium ''sequence'', the ''specific'' equilibrium state &#8212; henceforth labeled as having the ''critical'' radius, <math>~x_\mathrm{crit}</math> &#8212; that marks a transition from dynamically stable to dynamically unstable configurations is identified by setting  <math>~d^2\mathfrak{G}^*/dx^2 = 0</math>, that is, it is the configuration for which,
<table border="0" cellpadding="5" align="center">
 
<tr>
  <td align="right">
<math>~0</math>
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  <td align="center">
<math>~=</math>
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<math>~\biggl[\biggl(\frac{n+3}{n}\biggr) \biggl( \frac{3b}{n} \biggr) x^{(n-3)/n} + 6c x^4 - 2a  \biggr]_{x = x_\mathrm{eq}}</math>
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<math>~\Rightarrow ~~~
x_\mathrm{crit}^4
</math>
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<math>~=</math>
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<math>~
\frac{a}{3^2c}\biggl(\frac{n - 3}{n+1}\biggr) \, .
</math>
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Revision as of 21:02, 7 February 2019

Virial Equilibrium of Pressure-Truncated Polytropes

Here we will draw heavily from an accompanying Free Energy Synopsis.


Whitworth's (1981) Isothermal Free-Energy Surface
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In the context of spherically symmetric, pressure-truncated polytropic configurations, the relevant free-energy expression is,

<math>~\mathfrak{G}</math>

<math>~=</math>

<math>~W_\mathrm{grav} + U_\mathrm{int} + P_e V \, .</math>

When rewritten in a suitably dimensionless form — see two useful alternatives, below — this expression becomes,

<math>~\mathfrak{G}^*</math>

<math>~=</math>

<math>~- a x^{-1} + bx^{-3/n} + c x^3 \, ,</math>

where <math>~x</math> is the configuration's dimensionless radius and <math>~a</math>, <math>~b</math>, and <math>~c</math> are constants. We therefore have,

<math>~\frac{d\mathfrak{G}^*}{dx}</math>

<math>~=</math>

<math>~\frac{1}{x^2} \biggl[ a - \biggl( \frac{3b}{n} \biggr) x^{(n-3)/n} + 3c x^4 \biggr] \, ,</math>

and,

<math>~\frac{d^2\mathfrak{G}^*}{dx^2}</math>

<math>~=</math>

<math>~\frac{1}{x^3} \biggl[\biggl(\frac{n+3}{n}\biggr) \biggl( \frac{3b}{n} \biggr) x^{(n-3)/n} + 6c x^4 - 2a \biggr] \, .</math>

Virial equilibrium is obtained when <math>~d\mathfrak{G}^*/dx = 0</math>, that is, when

<math>~0</math>

<math>~=</math>

<math>~a - \biggl( \frac{3b}{n} \biggr) x^{(n-3)/n} + 3c x^4</math>

<math>~\Rightarrow ~~~ \biggl( \frac{3b}{n} \biggr) x_\mathrm{eq}^{(n-3)/n} </math>

<math>~=</math>

<math>~ a + 3c x_\mathrm{eq}^4 \, .</math>

And along an equilibrium sequence, the specific equilibrium state — henceforth labeled as having the critical radius, <math>~x_\mathrm{crit}</math> — that marks a transition from dynamically stable to dynamically unstable configurations is identified by setting <math>~d^2\mathfrak{G}^*/dx^2 = 0</math>, that is, it is the configuration for which,

<math>~0</math>

<math>~=</math>

<math>~\biggl[\biggl(\frac{n+3}{n}\biggr) \biggl( \frac{3b}{n} \biggr) x^{(n-3)/n} + 6c x^4 - 2a \biggr]_{x = x_\mathrm{eq}}</math>

<math>~\Rightarrow ~~~ x_\mathrm{crit}^4 </math>

<math>~=</math>

<math>~ \frac{a}{3^2c}\biggl(\frac{n - 3}{n+1}\biggr) \, . </math>

See Also


Whitworth's (1981) Isothermal Free-Energy Surface

© 2014 - 2021 by Joel E. Tohline
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Recommended citation:   Tohline, Joel E. (2021), The Structure, Stability, & Dynamics of Self-Gravitating Fluids, a (MediaWiki-based) Vistrails.org publication, https://www.vistrails.org/index.php/User:Tohline/citation