Difference between revisions of "User:Tohline/SSC/Stability/Isothermal"

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(Begin new chapter on radial oscillations of truncated isothermal spheres)
 
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=Radial Oscillations of Pressure-Truncated Isothermal Spheres=
=Radial Oscillations of Pressure-Truncated Isothermal Spheres=
Here we draw primarily from the following three sources:
* &sect;5.3.8 (p. 372) of Horedt's treatise on ''Polytropes''
* [http://adsabs.harvard.edu/abs/1968MNRAS.140..109Y S. Yabushita (1968, MNRAS, 140, 109)] &#8212; ''Jeans's Type Gravitational Instability of Finite Isothermal Gas Spheres''
* [http://adsabs.harvard.edu/abs/1974MNRAS.168..427T L. G. Taff &amp; H. M. Horn (1974, MNRAS, 168, 427-432)] &#8212; ''Radial Pulsations of Finite Isothermal Gas Spheres''
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Revision as of 20:53, 7 November 2016

Radial Oscillations of Pressure-Truncated Isothermal Spheres

Here we draw primarily from the following three sources:


Whitworth's (1981) Isothermal Free-Energy Surface
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Groundwork

Linearized Wave Equation

In an accompanying discussion, we derived the so-called,

Adiabatic Wave (or Radial Pulsation) Equation

LSU Key.png

<math>~ \frac{d^2x}{dr_0^2} + \biggl[\frac{4}{r_0} - \biggl(\frac{g_0 \rho_0}{P_0}\biggr) \biggr] \frac{dx}{dr_0} + \biggl(\frac{\rho_0}{\gamma_\mathrm{g} P_0} \biggr)\biggl[\omega^2 + (4 - 3\gamma_\mathrm{g})\frac{g_0}{r_0} \biggr] x = 0 </math>


whose solution gives eigenfunctions that describe various radial modes of oscillation in spherically symmetric, self-gravitating fluid configurations.

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