Difference between revisions of "User:Tohline/SSC/Stability/InstabilityOnsetOverview"
(Begin new overview chapter) |
|||
Line 42: | Line 42: | ||
</div> | </div> | ||
Yabushita ([http://adsabs.harvard.edu/abs/1974MNRAS.167…95Y 1974], [http://adsabs.harvard.edu/abs/1975MNRAS.172..441Y 1975]) showed that one valid | Yabushita ([http://adsabs.harvard.edu/abs/1974MNRAS.167…95Y 1974], [http://adsabs.harvard.edu/abs/1975MNRAS.172..441Y 1975]) showed that one valid, | ||
<div align="center"> | <div align="center"> | ||
<table border="0" cellpadding="5" align="center"> | <table border="0" cellpadding="5" align="center"> | ||
<tr> | |||
<td align="center" colspan="3"><font color="maroon"><b>Precise Solution to the Isothermal LAWE</b></font></td> | |||
</tr> | |||
<tr> | <tr> | ||
<td align="right"> | <td align="right"> | ||
<math>~ | <math>~\sigma_c^2 = 0</math> | ||
</td> | </td> | ||
<td align="center"> | <td align="center"> | ||
and | |||
</td> | </td> | ||
<td align="left"> | <td align="left"> | ||
<math>~1 - \biggl( \frac{1}{\xi e^{-\psi}}\biggr) \frac{d\psi}{d\xi} \, .</math> | <math>~x = 1 - \biggl( \frac{1}{\xi e^{-\psi}}\biggr) \frac{d\psi}{d\xi} \, .</math> | ||
</td> | </td> | ||
</tr> | </tr> | ||
Line 77: | Line 79: | ||
</div> | </div> | ||
the relevant configuration is precisely defined by the surface condition, xxx, which is identical to the configuration at the turning point. | the relevant configuration is precisely defined by the surface condition, xxx, which is identical to the configuration at the turning point. | ||
==Polytropic== | ==Polytropic== |
Revision as of 16:24, 19 March 2017
Overview: Marginally Unstable Pressure-Truncated Configurations
Additional details may be found here.
| Tiled Menu | Tables of Content | Banner Video | Tohline Home Page | |
Isothermal
The internal structure of a detailed force-balance model is provided via the function, <math>~\psi(\xi)</math>, which is a solution to the,
Isothermal Lane-Emden Equation
|
Equilibrium sequence for pressure-truncated configurations is displayed in three ways.
Figure 1: Bonnor's P-V Diagram |
|
This equation — in the following, slightly rewritten form — can be found among our selected set of key equations associated with the study of radial pulsation, and will henceforth be referred to as the,
Isothermal LAWE
<math>~0 = \frac{d^2x}{d\xi^2} + \biggl[4 - \xi \biggl( \frac{d\psi}{d\xi} \biggr) \biggr] \frac{1}{\xi} \cdot \frac{dx}{d\xi} + \biggl[ \biggl( \frac{\sigma_c^2}{6\gamma_\mathrm{g}}\biggr)\xi^2 - \alpha \xi \biggl( \frac{d\psi}{d\xi} \biggr) \biggr] \frac{x}{\xi^2} </math> |
|
where: <math>~\sigma_c^2 \equiv \frac{3\omega^2}{2\pi G\rho_c}</math> and, <math>~\alpha \equiv \biggl(3 - \frac{4}{\gamma_\mathrm{g}}\biggr)</math> |
Yabushita (1974, 1975) showed that one valid,
Precise Solution to the Isothermal LAWE | ||
<math>~\sigma_c^2 = 0</math> |
and |
<math>~x = 1 - \biggl( \frac{1}{\xi e^{-\psi}}\biggr) \frac{d\psi}{d\xi} \, .</math> |
When viewed in concert with the surface boundary condition,
<math>~\frac{d\ln x}{d\ln\xi}</math> |
<math>~=</math> |
<math>~- 3 \, ,</math> |
the relevant configuration is precisely defined by the surface condition, xxx, which is identical to the configuration at the turning point.
Polytropic
References
© 2014 - 2021 by Joel E. Tohline |