Editing
SSC/Stability/BiPolytropes
(section)
Jump to navigation
Jump to search
Warning:
You are not logged in. Your IP address will be publicly visible if you make any edits. If you
log in
or
create an account
, your edits will be attributed to your username, along with other benefits.
Anti-spam check. Do
not
fill this in!
=Equilibrium Models= The original text contained in this section has been commented out. <!-- The equilibrium sequences displayed in Figure 1 — for pressure-truncated polytropes — and in Figure 2 — for <math>(n_c, n_e) = (5, 1)</math> bipolytropes — were constructed by solving the second-order ODE that governs detailed force-balance throughout spherically symmetric configurations that obey polytropic equations of state. In Figure 1, the sequences labeled <math>n = 1</math> and <math>n = 5</math> can be specified entirely through analytical expressions; these are well-known analytic solutions to the Lane-Emden equation. In Figure 2, ''all seven equilibrium sequences'' are specifiable analytically; the location(s) of ''turning points'' along each sequence (when they exist) are also completely specifiable analytically. In this chapter we examine the relative stability of various equilibrium <math>(n_c, n_e) = (5, 1)</math> bipolytropes. A model is uniquely selected once we specify the radial location, <math>\xi_i</math>, of the core/envelope interface, and specify the ratio <math>\mu_e/\mu_c \le 1</math> of the mean-molecular weights of the gas in the envelope to the gas in the core. Once this pair of parameter values has been specified, the model's radius <math>R_\mathrm{eq}</math> and total mass <math>M_\mathrm{tot}</math> are known analytically, as is the relative size of the core — both in terms of its fractional radius, <math>q \equiv r_i/R_\mathrm{eq}</math>, and its fractional mass, <math>\nu \equiv m_\mathrm{core}/M_\mathrm{tot}</math>. Knowledge of the <math>(q, \nu)</math> parameter pair precisely identifies the selected model's location in the Figure 2 diagram. In line with the '''<font color="red">principal question</font>''' stated above, we are particularly interested in examining the relative stability of models that are associated with the "maximum-mass turning points" along bipolytropic sequences for which <math>\mu_e/\mu_c \le \tfrac{1}{3}</math> — see the solid green circular markers in Figure 2. -->
Summary:
Please note that all contributions to JETohlineWiki may be edited, altered, or removed by other contributors. If you do not want your writing to be edited mercilessly, then do not submit it here.
You are also promising us that you wrote this yourself, or copied it from a public domain or similar free resource (see
JETohlineWiki:Copyrights
for details).
Do not submit copyrighted work without permission!
Cancel
Editing help
(opens in new window)
Navigation menu
Personal tools
Not logged in
Talk
Contributions
Log in
Namespaces
Page
Discussion
English
Views
Read
Edit
View history
More
Search
Navigation
Main page
Tiled Menu
Table of Contents
Old (VisTrails) Cover
Appendices
Variables & Parameters
Key Equations
Special Functions
Permissions
Formats
References
lsuPhys
Ramblings
Uploaded Images
Originals
Recent changes
Random page
Help about MediaWiki
Tools
What links here
Related changes
Special pages
Page information