Editing
ParabolicDensity/Axisymmetric/Structure/Try1thru7
(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!
====Vertical Component==== We will focus, first, on the vertical component. Specifically, since both <math>\rho</math> and <math>\Phi_\mathrm{grav}</math> are known, the vertical gradient of the (unknown) scalar pressure is <table border="0" align="center" cellpadding="8"> <tr> <td align="right"><math>\frac{\partial P}{\partial z}</math></td> <td align="center"><math>=</math></td> <td align="left"> <math> - \rho ~ \frac{\partial}{\partial z} \biggl\{ \Phi_\mathrm{grav} \biggr\} </math> </td> </tr> </table> Multiply thru by <math>1/(\pi G \rho_c^2 a_\ell)</math>: <table border="0" align="center" cellpadding="8"> <tr> <td align="right"><math>\Rightarrow ~~~ \frac{1}{(\pi G\rho_c^2 a_\ell)} \cdot \frac{\partial P}{\partial z}</math></td> <td align="center"><math>=</math></td> <td align="left"> <math> \frac{\rho}{\rho_c} \cdot \frac{\partial}{\partial z} \biggl\{ \frac{\Phi_\mathrm{grav}}{(-\pi G\rho_c a_\ell)} \biggr\} </math> </td> </tr> <tr> <td align="right"><math>\Rightarrow ~~~ \frac{1}{(\pi G\rho_c^2 a_\ell^2)} \cdot \frac{\partial P}{\partial \zeta}</math></td> <td align="center"><math>=</math></td> <td align="left"> <math> \frac{\rho}{\rho_c} \cdot \frac{\partial}{\partial \zeta} \biggl\{ \frac{\Phi_\mathrm{grav}}{(-\pi G\rho_c a_\ell^2)} \biggr\} </math> </td> </tr> <tr> <td align="right"> </td> <td align="center"><math>=</math></td> <td align="left"> <math> \biggl[ 1 - \biggl( \frac{\varpi^2}{a_\ell^2} + \frac{z^2}{a_s^2}\biggr) \biggr] \cdot \frac{\partial}{\partial \zeta} \biggl\{ \frac{1}{2} I_\mathrm{BT} - \biggl[A_\ell \biggl(\frac{\varpi^2}{a_\ell^2}\biggr) + A_s \biggl( \frac{z^2}{a_\ell^2}\biggr) \biggr] + \frac{1}{2} \biggl[ A_{\ell \ell} a_\ell^2 \biggl(\frac{\varpi^4}{a_\ell^4}\biggr) + A_{ss} a_\ell^2 \biggl(\frac{z^4}{a_\ell^4}\biggr) + 2A_{\ell s}a_\ell^2 \biggl( \frac{\varpi^2 z^2}{a_\ell^4}\biggr) \biggr] \biggr\} </math> </td> </tr> <tr> <td align="right"> </td> <td align="center"><math>=</math></td> <td align="left"> <math> \biggl\{ 1 - \biggl[ \chi^2 + \zeta^2(1-e^2)^{-1}\biggr] \biggr\} \cdot \frac{\partial}{\partial \zeta} \biggl\{ \frac{1}{2} I_\mathrm{BT} - \biggl[A_\ell \chi^2 + A_s \zeta^2 \biggr] + \frac{1}{2} \biggl[ A_{\ell \ell} a_\ell^2 \chi^4 + A_{ss} a_\ell^2 \zeta^4 + 2A_{\ell s}a_\ell^2 \chi^2\zeta^2 \biggr] \biggr\} </math> </td> </tr> <tr> <td align="right"> </td> <td align="center"><math>=</math></td> <td align="left"> <math> \biggl\{ 1 - \biggl[ \chi^2 + \zeta^2(1-e^2)^{-1}\biggr] \biggr\} \cdot \biggl\{ - 2A_s \zeta + \biggl[ 2A_{ss} a_\ell^2 \zeta^3 + 2A_{\ell s}a_\ell^2 \chi^2\zeta \biggr] \biggr\} </math> </td> </tr> <tr> <td align="right"> </td> <td align="center"><math>=</math></td> <td align="left"> <math> 2\biggl\{ 1 - \biggl[ \chi^2 + \zeta^2(1-e^2)^{-1}\biggr] \biggr\} \cdot \biggl[ A_{\ell s}a_\ell^2 \chi^2\zeta - A_s \zeta + A_{ss} a_\ell^2 \zeta^3 \biggr] </math> </td> </tr> <tr> <td align="right"> </td> <td align="center"><math>=</math></td> <td align="left"> <math> 2\biggl\{ 1 - \biggl[ \chi^2 + \zeta^2(1-e^2)^{-1}\biggr] \biggr\} \cdot \biggl[ A_{\ell s}a_\ell^2 \chi^2\zeta - A_s \zeta + A_{ss} a_\ell^2 \zeta^3 \biggr] </math> </td> </tr> </table> where (unlike above) we are using the dimensionless lengths, <math>\chi \equiv \varpi/a_\ell</math> and <math>\zeta \equiv z/a_\ell</math>. Continuing to streamline this function, we have, <table border="0" align="center" cellpadding="8"> <tr> <td align="right"><math>\frac{1}{(2\pi G\rho_c^2 a_\ell^2)} \cdot \frac{\partial P}{\partial \zeta}</math></td> <td align="center"><math>=</math></td> <td align="left"> <math> \biggl[ A_{\ell s}a_\ell^2 \chi^2\zeta - A_s \zeta + A_{ss} a_\ell^2 \zeta^3 \biggr] - \chi^2\biggl[ A_{\ell s}a_\ell^2 \chi^2\zeta - A_s \zeta + A_{ss} a_\ell^2 \zeta^3 \biggr] - \zeta^2\biggl[ A_{\ell s}a_\ell^2 \chi^2\zeta - A_s \zeta + A_{ss} a_\ell^2 \zeta^3 \biggr](1-e^2)^{-1} </math> </td> </tr> <tr> <td align="right"> </td> <td align="center"><math>=</math></td> <td align="left"> <math> \biggl[ A_{\ell s}a_\ell^2 \chi^2\zeta - A_s \zeta + A_{ss} a_\ell^2 \zeta^3 \biggr] - \biggl[ A_{\ell s}a_\ell^2 \chi^4 \zeta - A_s \chi^2 \zeta + A_{ss} a_\ell^2 \chi^2 \zeta^3 \biggr] - \biggl[ A_{\ell s}a_\ell^2 \chi^2\zeta^3 - A_s \zeta^3 + A_{ss} a_\ell^2 \zeta^5 \biggr](1-e^2)^{-1} </math> </td> </tr> <tr> <td align="right"> </td> <td align="center"><math>=</math></td> <td align="left"> <math> \biggl[ A_{\ell s}a_\ell^2 \chi^2 - A_s \biggr]\zeta + A_{ss} a_\ell^2 \zeta^3 + \biggl[ A_s \chi^2 - A_{\ell s}a_\ell^2 \chi^4 \biggr]\zeta - A_{ss} a_\ell^2 \chi^2 \zeta^3 + \biggl[ A_s \zeta^3 - A_{\ell s}a_\ell^2 \chi^2\zeta^3 - A_{ss} a_\ell^2 \zeta^5 \biggr](1-e^2)^{-1} </math> </td> </tr> <tr> <td align="right"> </td> <td align="center"><math>=</math></td> <td align="left"> <math> \biggl[ A_{\ell s}a_\ell^2 \chi^2 - A_s + A_s \chi^2 - A_{\ell s}a_\ell^2 \chi^4 \biggr]\zeta + \biggl[ A_{ss} a_\ell^2 - A_{ss} a_\ell^2 \chi^2 + A_s(1-e^2)^{-1} - A_{\ell s}a_\ell^2 \chi^2(1-e^2)^{-1} \biggr]\zeta^3 - A_{ss} a_\ell^2(1-e^2)^{-1} \zeta^5 </math> </td> </tr> <tr> <td align="right"> </td> <td align="center"><math>=</math></td> <td align="left"> <math> \biggl[ - A_s + (A_{\ell s}a_\ell^2 + A_s )\chi^2 - A_{\ell s}a_\ell^2 \chi^4 \biggr]\zeta + \biggl\{ [A_s(1-e^2)^{-1} + A_{ss} a_\ell^2] - [A_{ss} a_\ell^2 + A_{\ell s}a_\ell^2 (1-e^2)^{-1}]\chi^2 \biggr\}\zeta^3 - A_{ss} a_\ell^2(1-e^2)^{-1} \zeta^5 \, . </math> </td> </tr> </table> So, let's see what happens if we assume that the pressure has the form, <table border="0" align="center" cellpadding="8"> <tr> <td align="right"><math>\frac{P_\mathrm{vert}}{(2\pi G\rho_c^2 a_\ell^2)} </math></td> <td align="center"><math>=</math></td> <td align="left"> <math>p_0 + p_2 \zeta^2 + p_4\zeta^4 + p_6\zeta^6 </math> </td> </tr> <tr> <td align="right"><math>\Rightarrow ~~~ \frac{1}{(2\pi G\rho_c^2 a_\ell^2)} \cdot \frac{\partial P_\mathrm{vert}}{\partial \zeta}</math></td> <td align="center"><math>=</math></td> <td align="left"> <math>2p_2 \zeta + 4p_4\zeta^3 + 6p_6\zeta^5 \, ,</math> </td> </tr> </table> in which case, <table border="0" align="center" cellpadding="8"> <tr> <td align="right"><math>\frac{P_\mathrm{vert}}{(2\pi G\rho_c^2 a_\ell^2)} </math></td> <td align="center"><math>=</math></td> <td align="left"> <math> p_0 + \frac{1}{2}\biggl[ - A_s + (A_{\ell s}a_\ell^2 + A_s )\chi^2 - A_{\ell s}a_\ell^2 \chi^4 \biggr] \zeta^2 + \frac{1}{4}\biggl\{[A_s (1-e^2)^{-1} + A_{ss} a_\ell^2] - [A_{ss} a_\ell^2 + A_{\ell s}a_\ell^2 (1-e^2)^{-1} ]\chi^2 \biggr\}\zeta^4 + \frac{1}{6}\biggl[ - A_{ss} a_\ell^2 (1-e^2)^{-1} \biggr]\zeta^6 \, . </math> </td> </tr> </table> <table border="1" align="center" width="80%" cellpadding="8"><tr><td align="left"> <font color="red">REMINDER:</font> From [[#2nd_Try|above]] … <table border="0" cellpadding="5" align="center"> <tr> <td align="right"> <math>\frac{\rho}{\rho_c}</math> </td> <td align="center"> <math>=</math> </td> <td align="left"> <math> 1 - \chi^2 - \zeta^2(1-e^2)^{-1} \, . </math> </td> </tr> </table> And, in the case of the spherically symmetric equilibrium configuration, the [[SSC/Structure/OtherAnalyticModels#Pressure|pressure distribution]] derived by {{ Prasad49 }} has the form, <table border="0" cellpadding="5" align="center"> <tr> <td align="right"> <math>\frac{P}{P_c}</math> </td> <td align="center"> <math>\sim</math> </td> <td align="left"> <math> \biggl(\frac{\rho}{\rho_c}\biggr)^2 \biggl[1 + \biggl(\frac{\rho}{\rho_c}\biggr)\biggr] \, . </math> </td> </tr> </table> In the context of rotationally flattened configurations, therefore, we might expect the (vertical) pressure distribution to be of the form, <table border="0" cellpadding="5" align="center"> <tr> <td align="right"> <math>\frac{P}{P_c}</math> </td> <td align="center"> <math>\sim</math> </td> <td align="left"> <math> \biggl[1 - \chi^2 - \zeta^2(1-e^2)^{-1}\biggr] \biggl[1 - \chi^2 - \zeta^2(1-e^2)^{-1}\biggr] \biggl[2 - \chi^2 - \zeta^2(1-e^2)^{-1}\biggr] </math> </td> </tr> <tr> <td align="right"> </td> <td align="center"> <math>\sim</math> </td> <td align="left"> <math> \biggl[2 - \chi^2 - \zeta^2(1-e^2)^{-1}\biggr] \biggl\{ \biggl[1 - \chi^2 - \zeta^2(1-e^2)^{-1}\biggr] -\chi^2\biggl[1 - \chi^2 - \zeta^2(1-e^2)^{-1}\biggr] - \zeta^2(1-e^2)^{-1}\biggl[1 - \chi^2 - \zeta^2(1-e^2)^{-1}\biggr] \biggr\} </math> </td> </tr> <tr> <td align="right"> </td> <td align="center"> <math>\sim</math> </td> <td align="left"> <math> \biggl[2 - \chi^2 - \zeta^2(1-e^2)^{-1}\biggr] \biggl\{ \biggl[1 - \chi^2 - \zeta^2(1-e^2)^{-1}\biggr] + \biggl[-\chi^2 + \chi^4 + \chi^2\zeta^2(1-e^2)^{-1}\biggr] + \biggl[- \zeta^2(1-e^2)^{-1} + \chi^2\zeta^2(1-e^2)^{-1} + \zeta^4(1-e^2)^{-2}\biggr] \biggr\} </math> </td> </tr> </table> </td></tr></table>
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