Editing
Apps/ImamuraHadleyCollaboration
(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!
====Tori with Small but Finite β==== Using perturbation theory with <math>~\beta</math> serving effectively as an order parameter, [http://adsabs.harvard.edu/abs/1985MNRAS.216..553B Blaes (1985)] extended his analytic analysis of slender tori to, what he refers to as, "more distorted thick tori." We prefer to describe them as tori with still small, but finite, values of <math>~\beta</math>. Blaes found that, for each ''m'', only the zeroth order co-rotation mode, [[#CorotationMode|described above]], becomes unstable at higher order. To leading order in <math>~\beta</math>, Blaes shows that (see his equations 1.10 and 1.11) the, now complex, eigenfunction is, <div align="center"> <table border="0" cellpadding="5" align="center"> <tr> <td align="right"> <math>~\delta W_{0,0,m}</math> </td> <td align="center"> <math>~\approx</math> </td> <td align="left"> <math>~C ~\exp[i(m\varphi + \sigma_{0,0,m} t)] \biggl\{ 1 + \beta^2 m^2\biggl[ 2\eta^2 \cos^2\theta - \frac{3\eta^2}{4(n+1)} - \frac{(4n+1)}{4(n+1)^2} ~\pm ~4i \biggl( \frac{3}{2n+2} \biggr)^{1/2}\eta\cos\theta \biggr]\biggr\} \, , </math> </td> </tr> </table> </div> and, to leading order in <math>~\beta</math>, the associated ''complex'' eigenfrequency is, <div align="center"> <table border="0" cellpadding="5" align="center"> <tr> <td align="right"> <math>~\sigma_{0,0,m} </math> </td> <td align="center"> <math>~\approx</math> </td> <td align="left"> <math>~-m \Omega_0 - ~i~m\Omega_0 \biggl( \frac{3}{2n+2} \biggr)^{1/2}\beta \, .</math> </td> </tr> </table> </div> In an [[Appendix/Ramblings/PPToriPt2A#Stability_Analyses_of_PP_Tori_.28Part_2.29|accompanying chapter]] that we have relegated to our [[Appendix/Ramblings#Ramblings|Ramblings Appendix]], we demonstrate in detail that this pair of ''complex'' expressions does provide a (leading order) solution to the "thick torus" eigenvalue problem. Notice that if <math>~\beta</math> is set to zero, these two expressions reduce to the (purely real) expressions for the ''j'' = ''k'' = 0, slender torus mode.
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