Editing
SSC/Stability/BiPolytropes/RedGiantToPN/Pt4
(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!
===Steps=== <table border="1" align="center" width="80%" cellpadding="8"><tr><td align="left"> <font color="maroon">STEP 1:</font> Specify the interface location from the perspective of the core; that is, specify <math>\xi_\mathrm{int}</math>, in which case, <table border="0" align="center" cellpadding="8"> <tr> <td align="right"> <math>(r_0)_\mathrm{int} = a_5\cdot \xi_\mathrm{int}</math> </td> <td align="center">=</td> <td align="left"> <math> \biggl[ K_5 G^{-1}\rho_c^{-4/5} \biggr]^{1 / 2}\biggl(\frac{3}{2\pi}\biggr)^{1 / 2} \xi_\mathrm{int} \, . </math> </td> </tr> </table> <font color="maroon">STEP 2:</font> Adopting the normalization <math>\phi_\mathrm{int} = 1</math>, determine numerous additional [[SSC/Structure/BiPolytropes/Analytic51#Step_6:_Envelope_Solution|equilibrium properties]] at the interface, such as … <table border="0" align="center" cellpadding="8" width="80%"> <tr><td align="center" colspan="4"> <table border="1" align="center" cellpadding="8"><tr><td align="center"><font color="darkgreen">Example numerical values inside parentheses assume <math>(\mu_e/\mu_c) = 1</math> and <math>\xi_\mathrm{int} = 1.668646016</math><br /><math>\Rightarrow~~~(r_0)_\mathrm{int}[ K_5^{-1} G\rho_c^{4/5} ]^{1 / 2} = 1.153014872 \, .</math></td></tr></table> </td> </tr> <tr> <td align="right"> <math>\theta_\mathrm{int}</math> </td> <td align="center">=</td> <td align="left"> <math> \biggl[1 + \frac{\xi^2_\mathrm{int}}{3}\biggr]^{-1 / 2} \, ; </math> </td> <td align="right">(0.720165375)</td> </tr> <tr> <td align="right"> <math>\biggl( \frac{d\theta}{d\xi} \biggr)_\mathrm{int}</math> </td> <td align="center">=</td> <td align="left"> <math> -~\frac{\xi_\mathrm{int}}{3}\biggl[1 + \frac{\xi^2_\mathrm{int}}{3}\biggr]^{-3 / 2} \, ; </math> </td> <td align="right">(- 0.207749350)</td> </tr> <tr> <td align="right"> <math>\eta_\mathrm{int}</math> </td> <td align="center">=</td> <td align="left"> <math> 3^{1 / 2}\biggl(\frac{\mu_e}{\mu_c}\biggr)\theta^2_\mathrm{int}\cdot \xi_\mathrm{int} \, ; </math> </td> <td align="right">(1.498957494)</td> </tr> <tr> <td align="right"> <math>\biggl( \frac{d\phi}{d\eta} \biggr)_\mathrm{int}</math> </td> <td align="center">=</td> <td align="left"> <math> 3^{1 / 2} \theta^{-3}_\mathrm{int}\cdot \biggl( \frac{d\theta}{d\xi} \biggr)_\mathrm{int} \, ; </math> </td> <td align="right">(- 0.963393227)</td> </tr> <tr> <td align="right"> <math>\Lambda_\mathrm{int}</math> </td> <td align="center">=</td> <td align="left"> <math> \frac{1}{\eta_\mathrm{int}} + \biggl( \frac{d\phi}{d\eta} \biggr)_\mathrm{int} \, ; </math> </td> <td align="right">(- 0.296262902)</td> </tr> <tr> <td align="right"> <math>A</math> </td> <td align="center">=</td> <td align="left"> <math> \eta_\mathrm{int}(1 + \Lambda^2_\mathrm{int})^{1 / 2} \, ; </math> </td> <td align="right">(1.563357124)</td> </tr> <tr> <td align="right"> <math>B</math> </td> <td align="center">=</td> <td align="left"> <math> \eta_\mathrm{int} - \frac{\pi}{2} + \tan^{-1}(\Lambda_\mathrm{int}) \, . </math> </td> <td align="right">(- 0.359863580)</td> </tr> <tr> <td align="right"> <math>\eta_\mathrm{surf}</math> </td> <td align="center">=</td> <td align="left"> <math> B + \pi \, . </math> </td> <td align="right">(2.781729074)</td> </tr> </table> <font color="maroon">STEP 3:</font> Throughout the core — that is, at all radial positions, <math>0 \le r_0 \le (r_0)_\mathrm{int}</math> — the displacement amplitude and its first and second derivatives, respectively, are given by the expressions, <table border="0" cellpadding="5" align="center" width="80%"> <tr> <td align="right"> <math>x</math> </td> <td align="center"> <math>=</math> </td> <td align="left"> <math> \biggl[1 - \frac{r_0^2}{15a_5^2} \biggr] = \biggl[1 - \frac{\xi^2}{15} \biggr] \, ; </math> </td> <td align="right">(0.814374698)</td> </tr> <tr> <td align="right"> <math>\Rightarrow ~~~r_0\cdot \frac{dx}{dr_0}</math> </td> <td align="center"> <math>=</math> </td> <td align="left"> <math> -~\frac{2r_0^2}{15a_5^2} = -~\frac{2\xi^2}{15} \, ; </math> </td> <td align="right">(- 0.371250604)</td> </tr> <tr> <td align="right"> <math>\Rightarrow ~~~ r_0^2 \cdot \frac{d^2x}{dr_0^2}</math> </td> <td align="center"> <math>=</math> </td> <td align="left"> <math> -~\frac{2r_0^2}{15a_5^2} = -~\frac{2\xi^2}{15} \, ; </math> </td> <td align="right">(- 0.371250604)</td> </tr> <tr> <td align="right"> also … <math> \biggl\{ \frac{d\ln x}{d\ln \xi} \biggr\}_\mathrm{core} = \biggl\{ \frac{d\ln x}{d\ln r_0} \biggr\}_\mathrm{core} = \frac{r_0}{x} \cdot \frac{dx}{dr_0}</math> </td> <td align="center"> <math>=</math> </td> <td align="left"> <math> \biggl[\frac{15}{15 - \xi^2} \biggr] \cdot \biggl[-~\frac{2\xi^2}{15 }\biggr] = \biggl[\frac{2\xi^2}{\xi^2 - 15} \biggr] \, . </math> </td> <td align="right">(-0.455871977)<sup>†</sup></td> </tr> </table> <font color="maroon">STEP #4:</font> From the determination of the logarithmic slope of the displacement function at the edge of the core — <i>i.e.,</i> at the core-envelope interface — determine the slope as viewed from the perspective of the envelope. <table border="0" cellpadding="5" align="center" width="80%"> <tr> <td align="right"> <math>~ \biggl\{ \frac{d\ln x}{d\ln r_0}\biggr|_\mathrm{int} \biggr\}_\mathrm{env} = \biggl\{ \frac{d\ln x}{d\ln \eta}\biggr|_\mathrm{int} \biggr\}_\mathrm{env} </math> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~3\biggl(\frac{\gamma_c}{\gamma_e} -1\biggr) + \frac{\gamma_c}{\gamma_e} \biggl\{ \frac{d\ln x}{d\ln \xi}\biggr|_\mathrm{int} \biggr\}_\mathrm{core} \, .</math> </td> <td align="right">(-1.473523186)<sup>†</sup></td> </tr> </table> ---- <sup>†</sup>This analytically determined value matches the [[SSC/Stability/BiPolytropes/Pt3#Eigenfunction_Details|previous determination]] that was obtained via numerical integration of the LAWE. </td></tr></table> [[SSC/Structure/BiPolytropes/Analytic51#Step_8:_Throughout_the_envelope_(ηi_≤_η_≤_ηs)|Throughout the envelope]] — that is, over the range, <math>(\eta_\mathrm{int} \le \eta \le \eta_\mathrm{surf})</math> — the radial coordinate, <math>r_0</math>, is a linear function of <math>\eta</math> and takes on values given by the expression, <table border="0" cellpadding="5" align="center" width="80%"> <tr> <td align="right"> <math> r_0 [K_5^{-1} G \rho_c^{4/5}]^{1 / 2} </math> </td> <td align="center"> <math>=</math> </td> <td align="left"> <math> \biggl[ \biggl(\frac{\mu_e}{\mu_c}\biggr)^{-1} \theta^{-2}_\mathrm{int} (2\pi)^{-1 / 2} \biggr]\cdot \eta </math> </td> <td align="right">(0.769211186 × η)</td> </tr> <tr> <td align="right"> <math> \Rightarrow ~~~1.153014872 </math> </td> <td align="center"> <math>\leq r_0 \leq</math> </td> <td align="left"> <math>2.139737121 \, . </math> </td> <td align="right"> </td> </tr> </table> [[SSC/Stability/BiPolytropes/Pt3#Eigenfunction_Details|From our earlier discussions]], Here we examine some of the properties of the fundamental-mode eigenfunctions that we have found are associated with marginally unstable, <math>~(n_c, n_e) = (5,1)</math> bipolytropes. <table border="0" align="right" width="40%"> <tr> <th align="center">Figure 5</th> </tr> <tr><td align="center"> [[File:Mod0MuRatio100.png|450px|Example eigenvector]] </td></tr> </table> Consider the model on the <math>~\mu_e/\mu_c = 1</math> sequence for which <math>~\sigma_c^2=0~</math>; key properties of this specific equilibrium model are enumerated in the first row of numbers provided in [[#Equilibrium_Properties_of_Marginally_Unstable_Models|Table 2, above]]. Figure 5 shows how our numerically derived, fundamental-mode eigenfunction, <math>~x = \delta r/r_0</math>, varies with the fractional radius over the entire range, <math>~0 \le r/R \le 1</math>. By prescription, the eigenfunction has a value of unity and a slope of zero at the center <math>~(r/R = 0)</math>. Integrating the LAWE outward from the center, through the model's core (blue curve segment), <math>~x</math> drops smoothly to the value <math>~x_i = 0.81437</math> at the interface <math>~(\xi_i = 1.6686460157 ~\Rightarrow~ q = r_\mathrm{core}/R_\mathrm{surf} = 0.53885819)</math>. Our numerical integration of the LAWE showed that, at the interface, the logarithmic slope of the ''core'' (blue) segment of the eigenfunction is, <table border="0" cellpadding="5" align="center"> <tr> <td align="right"> <math>~ \biggl\{ \frac{d\ln x}{d\ln r}\biggr|_i \biggr\}_\mathrm{core} = \biggl\{ \frac{d\ln x}{d\ln \xi}\biggr|_i \biggr\}_\mathrm{core} </math> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~- 0.455872 \, .</math> </td> </tr> </table> Next, following the [[#Interface|above discussion of matching conditions at the interface]], we determined that, from the perspective of the envelope, the slope of the eigenfunction at the interface must therefore be, <table border="0" cellpadding="5" align="center"> <tr> <td align="right"> <math>~ \biggl\{ \frac{d\ln x}{d\ln r}\biggr|_i \biggr\}_\mathrm{env} = \biggl\{ \frac{d\ln x}{d\ln \eta}\biggr|_i \biggr\}_\mathrm{env} </math> </td> <td align="center"> <math>~=</math> </td> <td align="left"> <math>~3\biggl(\frac{\gamma_c}{\gamma_e} -1\biggr) + \frac{\gamma_c}{\gamma_e} \biggl\{ \frac{d\ln x}{d\ln \xi}\biggr|_i \biggr\}_\mathrm{core} = -1.47352 \, .</math> </td> </tr> </table> Adopting this "env" slope along with the amplitude, <math>~x_i = 0.81437</math>, as the appropriate ''interface'' boundary conditions, we integrated the LAWE from the interface to the surface, obtaining the green-colored segment of the eigenfunction that is shown in Figure 5. The amplitude continued to steadily decrease, reaching a value of <math>~x_s = 0.38203</math>, at the model's surface <math>~(r/R = 1)</math>. At the surface, this ''envelope'' (green) segment of the eigenfunction exhibits a logarithmic slope that matches to eight significant digits the value that is [[#SurfaceCondition|expected from astrophysical arguments]] for this marginally unstable <math>~(\sigma_c^2=0)</math> model, namely, <div align="center"> <math>~ \frac{d\ln x}{d\ln \eta}\biggr|_s = \biggl[ \biggl( \frac{\rho_c}{\bar\rho} \biggr)\frac{\cancelto{0}{\sigma_c^2}}{2\gamma_e} - \biggl(3 - \frac{4}{\gamma_e}\biggr)\biggr] = -1 \, . </math> </div>
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