SSC/Stability/BiPolytropes/RedGiantToPN/Pt3: Difference between revisions

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Created page with "__FORCETOC__ =Main Sequence to Red Giant to Planetary Nebula (Part 2)= <table border="1" align="center" width="100%" colspan="8"> <tr> <td align="center" bgcolor="lightblue" width="25%"><br />Part I:  Background & Objective   </td> <td align="center" bgcolor="lightblue" width="25%"><br />Part II:    </td> <td align="center" bgcolor="lightblue" wi..."
 
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   <td align="center" bgcolor="lightblue" width="25%"><br />[[SSC/Stability/BiPolytropes/RedGiantToPN/Pt3|Part III:&nbsp; ]]
   <td align="center" bgcolor="lightblue" width="25%"><br />[[SSC/Stability/BiPolytropes/RedGiantToPN/Pt3|Yabushita68-Motivated Analysis]]
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==Yabushita68-Motivated Analysis==
==Yabushita68-Motivated Analysis==
In an [[SSC/Perturbations#2ndOrderODE|accompanying discussion]], we derived the so-called,
In an [[SSC/Perturbations#2ndOrderODE|accompanying discussion]], we derived the so-called,
<div align="center">
<font color="maroon"><b>Yabushita68-Motivated Polytropic LAWE</b></font><br />
{{ Math/EQ_RadialPulsation02 }}
</div>


=Related Discussions=
=Related Discussions=


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{{ SGFfooter }}

Revision as of 13:00, 6 January 2026

Main Sequence to Red Giant to Planetary Nebula (Part 2)


Part I:  Background & Objective

 


Part II: 

 


Yabushita68-Motivated Analysis

 


Part IV: 

 

Yabushita68-Motivated Analysis

In an accompanying discussion, we derived the so-called,


Yabushita68-Motivated Polytropic LAWE

0=d2xdξ2+[4(n+1)Q]1ξdxdξ+(n+1)[(σc26γg)ξ2θαQ]xξ2

where:    Q(ξ)dlnθdlnξ,    σc23ω22πGρc,     and,     α(34γg)


Related Discussions

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