Template:LAWEsolutions: Difference between revisions

Revision as of 17:23, 1 November 2023

Isolated n = 1 Polytrope

γ_{g} = 2

γ_{g} = \frac{5}{3}

Relevant Chapters

Key References:

Isolated n = 3 Polytrope
$γ_{g} = \frac{20}{13}$	Relevant Chapters Origin of Planetary Nebulae Radial Oscillations of n = 3 Polytropic Spheres
	Key References: 📚 Schwarzschild (1941)

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    <td align="left">Key References:
 <ul><li>{{ Chatterji51 }}</li></ul></td>
+</tr>
+</table>
+<table border="1" align="center" cellpadding="5">
+<tr>
+  <td align="center" colspan="2"><b>Isolated n = 3 Polytrope</b></td>
+</tr>
+<tr>
+  <td align="center" rowspan="2"><math>\gamma_g = \tfrac{20}{13}</math><br />[[File:Schwarzschild1941movie.gif|250px|n = 3 Eigenvectors]]</td>
+  <td align="left">Relevant Chapters
+<ul><li>[[Appendix/Ramblings/OriginOfPlanetaryNebulae#Isolated_n_=_3_Polytrope_with_γg_=_20/13|Origin of Planetary Nebulae]]</li>
+<li>[[SSC/Stability/n3PolytropeLAWE#Radial_Oscillations_of_n_.3D_3_Polytropic_Spheres|Radial Oscillations of n = 3 Polytropic Spheres]]</li>
+</ul></td>
+</tr>
+<tr>
+  <td align="left">Key References:
+<ul><li>{{ Schwarzschild41 }}</li></ul></td>
 </tr>
 </table>