SSC/Stability/BiPolytropes/RedGiantToPN/Pt3: Difference between revisions
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<font color="maroon"><b> | <font color="maroon"><b>Polytropic LAWE</b></font><br /> | ||
{{ Math/EQ_RadialPulsation02 }} | {{ Math/EQ_RadialPulsation02 }} | ||
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Let's now insert an additive constant, <math>C_0</math>, to this 2<sup>nd</sup>-order ODE as follows: | |||
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[[Image:LSUkey.png|25px|link=Appendix/EquationTemplates#Stability:_Radial_Pulsation]] | |||
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<math>C_0 = \frac{d^2x}{d\xi^2} + \biggl[ 4 - (n+1) Q \biggr] \frac{1}{\xi} \cdot \frac{dx}{d\xi} | |||
+ (n+1) \biggl[ \biggl( \frac{\sigma_c^2}{6\gamma_g } \biggr) \frac{\xi^2}{\theta} | |||
- \alpha Q\biggr] \frac{x}{\xi^2} </math> | |||
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where: <math>Q(\xi) \equiv - \frac{d\ln\theta}{d\ln\xi} \, ,</math> <math>\sigma_c^2 \equiv \frac{3\omega^2}{2\pi G\rho_c} \, ,</math> and, <math>\alpha \equiv \biggl(3 - \frac{4}{\gamma_\mathrm{g}}\biggr)</math> | |||
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=Related Discussions= | =Related Discussions= | ||
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Revision as of 13:06, 6 January 2026
Main Sequence to Red Giant to Planetary Nebula (Part 3)
Part I: Background & Objective
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Part II:
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Yabushita68-Motivated Analysis
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Part IV:
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Yabushita68-Motivated Analysis
In an accompanying discussion, we derived the so-called,
Let's now insert an additive constant, , to this 2nd-order ODE as follows:
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where: and, |
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Related Discussions
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Appendices: | VisTrailsEquations | VisTrailsVariables | References | Ramblings | VisTrailsImages | myphys.lsu | ADS | |