Difference between revisions of "User:Tohline/Math/EQ SSradiationTransport01"

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[[Image:LSU_Key.png|25px|link=https://www.vistrails.org/index.php/User:Tohline/Appendix/Equation_templates#Traditional_Equations_of_.28Spherical.29_Stellar_Structure]]
[[Image:LSU_Key.png|25px|link=http://www.vistrails.org/index.php/User:Tohline/Appendix/Equation_templates#Traditional_Equations_of_.28Spherical.29_Stellar_Structure]]
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<math>~\frac{dL_r}{dr} = 4\pi r^2 \rho \epsilon_\mathrm{nuc}</math>
<math>~\frac{dT}{dr} = - \frac{ 3 }{ 4a_\mathrm{rad} c}
\biggl(\frac{ \kappa \rho }{ T^3 }\biggr)
\frac{ L_r  }{ 4\pi r^2 }</math>
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Latest revision as of 03:46, 28 October 2018

LSU Key.png

<math>~\frac{dT}{dr} = - \frac{ 3 }{ 4a_\mathrm{rad} c} \biggl(\frac{ \kappa \rho }{ T^3 }\biggr) \frac{ L_r }{ 4\pi r^2 }</math>