Difference between revisions of "User:Tohline/Math/EQ SSenergyConservation01"
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Revision as of 03:35, 28 October 2018
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<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> |
