Difference between revisions of "User:Tohline/Math/EQ SSenergyConservation01"

Latest revision as of 03:46, 28 October 2018

<math>~\frac{dL_r}{dr} = 4\pi r^2 \rho \epsilon_\mathrm{nuc}</math>

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