Changes between Version 24 and Version 25 of u/bliu/pnfldiff

Timestamp:

08/15/18 14:41:51 (6 years ago)

Author:

Baowei Liu

Comment:

—

u/bliu/pnfldiff

@@ -29 +29 @@
 $ I = -\nabla\cdot J$[[BR]]
 
-J is the flux of ionizing photons. Inside the front where the gas is nearly completely ionized the recombination rate[[BR]]
+J is the flux of ionizing photons. Inside the front where the gas is nearly completely ionized.
+
+The recombination rate[[BR]]
 
 $ r=\alpha n_{e}^{2} $[[BR]]
 
-The thermal energy of the gas per unit mass [[BR]]
+at T~10000K, $\alpha=2.6\times10^{-13} cm^{3}s^{-1}$[[BR]]
 
-$E=(3/2)\kappa T(n+n_{e})/\rho$
-
-$\frac{\partial E}{\partial t}=-(\bold{U}_{rel}\cdot\nabla)E-\frac{P}{\rho}(\nabla\cdot \bold{u})-\frac{\Lambda-\Gamma}{\rho}$[[BR]]
 
 Optical depth of the interior:[[BR]]
@@ -46 +45 @@
 
 $x=n_{e}/n$ is the ionization fraction[[BR]]
+
+
+
+The thermal energy of the gas per unit mass [[BR]]
+
+$E=(3/2)\kappa T(n+n_{e})/\rho$
+
+$\frac{\partial E}{\partial t}=-(\bold{U}_{rel}\cdot\nabla)E-\frac{P}{\rho}(\nabla\cdot \bold{u})-\frac{\Lambda-\Gamma}{\rho}$[[BR]]
 
 
@@ -79 +86 @@
 10. [http://www.astronomy.ohio-state.edu/~pogge/Ast871/Notes/Ionized.pdf ionizaed]
 
-11. [https://en.wikipedia.org/wiki/Beer%E2%80%93Lambert_law Beer–Lambert law]
+
 
 == related code ==