Changes between Version 5 and Version 6 of u/erica/radpredictionsink

Timestamp:

04/05/16 15:04:27 (9 years ago)

Author:

Erica Kaminski

Comment:

—

u/erica/radpredictionsink

@@ -81 +81 @@
 Consider this is the case for small pre-stellar cores, and perhaps why radiative feedback is so important. With high mass star formation it will inevitably take longer to heat the gas.
 
-Here are my initial energy budgets:
+Here are my initial energy density budgets:
 
-|| Erad || aT^4^=7.565e-11 erg/cm^3^ ||
+|| Erad || aT^4^=7.565e-11 erg/cm^3^||
 || Egas || nKT=1.656e-7 erg/cm^3^ ||
-|| Estar ||  ||
 
+Here is the total initial energy budgets:
+|| Erad || aT^4^=(7.565e-11 erg/cm^3^)*(7.7e+49)=6e+39 erg||
+|| Egas || nKT=1.656e-7 erg/cm^3^=1e+43 erg ||
+
+And the total energy radiated by the star in a diffusion time:
+|| Estar || L*tdiff= ||
+