Version 7 (modified by 12 years ago) ( diff ) | ,
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PURE FUNCTION H2_critical_cool(nH2, T)
Defined in
contrib/astro/physics/cool/cool.f90
Inputs
- nH2
- T
Description
- Not used. This function has been commented out.
- This seems to have been a way to bridge H2 cooling between the high and low density regimes.
- Values are in erg/cm3/s
Called in
contrib/astro/physics/cool/cool.f90, in the subroutine initneqCool
Functions Used
- fj (PURE) (j)
- boltzmann population fraction for rotational state j
- fv (PURE) (v)
- boltzmann population fraction for vibrational state v
- gs (PURE) (j)
- degeneracy of rotational state j
- Bv (PURE) (v)
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