Version 8 (modified by 12 years ago) ( diff ) | ,
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PURE FUNCTION H_recomb(nHII,ne,T)
Defined in
contrib/astro/physics/cool/cool.f90
Inputs
- nHII (=1.d0)
- ne (=1.d0)
- T (in K)
Description
- Calculates rates for HII + e- recombination using the expression of Verner & Ferland (1996ApJS..103..467V):
- H_recomb = nHII*ne* (a / [sqrt(T/T0)*(1+sqrt(T/T0))(1-b)*(1+sqrt(Tin/T1))(1+b)])
- where a,b,T0,T1 are constants, and Tin = max(200.,T) (I'm not sure why)
- H_recomb = nHII*ne* (a / [sqrt(T/T0)*(1+sqrt(T/T0))(1-b)*(1+sqrt(Tin/T1))(1+b)])
- Values are nominally in cm-3 s-1, however:
- When used in initneqCool, nHII & ne are inputted as 1.d0.
- The actual densities aren't multiplied in until the tables are used in i_evolove.f90 to calculate the actual cooling rates.
- Is used in Subroutine initneqCool (in cool.f90) to build table of cooling values for this process
Called in
contrib/astro/physics/cool/cool.f90, in SUBROUTINE initneqCool
Modules Used ![(?)](/astrobear/chrome/wikiextras-icons-16/question.png)
None
Functions Used
None
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