Version 5 (modified by 12 years ago) ( diff ) | ,
---|
(Back to Bearclaw Outline)
PURE FUNCTION kd (i,T)
Defined in
contrib/astro/physics/cool/cool.f90
Inputs
- i (represents species: H=1, H2=2, He=3, e=4)
- T
Description
- Calculates collisional dissociation rates, kd, for high & low density limits, and interpolates between them, for collisions between H2 and H, H2, He, or e
Specifics
- For high density limits:
- Collisions with H and H2 use Lepp & Shull: kdH = kdH_LS
- No high density limit collisions between H2 and He or e.
- Low density limits:
- For H & H2:
- A critical density is calculated (different expression for H & H2) as the delineation between high & low density limits
- kd is then calculated by interpolating between kdH and kdL using the expression from Lepp & Shull
Called in
contrib/astro/physics/cool/cool.f90 in SUBROUTINE H2_diss
Modules Used
Functions Used
PURE_FUNCTION_kdH_LS
Defined in
contrib/astro/physics/cool/cool.f90
Inputs
Description
Called in
Modules Used
Functions Used
PURE_FUNCTION_kdL_MK
Defined in
contrib/astro/physics/cool/cool.f90
Inputs
Description
Called in
Modules Used
Functions Used
PURE_FUNCTION_kdL_DM
Defined in
contrib/astro/physics/cool/cool.f90
Inputs
Description
Called in
Modules Used
Functions Used
PURE_FUNCTION_kdL_LS
Defined in
contrib/astro/physics/cool/cool.f90
Inputs
Description
This function seems to be obsolete.
Called in
Modules Used
Functions Used
Note:
See TracWiki
for help on using the wiki.