OP Computations of radiative accelerations
Mass-Fractions Metal Fractional Composition (default = solar)
Hydrogen Mass-Fraction (X)
Metal Mass-Fraction (Z)
Note: metal abundances are re-normalised to the value of Z which has been set --- it is necessary to specify only the relative abundance for each metal.
 
C (Z=6)
N (Z=7)
O (Z=8)
Ne (Z=10)
Na (Z=11)
Mg (Z=12)
Al (Z=13)
Si (Z=14)
S (Z=16)
Ar (Z=18)
Ca (Z=20)
Cr (Z=24)
Mn (Z=25)
Fe (Z=26)
Ni (Z=28)

Output options
Please choose ONE of the following output options:
An intermediate file containing radiative acceleration data for a selected element and a range of its abundance multiplier (χ) to be used locally for interpolation with the code accfit.tar.gz
 
log10(χ) range
   
Selected element
Initial
Interval
No. points
 
 
Radiative accelerations, RMOs, and diffusion coefficients for a selected element, a range of its abundance multiplier (χ) and a stellar model (Teff and depth profile {log10(T) , log10(ρ), r/R*}).
 
log10(χ) range
   
Selected element
Initial
Interval
No. points
 
Teff
 
Please introduce local file with depth profile
(see example)
 
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