- #1
mccizmt2
- 5
- 0
I am trying to write some code to produce a model of a star. I've done loads of research and come to the conclusion that for ease i want to represent the opacity in my model with the power law.
k=k(0)*(rho^alpha)*(T^beta)
this seems very straight forward apart from the fact that in every source I've looked at it states how easy this equation is to use etc but never actually tells you how to calculate the constant k(0). Which i presume is opacity at the centre of the star. Could somebody please help me.
Thanks
k=k(0)*(rho^alpha)*(T^beta)
this seems very straight forward apart from the fact that in every source I've looked at it states how easy this equation is to use etc but never actually tells you how to calculate the constant k(0). Which i presume is opacity at the centre of the star. Could somebody please help me.
Thanks