- #1
Leonardo Machado
- 57
- 2
Good evening.
I'm currently studing dense matter and nuclear matter above 10^8 g/cm^3, and i know well how to insert a beta equilibirum condition in a free Fermi gás at T=0.
[tex] \sqrt{K^2_{F,n}+m^2_n}=\sqrt{K^2_{F,p}+m^2_p}+\sqrt{K^2_{F,e}+m^2_e}[/tex]
But how do i insert the same condition of radioactive equilibrium for an interacting model ?
I'm currently studing dense matter and nuclear matter above 10^8 g/cm^3, and i know well how to insert a beta equilibirum condition in a free Fermi gás at T=0.
[tex] \sqrt{K^2_{F,n}+m^2_n}=\sqrt{K^2_{F,p}+m^2_p}+\sqrt{K^2_{F,e}+m^2_e}[/tex]
But how do i insert the same condition of radioactive equilibrium for an interacting model ?