Consider a system with high-energy neutrinos (higher than rest mass energies of protons & neutrons) where the energy of a neutrino is specified as $E = p + sB$, $p$ being the magnitude of the momentum and $s$ its spin. $B$ is a constant external magnetic field.
I need to show using 'simple statistical mechanics' that the number density of neutrons is expected to be higher than that of protons.
I am aware that the situation is akin to a white dwarf/neutron star, and from this question I know that the electron degeneracy makes it energetically favorable for an electron capture process:
$$p+e→n+\nu_e$$
I think the 'simple statistical mechanics' that I need to use is the two-level occupation ratio:
$$ \frac{n}{p} = exp(-\frac{\Delta E}{kT}) $$
but how does one go from the information given to me to being able to apply the above?
Edit: After some more reading, I realize that I can relate $E_F$ to number densities. Assuming degenerate electron gas, which terms in the conservation laws can I relate to their Fermi energies and thus invoke the relationship to their respective number densities?
I am mildly certain electron energy/momentum terms can be replaced with their Fermi values due to the neutron star being a degenerate electron gas scenario. What else am I missing?