Proto-neutron Star with Trapped Neutrinos

초록

We investigate the structure of a proto-neutron star with trapped neutrinos by using quantum hadrodynamics (QHD). We assume that a part of neutrinos produced by beta equilibrium may be trapped and the ratio of trapped neutrinos may depend on the density. With these assumptions, we calculated the population of baryons and leptons, equation of state, the mass-radius relation of a proto-neutron star under isentropic conditions.

키워드