Protoneutron stars and neutron stars
D. Gondek-Rosinska, P. Haensel, J. L. Zdunik
Abstract
We find constraints on minimum and maximum mass of ordinary neutron stars imposed by their early evolution (protoneutron star stage). We calculate models of protoneutron stars using a realistic standard equation of state of hot, dense matter valid for both supranuclear and subnuclear densities. Results for different values of the nuclear incompressibility are presented.
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