2026-07-072026-07-07http://salesiana.dossiersoluciones.com/handle/123456789/2298We 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.ASP Conference Series "Pulsar Astronomy - 2000 and Beyond", eds Kramer, Wex, Wielebinski, Vol 202, 663Astrophysicstext