Protoneutron stars and neutron stars

2000/12/29 by D. Rosińska, D. Gondek-Rosinska, Gondek-Rosinska, D. +4
Earth and Planetary Sciences · Physics and Astronomy · #Astrophysics (astro-ph) #FOS: Physical sciences #Gamma-ray bursts and supernovae #Geological and Geophysical Studies #Pulsars and Gravitational Waves Research #astro-ph

paper · pdf · doi:10.48550/arxiv.astro-ph/0012543

ASP Conference Series "Pulsar Astronomy - 2000 and Beyond", eds Kramer, Wex, Wielebinski, Vol 202, 663

arxiv created 2000/12/29 · openalex publication_date 2000/12/29 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28

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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