Protoneutron stars and neutron stars
Astrophysics
2007-05-23 v1
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.
Keywords
Cite
@article{arxiv.astro-ph/0012543,
title = {Protoneutron stars and neutron stars},
author = {D. Gondek-Rosinska and P. Haensel and J. L. Zdunik},
journal= {arXiv preprint arXiv:astro-ph/0012543},
year = {2007}
}
Comments
ASP Conference Series "Pulsar Astronomy - 2000 and Beyond", eds Kramer, Wex, Wielebinski, Vol 202, 663