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Protoneutron stars and neutron stars
Published online by Cambridge University Press: 12 April 2016
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.
- Type
- Part 9. Population and Neutron Star Properties
- Information
- International Astronomical Union Colloquium , Volume 177: Pulsar Astronomy - 2000 and Beyond , 2000 , pp. 663 - 664
- Copyright
- Copyright © Astronomical Society of the Pacific 2000