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Neutron Star Models

Published online by Cambridge University Press:  14 August 2015

V. Canuto  and
Richard L. Bowers
V. Canuto
Affiliation:
NASA Goddard Institute for Space Studies, New York, N.Y., USA Department of Physics, CCNY, New York, N.Y., USA
Richard L. Bowers
Affiliation:
Lawrence Livermore National Laboratory, Livermore, CA, USA

Abstract

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The current state of neutron star structure calculations is reviewed. Uncertainties in the equation of state for matter at and above nuclear density remain. The role of the delta resonance, pion condensates, and quark matter is reviewed. Despite uncertainties, we find that recent models yield stable neutron star masses which are consistent with observational estimates.

Type
VII. Properties of Neutron Stars
Information
Symposium - International Astronomical Union , Volume 95: Pulsars , 1981 , pp. 321 - 330
Copyright
Copyright © Reidel 1981 

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