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Neutron star modelsThe 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. It is found that recent models yield stable neutron star masses which are consistent with observational estimates.
Document ID
19820049425
Acquisition Source
Legacy CDMS
Document Type
Conference Proceedings
Authors
Canuto, V. (NASA Goddard Institute for Space Studies; City College New York, NY, United States)
Bowers, R. L. (California, University Lawrence Livermore Laboratory, Livermore, CA, United States)
Date Acquired
August 10, 2013
Publication Date
January 1, 1981
Subject Category
Astrophysics
Meeting Information
Meeting: Pulsars: 13 years of research on neutron stars
Location: Bonn
Start Date: August 26, 1980
End Date: August 29, 1980
Accession Number
82A32960
Distribution Limits
Public
Copyright
Other

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