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Neutron Star Interiors

Published online by Cambridge University Press:  04 August 2017

Charles Alcock
Charles Alcock*
Affiliation:
Department of Physics, Massachusetts Institute of Technology, Cambridge, MA 02139 U.S.A.

Abstract

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The current status of the theory of neutron star interiors is reviewed. The various phases of matter that might exist are discussed and their relation to other areas of astrophysics briefly noted. Observational distinction between the models is not simply obtained; analysis of pulsar post-glitch relation, of neutron star precession and neutron star cooling are promising in this regard.

Type
V. Neutron Star Physics
Information
Symposium - International Astronomical Union , Volume 125: The Origin and Evolution of Neutron Stars , 1987 , pp. 413 - 424
Copyright
Copyright © Reidel 1987 

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