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Physics of the Neutron Star

Published online by Cambridge University Press:  07 February 2017

A. G. W. Cameron
A. G. W. Cameron*
Affiliation:
Belfer Graduate School of Science, Yeshiva University, New York, N.Y., U.S.A. Goddard Institute for Space Studies, NASA, New York, N.Y., U.S.A.

Abstract

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Some characteristics of neutron star models are described. These include: the physics of the crystalline crust, the superfluid properties of the neutrons and protons, and the presence of rotational vortices in these superfluids. The possible relationship of some of these properties to the behavior of the Crab Nebula pulsar is described.

Type
Session 6
Information
Symposium - International Astronomical Union , Volume 46: The Crab Nebula , 1971 , pp. 323 - 333
Copyright
Copyright © Reidel 1971 

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