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Neutron starsQuantum-mechanical processes associated with the presence of high magnetic fields and the effect of such fields on the evolution of neutron stars are reviewed. A technical description of the interior of a neutron star is presented. The neutron star-pulsar relation is reviewed and consideration is given to supernovae explosions, flux conservation in neutron stars, gauge-invariant derivation of the equation of state for a strongly magnetized gas, neutron beta-decay, and the stability condition for a neutron star.
Document ID
19790035105
Document Type
Other - Collected Works
Authors
Canuto, V. (NASA Goddard Institute for Space Studies New York, N.Y., United States)
Date Acquired
August 9, 2013
Publication Date
January 1, 1978
Subject Category
Astrophysics
Accession Number
79A19118
Distribution Limits
Public
Copyright
Other

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