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Properties and Synthesis of Heavy Nuclei and Properties of Neutron Star Matter

Published online by Cambridge University Press:  14 August 2015

J. Robert Buchler
J. Robert Buchler*
Affiliation:
Belfer Graduate School of Science, Yeshiva University, New York, N.Y., U.S.A.

Abstract

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The nuclear Thomas-Fermi model which is based on nuclear matter calculations has been successfully applied to the study of the bulk properties of nuclei. It is ideally suited for extrapolation into the region of very neutron-rich and of superheavy nuclei. It is therefore a valuable approach for r-process calculations as well as for the study of neutron star matter at subnuclear densities.

Type
Research Article
Information
Symposium - International Astronomical Union , Volume 53: Physics of Dense Matter , 1974 , pp. 67 - 75
Copyright
Copyright © Reidel 1974 

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