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Properties and synthesis of heavy nuclei and properties of neutron star matterThe 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.
Document ID
19740049632
Acquisition Source
Legacy CDMS
Document Type
Conference Proceedings
Authors
Buchler, J. R.
(Yeshiva University New York, N.Y., United States)
Date Acquired
August 7, 2013
Publication Date
January 1, 1974
Subject Category
Physics, Atomic, Molecular, And Nuclear
Meeting Information
Meeting: Symposium on Physics of dense matter
Location: Boulder, CO
Start Date: August 21, 1972
End Date: August 25, 1972
Accession Number
74A32382
Distribution Limits
Public
Copyright
Other

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