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)