Properties of nuclei in astrophysical environments: Binding energies, weak-interaction rates

Details Properties of nuclei in astrophysical environments: Binding energies, weak-interaction rates Properties of nuclei in astrophysical environments: Binding energies, weak-interaction rates

Dec 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992stin...9417628t&link_type=abstract

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Physics

Nuclear Physics

Ionization, Nuclear Astrophysics, Nuclei (Nuclear Physics), Weak Energy Interactions, Boltzmann Distribution, Hartree Approximation, Neutron Stars, Stellar Evolution, Supernovae

Scientific paper

Some of the problems related to the evaluation of binding energies (masses) and weak interaction rates in nuclei of astrophysical interest are discussed. Selected examples of those arising in stellar evolution and nucleosynthesis studies are considered. Judging from the progress made in developing new experiment techniques, it can be expected that some data in the quest will become available in the near future. This concerns masses and beta decay half lives of neutron rich nuclei involved in the r-process nucleosynthesis

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