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- W2615369300 abstract "We examine a relationship between the phenomenological equation of state (EOS) of nuclear matter near normal nuclear density and neutron-rich nuclei in laboratories and in neutron-star crusts. In this study, we use about 200 EOS ’s, which are systematically constructed in such a way as to provide a reasonable fit to empirical masses and radii of stable nuclei by simplified Thomas-Fermi calculations. As for neutron-rich nuclei in laboratories, matter radii and masses are shown to be functions of the symmetry energy density derivative coefficient L. We also find that the boundary density between the core and crust of neutron stars is a decreasing function of L. We expect that future systematic measurements of the matter radii and masses of neutron-rich nuclei could help deduce the L value, which in turn could give useful information about nuclei in neutron-star crusts." @default.
- W2615369300 created "2017-05-26" @default.
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- W2615369300 date "2005-09-21" @default.
- W2615369300 modified "2023-09-26" @default.
- W2615369300 title "Equation of state of nuclear matter and nuclei in laboratories and neutron-star crusts" @default.
- W2615369300 hasPublicationYear "2005" @default.
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