Neutron star properties from modern meson-exchange potential models
Bao, Engvik, Hjorth-Jensen, Osnes, Oestgaard
Abstract
We calculate the total mass, radius, moment of inertia and surface gravitational redshift for neutron stars using various equations of state. The latter are derived from recent meson-exchange potential models, employing both a relativistic and a non-relativistic Brueckner-Hartree-Fock approach.
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