Neutron star properties and the equation of state of neutron-rich matter

Details Neutron star properties and the equation of state of neutron-rich matter Neutron star properties and the equation of state of neutron-rich matter

2006-01-22

arxiv.org/abs/nucl-th/0601065v3

Phys.Rev. C74 (2006) 025808

Physics

Nuclear Physics

Nuclear Theory

13 pages, 9 figures, 1 table; Revised version, accepted for publication in Physical Review C

Scientific paper

10.1103/PhysRevC.74.025808

We calculate total masses and radii of neutron stars (NS) for pure neutron matter and nuclear matter in beta-equilibrium. We apply a relativistic nuclear matter equation of state (EOS) derived from Dirac-Brueckner-Hartree-Fock (DBHF) calculations. We use realistic nucleon-nucleon (NN) interactions defined in the framework of the meson exchange potential models. Our results are compared with other theoretical predictions and recent observational data. Suggestions for further study are discussed.

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