dorsal/arxiv
View SchemaNeutron star properties and the equation of state of neutron-rich matter
| Authors | Plamen G. Krastev, Francesca Sammarruca |
|---|---|
| Categories | |
| ArXiv ID | nucl-th/0601065 |
| URL | https://arxiv.org/abs/nucl-th/0601065 |
| DOI | 10.1103/PhysRevC.74.025808 |
| Journal | Phys.Rev. C74 (2006) 025808 |
Abstract
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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"abstract": "We calculate total masses and radii of neutron stars (NS) for pure neutron\nmatter and nuclear matter in beta-equilibrium. We apply a relativistic nuclear\nmatter equation of state (EOS) derived from Dirac-Brueckner-Hartree-Fock (DBHF)\ncalculations. We use realistic nucleon-nucleon (NN) interactions defined in the\nframework of the meson exchange potential models. Our results are compared with\nother theoretical predictions and recent observational data. Suggestions for\nfurther study are discussed.",
"arxiv_id": "nucl-th/0601065",
"authors": [
"Plamen G. Krastev",
"Francesca Sammarruca"
],
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"doi": "10.1103/PhysRevC.74.025808",
"journal_ref": "Phys.Rev. C74 (2006) 025808",
"title": "Neutron star properties and the equation of state of neutron-rich matter",
"url": "https://arxiv.org/abs/nucl-th/0601065"
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