{
  "annotation_id": "e7892c7e-f963-4331-aa08-674fe66e9896",
  "date_created": "2026-03-02T18:00:08.467000Z",
  "date_modified": "2026-03-02T18:00:08.467000Z",
  "file_hash": "4ce23ca955b3156c08830ac3ff2e30457ad3d6ae89c4fbd207cd950858bd2d35",
  "private": false,
  "record": {
    "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"
    ],
    "categories": [
      "nucl-th"
    ],
    "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"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "b19eaa1a-cf34-4a30-851b-fff8f5090d94",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}