{
  "annotation_id": "807ffcf2-23e7-4112-9b28-eef09b8939bc",
  "date_created": "2026-03-02T18:00:21.981000Z",
  "date_modified": "2026-03-02T18:00:21.981000Z",
  "file_hash": "6850f32e620d2662192f67963b010f274e0b4dc573b3214b3b2f212c7d6a71b3",
  "private": false,
  "record": {
    "abstract": "We study the properties of neutron stars adopting relativistic equations of\nstate of neutron star matter, calculated in the framework of the relativistic\nBrueckner-Hartree-Fock approximation for electrically charge neutral neutron\nstar matter in beta-equilibrium. For higher densities more baryons (hyperons\netc.) are included by means of the relativistic Hartree- or Hartree-Fock\napproximation. The special features of the different approximations and\ncompositions are discussed in detail. Besides standard neutron star properties\nspecial emphasis is put on the limiting periods of neutron stars, for which the\nKepler criterion and gravitation-reaction instabilities are considered.\nFurthermore the cooling behaviour of neutron stars is investigated, too. For\ncomparison we give also the outcome for some nonrelativistic equations of\nstate.",
    "arxiv_id": "nucl-th/9711025",
    "authors": [
      "H. Huber",
      "F. Weber",
      "M. K. Weigel",
      "Ch. Schaab"
    ],
    "categories": [
      "nucl-th",
      "astro-ph"
    ],
    "doi": "10.1142/S0218301398000130",
    "journal_ref": "Int.J.Mod.Phys. E7 (1998) 301-340",
    "title": "Neutron star properties with relativistic equations of state",
    "url": "https://arxiv.org/abs/nucl-th/9711025"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "8b9d6ca6-d3c7-48f2-97c3-7c5c33169e29",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}