{
  "annotation_id": "a0083172-2c10-426d-b1cb-f5702de57a8c",
  "date_created": "2026-03-02T18:00:14.166000Z",
  "date_modified": "2026-03-02T18:00:14.166000Z",
  "file_hash": "ca9d38f9bf4126a563f16e3add1a9be10cb0998f07200e8b592f421a48bc2a96",
  "private": false,
  "record": {
    "abstract": "We calculate properties of neutron stars such as mass and radius using a\nrelativistic Dirac-Brueckner-hartree-Fock apprach for asymmetric nuclear\nmatter. For pure neutron matter we find the maximum mass to be 2.4 solar masses\nwith a radius of 12 km. For a proton fraction of 30% we find a max mass of 2.1\nsolar masses and a radius of 10.5 km. The implications are discussed.",
    "arxiv_id": "nucl-th/9406028",
    "authors": [
      "L. Engvik",
      "M. Hjorth-Jensen",
      "E. Osnes",
      "G. Bao",
      "E. Oestgaard"
    ],
    "categories": [
      "nucl-th"
    ],
    "doi": "10.1103/PhysRevLett.73.2650",
    "journal_ref": "Phys.Rev.Lett. 73 (1994) 2650-2653",
    "title": "Asymmetric nuclear matter and neutron star properties",
    "url": "https://arxiv.org/abs/nucl-th/9406028"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "f9e1b4dd-de76-41fc-8718-06cada54d123",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}