{
  "annotation_id": "4b3b8cc2-f32a-4c36-90d5-7541a397515d",
  "date_created": "2026-03-02T18:00:04.343000Z",
  "date_modified": "2026-03-02T18:00:04.343000Z",
  "file_hash": "30aea64d712703b693dcce31a8c6daf77e5782b7f877a93611cf6f82754dac36",
  "private": false,
  "record": {
    "abstract": "We investigate the equations of state for pure neutron matter and strange\nhadronic matter in $\\beta$-equilibrium, including $\\Lambda$, $\\Sigma$ and $\\Xi$\nhyperons. The masses and radii of pure neutron stars and strange hadronic stars\nare obtained. For a pure neutron star, the maximum mass is about $1.8\nM_{\\mathrm{sun}}$, while for a strange hadronic star, the maximum mass is\naround $1.45 M_{\\mathrm{sun}}$. The typical radii of pure neutron stars and\nstrange hadronic stars are about 11.0-12.3 km and 10.7-11.7 km, respectively.",
    "arxiv_id": "nucl-th/0506014",
    "authors": [
      "P. Wang",
      "S. Lawley",
      "D. B. Leinweber",
      "A. W. Thomas",
      "A. G. Williams"
    ],
    "categories": [
      "nucl-th"
    ],
    "doi": "10.1103/PhysRevC.72.045801",
    "journal_ref": "Phys.Rev.C72:045801,2005",
    "title": "Neutron stars and strange stars in the chiral SU(3) quark mean field   model",
    "url": "https://arxiv.org/abs/nucl-th/0506014"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "2f76d070-79a2-4959-b1e8-5fbab33e4129",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}