{
  "annotation_id": "da4372d8-90a3-4308-9651-7adf0d0e4fb0",
  "date_created": "2026-03-02T18:00:11.913000Z",
  "date_modified": "2026-03-02T18:00:11.913000Z",
  "file_hash": "929004899d7f0d27e7212fed8abbd616c4b90735648d809525079f985df17de2",
  "private": false,
  "record": {
    "abstract": "We confirmed the following idea by numerical calculation: The extended\nstructure of baryons may make the nuclear equation of state stiffer at higher\ndensity while keeping the compression modulus for normal nuclear matter around\nits empirical value $K=240MeV$.The model built in this wayy fits all empirical\ndata for normal nuclear matter and gives the mass limit of neutron stars\ncompatible with the observation.",
    "arxiv_id": "nucl-th/9210019",
    "authors": [
      "Qi-Ren Zhang",
      "Bo-Qiang Ma",
      "Walter Greiner"
    ],
    "categories": [
      "nucl-th",
      "astro-ph"
    ],
    "doi": "10.1088/0954-3899/18/12/020",
    "journal_ref": "J.Phys. G18 (1992) 2051-2060",
    "title": "Finite volume of baryons and the mass limit for neutron stars",
    "url": "https://arxiv.org/abs/nucl-th/9210019"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "cdde8198-37a0-4a7c-ac5a-6c8ff09ea2e1",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}