{
  "annotation_id": "9476cd01-06d3-4a14-a1b5-88a69b46e0ce",
  "date_created": "2026-03-02T18:00:01.591000Z",
  "date_modified": "2026-03-02T18:00:01.591000Z",
  "file_hash": "4918a2498e63ac8439f86ac6ccc864702383c20191224467fcff86ddde3f1f5f",
  "private": false,
  "record": {
    "abstract": "The linear chiral SU(3)*SU(3) model is applied to describe properties of the\ncompact star matter inside the quark, protoneutron and neutron star.The leads\nto the neutron star with the value of maximum mass close to 1.5 solar mass and\nradius 11 km and with the reduced value of proton fraction and very compact\nhyperon core.",
    "arxiv_id": "nucl-th/0411022",
    "authors": [
      "Ryszard Manka",
      "Ilona Bednarek"
    ],
    "categories": [
      "nucl-th"
    ],
    "journal_ref": "Fizika B13 (2004) 355-364",
    "title": "The compact star in the SU(3) sigma model",
    "url": "https://arxiv.org/abs/nucl-th/0411022"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "57cd7fc3-3953-4e3f-8041-1f4bd9bbb695",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}