{
  "annotation_id": "2b9b35e5-d45c-46e6-a007-69ab14a81361",
  "date_created": "2026-03-02T18:00:25.309000Z",
  "date_modified": "2026-03-02T18:00:25.309000Z",
  "file_hash": "75058c2eb5091881d7d10dabef5d1aa68e31256bee998e799799715bfb06c8b6",
  "private": false,
  "record": {
    "abstract": "Recent equations of state for dense nuclear matter are discussed with\npossible phase transitions arising in neutron stars such as pion, kaon and\nhyperon kondensation, superfluidity and quark matter. Specifically, we treat\nthe nuclear to quark matter phase transition, the possible mixed phase and its\nstructure. A number of numerical calculations of rotating neutron stars with\nand without phase transitions are given and compared to observed masses, radii,\ntemperatures and glitches.",
    "arxiv_id": "nucl-th/9902033",
    "authors": [
      "H. Heiselberg",
      "M. Hjorth-Jensen"
    ],
    "categories": [
      "nucl-th",
      "astro-ph",
      "hep-ph"
    ],
    "doi": "10.1016/S0370-1573(99)00110-6",
    "journal_ref": "Phys.Rept. 328 (2000) 237-327",
    "title": "Phases of dense matter in neutron stars",
    "url": "https://arxiv.org/abs/nucl-th/9902033"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "fab1d94d-fbbc-4647-b92c-8dde3a235dce",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}