{
  "annotation_id": "6e2e5581-a5ed-4d87-91ee-3e0c3f49f3b0",
  "date_created": "2026-03-02T18:00:01.252000Z",
  "date_modified": "2026-03-02T18:00:01.252000Z",
  "file_hash": "471b2fd825f6b131411f67c541be76e2394a78b8dcefff525fdefbe231d1faa2",
  "private": false,
  "record": {
    "abstract": "For neutron stars with hyperon-mixed core, neutrino emissivity is studied\nunder the equation of state, obtained by introducing repulsive three-body force\nuniversal for all baryons so as to assure the maximum mass compatible with the\nobservation. By paying attention to the density-dependence of critical\ntemperatures of baryon superfluids, which reflect the nature of baryon-baryon\ninteraction and control neutron star cooling, we show what neutrino emission\nprocesses are efficient in the regions with and without hyperon mixing and\nremark its implications related to neutron star cooling.",
    "arxiv_id": "nucl-th/0402011",
    "authors": [
      "T. Takatsuka",
      "R. Tamagaki"
    ],
    "categories": [
      "nucl-th"
    ],
    "doi": "10.1143/PTP.112.37",
    "journal_ref": "Prog.Theor.Phys. 112 (2004) 37-72",
    "title": "Baryon superfluidity and neutrino emissivity of neutron stars",
    "url": "https://arxiv.org/abs/nucl-th/0402011"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "b53f6fa6-b9d8-4ae6-9efa-e709dc0f75a4",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}