{
  "annotation_id": "f92baa63-0ce2-4806-855e-b9a01cc815d7",
  "date_created": "2026-03-02T18:00:14.496000Z",
  "date_modified": "2026-03-02T18:00:14.496000Z",
  "file_hash": "b23b568f4d725960cc1dc06c90a4abc241dcf879cc6dfeb190814c3515318383",
  "private": false,
  "record": {
    "abstract": "The neutrino emissivity of compact stars is investigated in this work. We\nconsider stars consisting of nuclear as well as quark matter for this purpose.\nDifferent models are used to calculate the composition of nuclear and quark\nmatter and the neutrino emissivity. Depending on the model under consideration,\nthe neutrino emissivity of nuclear as well as quark matter varies over a wide\nrange. We find that for nuclear matter, the direct URCA processes are allowed\nfor most of the relativistic models without and with strange baryons, whereas\nfor the nonrelativistic models this shows a strong dependence on the type of\nnuclear interaction employed. When the direct URCA processes are allowed, the\nneutrino emissivity of hadronic matter is larger than that of the quark matter\nby several orders of magnitude. We also find that the neutrino emissivity\ndeparts from $T^6$ behavior when the temperature is larger than the difference\nin the Fermi momenta of the particles, participating in the neutrino-producing\nreactions.",
    "arxiv_id": "nucl-th/9509011",
    "authors": [
      "Sanjay K. Ghosh",
      "S. C. Phatak",
      "P. K. Sahu"
    ],
    "categories": [
      "nucl-th"
    ],
    "doi": "10.1142/S0218301396000190",
    "journal_ref": "Int.J.Mod.Phys. E5 (1996) 385-402",
    "title": "Neutrino Emissivity of Dense Stars",
    "url": "https://arxiv.org/abs/nucl-th/9509011"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "2fb31363-4042-4886-b1a5-904eb18ac4b3",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}