{
  "annotation_id": "fd657604-4930-40b2-9293-c3fafc4744f5",
  "date_created": "2026-03-02T18:00:28.096000Z",
  "date_modified": "2026-03-02T18:00:28.096000Z",
  "file_hash": "283926c399e0b6321d7caa90e819f54647a57779ba84d887bf3ba49bcc0b242f",
  "private": false,
  "record": {
    "abstract": "In this paper the equation of state of hot neutron matter is calculated.\n  Involving the Oppenheimer-Volkov-Tolman equation global parameters of a\nneutron star at the finite temperature are obtained. The objective of our work\nwas to study the influence of the temperature on the main parameters of a\nneutron star.",
    "arxiv_id": "nucl-th/9912039",
    "authors": [
      "Ilona Bednarek",
      "Ryszard Manka"
    ],
    "categories": [
      "nucl-th"
    ],
    "doi": "10.1238/Physica.Regular.061a00544",
    "title": "The hot neutron star",
    "url": "https://arxiv.org/abs/nucl-th/9912039"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "eee81ff3-5ca5-4c51-abd5-375abce09bbc",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}