{
  "annotation_id": "e2e69faf-c021-48e6-b052-8d3920bf736d",
  "date_created": "2026-03-02T18:00:25.254000Z",
  "date_modified": "2026-03-02T18:00:25.254000Z",
  "file_hash": "6450b2da47183731b3136723a6172dc5f052408bda208d57de343cbeb6c47701",
  "private": false,
  "record": {
    "abstract": "The phase transition between the nuclear matter and the quark matter is\nexamined. The relativistic mean field theory(RMF) is consider with interacting\nnucleons and mesons using TM1 parameter set for the nuclear matter equations of\nstate. It is found that the trasition point depends on coupling constant\n$\\alpha_s$ and bag pressure. From the study of the structure of a hybrid\nneutron star, it is observed that the star contains quark matter in the\ninterior and neutron matter on the outer perifery.",
    "arxiv_id": "nucl-th/9811041",
    "authors": [
      "S. Acharya",
      "L. Maharana",
      "R. Mohanty",
      "P. K. Panda"
    ],
    "categories": [
      "nucl-th"
    ],
    "doi": "10.1142/S0218301399000082",
    "journal_ref": "Int.J.Mod.Phys. E8 (1999) 107-120",
    "title": "Phase Transition and Hybrid Star in a Nonlinear $\\sigma - \\omega$ model",
    "url": "https://arxiv.org/abs/nucl-th/9811041"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "9f2a23de-2b52-4b33-a152-d909a75ef5fe",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}