{
  "annotation_id": "a39e718a-6e44-40cb-a184-05576fa84d59",
  "date_created": "2026-03-02T18:00:01.089000Z",
  "date_modified": "2026-03-02T18:00:01.089000Z",
  "file_hash": "9deadd03bb96e52266e4281dfbcab87ca714e7e308a211b79389705697cf190a",
  "private": false,
  "record": {
    "abstract": "We analyse the temperature dependence of pairing correlations in the inner\ncrust matter of neutron stars. The study is done in a finite-temperature HFB\napproach and by using a zero range pairing force adjusted to the pairing\nproperties of infinite neutron matter. Within the same approach we investigate\nhow the specific heat of the inner crust depends on temperature, matter\ninhomogeneity, and the assumption used for the pairing force. It is shown that\nin a physical relevant range of densities the pairing properties of inner crust\nmatter depend significantly on temperature. The finite-temperature HFB\ncalculations show also that the specific heat is rather sensitive to the\npresence of nuclear clusters inside the inner crust. However, the most dramatic\nchange of the specific heat is determined by the scenario used for the neutron\nmatter superfluidity.",
    "arxiv_id": "nucl-th/0403019",
    "authors": [
      "N. Sandulescu"
    ],
    "categories": [
      "nucl-th",
      "astro-ph"
    ],
    "doi": "10.1103/PhysRevC.70.025801",
    "journal_ref": "Phys.Rev. C70 (2004) 025801",
    "title": "Nuclear Superfluidity and Specific Heat in the Inner Crust of Neutron   Stars",
    "url": "https://arxiv.org/abs/nucl-th/0403019"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "3709e98d-e75b-4310-b02b-2b37cc435eb0",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}