{
  "annotation_id": "852fc57b-d3cc-480c-80eb-97d547bb8f13",
  "date_created": "2026-03-02T18:00:00.671000Z",
  "date_modified": "2026-03-02T18:00:00.671000Z",
  "file_hash": "8028050df63750acba2889357b4a1d7b50f2d383109b3f76deee37bcf573682d",
  "private": false,
  "record": {
    "abstract": "Superfluid properties of the inner crust matter of neutron stars, formed by\nnuclear clusters immersed in a dilute neutron gas, are analysed in a self-\nconsistent HFB approach. The calculations are performed with two pairing\nforces, fixed so as to obtain in infinite nuclear matter the pairing gaps\nprovided by the Gogny force or by induced interactions. It is shown that the\nnuclear clusters can either suppress or enhance the pairing correlations inside\nthe inner crust matter, depending on the density of the surrounding neutrons.\nThe profile of the pairing field in the inner crust is rather similar for both\npairing forces, but the values of the pairing gaps are drastically reduced for\nthe force which simulates the polarisation effects in infinite neutron matter.",
    "arxiv_id": "nucl-th/0402032",
    "authors": [
      "N. Sandulescu",
      "Nguyen Van Giai",
      "R. J. Liotta"
    ],
    "categories": [
      "nucl-th"
    ],
    "doi": "10.1103/PhysRevC.69.045802",
    "journal_ref": "Phys.Rev. C69 (2004) 045802",
    "title": "Superfluid Properties of the Inner Crust of Neutron Stars",
    "url": "https://arxiv.org/abs/nucl-th/0402032"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "38afc91e-3fa5-41b7-8cd0-73ba326ccccf",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}