{
  "annotation_id": "a63d1bd7-541a-4704-b9e9-9e3680bd607f",
  "date_created": "2026-03-02T18:00:11.524000Z",
  "date_modified": "2026-03-02T18:00:11.524000Z",
  "file_hash": "73e82869813add09878e090db4ab1999e25a3ca08424a2a1d76a6bbf5067da1c",
  "private": false,
  "record": {
    "abstract": "Nuclear superfludity in exotic nuclei close to the drip lines and in the\ninner crust matter of neutron stars have common features which can be treated\nwith the same theoretical tools. In the first part of my lecture I discuss how\ntwo such tools, namely the HFB approach and the linear response theory can be\nused to describe the pairing correlations in weakly bound nuclei, in which the\nunbound part of the energy spectrum becomes important. Then, using the same\nmodels, I shall discuss how the nuclear superfluidity can affect the thermal\nproperties of the inner crust of neutron stars.",
    "arxiv_id": "nucl-th/0612047",
    "authors": [
      "Nicolae Sandulescu"
    ],
    "categories": [
      "nucl-th"
    ],
    "doi": "10.1142/9789812770417_0013",
    "title": "Nuclear Superfluidity in Exotic Nuclei and Neutron Stars",
    "url": "https://arxiv.org/abs/nucl-th/0612047"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "23e1d9bb-de1d-4f36-8a59-5271e2c478dc",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}