{
  "annotation_id": "07a57aeb-2aac-49cd-ae7c-37908b45b373",
  "date_created": "2026-03-02T18:00:12.027000Z",
  "date_modified": "2026-03-02T18:00:12.027000Z",
  "file_hash": "61dd147883b2338ce95e8b5f1695ea4185b0486fe2e93a1b31234fdb27467d10",
  "private": false,
  "record": {
    "abstract": "We analyse the effect of neutron superfluidity on the cooling time of inner\ncrust matter in neutron stars, in the case of a rapid cooling of the core. The\nspecific heat of the inner crust, which determines the thermal response of the\ncrust, is calculated in the framework of HFB approach at finite temperature.\nThe calculations are performed with two paring forces chosen to simulate the\npairing properties of uniform neutron matter corresponding respectively to\nGogny-BCS approximation and to many-body techniques including polarisation\neffects. Using a simple model for the heat transport across the inner crust, it\nis shown that the two pairing forces give very different values for the cooling\ntime.",
    "arxiv_id": "nucl-th/0703064",
    "authors": [
      "C. Monrozeau",
      "J. Margueron",
      "N. Sandulescu"
    ],
    "categories": [
      "nucl-th"
    ],
    "doi": "10.1103/PhysRevC.75.065807",
    "journal_ref": "Phys.Rev.C75:065807,2007",
    "title": "Nuclear Superfluidity and Cooling Time of Neutron-Star Crust",
    "url": "https://arxiv.org/abs/nucl-th/0703064"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "90860af6-9a56-4385-9bee-c280e8608bde",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}