{
  "annotation_id": "490d5f85-53fb-4fb5-8935-afb422333716",
  "date_created": "2026-03-02T18:00:21.917000Z",
  "date_modified": "2026-03-02T18:00:21.917000Z",
  "file_hash": "7eb8fc749b71fa11bd33488b69186cc49f179b1ae3055e9799a3348acbf407ff",
  "private": false,
  "record": {
    "abstract": "The microscopic structure of an isolated vortex line in superfluid neutron\nstar matter is studied by solving the Bogoliubov-de Gennes equations. Our\ncalculation, which is the starting point for a microscopic calculation of\npinning forces in neutron stars, shows that the size of the vortex core varies\ndifferently with density, and is in general smaller than assumed in some\nearlier calculations of vortex pinning in neutron star crusts. The implications\nof this result are discussed",
    "arxiv_id": "nucl-th/9808057",
    "authors": [
      "F. V. De Blasio",
      "O. Elgaroy"
    ],
    "categories": [
      "nucl-th",
      "astro-ph"
    ],
    "doi": "10.1103/PhysRevLett.82.1815",
    "journal_ref": "Phys.Rev.Lett.82:1815-1818,1999",
    "title": "Microscopic structure of a vortex line in superfluid neutron star matter",
    "url": "https://arxiv.org/abs/nucl-th/9808057"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "0f278a65-27e0-4841-a0c5-a3c7a0e9a7d3",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}