{
  "annotation_id": "dc91a738-5a9c-4feb-a6ac-71242b4f5b73",
  "date_created": "2026-03-02T18:00:15.416000Z",
  "date_modified": "2026-03-02T18:00:15.416000Z",
  "file_hash": "fccb9384cb91ec15fd4c0a56a019ad3e7855030dcb88bd1b240552b8a9849de1",
  "private": false,
  "record": {
    "abstract": "In this work we present results for pairing gaps in $\\beta$--stable neutron\nstar matter with electrons and muons using a relativistic\nDirac--Brueckner--Hartree--Fock approach, starting with modern meson--exchange\nmodels for the nucleon--nucleon interaction. Results are given for\nsuperconducting $^1S_0$ protons and $^3P_2$ and $^1D_2$ neutron superfluids. A\ncomparison is made with recent non--relativistic calculations and the\nimplications for neutron star cooling are discussed.",
    "arxiv_id": "nucl-th/9604041",
    "authors": [
      "Oe. Elgaroey",
      "L. Engvik",
      "M. Hjorth-Jensen",
      "E. Osnes"
    ],
    "categories": [
      "nucl-th"
    ],
    "doi": "10.1103/PhysRevLett.77.1428",
    "journal_ref": "Phys.Rev.Lett.77:1428-1431,1996",
    "title": "Superfluidity in beta-stable neutron star matter",
    "url": "https://arxiv.org/abs/nucl-th/9604041"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "8d48d24e-a542-446f-b1f6-ffba4fe79f81",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}