{
  "annotation_id": "024c1fd0-d5fe-4566-910e-d8e40a618c1d",
  "date_created": "2026-03-02T18:00:14.829000Z",
  "date_modified": "2026-03-02T18:00:14.829000Z",
  "file_hash": "b6702af72f86e457f065275a66eaaf1a6d3918a66268d3984922fae237d77865",
  "private": false,
  "record": {
    "abstract": "In this work we calculate neutron and proton energy gaps in neutron star\nmatter, using the Bonn meson--exchange interactions and a model--space approach\nto the gap equation. This approach allows a consistent calculation of energy\ngaps and single particle energies with the model--space\nBrueckner--Hartree--Fock (MBHF) method, without double counting of\ntwo--particle correlations. Neutron energy gaps are calculated at zero and\nfinite temperature. Proton energy gaps are calculated at beta equilibrium, and\nit is shown that the inclusion of muons has a significant effect. The results\nare compared with those of other works, and the implications for neutron star\nphysics are briefly discussed.",
    "arxiv_id": "nucl-th/9602020",
    "authors": [
      "O. Elgaroy",
      "L. Engvik",
      "M. Hjorth-Jensen",
      "E. Osnes"
    ],
    "categories": [
      "nucl-th"
    ],
    "doi": "10.1016/0375-9474(96)00152-2",
    "journal_ref": "Nucl.Phys. A604 (1996) 466-490",
    "title": "Model--space approach to $^{1}S_{0}$ neutron and proton pairing with the   Bonn meson--exchange potentials",
    "url": "https://arxiv.org/abs/nucl-th/9602020"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "7eb8bdda-5e1c-4975-b57a-387971e1a528",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}