{
  "annotation_id": "d99d59ef-0344-4e7a-8d57-487c48474bcc",
  "date_created": "2026-03-02T18:00:25.262000Z",
  "date_modified": "2026-03-02T18:00:25.262000Z",
  "file_hash": "a45cd01dbc6a5723e09a211864b3dd24193b36cff64ee4e7d9f6e43253636beb",
  "private": false,
  "record": {
    "abstract": "Brueckner-Hartree-Fock calculations are performed for nuclear matter with an\nexact treatment of the Pauli exclusion operator in the Bethe-Goldstone\nequation. The differences in the calculated binding energy, compared to the\nangle-average approximation, which is commonly used, are non-negligible. These\ndifference exhibits a specific density dependence, which shifts the calculated\nsaturation point towards smaller densities. This effect is observed for various\nversions of modern models for the NN interaction.",
    "arxiv_id": "nucl-th/9812011",
    "authors": [
      "E. Schiller",
      "H. M\u00fcther",
      "P. Czerski"
    ],
    "categories": [
      "nucl-th"
    ],
    "doi": "10.1103/PhysRevC.59.2934 10.1103/PhysRevC.60.059901",
    "journal_ref": "Phys.Rev.C59:2934-2936,1999; Erratum-ibid.C60:059901,1999",
    "title": "Pauli exclusion operator and binding energy of nuclear matter",
    "url": "https://arxiv.org/abs/nucl-th/9812011"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "82a930fc-c5cc-4206-aced-c82733d3c195",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}