{
  "annotation_id": "cb797e58-f395-4ba8-8492-b7eb64e64b3c",
  "date_created": "2026-03-02T18:00:01.190000Z",
  "date_modified": "2026-03-02T18:00:01.190000Z",
  "file_hash": "7eef4c10cf1d9fcb5b11e85709bbe4b55d3c063293c2e9edc85061d452b2f6f1",
  "private": false,
  "record": {
    "abstract": "Astrophysical reaction rates are sensitive to the parity distribution at low\nexcitation energies. We combine a formula for the energy-dependent parity\ndistribution with a microscopic-macroscopic nuclear level density. This\napproach describes well the transition from low excitation energies, where a\nsingle parity dominates, to high excitations where the two densities are equal.",
    "arxiv_id": "nucl-th/0407043",
    "authors": [
      "D. Mocelj",
      "T. Rauscher",
      "G. Martinez-Pinedo",
      "K. Langanke",
      "L. Pacearescu",
      "A. Faessler",
      "F. -K. Thielemann"
    ],
    "categories": [
      "nucl-th"
    ],
    "doi": "10.1016/j.nuclphysa.2005.05.032",
    "journal_ref": "Nucl.Phys. A758 (2005) 154-157",
    "title": "Parity-Dependence in the Nuclear Level Density",
    "url": "https://arxiv.org/abs/nucl-th/0407043"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "5958a7eb-e980-438c-8512-bfea1fcb839c",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}