{
  "annotation_id": "43045652-2a82-4cf6-8149-6f49c93fd10a",
  "date_created": "2026-03-02T18:00:18.887000Z",
  "date_modified": "2026-03-02T18:00:18.887000Z",
  "file_hash": "cf8ff48455c009b48ccfad271bd074f1a51a250a5c90c1c705f2b20a219002c8",
  "private": false,
  "record": {
    "abstract": "The prediction of cross sections for nuclei far off stability is crucial in\nthe field of nuclear astrophysics. For spherical nuclei close to the dripline\nthe statistical model (Hauser-Feshbach) approach is not applicable and direct\ncontributions may dominate the cross sections. For neutron-rich, even-even Sn\ntargets, we compare the resulting neutron capture cross sections when\nconsistently taking the input for the direct capture calculations from three\ndifferent microscopic models. The results underline the sensitivity of cross\nsections calculated in the direct model to nuclear structure models which can\nlead to high uncertainties when lacking experimental information.",
    "arxiv_id": "nucl-th/9609007",
    "authors": [
      "T. Rauscher",
      "K. -L. Kratz",
      "H. Oberhummer",
      "J. Dobaczewski",
      "P. Moeller",
      "M. Sharma"
    ],
    "categories": [
      "nucl-th",
      "astro-ph"
    ],
    "doi": "10.1016/S0375-9474(97)00265-0",
    "journal_ref": "Nucl.Phys. A621 (1997) 327c-330c",
    "title": "Uncertainties In Direct Neutron Capture Calculations Due To Nuclear   Structure Models",
    "url": "https://arxiv.org/abs/nucl-th/9609007"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "9bac5aee-7e52-45b0-a825-d670e6a6ad3f",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}