{
  "annotation_id": "4c551921-498d-4282-8816-264d1985e9ad",
  "date_created": "2026-03-02T18:00:08.131000Z",
  "date_modified": "2026-03-02T18:00:08.131000Z",
  "file_hash": "f4dc8be080924d7594ab12b437ac792153f3e4203bae2b20e11ad4692bdeeaec",
  "private": false,
  "record": {
    "abstract": "Precise nuclear reaction rates are needed for a detailed description of the\nproduction of elements in primordial nucleosynthesis and during the hydrostatic\nburning of stars to constrain the astrophysical models. The relevant reactions\nare extremely difficult to measure directly in the laboratory at the small\nastrophysical energies. In recent years direct reactions methods have been\ndeveloped and applied to extract low-energy astrophysical S factors. The\napplication of these methods requires a combination of experimental and\ntheoretical efforts. This contribution focuses on the underlying reaction\ntheories that have to be well understood in order to assess the precision and\nlimitations of the various approaches.",
    "arxiv_id": "nucl-th/0607015",
    "authors": [
      "C. A. Bertulani"
    ],
    "categories": [
      "nucl-th"
    ],
    "journal_ref": "PoSNIC-IX:040,2006",
    "title": "Direct reactions in/for astrophysics",
    "url": "https://arxiv.org/abs/nucl-th/0607015"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "52c77b85-5b6a-4de9-b084-1ec5fea5570c",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}