{
  "annotation_id": "8d2fa8f3-5cd0-4926-acc7-adf1e0024ff6",
  "date_created": "2026-03-02T18:00:25.905000Z",
  "date_modified": "2026-03-02T18:00:25.905000Z",
  "file_hash": "691b97d301a7aeccf6bda3a05a8f0cd713d079a51febde8b7c73905fbb88ed01",
  "private": false,
  "record": {
    "abstract": "The reaction rates of neutron capture reactions on light nuclei are important\nfor reliably simulating nucleosynthesis in a variety of stellar scenarios.\nNeutron capture reaction rates on neutron-rich C-, N-, and O-isotopes are\ncalculated in the framework of a hybrid compound and direct capture model. The\nresults are tabulated and compared with the results of previous calculations as\nwell as with experimental results.",
    "arxiv_id": "nucl-th/9908087",
    "authors": [
      "H. Herndl",
      "R. Hofinger",
      "J. Jank",
      "H. Oberhummer",
      "J. Goerres",
      "M. Wiescher",
      "F. -K. Thielemann",
      "B. A. Brown"
    ],
    "categories": [
      "nucl-th",
      "astro-ph",
      "nucl-ex"
    ],
    "doi": "10.1103/PhysRevC.60.064614",
    "journal_ref": "Phys.Rev.C60:064614,1999",
    "title": "Reaction rates for Neutron Capture Reactions to C-, N- and O-isotopes to   the neutron rich side of stability",
    "url": "https://arxiv.org/abs/nucl-th/9908087"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "5658543e-7a6f-4290-a87b-bb565cbdd085",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}