{
  "annotation_id": "1ff80ae9-0bd4-4404-a44a-f22ddb201d09",
  "date_created": "2026-03-02T18:00:21.721000Z",
  "date_modified": "2026-03-02T18:00:21.721000Z",
  "file_hash": "e1f8e706109714e1e6dd4b5b840fb7a12e742363337639d5ef5a408207ba4aff",
  "private": false,
  "record": {
    "abstract": "Updated stellar rates for the reaction 23Mg(p,gamma)24Al are calculated by\nusing all available experimental information on 24Al excitation energies.\nProton and gamma-ray partial widths for astrophysically important resonances\nare derived from shell model calculations. Correspondences of experimentally\nobserved 24Al levels with shell model states are based on application of the\nisobaric multiplet mass equation. Our new rates suggest that the\n23Mg(p,gamma)24Al reaction influences the nucleosynthesis in the mass A\u003e20\nregion during thermonuclear runaways on massive white dwarfs.",
    "arxiv_id": "nucl-th/9806018",
    "authors": [
      "H. Herndl",
      "M. Fantini",
      "C. Iliades",
      "P. M. Endt",
      "H. Oberhummer"
    ],
    "categories": [
      "nucl-th",
      "astro-ph"
    ],
    "doi": "10.1103/PhysRevC.58.1798",
    "journal_ref": "Phys.Rev.C58:1798-1803,1998",
    "title": "Thermonuclear Reaction Rate of 23Mg(p,gamma)24$Al",
    "url": "https://arxiv.org/abs/nucl-th/9806018"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "c389ac8f-9b39-4039-92f6-99f57bd6fbec",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}