{
  "annotation_id": "a3980491-20e5-481d-85aa-1f62d4a18425",
  "date_created": "2026-03-02T18:00:01.136000Z",
  "date_modified": "2026-03-02T18:00:01.136000Z",
  "file_hash": "7965b933ab6a5447a1f6e0007bc73d1a8ebab5f0ec31c0452e068ca188950728",
  "private": false,
  "record": {
    "abstract": "This talk reviews three inputs important to neutrino-induced nucleosynthesis\nin a supernova: 1) \"standard\" properties of the supernova neutrino flux, 2)\neffects of phenomena like neutrino oscillations on that flux, and 3) nuclear\nstructure issues in estimating cross sections for neutrino-nucleus\ninteractions. The resulting possibilities for neutrino-induced nucleosynthesis\n-- the neutrino-process -- in massive stars are discussed. This includes two\nrelatively recent extensions of neutrino-process calculations to heavier\nnuclei, one focused on understanding the origin of 138La and 180Ta and the\nsecond on the effects following r-process freezeout. From calculations of the\nneutrino post-processing of the r-process distribution, limits can be placed on\nthe neutrino fluence after freezeout and thus on the dynamic timescale for the\nexpansion of the \"hot bubble.\"",
    "arxiv_id": "nucl-th/0406012",
    "authors": [
      "W. C. Haxton"
    ],
    "categories": [
      "nucl-th",
      "astro-ph",
      "hep-ph"
    ],
    "doi": "10.1142/9789812702470_0009",
    "title": "Supernova Neutrino-Nucleus Physics and the r-process",
    "url": "https://arxiv.org/abs/nucl-th/0406012"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "14c5f079-1d33-4fe1-8c86-00b63e7231ab",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}