{
  "annotation_id": "e600554c-0421-4c9e-acab-3b0cce639e86",
  "date_created": "2026-03-02T18:00:12.083000Z",
  "date_modified": "2026-03-02T18:00:12.083000Z",
  "file_hash": "b18c1e941219ce7aaf8d082b222a202ead949c9bfae11402eafb329cc399fff3",
  "private": false,
  "record": {
    "abstract": "We discuss and improve a recent treatment of the absorption of solar\nneutrinos by ${}^{127}$I, in connection with a proposed solar neutrino\ndetector. With standard-solar-model fluxes and an in-medium value of -1.0 for\nthe axial-vector coupling constant $g_A$, we obtain a ${}^8$B-neutrino cross\nsection of 3.3$\\times 10^{-42}$, about 50\\% larger than in our previous work,\nand a ${}^7$Be cross section that is less certain but nevertheless also larger\nthan before. We then apply the improved techniques to higher incoming energies\nthat obtain at the LAMPF beam dump, where an experiment is underway to finalize\na calibration of the ${}^{127}$I with electron neutrinos from muon decay. We\nfind that forbidden operators, which play no role in solar-neutrino absorption,\ncontribute nonnegligibly to the LAMPF cross section, and that the preliminary\nLAMPF mean value is significantly larger than our prediction.",
    "arxiv_id": "nucl-th/9402022",
    "authors": [
      "J. Engel",
      "S. Pittel",
      "P. Vogel"
    ],
    "categories": [
      "nucl-th"
    ],
    "doi": "10.1103/PhysRevC.50.1702",
    "journal_ref": "Phys.Rev.C50:1702-1708,1994",
    "title": "Capture of Solar and Higher-Energy Neutrinos by Iodine 127",
    "url": "https://arxiv.org/abs/nucl-th/9402022"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "fa49ae20-e1b3-455d-a026-dabc292dbdbd",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}