{
  "annotation_id": "c7984fc7-bcfa-4be0-87de-03a599a12997",
  "date_created": "2026-03-02T18:00:15.357000Z",
  "date_modified": "2026-03-02T18:00:15.357000Z",
  "file_hash": "b3f8ae3259c09998ee418d9a16e320d79ad7ccbd0eca6084f545871b15fdd8cd",
  "private": false,
  "record": {
    "abstract": "Shell-model calculations of solar neutrino absorption cross sections for\n$^{40}$Ar, the proposed component of the ICARUS detector, are presented. It is\nfound that low-lying Gamow-Teller transitions lead to a significant enhancement\nof the absorption rate over that expected from the Fermi transition between the\nisobaric analog states, leading to an overall absorption rate of 6.7 SNU. We\nalso note that the pertinent Gamow-Teller transitions in $^{\\sss 40}$Ar are\nexperimentally accessible from the $\\beta$-decay of the mirror nucleus $^{\\sss\n40}$Ti. Predictions for the branching ratios to states in $^{\\sss 40}$Sc are\npresented, and the theoretical halflife of 53~ms is found to be in good\nagreement with the experimental value of $56^{+18}_{-12}$~ms.",
    "arxiv_id": "nucl-th/9405007",
    "authors": [
      "W. E. Ormand",
      "P. M. Pizzochero",
      "P. F. Bortignon",
      "R. A. Broglia"
    ],
    "categories": [
      "nucl-th"
    ],
    "doi": "10.1016/0370-2693(94)01605-C",
    "journal_ref": "Phys.Lett. B345 (1995) 343-350",
    "title": "Neutrino Capture Cross Sections for Ar-40 and beta-decay of Ti-40",
    "url": "https://arxiv.org/abs/nucl-th/9405007"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "5f2fde57-5a9c-433c-926c-13409944112c",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}