{
  "annotation_id": "0ddf1f37-5acb-4bb7-8359-01aaa2c6c4ee",
  "date_created": "2026-03-02T18:00:14.929000Z",
  "date_modified": "2026-03-02T18:00:14.929000Z",
  "file_hash": "51ef3e139675e65f4ae83f6092785d5e76091571be37401c935731aaa6886167",
  "private": false,
  "record": {
    "abstract": "We argue that, prior to the recent GALLEX $^{51}$Cr source experiment, the\nexcited state contributions to the $^{71}$Ga capture cross section for\n$^{51}$Cr and $^7$Be neutrinos were poorly constrained, despite forward-angle\n(p,n) measurements. We describe the origin of the uncertainties and estimate\ntheir extent. We explore the implications of the source experiment for solar\nneutrino capture in light of these uncertainties. A reanalysis of the $^7$Be\nand $^8$B flux constraints and MSW solutions of the solar neutrino puzzle is\npresented.",
    "arxiv_id": "nucl-th/9503017",
    "authors": [
      "Naoya Hata",
      "Wick Haxton"
    ],
    "categories": [
      "nucl-th",
      "astro-ph",
      "hep-ph"
    ],
    "doi": "10.1016/0370-2693(95)00598-F",
    "journal_ref": "Phys.Lett. B353 (1995) 422-431",
    "title": "Implications of the GALLEX Source Experiment for the Solar Neutrino   Problem",
    "url": "https://arxiv.org/abs/nucl-th/9503017"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "a7f90adb-6949-4a35-a5da-5c95a83ed63c",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}