{
  "annotation_id": "d00de086-63e7-40d1-ac44-75761ea12762",
  "date_created": "2026-03-02T18:00:22.406000Z",
  "date_modified": "2026-03-02T18:00:22.406000Z",
  "file_hash": "5c17f94838941629c18e3f8ebe75206606a54031478a5bb5c988367eae316573",
  "private": false,
  "record": {
    "abstract": "The sensitivity of the Sudbury Neutrino Observatory (SNO) to measure the\nshape of the recoil electron spectrum in the charged-current reaction of\n$^{8}$B solar neutrinos interacting with deuterium can be improved if the\nresults of a $^{8}$Li beta-decay calibration experiment are included in the\ntest. We calculate an improvement in sensitivity, under certain idealistic\nassumptions, of about a factor of 2, sufficient to resolve different\nneutrino-oscillation solutions to the solar-neutrino problem. We further\nexamine the role of recoil and radiative corrections on both the $^{8}$B\nneutrino spectrum and the $^{8}$Li electron spectrum and conclude that the\ninfluence of these effects on the ratio of the two spectra as measured by SNO\nis very small.",
    "arxiv_id": "nucl-th/9802078",
    "authors": [
      "G. Jonkmans",
      "I. S. Towner",
      "B. Sur"
    ],
    "categories": [
      "nucl-th"
    ],
    "doi": "10.1103/PhysRevC.58.1278",
    "journal_ref": "Phys.Rev.C58:1278-1287,1998",
    "title": "8Li electron spectrum versus 8B neutrino spectrum: implications for the   Sudbury Neutrino Observatory",
    "url": "https://arxiv.org/abs/nucl-th/9802078"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "7343603f-2597-4395-9442-a7f05779fde2",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}