{
  "annotation_id": "8e66684e-fa08-46cd-a624-c601969d56c6",
  "date_created": "2026-03-02T18:01:00.751000Z",
  "date_modified": "2026-03-02T18:01:00.751000Z",
  "file_hash": "007367c3d474ec4957c5fc5a006a00c48179687d450ff1c3b26170c12f41d423",
  "private": false,
  "record": {
    "abstract": "We show that liquid organic scintillator detectors (e.g., KamLAND and\nBorexino) can measure the 8B solar neutrino flux by means of the nu_e charged\ncurrent interaction with the 13C nuclei naturally contained in the\nscintillators. The neutrino events can be identified by exploiting the time and\nspace coincidence with the subsequent decay of the produced 13N nuclei. We\nperform a detailed analysis of the background in KamLAND, Borexino and in a\npossible liquid scintillator detector at SNOLab, showing that the 8B solar\nneutrino signal can be extracted with a reasonable uncertainty in a few years\nof data taking. KamLAND should be able to extract about 18 solar neutrino\nevents from the already collected data. Prospects for gigantic scintillator\ndetectors (such as LENA) are also studied.",
    "arxiv_id": "physics/0506171",
    "authors": [
      "A. Ianni",
      "D. Montanino",
      "F. L. Villante"
    ],
    "categories": [
      "physics.ins-det",
      "astro-ph",
      "hep-ex",
      "hep-ph"
    ],
    "doi": "10.1016/j.physletb.2005.08.122",
    "journal_ref": "Phys.Lett. B627 (2005) 38-48",
    "title": "How to observe 8B solar neutrinos in liquid scintillator detectors",
    "url": "https://arxiv.org/abs/physics/0506171"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "7359f442-89fa-4ec3-bde9-34db084e4eea",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}