{
  "annotation_id": "dc85b0ca-ac28-447e-97e3-30e4f7b9a4e8",
  "date_created": "2026-03-02T18:00:15.303000Z",
  "date_modified": "2026-03-02T18:00:15.303000Z",
  "file_hash": "a520b315f32ee26839dd4b9693d195d98c8e1e46e9973b056b45853ea7fba7b9",
  "private": false,
  "record": {
    "abstract": "We suggest that photons with energies between 5 and 10 MeV, generated by the\n($\\nu,\\nu\u0027p\\gamma$) and ($\\nu,\\nu\u0027n\\gamma$) reactions on $^{16}$O, constitute a\nsignal which allows a unique identification of supernova $\\nu_\\mu$ and\n$\\nu_\\tau$ neutrinos in water \\v{C}erenkov detectors. We calculate the yield of\nsuch $\\gamma$ events and estimate that a few hundred of them would be detected\nin Superkamiokande for a supernova at 10 kpc distance.",
    "arxiv_id": "nucl-th/9511032",
    "authors": [
      "K. Langanke",
      "P. Vogel",
      "E. Kolbe"
    ],
    "categories": [
      "nucl-th",
      "astro-ph"
    ],
    "doi": "10.1103/PhysRevLett.76.2629",
    "journal_ref": "Phys.Rev.Lett. 76 (1996) 2629-2632",
    "title": "Signal for supernova $\\nu_\\mu$ and $\\nu_\\tau$ neutrinos in water   \\v{C}erenkov detectors",
    "url": "https://arxiv.org/abs/nucl-th/9511032"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "d55a2d50-4bec-41c2-a81c-b939408b3d4c",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}