{
  "annotation_id": "275fae61-5c81-47fd-9d75-3e65cd481e44",
  "date_created": "2026-03-02T18:00:12.029000Z",
  "date_modified": "2026-03-02T18:00:12.029000Z",
  "file_hash": "f6b346ee428d209f97b98a02f00d8602dbd9112ad3f61641b97d8a3850106fe7",
  "private": false,
  "record": {
    "abstract": "We examine several phenomena beyond the scope of Fermi-gas models that affect\nthe quasielastic scattering (from oxygen) of neutrinos in the 0.1 -- 3.0 GeV\nrange. These include Coulomb interactions of outgoing protons and leptons, a\nrealistic finite-volume mean field, and the residual nucleon-nucleon\ninteraction. None of these effects are accurately represented in the Monte\nCarlo simulations used to predict event rates due to $\\mu$ and $e$ neutrinos\nfrom cosmic-ray collisions in the atmosphere. We nevertheless conclude that the\nneglected physics cannot account for the anomalous $\\mu$ to $e$ ratio observed\nat Kamiokande and IMB, and is unlikely to change absolute event rates by more\nthan 10--15\\%. We briefly mention other phenomena, still to be investigated in\ndetail, that may produce larger changes.",
    "arxiv_id": "nucl-th/9304017",
    "authors": [
      "J. Engel",
      "E. Kolbe",
      "K. Langanke",
      "P. Vogel"
    ],
    "categories": [
      "nucl-th",
      "hep-ph"
    ],
    "doi": "10.1103/PhysRevD.48.3048",
    "journal_ref": "Phys.Rev.D48:3048-3054,1993",
    "title": "Quasielastic neutrino scattering from oxygen and the atmospheric   neutrino problem",
    "url": "https://arxiv.org/abs/nucl-th/9304017"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "41374887-e444-42e0-ac9b-f68c0f5a6751",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}