{
  "annotation_id": "e7c6987b-023c-46db-8013-2025e1d3092d",
  "date_created": "2026-03-02T18:00:15.182000Z",
  "date_modified": "2026-03-02T18:00:15.182000Z",
  "file_hash": "81044f7a36f2d897657d416ee3ac140c0206b6c821929f82d11173ccfcc11880",
  "private": false,
  "record": {
    "abstract": "We develop the Redfield equation for delta-correlated gaussian noise and\napply it to the case of two neutrino flavor or spin precession in the presence\nof a noisy matter density or magnetic field, respectively. The criteria under\nwhich physical fluctuations can be well approximated by the delta-correlated\ngaussian noise for the above cases are examined. Current limits on the possible\nneutrino magnetic moment and solar magnetic field suggest that a reasonably\nnoisy solar magnetic field would not appreciably affect the solar electron\nneutrino flux. However, if the solar electron density has fluctuations of a few\npercent of the local density and a small enough correlation length, the MSW\neffect is suppressed for a range of parameters.",
    "arxiv_id": "nucl-th/9406003",
    "authors": [
      "F. N. Loreti",
      "A. B. Balantekin"
    ],
    "categories": [
      "nucl-th",
      "astro-ph",
      "hep-ph"
    ],
    "doi": "10.1103/PhysRevD.50.4762",
    "journal_ref": "Phys.Rev.D50:4762-4770,1994",
    "title": "Neutrino Oscillations in Noisy Media",
    "url": "https://arxiv.org/abs/nucl-th/9406003"
  },
  "schema_id": "dorsal/arxiv",
  "source": {
    "execution_id": "dd454de4-da1c-428f-900e-8c8f420975b8",
    "id": "arXiv Dataset IDs",
    "type": "Model",
    "variant": "snapshot-2026-03-01",
    "version": "0.1.0"
  },
  "user_id": 1000002
}