{"paper":{"title":"Analysis of a three flavor neutrino oscillation fit to recent Super-Kamiokande data","license":"","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"Christoph Meier, Tommy Ohlsson","submitted_at":"1999-10-07T15:27:15Z","abstract_excerpt":"We have analyzed the most recent available Super-Kamiokande data in a three flavor neutrino oscillation model. We have here neglected possible matter effects and performed a fit to atmospheric and solar Super-Kamiokande data. We have investigated a large parameter range, where the mixing angles were restricted to $0 \\leq \\theta_i \\leq \\pi/2$, $ i=1,2,3$, and the mass squared differences were taken to be in the intervals $10^{-11} {\\rm eV}^2 \\leq \\Delta m^2 \\leq 10^{-2} {\\rm eV}^2$ and $10^{-4} {\\rm eV}^2 \\leq \\Delta M^2 \\leq 10 {\\rm eV}^2$. This yielded a best solution characterized by the par"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"hep-ph/9910270","kind":"arxiv","version":2},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"}