{"paper":{"title":"Analysis of neutrino oscillation in three-flavor neutrinos","license":"","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"O. Inagaki, T. Sakai, T. Teshima","submitted_at":"1998-01-13T09:05:20Z","abstract_excerpt":"We analyzed the solar, terrestrial and atmospheric neutrinos experiments using the three-flavor neutrino framework and got the allowed regions for parameters (\\Delta m_{12}^2, \\sin^22\\theta_{12}, \\Delta m_{23}^2, \\theta_{13}, \\theta_{23}). In solar neutrino experiments, we got the large angle solution (\\Delta m_{12}^2, \\sin^22\\theta_{12})=(4x10^{-6}\n - 7x10^{-5}eV^2, 0.6 - 0.9) and small angle solution (3x10^{-6} - 1.2x10^{-5}eV^2, 0.003 - 0.01) for \\theta_{13}=0^\\circ - 20^\\circ. From the terrestrial and atmospheric neutrino experiments, we got the allowed regions (\\theta_{13}<4^\\circ, 24^\\ci"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"hep-ph/9801276","kind":"arxiv","version":1},"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"}