{"paper":{"title":"Global analysis of Solar neutrino oscillation evidence including SNO and implications for Borexino","license":"","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"E. Torrente-Lujan, M. Picariello, P. Aliani, V. Antonelli","submitted_at":"2001-11-29T18:36:02Z","abstract_excerpt":"An updated analysis of all available neutrino oscillation evidence in Solar experiments including the latest $SNO$ data is presented. Predictions for total rates and day-night asymmetry in Borexino are calculated. Our analysis features the use of exhaustive computation of the neutrino oscillation probabilities and the use of an improved statistical $\\chi^2$ minimization.\n  In the framework of two neutrino oscillations we conclude that the best fit to the data is obtained in the LMA region with parameters $(\\Delta m^2, \\tan^2\\theta) = (5.2 \\times 10^{-5} \\eV^2, 0.47)$, ($\\chi^2_{min}/n=0.82$, $"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"hep-ph/0111418","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"}