{"paper":{"title":"Can a mass inversion save solar neutrino oscillations from the Los Alamos neutrino?","license":"","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"G. Raffelt (MPI f. Physik, J.~Silk (UC Berkeley), Munich)","submitted_at":"1995-02-15T12:35:23Z","abstract_excerpt":"In the light of the $\\nu_\\mu\\to\\nu_e$ neutrino oscillations which may have been observed at the LSND experiment we explore the consequences of two inverted mass schemes where solar neutrino oscillations occur between $\\nu_e$ and $\\nu_\\tau$. The favored LSND value $\\Delta m^2=6\\,\\eV^2$ leads to $m_{\\nu_e}\\approx m_{\\nu_\\tau}\\approx 2.5\\,\\eV$ and $m_{\\nu_\\mu}\\approx0$ so that cosmology can benefit from a recently proposed ``cold plus hot dark matter'' structure formation scenario with two equal mass light neutrinos (C$\\nu^2$DM). Solar neutrino oscillations ($\\nu_e\\to\\nu_\\tau$) can occur with one"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"hep-ph/9502306","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"}