{"paper":{"title":"Getting the Most from Detection of Galactic Supernova Neutrinos in Future Large Liquid-Scintillator Detectors","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"Jia-Shu Lu, Shun Zhou, Yu-Feng Li","submitted_at":"2016-05-25T09:57:39Z","abstract_excerpt":"Future large liquid-scintillator detectors can be implemented to observe neutrinos from a core-collapse supernova (SN) in our galaxy in various reaction channels: (1) The inverse beta decay $\\overline{\\nu}^{}_e + p \\to n + e^+$; (2) The elastic neutrino-proton scattering $\\nu + p \\to \\nu + p$; (3) The elastic neutrino-electron scattering $\\nu + e^- \\to \\nu + e^-$; (4) The charged-current $\\nu^{}_e$ interaction $\\nu^{}_e + {^{12}}{\\rm C} \\to e^- + {^{12}}{\\rm N}$; (5) The charged-current $\\overline{\\nu}^{}_e$ interaction $\\overline{\\nu}^{}_e + {^{12}}{\\rm C} \\to e^+ + {^{12}}{\\rm B}$; (6) The n"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1605.07803","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"}