{"paper":{"title":"Study of the effect of neutrino oscillation on the supernova neutrino signal with the LVD detector","license":"","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"A. Pesci, A. Porta, A.S. Malguin, A. Zichichi, C. Castagnoli, C. Vigorito, E. Kemp, F. Vissani, G. Bari, G. Sartorelli, G.T. Zatsepin, H. Menghetti, I. A. Pless, L. Votano, M. Aglietta, M. Garbini, M. Selvi, O. G. Ryazhskaya, O. Saavedra, P. Antonioli, P. Galeotti, P. Giusti, P. L. Ghia, V.F. Yakushev, V. G. Ryasny, W. Fulgione","submitted_at":"2003-07-23T07:11:09Z","abstract_excerpt":"We present an update of our previous study (astro-ph/0112312) on how $\\nu$ oscillations affect the signal from a supernova core collapse observed in the LVD detector at LNGS. In this paper we use a recent, more precise determination of the cross section (astro-ph/0302055) to calculate the expected number of inverse beta decay events, we introduce in the simulation also the $\\nu$-{\\rm Fe} interactions, we include the Earth matter effects and, finally, we study also the inverted mass hierarchy case."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"hep-ph/0307287","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"}