{"paper":{"title":"Search for high-energy neutrinos from bright GRBs with ANTARES","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A. Albert, A. Capone, A. Coleiro, A. Creusot, A. Deschamps, A. Enzenh\\\"ofer, A. Gleixner, A.J. Heijboer, A. Kouchner, A. Margiotta, A. Marinelli, A. Mathieu, A. Moussa, A. S\\'anchez-Losa, A. Trovato, A. Vizzoca, B. Baret, B. Vallage, C. Distefano, C. Donzaud, C. Hugon, C. Lachaud, C. Mueller, C. Pellegrino, C. Perrina, C. Racca, C. Sieger, C. T\\\"onnis, C. Vall\\'ee, C.W. James, D. Dornic, D. Drouhin, D. Els\\\"asser, D. F. E. Samtleben, D. Kie{\\ss}ling, D. Lef\\`evre, D. Turpin, D. Vivolo, E. Leonora, E. Nezri, F. Sch\\\"ussler, G. Anton, G. De Bonis, G.E. P\\u{a}v\\u{a}la\\c{s}, G. Illuminati, G. Riccobene, H. Costantini, H. Glotin, H. van Haren, I. Di Palma, I. El Bojaddaini, I. Felis, I. Kreykenbohm, I. Salvadori, J.A.B. Coelho, J.A. Mart\\'inez-Mora, J. Barrios-Mart\\'i, J. Brunner, J. Busto, J. Carr, J.D. Zornoza, J. Hofest\\\"adt, J. H\\\"o{\\ss}l, J.-J. Aubert, J.J. Hern\\'andez-Rey, J. Schnabel, J. Wilms, J. Z\\'u\\~niga, K. Geyer, K. Graf, K. Melis, K. Roensch, L.A. Fusco, L. Caramete, L. Quinn, M. Andr\\'e, M. Anghinolfi, M. Ardid, M.C. Bouwhuis, M. Circella, M. de Jong, M. Jongen, M. Kadler, M. Kreter, M. Lotze, M. Marcelin, M. Salda\\~na, M. Sanguineti, M. Spurio, M. Taiuti, M. Tselengidou, O. Kalekin, P. Coyle, P. Gay, P. Migliozzi, P. Piattelli, P. Sapienza, R. Bormuth, R. Bruijn, R. Coniglione, R. Gracia Ruiz, R. Lahmann, R. Mele, S. Basa, S. Biagi, S. Bourret, S. Celli, S. Galat\\`a, S. Gei{\\ss}els\\\"oder, S. Hallmann, S. Loucatos, S. Wagner, T. Avgitas, T. Chiarusi, T. Eberl, T. Gr\\'egoire, Th. Stolarczyk, T. Michael, T. Pradier, T. Seitz, U. Katz, V. Bertin, V. Giordano, V. Kulikovskiy, V. Popa, V. Van Elewyck, Y. Hello, Y. Tayalati","submitted_at":"2016-12-27T12:02:55Z","abstract_excerpt":"Gamma-ray bursts are thought to be sites of hadronic acceleration, thus neutrinos are expected from the decay of charged particles, produced in p{\\gamma} interactions. The methods and results of a search for muon neutrinos in the data of the ANTARES neutrino telescope from four bright GRBs (GRB 080916C, GRB 110918A, GRB 130427A and GRB 130505A) observed between 2008 and 2013 are presented. Two scenarios of the fireball model have been investigated: the internal shock scenario, leading to the production of neutrinos with energies mainly above 100 TeV, and the photospheric scenario, characterise"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1612.08589","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"}