An offline search for a neutrino counterpart to gravitational -wave (GW) events detected during the second observation run (02) of Advanced-LIGO and Advanced Virgo performed with ANTARES data is presented. In addition to the search for long tracks induced by pp, (17i,) charged current interactions, a search for showering events induced by interactions of neutrinos of any flavour is conducted. The severe spatial and time coincidence provided by the gravitational -wave alert allows regions above the detector horizon to be probed, extending the ANTARES sensitivity over the entire sky. The results of this all -neutrino -flavour and all -sky time dependent analysis are presented. The search for prompt neutrino emission within 500 s around the time of six GW events yields no neutrino counterparts. Upper limits on the neutrino spectral fluence and constraints on the isotropic energy radiated via high-energy neutrinos (from a few TeV to a few tens of PeV) are set for each GW event analysed.
Search for neutrino counterparts of gravitational-wave events detected by LIGO and Virgo during run O2 with the ANTARES telescope / Albert, A; Andre, M; Anghinolfi, M; Anton, G; Ardid, M; Aubert, Jj; Aublin, J; Baret, B; Basa, S; Belhorma, B; Bertin, V; Biagi, S; Bissinger, M; Boumaaza, J; Bouta, M; Bouwhuis, Mc; Branzas, H; Bruijn, R; Brunner, J; Busto, J; Capone, A; Caramete, L; Carr, J; Celli, S; Chabab, M; Chau, Tn; El Moursli, Rc; Chiarusi, T; Circella, M; Coleiro, A; Colomer-Molla, M; Coniglione, R; Coyle, P; Creusot, A; Diaz, Af; de Wasseige, G; Deschamps, A; Distefano, C; Di Palma, I; Domi, A; Donzaud, C; Dornic, D; Drouhin, D; Eberl, T; El Khayati, N; Enzenhofer, A; Ettahiri, A; Fermani, P; Ferrara, G; Filippini, F; Fusco, L; Gay, P; Glotin, H; Gozzini, R; Ruiz, Rg; Graf, K; Guidi, C; Hallmann, S; van Haren, H; Heijboer, Aj; Hello, Y; Hernandez-Rey, Jj; Hoessl, J; Hofestadt, J; Huang, F; Illuminati, G; James, Cw; de Jong, M; de Jong, P; Jongen, M; Kadler, M; Kalekin, O; Katz, U; Khan-Chowdhury, Nr; Kouchner, A; Kreykenbohm, I; Kulikovskiy, V; Lahmann, R; Le Breton, R; Lefevre, D; Leonora, E; Levi, G; Lincetto, M; Lopez-Coto, D; Loucatos, S; Maggi, G; Manczak, J; Marcelin, M; Margiotta, A; Marinelli, A; Martinez-Mora, Ja; Mele, R; Melis, K; Migliozzi, P; Moser, M; Moussa, A; Muller, R; Nauta, L; Navas, S; Nezri, E; Nielsen, C; Nunez-Castineyra, A; O'Fearraigh, B; Organokov, M; Pavalas, Ge; Pellegrino, C; Perrin-Terrin, M; Piattelli, P; Poire, C; Popa, V; Pradier, T; Randazzo, N; Reck, S; Riccobene, G; Sanchez-Losa, A; Samtleben, Dfe; Sanguineti, M; Sapienza, P; Schussler, F; Spurio, M; Stolarczyk, T; Strandberg, B; Taiuti, M; Tayalati, Y; Thakore, T; Tingay, Sj; Trovato, A; Vallage, B; Van Elewyck, V; Versari, F; Viola, S; Vivolo, D; Wilms, J; Zaborov, D; Zegarelli, A; Zornoza, Jd; Zuniga, J. - In: THE EUROPEAN PHYSICAL JOURNAL. C, PARTICLES AND FIELDS. - ISSN 1434-6044. - 80:5(2020), pp. 1-9. [10.1140/epjc/s10052-020-8015-6]
Search for neutrino counterparts of gravitational-wave events detected by LIGO and Virgo during run O2 with the ANTARES telescope
Trovato A;
2020-01-01
Abstract
An offline search for a neutrino counterpart to gravitational -wave (GW) events detected during the second observation run (02) of Advanced-LIGO and Advanced Virgo performed with ANTARES data is presented. In addition to the search for long tracks induced by pp, (17i,) charged current interactions, a search for showering events induced by interactions of neutrinos of any flavour is conducted. The severe spatial and time coincidence provided by the gravitational -wave alert allows regions above the detector horizon to be probed, extending the ANTARES sensitivity over the entire sky. The results of this all -neutrino -flavour and all -sky time dependent analysis are presented. The search for prompt neutrino emission within 500 s around the time of six GW events yields no neutrino counterparts. Upper limits on the neutrino spectral fluence and constraints on the isotropic energy radiated via high-energy neutrinos (from a few TeV to a few tens of PeV) are set for each GW event analysed.| File | Dimensione | Formato | |
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