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Sensitivity of the KM3NeT/ARCA neutrino telescope to point-like neutrino sources

Title: Sensitivity of the KM3NeT/ARCA neutrino telescope to point-like neutrino sources
Authors: Aiello S; Akrame SE; Ameli F; Anassontzis EG; Andre M; Androulakis G; Anghinolfi M; Anton G; Ardid M; Aublin J; Avgitas T; Bagatelas C; Barbarino G; Baret B; Barrios-Marti J; Belias A; Berbee E; van den Berg A; Bertin V; Biagi S; Biagioni A; Biernoth C; Boumaaza J; Bourret S; Bouta M; Bouwhuis M; Bozza C; Branzas H; Bruchner M; Bruijn R; Brunner J; Buis E; Buompane R; Busto J; Calvo D; Capone A; Celli S; Chabab M; Chau N; Cherubini S; Chiarella V; Chiarusi T; Circella M; Cocimano R; Coelho JAB; Coleiro A; Molla MC; Coniglione R; Coyle P; Creusot A; Cuttone G; D'Onofrio A; Dallier R; De Sio C; Di Palma I; Diaz AF; Diego-Tortosa D; Distefano C; Domi A; Dona R; Donzaud C; Dornic D; Dorr M; Durocher M; Eberl T; van Eijk D; El Bojaddaini I; Eljarrari H; Elsaesser D; Enzenhofer A; Fermani P; Ferrara G; Filipovic MD; Fusco LA; Gal T; Garcia A; Garufi F; Gialanella L; Giorgio E; Giuliante A; Gozzini SR; Gracia R; Graf K; Grasso D; Gregoire T; Grella G; Hallmann S; Hamdaoui H; van Haren H; Heid T; Heijboer A; Hekalo A; Hernandez-Rey JJ; Hofestadt J; Illuminati G; James CW; Jongen M; de Jong M; de Jong P; Kadler M; Kalaczynski P; Kalekin O; Katz UF; Chowdhury NRK; Kiessling D; Koffeman EN; Kooijman P; Kouchner A; Kreter M; Kulikovskiy V; Kannichankandy MK; Lahmann R; Larosa G; Le Breton R; Leone F; Leonora E; Levi G; Lincetto M; Lonardo A; Longhitano F; Coto DL; Lotze M; Maderer L; Maggi G; Manczak J; Mannheim K; Margiotta A; Marinelli A; Markou C; Martin L; Martinez-Mora JA; Martini A; Marzaioli F; Mele R; Melis KW; Migliozzi P; Migneco E; Mijakowski P; Miranda LS; Mollo CM; Morganti M; Moser M; Moussa A; Muller R; Musumeci M; Nauta L; Navas S; Nicolau CA; Nielsen C; Fearraigh BO; Organokov M; Orlando A; Ottonello S; Panagopoulos V; Papalashvili G; Papaleo R; Pavalas GE; Pellegrino C; Perrin-Terrin M; Piattelli P; Pikounis K; Pisanti O; Poire C; Polydefki G; Popa V; Post M; Pradier T; Puhlhofer G; Pulvirenti S; Quinn L; Raffaelli F; Randazzo N; Razzaque S; Real D; Resvanis L; Reubelt J; Riccobene G; Richer M; Rigalleau L; Rovelli A; Saffer M; Salvadori I; Samtleben DFE; Losa AS; Sanguineti M; Santangelo A; Santonocito D; Sapienza P; Schumann J; Sciacca V; Seneca J; Sgura I; Shanidze R; Sharma A; Simeone F; Sinopoulou A; Spisso B; Spurio M; Stavropoulos D; Steijger J; Stellacci SM; Strandberg B; Stransky D; Stuven T; Taiuti M; Tatone F; Tayalati Y; Tenllado E; Thakore T; Trovato A; Tzamariudaki E; Tzanetatos D; Van Elewyck V; Versari F; Viola S; Vivolo D; Wilms J; de Wolf E; Zaborov D; Zornoza JD; Zuniga J
Contributors: Aiello, S; Akrame, Se; Ameli, F; Anassontzis, Eg; Andre, M; Androulakis, G; Anghinolfi, M; Anton, G; Ardid, M; Aublin, J; Avgitas, T; Bagatelas, C; Barbarino, G; Baret, B; Barrios-Marti, J; Belias, A; Berbee, E; van den Berg, A; Bertin, V; Biagi, S; Biagioni, A; Biernoth, C; Boumaaza, J; Bourret, S; Bouta, M; Bouwhuis, M; Bozza, C; Branzas, H; Bruchner, M; Bruijn, R; Brunner, J; Buis, E; Buompane, R; Busto, J; Calvo, D; Capone, A; Celli, S; Chabab, M; Chau, N; Cherubini, S; Chiarella, V; Chiarusi, T; Circella, M; Cocimano, R; Coelho, Jab; Coleiro, A; Molla, Mc; Coniglione, R; Coyle, P; Creusot, A; Cuttone, G; D'Onofrio, A; Dallier, R; De Sio, C; Di Palma, I; Diaz, Af; Diego-Tortosa, D; Distefano, C; Domi, A; Dona, R; Donzaud, C; Dornic, D; Dorr, M; Durocher, M; Eberl, T; van Eijk, D; El Bojaddaini, I; Eljarrari, H; Elsaesser, D; Enzenhofer, A; Fermani, P; Ferrara, G; Filipovic, Md; Fusco, La; Gal, T; Garcia, A; Garufi, F; Gialanella, L; Giorgio, E; Giuliante, A; Gozzini, Sr; Gracia, R; Graf, K; Grasso, D; Gregoire, T; Grella, G; Hallmann, S; Hamdaoui, H; van Haren, H; Heid, T; Heijboer, A; Hekalo, A; Hernandez-Rey, Jj; Hofestadt, J; Illuminati, G; James, Cw; Jongen, M; de Jong, M; de Jong, P; Kadler, M
Publication Year: 2019
Collection: Università degli studi di Trieste: ArTS (Archivio della ricerca di Trieste)
Subject Terms: Astrophysical neutrino source; Cherenkov underwater neutrino telescope; KM3NeT
Description: KM3NeT will be a network of deep-sea neutrino telescopes in the Mediterranean Sea. The KM3NeT/ARCA detector, to be installed at the Capo Passero site (Italy), is optimised for the detection of high-energy neutrinos of cosmic origin. Thanks to its geographical location on the Northern hemisphere, KM3NeT/ARCA can observe upgoing neutrinos from most of the Galactic Plane, including the Galactic Centre. Given its effective area and excellent pointing resolution, KM3NeT/ARCA will measure or significantly constrain the neutrino flux from potential astrophysical neutrino sources. At the same time, it will test flux predictions based on gamma-ray measurements and the assumption that the gamma-ray flux is of hadronic origin. Assuming this scenario, discovery potentials and sensitivities for a selected list of Galactic sources and to generic point sources with an E-2 spectrum are presented. These spectra are assumed to be time independent. The results indicate that an observation with 3 sigma significance is possible in about six years of operation for the most intense sources, such as Supernovae Remnants RX J1713.7-3946 and Vela Jr. If no signal will be found during this time, the fraction of the gamma-ray flux coming from hadronic processes can be constrained to be below 50% for these two objects. (C) 2019 The Authors. Published by Elsevier B.V.
Document Type: article in journal/newspaper
Language: English
Relation: info:eu-repo/semantics/altIdentifier/wos/WOS:000470047300008; volume:111; firstpage:100; lastpage:110; numberofpages:11; journal:ASTROPARTICLE PHYSICS; https://hdl.handle.net/11368/3003242
DOI: 10.1016/j.astropartphys.2019.04.002
Availability: https://hdl.handle.net/11368/3003242; https://doi.org/10.1016/j.astropartphys.2019.04.002
Rights: info:eu-repo/semantics/openAccess
Accession Number: edsbas.E40B8F22
Database: BASE