TY - JOUR
T1 - Sensitivity estimates for diffuse, point-like and extended neutrino sources with KM3NeT/ARCA
AU - KM3NeT Collaboration
AU - Caiffi, B.
AU - Garcia Soto, A.
AU - Heijboer, A.
AU - Kulikovskiy, V.
AU - Muller, R. S.
AU - Sanguineti, M.
AU - Ageron, M.
AU - Aiello, S.
AU - Albert, A.
AU - Alshamsi, M.
AU - Alves Garre, S.
AU - Aly, Z.
AU - Ambrosone, A.
AU - Ameli, F.
AU - Andre, M.
AU - Androulakis, G.
AU - Anghinolfi, M.
AU - Anguita, M.
AU - Anton, G.
AU - Ardid, M.
AU - Ardid, S.
AU - Assal, W.
AU - Aublin, J.
AU - Bagatelas, C.
AU - Baret, B.
AU - Basegmez du Pree, S.
AU - Bendahman, M.
AU - Benfenati, F.
AU - Berbee, E.
AU - van den Berg, A. M.
AU - Bertin, V.
AU - Beurthey, S.
AU - van Beveren, V.
AU - Biagi, S.
AU - Billault, M.
AU - Bissinger, M.
AU - Boettcher, M.
AU - Bou Cabo, M.
AU - Boumaaza, J.
AU - Bouta, M.
AU - Boutonnet, C.
AU - Bouvet, G.
AU - Bouwhuis, M.
AU - Bozza, C.
AU - Brânzaş, H.
AU - Bruijn, R.
AU - Brunner, J.
AU - Bruno, R.
AU - Buis, E.
AU - Razzaque, S.
N1 - Publisher Copyright:
© Copyright owned by the author(s).
PY - 2022/3/18
Y1 - 2022/3/18
N2 - The identification of cosmic objects emitting high energy neutrinos could provide new insights about the Universe and its active sources. The existence of these cosmic neutrinos has been proven by the IceCube collaboration, but the big question of which sources these neutrinos originate from, remains unanswered. The KM3NeT detector for Astroparticle Research with Cosmics in the Abyss (ARCA), with a cubic kilometer instrumented volume, is currently being built in the Mediterranean Sea. It will excel at identifying cosmic neutrino sources due to its unprecedented angular resolution for muon neutrinos (< 0.2◦ for E > 10 TeV neutrinos). KM3NeT has a view of the sky complementary to IceCube, and is sensitive to neutrinos across a wide range of energies. In order to identify the signature of cosmic neutrino sources in the background of atmospheric neutrinos and muons, statistical methods are being developed and tested with Monte-Carlo pseudo-experiments. This contribution presents the most recent sensitivity estimates for diffuse, point-like and extended neutrino sources with KM3NeT/ARCA.
AB - The identification of cosmic objects emitting high energy neutrinos could provide new insights about the Universe and its active sources. The existence of these cosmic neutrinos has been proven by the IceCube collaboration, but the big question of which sources these neutrinos originate from, remains unanswered. The KM3NeT detector for Astroparticle Research with Cosmics in the Abyss (ARCA), with a cubic kilometer instrumented volume, is currently being built in the Mediterranean Sea. It will excel at identifying cosmic neutrino sources due to its unprecedented angular resolution for muon neutrinos (< 0.2◦ for E > 10 TeV neutrinos). KM3NeT has a view of the sky complementary to IceCube, and is sensitive to neutrinos across a wide range of energies. In order to identify the signature of cosmic neutrino sources in the background of atmospheric neutrinos and muons, statistical methods are being developed and tested with Monte-Carlo pseudo-experiments. This contribution presents the most recent sensitivity estimates for diffuse, point-like and extended neutrino sources with KM3NeT/ARCA.
UR - http://www.scopus.com/inward/record.url?scp=85145021668&partnerID=8YFLogxK
M3 - Conference article
AN - SCOPUS:85145021668
SN - 1824-8039
VL - 395
JO - Proceedings of Science
JF - Proceedings of Science
M1 - 1077
T2 - 37th International Cosmic Ray Conference, ICRC 2021
Y2 - 12 July 2021 through 23 July 2021
ER -