TY - JOUR
T1 - The next generation neutrino telescope
T2 - 38th International Cosmic Ray Conference, ICRC 2023
AU - The IceCube-Gen2 Collaboration
AU - Abbasi, R.
AU - Ackermann, M.
AU - Adams, J.
AU - Agarwalla, S. K.
AU - Aguilar, J. A.
AU - Ahlers, M.
AU - Alameddine, J. M.
AU - Amin, N. M.
AU - Andeen, K.
AU - Anton, G.
AU - Argüelles, C.
AU - Ashida, Y.
AU - Athanasiadou, S.
AU - Audehm, J.
AU - Axani, S. N.
AU - Bai, X.
AU - Balagopal, A. V.
AU - Baricevic, M.
AU - Barwick, S. W.
AU - Basu, V.
AU - Bay, R.
AU - Becker Tjus, J.
AU - Beise, J.
AU - Bellenghi, C.
AU - Benning, C.
AU - BenZvi, S.
AU - Berley, D.
AU - Bernardini, E.
AU - Besson, D. Z.
AU - Bishop, A.
AU - Blaufuss, E.
AU - Blot, S.
AU - Bohmer, M.
AU - Bontempo, F.
AU - Book, J. Y.
AU - Borowka, J.
AU - Boscolo Meneguolo, C.
AU - Böser, S.
AU - Botner, O.
AU - Böttcher, J.
AU - Bouma, S.
AU - Bourbeau, E.
AU - Braun, J.
AU - Brinson, B.
AU - Brostean-Kaiser, J.
AU - Burley, R. T.
AU - Busse, R. S.
AU - Cowen, Douglas
AU - Fox, Derek Brindley
AU - Wissel, S.
N1 - Publisher Copyright:
© Copyright owned by the author(s) under the terms of the Creative Commons.
PY - 2024/9/27
Y1 - 2024/9/27
N2 - The IceCube Neutrino Observatory, a cubic-kilometer-scale neutrino detector at the geographic South Pole, has reached a number of milestones in the field of neutrino astrophysics: the discovery of a high-energy astrophysical neutrino flux, the temporal and directional correlation of neutrinos with a flaring blazar, and a steady emission of neutrinos from the direction of an active galaxy of a Seyfert II type and the Milky Way. The next generation neutrino telescope, IceCube-Gen2, currently under development, will consist of three essential components: an array of about 10,000 optical sensors, embedded within approximately 8 cubic kilometers of ice, for detecting neutrinos with energies of TeV and above, with a sensitivity five times greater than that of IceCube; a surface array with scintillation panels and radio antennas targeting air showers; and buried radio antennas distributed over an area of more than 400 square kilometers to significantly enhance the sensitivity of detecting neutrino sources beyond EeV. This contribution describes the design and status of IceCube-Gen2 and discusses the expected sensitivity from the simulations of the optical, surface, and radio components.
AB - The IceCube Neutrino Observatory, a cubic-kilometer-scale neutrino detector at the geographic South Pole, has reached a number of milestones in the field of neutrino astrophysics: the discovery of a high-energy astrophysical neutrino flux, the temporal and directional correlation of neutrinos with a flaring blazar, and a steady emission of neutrinos from the direction of an active galaxy of a Seyfert II type and the Milky Way. The next generation neutrino telescope, IceCube-Gen2, currently under development, will consist of three essential components: an array of about 10,000 optical sensors, embedded within approximately 8 cubic kilometers of ice, for detecting neutrinos with energies of TeV and above, with a sensitivity five times greater than that of IceCube; a surface array with scintillation panels and radio antennas targeting air showers; and buried radio antennas distributed over an area of more than 400 square kilometers to significantly enhance the sensitivity of detecting neutrino sources beyond EeV. This contribution describes the design and status of IceCube-Gen2 and discusses the expected sensitivity from the simulations of the optical, surface, and radio components.
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M3 - Conference article
AN - SCOPUS:85212255292
SN - 1824-8039
VL - 444
JO - Proceedings of Science
JF - Proceedings of Science
M1 - 994
Y2 - 26 July 2023 through 3 August 2023
ER -