TY - JOUR
T1 - The Giant Radio Array for Neutrino Detection (GRAND)
T2 - 35th International Cosmic Ray Conference, ICRC 2017
AU - Fang, Ke
AU - Álvarez-Muñiz, Jaime
AU - Batista, Rafael Alves
AU - Bustamante, Mauricio
AU - Carvalho, Washington
AU - Charrier, Didier
AU - Cognard, Ismaël
AU - De Jong, Sijbrand
AU - De Vries, Krijn D.
AU - Finley, Chad
AU - Gou, Quanbu
AU - Gu, Junhua
AU - Guépin, Claire
AU - Hanson, Jordan
AU - Hu, Hongbo
AU - Kotera, Kumiko
AU - Le Coz, Sandra
AU - Mao, Yi
AU - Martineau-Huynh, Olivier
AU - Medina, Clementina
AU - Mostafa, Miguel
AU - Mottez, Fabrice
AU - Murase, Kohta
AU - Niess, Valentin
AU - Oikonomou, Foteini
AU - Schröder, Frank
AU - Tasse, Cyril
AU - Timmermans, Charles
AU - Renault-Tinacci, Nicolas
AU - Tueros, Matías
AU - Wu, Xiang Ping
AU - Zarka, Philippe
AU - Zech, Andreas
AU - Zhang, Yi
AU - Zheng, Qian
AU - Zilles, Anne
N1 - Publisher Copyright:
© Copyright owned by the author(s) under the terms of the Creative Commons Attribution-Non Commercial-No Derivatives 4.0 International License (CC BY-NC-ND 4.0).
PY - 2017
Y1 - 2017
N2 - The Giant Radio Array for Neutrino Detection (GRAND) aims at detecting ultra-high energy extraterrestrial neutrinos via the extensive air showers induced by the decay of tau leptons created in the interaction of neutrinos under the Earth's surface. Consisting of an array of ∼105 radio antennas deployed over ∼2 × 105km2, GRAND plans to reach, for the first time, an all-flavor sensitivity of ∼1.5 × 10-10GeVcm-2 s-1 sr-1 above 5 × 1017 eV and a sub-degree angular resolution, beyond the reach of other planned detectors. We describe here preliminary designs and simulation results, plans for the ongoing, staged approach to the construction of GRAND, and the rich research program made possible by GRAND's design sensitivity and angular resolution.
AB - The Giant Radio Array for Neutrino Detection (GRAND) aims at detecting ultra-high energy extraterrestrial neutrinos via the extensive air showers induced by the decay of tau leptons created in the interaction of neutrinos under the Earth's surface. Consisting of an array of ∼105 radio antennas deployed over ∼2 × 105km2, GRAND plans to reach, for the first time, an all-flavor sensitivity of ∼1.5 × 10-10GeVcm-2 s-1 sr-1 above 5 × 1017 eV and a sub-degree angular resolution, beyond the reach of other planned detectors. We describe here preliminary designs and simulation results, plans for the ongoing, staged approach to the construction of GRAND, and the rich research program made possible by GRAND's design sensitivity and angular resolution.
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M3 - Conference article
AN - SCOPUS:85046058241
SN - 1824-8039
JO - Proceedings of Science
JF - Proceedings of Science
Y2 - 10 July 2017 through 20 July 2017
ER -