Authors: Ke Fang, Jaime Alvarez-Muniz, Rafael Alves Batista, Mauricio Bustamante, Washington Carvalho, Didier Charrier, Ismaël Cognard, Sijbrand de Jong, Krijn D. de Vries, Chad Finley, Quanbu GOU, Junhua Gu, Claire Guépin, Jordan Hanson, hongbo HU, Kumiko Kotera, Sandra Le Coz, Yi Mao, Olivier Martineau-Huynh, Clementina Medina, Miguel Mostafa, Fabrice Mottez, Kohta Murase, Valentin Niess, Foteini Oikonomou, Frank Schroeder, Cyril Tasse, Charles Timmermans, Nicolas Renault-Tinacci, Matias Jorge Tueros, Xiangping Wu, Philippe Zarka, Andreas Zech, Yi Zhang, Qian Zheng, Anne Zilles
Venue: Proceedings of 35th International Cosmic Ray Conference — PoS(ICRC2017)
Type: Publication
Abstract: 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 $\sim10^5$ radio antennas deployed over $\sim 2\times10^5\,\rm {km}^2$, GRAND plans to reach, for the first time, an all-flavor sensitivity of $\sim1.5\times10^{-10} \,\rm GeV\, cm^{-2} \,s^{-1}\, sr^{-1}$ above $5\times10^{17}$ eV and a sub-degree angular resolution, beyond...
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Topics: 
Particle physics
Astrophysics
DOI:
10.22323/1.301.0996
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