Science and Design for the Giant Radio Array for Neutrino Detection

Miguel Mostafa,Jaime Álvarez-Muñiz,Rafael Alves Batista,Aswathi V. Balagopal,Julien Bolmont,Mauricio Bustamante,Washington Carvalho, Didier Charrier, Ling-Mei Cheng,Ismaël Cognard,Zigao Dai,Valentin Decoene,Sijbrand De Jong,Peter B. Denton,Krijn D. De Vries,Ralph Engel,Ke Fang,Stefano Gabici,QuanBu Gou,Junhua Gu,Claire Guépin,Li Guo,Rene Habraken,Andreas Haungs,Hongbo Hu,Yan Huang,Kumiko Kotera, Bruno Lago, Sandra Le Coz,Jean-Philippe Lenain,KuanJun Li, Ruoyu Liu,Olivier Martineau-Huynh, Rogerio Menezes de Almeida, Fabrice Mottez, Jean Mouette, Marcio Muller,Kohta Murase,Valentin Niess,Foteini Oikonomou, Tanguy Pieorg,Simon Prunet,Xiangli Qian,Bo Qin,Markus Roth,Frank G. Schröder,Fabian Schüssler,Cyril Tasse, Charles Timmermans,João Torres de Mello Neto,Matías Tueros,Xiangyu Wang,Xiangping Wu,Lili Yang,Philippe Zarka,Andreas Zech,B. Theodore Zhang,Jianli Zhang, Pengfei Zhang,Yi Zhang,Qian Zheng,Anne Zilles

Bulletin of the American Astronomical Society（2019）

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摘要

GRAND is a planned large-scale observatory of ultra-high energy (UHE) cosmic messengers with energies exceeding 10⁸ GeV. The ultimate goal is to solve the long-standing mystery of the origin of UHE cosmic rays. Three key features of GRAND will make this possible: its large exposure, sub-degree angular resolution, and sensitivity to UHE particles.

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