Science and Design for the Giant Radio Array for Neutrino Detection - Observatoire de Paris
Conference Papers Year : 2019

Science and Design for the Giant Radio Array for Neutrino Detection

Miguel Mostafa
  • Function : Author
Jaime Álvarez-Muñiz
  • Function : Author
Rafael Alves Batista
  • Function : Author
Aswathi V. Balagopal
  • Function : Author
Mauricio Bustamante
  • Function : Author
Washington Carvalho
  • Function : Author
Ling-Mei Cheng
  • Function : Author
Zigao Dai
  • Function : Author
Sijbrand de Jong
  • Function : Author
Peter B. Denton
  • Function : Author
Krijn D. de Vries
  • Function : Author
Ralph Engel
  • Function : Author
Ke Fang
  • Function : Author
Quanbu Gou
  • Function : Author
Junhua Gu
  • Function : Author
Li Guo
  • Function : Author
Rene Habraken
  • Function : Author
Andreas Haungs
  • Function : Author
Hongbo Hu
  • Function : Author
Yan Huang
  • Function : Author
Bruno Lago
  • Function : Author
Sandra Le Coz
  • Function : Author
Kuanjun Li
  • Function : Author
Ruoyu Liu
  • Function : Author
Rogerio Menezes de Almeida
  • Function : Author
Marcio Muller
  • Function : Author
Kohta Murase
  • Function : Author
Foteini Oikonomou
  • Function : Author
Tanguy Pieorg
  • Function : Author
Xiangli Qian
  • Function : Author
Bo Qin
  • Function : Author
Markus Roth
  • Function : Author
Frank G. Schröder
  • Function : Author
Charles Timmermans
  • Function : Author
João Torres de Mello Neto
  • Function : Author
Matías Tueros
  • Function : Author
Xiangyu Wang
  • Function : Author
Xiangping Wu
  • Function : Author
Lili Yang
  • Function : Author
B. Theodore Zhang
  • Function : Author
Jianli Zhang
  • Function : Author
Pengfei Zhang
  • Function : Author
Yi Zhang
  • Function : Author
Qian Zheng
  • Function : Author

Abstract

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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Dates and versions

obspm-04009757 , version 1 (01-03-2023)

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Cite

Miguel Mostafa, Jaime Álvarez-Muñiz, Rafael Alves Batista, Aswathi V. Balagopal, Julien Bolmont, et al.. Science and Design for the Giant Radio Array for Neutrino Detection. Astro2020: Decadal Survey on Astronomy and Astrophysics, APC white papers, no. 92; Bulletin of the American Astronomical Society, 2019, à renseigner, Unknown Region. 18 p. ⟨obspm-04009757⟩
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