Accès ouvert déclaré
2023
preprint
The Giant Radio Array for Neutrino Detection (GRAND) Collaboration -- Contributions to the 38th International Cosmic Ray Conference (ICRC 2023)
Rafael Alves Batista, A. Benoit-Lévy, Teresa Bister, Mauricio Bustamante, Yiren Chen, Ling-Mei Cheng, Simon Chiche, Jean-Marc Colley, Pablo Correa, Nicoleta Cucu Laurenciu, Zi-Gao Dai, Beatriz de Errico, S. J. de Jong, K. D. de Vries, Peter B. Denton, Kaikai Duan, Bohao Duan, Ralph Engel, Yi-Zhong Fan, Arsène Ferrière, Q. B. Gou, Junhua Gu, Marion Guelfand, Jian‐Hua Guo, Vaidhai Gupta, Claire Guépin, Lukas Gülzow, A. Haungs, Haoning He, E. Hivon, Hongbo Hu, Xiaoyuan Huang, Yan Huang, T. Huege, Wen Jiang, Ramesh Koirala, Kumiko Kotera, Jelena Köhler, Bruno L. Lago, Sandra Le Coz, François Legrand, A. Leisos, Rui Li, Cheng Liu, Ruo-Yu Liu, Wei Liu, Peng-Xiong Ma, Oscar Macías, F. Magnard, O. Martineau‐Huynh, Ananstasiia Mikhno, P. Mitra, M. Mostafá, F. Mottez, J. Mouette, Kohta Murase, V. Niess, Stavros Nonis, S. Ogio, Foteini Oikonomou, T. Pierog, L. W. Piotrowski, Pierre Poisvert, S. Prunet, Xiang-Li Qian, M. Roth, T. Sako, Harm Schoorlemmer, Bart Steeman, Dániel Szálas-Motesiczky, Szymon Sławiński, Anne Timmermans, Charles Timmermans, A. Tsirigotis, Matias Jorge Tueros, Shen Wang, Xiang‐Yu Wang, Xu Wang, Da-Ming Wei, Xiangping Wu, Xue-Feng Wu, Xin Xu, Xing Xu, Lili Yang, Xuan Yang, Qiang Yuan, P. Zarka, Houdun Zeng, Chao Zhang, Jianli Zhang, Kewen Zhang, Pengfei Zhang, Songbo Zhang, H. Zhou
1Citations signalées, ce qui n’est pas une note de qualité
0Institutions déclarées
0Pays d’affiliation déclarés
Le résumé fourni par la source
The Giant Radio Array for Neutrino Detection (GRAND) is an envisioned observatory of ultra-high-energy particles of cosmic origin, with energies in excess of 100 PeV. GRAND uses large surface arrays of autonomous radio-detection units to look for the radio emission from extensive air showers that are triggered by the interaction of ultra-high-energy cosmic rays, gamma rays, and neutrinos in the atmosphere or underground. In particular, for ultra-high-energy neutrinos, the future final phase of GRAND aims to be sensitive enough to discover them in spite of their plausibly tiny flux. Presently, three prototype GRAND radio arrays are in operation: GRANDProto300, in China, GRAND@Auger, in Argentina, and GRAND@Nancay, in France. Their goals are to field-test the design of the radio-detection units, understand the radio background to which they are exposed, and develop tools for diagnostic, data gathering, and data analysis. This list of contributions to the 38th International Cosmic Ray Conference (ICRC 2023) presents an overview of GRAND, in its present and future incarnations, and a look at the first data collected by GRANDProto13, the first phase of GRANDProto300.
Ce résumé expose les affirmations des auteurs. BNTIC ne l’interprète pas comme une validation indépendante des résultats.
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Les sujets associés
Astrophysics and Cosmic PhenomenaNeutrino Physics ResearchDark Matter and Cosmic Phenomena