Paper

Towards the Giant Radio Array for Neutrino Detection (GRAND): the GRANDProto300 and GRAND@Auger prototypes

Magnard, Frédéric, Ogio, Shoichi, Wang, Xu, Weissling, Emily, de Errico, Beatriz, Köhler, Jelena, Ma, Pengxiong, Macias, Oscar, Haungs, Andreas, Fan, Yizhong, Cheng, LingMei, Sławiński, Szymon, Tsirigotis, Apostolos, Liu, Cheng, Tueros, Matías, Wang, Xiangyu, Lago, Bruno L, Shinde, Sarvesh, Huang, Guoyuan, Zhou, Hao, Zhang, Chao, Koirala, Ramesh, Gu, Junhua, Zhang, Jianli, Zhang, Pengfei, Colley, Jean-Marc, Leisos, Antonios, Zarka, Philippe, Bustamante, Mauricio, Yang, Fufu, Yang, Xuan, Li, Xingyu, Zhang, Yi, Marcowith, Alexandre, Guelfand, Marion, Lai, Zhisen, Zhang, Qingchi, Dai, Zigao, Gou, QuanBu, Vittakis, George, Prunet, Simon, Nonis, Stavros, Huang, Xiaoyuan, Pan, Hongwei, Legrand, François, Guépin, Claire, McKinley, Thomas, Sako, Takashi, Murase, Kohta, Wu, Juan, He, Haoning, Mostafá, Miguel, Wang, Shen, Voisin, Vincent, Guo, Jianhua, Chen, Yiren, Szálas-Motesiczky, Dániel, Lech Wiktor Piotrowski, Minodier, Paul, Denton, Peter B, Niess, Valentin, de Almeida, Rogerio M, Huang, Yan, Wang, Hanrui, Wu, Xiangping, Laurenciu, Nicoleta Cucu, Prévotat, Clément, GRAND Collaboration, Guo, Yiqing, Bister, Teresa, Hu, Hongbo, Ti

2026

Overview

The Giant Radio Array for Neutrino Detection (GRAND) is a proposed multi-messenger observatory of Ultra-High-Energy (UHE) particles of cosmic origin. Its main goal is to find the long-sought origin of UHE cosmic rays by detecting large numbers of them and the secondary particles created by their interactions like gamma rays and neutrinos. The GRAND Collaboration plans to achieve this using large arrays of radio antennas that look for the radio signals emitted by the air showers initiated by the interactions of the UHE particles in the atmosphere. Since 2023, three small-scale prototype GRAND arrays have been in operation: GRAND@Nançay in France, GRAND@Auger in Argentina, and GRANDProto300 in China. Together, their goal is to validate the detection principle of GRAND under prolonged field conditions, achieving efficient, autonomous radio-detection of air showers. We describe the hardware, software, layout, and operation of the GRAND prototypes. Using their data, we show a first characterization of the local electromagnetic environment of each site and a measurement of the Galactic synchrotron emission. Despite challenges, the successful operation of the prototypes confirms that the GRAND instrumentation is apt to address the goals of the experiment and lays the groundwork for its ensuing stages.

• Publisher: Cornell University Library, arXiv.org
• Subject: Antenna arrays / Cosmic ray showers / Cosmic rays / Gamma rays / Neutrinos / Prototypes / Radio antennas / Radio signals