巨型中微子探测射电阵列 (GRAND)：现状与展望
天体物理仪器与方法
2017-08-18 v1 高能天体物理现象
摘要
巨型中微子探测射电阵列 (GRAND) 旨在通过探测中微子在地球表面下方相互作用产生的 tau 轻子衰变所引发的广延大气簇射，来探测超高能地外中微子。GRAND 由部署在约 区域上的 个射电天线阵列组成，计划首次达到在 eV 以上约 的全味道灵敏度和亚度级角分辨率，这超越了其他计划中的探测器的探测范围。我们在此描述了初步设计和模拟结果、当前分阶段建设 GRAND 的计划，以及由 GRAND 的设计灵敏度和角分辨率所实现的丰富研究项目。
引用
@article{arxiv.1708.05128,
title = {The Giant Radio Array for Neutrino Detection (GRAND): Present and Perspectives},
author = {Ke Fang and Jaime Álvarez-Muñiz and Rafael Alves Batista and Mauricio Bustamante and Washington Carvalho and Didier Charrier and Ismaël Cognard and Sijbrand De Jong and Krijn D. de Vries and Chad Finley and Quanbu Gou and Junhua Gu and Claire Guépin and Jordan Hanson and Hongbo Hu and Kumiko Kotera and Sandra Le Coz and Yi Mao and Olivier Martineau-Huynh and Clementina Medina and Miguel Mostafa and Fabrice Mottez and Kohta Murase and Valentin Niess and Foteini Oikonomou and Frank Schröder and Cyril Tasse and Charles Timmermans and Nicolas Renault-Tinacci and Matías Tueros and Xiang-Ping Wu and Philippe Zarka and Andreas Zech and Yi Zhang and Qian Zheng and Anne Zilles},
journal= {arXiv preprint arXiv:1708.05128},
year = {2017}
}
备注
Proceedings of the 35th International Cosmic Ray Conference (ICRC2017), Bexco, Busan, Korea