【作者单位】1College of Physics, Chongqing University, No. 55 Daxuecheng South Road, High-tech District, Chongqing, 401331, People's Republic of China;2Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, People's Republic of China;guoyq@ihep.ac.cn;3Tsung-Dao Lee Institute, Shanghai Jiao Tong University, 200240 Shanghai, People's Republic of China;zwang0723@sjtu.edu.cn;4School of Physics and Astronomy, Yunnan University, Yunnan 650091, People's Republic of China;5The Key Laboratory of Cosmic Rays (Tibet University), Ministry of Education, Lhasa 850000, Tibet, People's Republic of China;6University of Chinese Academy of Sciences, 19 A Yuquan Road, Shijingshan District, Beijing, 100049, People's Republic of China;7College of Physics, Sichuan University, Chengdu, 610064, People's Republic of China;8School of Intelligent Engineering, Shandong Management University, Jinan, 250357, People's Republic of China;9Suzhou Aerospace Information Research Institute, Suzhou 215123, People's Republic of China;10Key Laboratory of Dark Matter and Space Astronomy, Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing 210008, People's Republic of China
【年份】2023
【卷号】Vol.958 No.1
【页码】87
【ISSN】0004-637X
【摘要】 Recent ground-based observations of TeV photons have significantly deepened our understanding of the nature of gamma-ray bursts . However, many fundamental problems remain unsolved concerning the physical mechanisms behind GRBs, necessitating the nee...
