Prospects for the detection of the prompt very-high-energy emission from γ-ray bursts with the High Altitude Detection of Astronomical Radiation experiment
【作者单位】1School of Physics and Technology, Wuhan University, Wuhan; 430072, China;2Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing; 100049, China;3College of Physics, Sichuan University, Chengdu; 610064, China;4School of Intelligent Engineering, Shandong Management University, Jinan; 250357, China;5The Key Laboratory of Cosmic Rays (Tibet University), Ministry of Education, Tibet, Lhasa; 850000, China;6Key Laboratory of Dark Matter and Space Astronomy, Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing; 210008, China;7University of Chinese Academy of Sciences, 19 A Yuquan Rd, Shijingshan District, Beijing; 100049, China;8Tsung-Dao Lee Institute, Shanghai Jiao Tong University, Shanghai; 200240, China
【年份】2021
【摘要】 The observation of very-high-energy γ-ray emission from γ-ray bursts , especially in the prompt phase, will provide critical information for understanding many aspects of their nature including the physical environment, the relativistic bulk motion,...
