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】1 School of Physics and Technology, Wuhan University, Wuhan 430072, People's Republic of China;hcai@whu.edu.cn; 2 Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, People's Republic of China;yaoyh@ihep.ac.cn, guoyq@ihep.ac.cn; 3 College of Physics, Sichuan University, Chengdu 610064, People's Republic of China; 4 School of Intelligent Engineering, Shandong Management University, Jinan 250357, People's Republic of China; 5 The Key Laboratory of Cosmic Rays (Tibet University), Ministry of Education, Lhasa 850000, Tibet, People's Republic of China;chentl@ihep.ac.cn; 6 Key Laboratory of Dark Matter and Space Astronomy, Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing 210008, People's Republic of China; 7 University of Chinese Academy of Sciences, 19 A Yuquan Road, Shijingshan District, Beijing 100049, People's Republic of China; 8 Tsung-Dao Lee Institute, Shanghai Jiao Tong University, Shanghai 200240, People's Republic of China
【年份】2021
【卷号】Vol.923 No.1
【页码】112
【ISSN】0004-637x
【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,...
