【作者单位】1Key Laboratory of Dark Matter and Space Astronomy, Purple Mountain Observatory, Chinese Academy of Sciences, 9 Jiangsu, Nanjing; 210023, China;2University of Science and Technology of China, Anhui, Hefei; 230026, China;3Institute of Frontier and Interdisciplinary Science, Shandong University, Shandong, Qingdao; 266237, China;4Key Laboratory of Particle Astrophyics & Experimental Physics Division & Computing Center, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing; 100049, China;5University of Chinese Academy of Sciences, Beijing; 100049, China;6TIANFU Cosmic Ray Research Center, Sichuan, Chengdu, China;7Dublin Institute for Advanced Studies, 31 Fitzwilliam Place, 2 Dublin, Ireland;8Max-Planck-Institut for Nuclear Physics, P.O. Box 103980, Heidelberg; 69029, Germany;9State Key Laboratory of Particle Detection and Electronics, China;10School of Physical Science and Technology, School of Information Science and Technology, Southwest Jiaotong University, Sichuan, Chengdu; 610031, China;11College of Physics, Sichuan University, Sichuan, Chengdu; 610065, China;12School of Astronomy and Space Science, Nanjing University, Jiangsu, Nanjing; 210023, China;13Center for Astrophysics, Guangzhou University, Guangdong, Guangzhou; 510006, China;14School of Physics and Technology, Wuhan University, Hubei, Wuhan; 430072, China;15Key Laboratory of Dark Matter and Space Astronomy, Purple Mountain Observatory, Chinese Academy of Sciences, Jiangsu, Nanjing; 210023, China;16Hebei Normal University, Hebei, Shijiazhuang; 050024, China;17Key Laboratory for Research in Galaxies and Cosmology, Shanghai Astronomical Observatory, Chinese Academy of Sciences, Shanghai; 200030, China;18Key Laboratory of Cosmic Rays (Tibet University), Ministry of Education, Tibet, Lhasa; 850000, China;19National Astronomical Observatories, Chinese Academy of Sciences, Beijing; 100101, China;20School of Physics and Astronomy, School of Physics (Guangzhou), Sun Yat-sen University, Guangdong, Zhuhai; 519000, China;21Dipartimento di Fisica dellUniversità di Napoli `Federico II', Complesso Universitario di Monte SantAngelo, via Cinthia, Napoli; 80126, Italy;22School of Physics and Astronomy, Yunnan University, Yunnan, Kunming; 650091, China;23Departement de Physique Nucleaire et Corpusculaire, Faculte de Sciences, Universite de Geneve, 24 Quai Ernest Ansermet, Geneva; 1211, Switzerland;24Department of Engineering Physics, Tsinghua University, Beijing; 100084, China;25School of Physics and Microelectronics, Zhengzhou University, Henan, Zhengzhou; 450001, China;26Institute for Nuclear Research of Russian Academy of Sciences, Moscow; 117312, Russia;27School of Physics, Peking University, Beijing; 100871, China;28School of Physical Science and Technology, Guangxi University, Guangxi, Nanning; 530004, China;29Tsung-Dao Lee Institute, School of Physics and Astronomy, Shanghai Jiao Tong University, Shanghai; 200240, China;30Yunnan Observatories, Chinese Academy of Sciences, Yunnan, Kunming; 650216, China;31Department of Physics, Faculty of Science, Mahidol University, Bangkok; 10400, Thailand;32Moscow Institute of Physics and Technology, Moscow; 141700, Russia;33Key Laboratory of Radio Astronomy, Purple Mountain Observatory, Chinese Academy of Sciences, Jiangsu, Nanjing; 210023, China;34National Space Science Center, Chinese Academy of Sciences, Beijing; 100190, China
【召开年】2021
【会议地点】Virtual, Berlin, Germany
【摘要】 Galactic diffuse gamma ray emission is introduced by the galactic cosmic rays interacting with the interstellar medium and/or radiation fields . Studying galactic diffuse TeV γ-ray emission would help to understand mechanisms of acceleration and pr...