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J-GLOBAL ID：201902266305469899   整理番号：19A2285276

宇宙物理源からの100TeV以上のエネルギーによる光子の最初の検出【JST・京大機械翻訳】

First Detection of Photons with Energy beyond 100 TeV from an Astrophysical Source

著者 (98件)： Amenomori M. (Department of Physics, Hirosaki University, Hirosaki 036-8561, Japan) ,  Bao Y. W. (School of Astronomy and Space Science, Nanjing University, Nanjing 210093, China) ,  Bi X. J. (Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China) ,  Chen D. (National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China) ,  Chen T. L. (Physics Department of Science School, Tibet University, Lhasa 850000, China) ,  Chen W. Y. (Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China) ,  Chen Xu (Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China) ,  Chen Xu (University of Chinese Academy of Sciences, Beijing 100049, China) ,  Chen Y. (School of Astronomy and Space Science, Nanjing University, Nanjing 210093, China) ,  Cirennima (Physics Department of Science School, Tibet University, Lhasa 850000, China) ,  Cui S. W. (Department of Physics, Hebei Normal University, Shijiazhuang 050016, China) ,  Danzengluobu (Physics Department of Science School, Tibet University, Lhasa 850000, China) ,  Ding L. K. (Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China) ,  Fang J. H. (Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China) ,  Fang J. H. (University of Chinese Academy of Sciences, Beijing 100049, China) ,  Fang K. (Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China) ,  Feng C. F. (Department of Physics, Shandong University, Jinan 250100, China) ,  Feng Zhaoyang (Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China) ,  Feng Z. Y. (Institute of Modern Physics, SouthWest Jiaotong University, Chengdu 610031, China) ,  Gao Qi (Physics Department of Science School, Tibet University, Lhasa 850000, China) ,  Gou Q. B. (Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China) ,  Guo Y. Q. (Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China) ,  He H. H. (Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China) ,  He Z. T. (Department of Physics, Hebei Normal University, Shijiazhuang 050016, China) ,  Hibino K. (Faculty of Engineering, Kanagawa University, Yokohama 221-8686, Japan) ,  Hotta N. (Faculty of Education, Utsunomiya University, Utsunomiya 321-8505, Japan) ,  Hu Haibing (Physics Department of Science School, Tibet University, Lhasa 850000, China) ,  Hu H. B. (Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China) ,  Huang J. (Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China) ,  Jia H. Y. (Institute of Modern Physics, SouthWest Jiaotong University, Chengdu 610031, China) ,  Jiang L. (Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China) ,  Jin H. B. (National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China) ,  Kajino F. (Department of Physics, Konan University, Kobe 658-8501, Japan) ,  Kasahara K. (Research Institute for Science and Engineering, Waseda University, Tokyo 169-8555, Japan) ,  Katayose Y. (Faculty of Engineering, Yokohama National University, Yokohama 240-8501, Japan) ,  Kato C. (Department of Physics, Shinshu University, Matsumoto 390-8621, Japan) ,  Kato S. (Institute for Cosmic Ray Research, University of Tokyo, Kashiwa 277-8582, Japan) ,  Kawata K. (Institute for Cosmic Ray Research, University of Tokyo, Kashiwa 277-8582, Japan) ,  Kozai M. (Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (ISAS/JAXA), Sagamihara 252-5210, Japan) ,  Labaciren (Physics Department of Science School, Tibet University, Lhasa 850000, China) ,  Le G. M. (National Center for Space Weather, China Meteorological Administration, Beijing 100081, China) ,  Li A. F. (School of Information Science and Engineering, Shandong Agriculture University, Taian 271018, China) ,  Li A. F. (Department of Physics, Shandong University, Jinan 250100, China) ,  Li A. F. (Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China) ,  Li H. J. (Physics Department of Science School, Tibet University, Lhasa 850000, China) ,  Li W. J. (Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China) ,  Li W. J. (Institute of Modern Physics, SouthWest Jiaotong University, Chengdu 610031, China) ,  Lin Y. H. (Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China) ,  Lin Y. H. (University of Chinese Academy of Sciences, Beijing 100049, China) ,  Liu B. (School of Astronomy and Space Science, Nanjing University, Nanjing 210093, China) ,  Liu C. (Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China) ,  Liu J. S. (Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China) ,  Liu M. Y. (Physics Department of Science School, Tibet University, Lhasa 850000, China) ,  Lou Y.-Q. (Physics Department, Astronomy Department and Tsinghua Center for Astrophysics, Tsinghua-National Astronomical Observatories of China joint Research Center for Astrophysics, Tsinghua University, Beijing 100084, China) ,  Lu H. (Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China) ,  Meng X. R. (Physics Department of Science School, Tibet University, Lhasa 850000, China) ,  Mitsui H. (Faculty of Engineering, Yokohama National University, Yokohama 240-8501, Japan) ,  Munakata K. (Department of Physics, Shinshu University, Matsumoto 390-8621, Japan) ,  Nakamura Y. (Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China) ,  Nanjo H. (Department of Physics, Hirosaki University, Hirosaki 036-8561, Japan) ,  Nishizawa M. (National Institute of Informatics, Tokyo 101-8430, Japan) ,  Ohnishi M. (Institute for Cosmic Ray Research, University of Tokyo, Kashiwa 277-8582, Japan) ,  Ohta I. (Sakushin Gakuin University, Utsunomiya 321-3295, Japan) ,  Ozawa S. (Research Institute for Science and Engineering, Waseda University, Tokyo 169-8555, Japan) ,  Qian X. L. (Department of Mechanical and Electrical Engineering, Shandong Management University, Jinan 250357, China) ,  Qu X. B. (College of Science, China University of Petroleum, Qingdao, 266555, China) ,  Saito T. (Tokyo Metropolitan College of Industrial Technology, Tokyo 116-8523, Japan) ,  Sakata M. (Department of Physics, Konan University, Kobe 658-8501, Japan) ,  Sako T. K. (Institute for Cosmic Ray Research, University of Tokyo, Kashiwa 277-8582, Japan) ,  Sengoku Y. (Faculty of Engineering, Yokohama National University, Yokohama 240-8501, Japan) ,  Shao J. (Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China) ,  Shao J. (Department of Physics, Shandong University, Jinan 250100, China) ,  Shibata M. (Faculty of Engineering, Yokohama National University, Yokohama 240-8501, Japan) ,  Shiomi A. (College of Industrial Technology, Nihon University, Narashino 275-8576, Japan) ,  Sugimoto H. (Shonan Institute of Technology, Fujisawa 251-8511, Japan) ,  Takita M. (Institute for Cosmic Ray Research, University of Tokyo, Kashiwa 277-8582, Japan) ,  Tan Y. H. (Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China) ,  Tateyama N. (Faculty of Engineering, Kanagawa University, Yokohama 221-8686, Japan) ,  Torii S. (Research Institute for Science and Engineering, Waseda University, Tokyo 169-8555, Japan) ,  Tsuchiya H. (Japan Atomic Energy Agency, Tokai-mura 319-1195, Japan) ,  Udo S. (Faculty of Engineering, Kanagawa University, Yokohama 221-8686, Japan) ,  Wang H. (Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China) ,  Wu H. R. (Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China) ,  Xue L. (Department of Physics, Shandong University, Jinan 250100, China) ,  Yagisawa K. (Faculty of Engineering, Yokohama National University, Yokohama 240-8501, Japan) ,  Yamamoto Y. (Department of Physics, Konan University, Kobe 658-8501, Japan) ,  Yang Z. (Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China) ,  Yuan A. F. (Physics Department of Science School, Tibet University, Lhasa 850000, China) ,  Zhai L. M. (National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China) ,  Zhang H. M. (Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China) ,  Zhang J. L. (Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China) ,  Zhang X. (School of Astronomy and Space Science, Nanjing University, Nanjing 210093, China) ,  Zhang X. Y. (Department of Physics, Shandong University, Jinan 250100, China) ,  Zhang Y. (Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China) ,  Zhang Yi (Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China) ,  Zhang Ying (Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China) ,  Zhaxisangzhu (Physics Department of Science School, Tibet University, Lhasa 850000, China) ,  Zhou X. X. (Institute of Modern Physics, SouthWest Jiaotong University, Chengdu 610031, China)
資料名： Physical Review Letters  (Physical Review Letters)
巻： 123  号： 5  ページ： 051101  発行年： 2019年 
JST資料番号： H0070A  ISSN： 0031-9007  CODEN： PRLTAO  資料種別： 逐次刊行物 (A)
記事区分： 原著論文  発行国： アメリカ合衆国 (USA)  言語： 英語 (EN)

抄録/ポイント： 地下水Cherenkov型ミュー検出器アレイによるチベットの空気シャワー配列によって観測されたCrab Nebulaからの最高エネルギー光子について報告する。空気シャワーで測定されたμ粒子数の基準に基づいて,エネルギー[数式:原文を参照]による宇宙線背景イベントの99.92%を抑制することに成功した。結果として,[数式:原文を参照]統計的有意性に対応する5.5の背景イベントに対して,[数式:原文を参照]を伴う24のフォトニック様イベントを観察した。これは天体物理源からの[数式:原文を参照]による光子の最初の検出である。Copyright 2019 The American Physical Society All rights reserved. Translated from English into Japanese by JST.【JST・京大機械翻訳】

シソーラス用語： 宇宙線 ,  チベット自治区 ,  空気シャワー ,  μ粒子 ,  地下水 ,  検出器 ,  *光子 ,  *宇宙物理学

分類 (1件)： 空気シャワー  (DB02070T)

タイトルに関連する用語 (3件)： 宇宙物理 ,  エネルギー ,  光子