文献

J-GLOBAL ID：201902291479228712   整理番号：19A0556756

望遠鏡アレイ実験で測定した超高エネルギー宇宙線空気シャワーからのミューオンの研究【JST・京大機械翻訳】

Study of muons from ultrahigh energy cosmic ray air showers measured with the Telescope Array experiment

著者 (120件)： Abbasi R. U. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, Utah, USA) ,  Abe M. (The Graduate School of Science and Engineering, Saitama University, Saitama, Saitama, Japan) ,  Abu-Zayyad T. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, Utah, USA) ,  Allen M. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, Utah, USA) ,  Azuma R. (Graduate School of Science and Engineering, Tokyo Institute of Technology, Meguro, Tokyo, Japan) ,  Barcikowski E. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, Utah, USA) ,  Belz J. W. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, Utah, USA) ,  Bergman D. R. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, Utah, USA) ,  Blake S. A. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, Utah, USA) ,  Cady R. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, Utah, USA) ,  Cheon B. G. (Department of Physics and The Research Institute of Natural Science, Hanyang University, Seongdong-gu, Seoul, Korea) ,  Chiba J. (Department of Physics, Tokyo University of Science, Noda, Chiba, Japan) ,  Chikawa M. (Department of Physics, Kindai University, Higashi Osaka, Osaka, Japan) ,  Di Matteo A. (Service de Physique Theorique, Universite Libre de Bruxelles, Brussels, Belgium) ,  Fujii T. (Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Chiba, Japan) ,  Fujita K. (Graduate School of Science, Osaka City University, Osaka, Osaka, Japan) ,  Fukushima M. (Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Chiba, Japan) ,  Fukushima M. (Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, the University of Tokyo, Kashiwa, Chiba, Japan) ,  Furlich G. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, Utah, USA) ,  Goto T. (Graduate School of Science, Osaka City University, Osaka, Osaka, Japan) ,  Hanlon W. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, Utah, USA) ,  Hayashi M. (Information Engineering Graduate School of Science and Technology, Shinshu University, Nagano, Nagano, Japan) ,  Hayashi Y. (Graduate School of Science, Osaka City University, Osaka, Osaka, Japan) ,  Hayashida N. (Faculty of Engineering, Kanagawa University, Yokohama, Kanagawa, Japan) ,  Hibino K. (Faculty of Engineering, Kanagawa University, Yokohama, Kanagawa, Japan) ,  Honda K. (Interdisciplinary Graduate School of Medicine and Engineering, University of Yamanashi, Kofu, Yamanashi, Japan) ,  Ikeda D. (Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Chiba, Japan) ,  Inoue N. (The Graduate School of Science and Engineering, Saitama University, Saitama, Saitama, Japan) ,  Ishii T. (Interdisciplinary Graduate School of Medicine and Engineering, University of Yamanashi, Kofu, Yamanashi, Japan) ,  Ishimori R. (Graduate School of Science and Engineering, Tokyo Institute of Technology, Meguro, Tokyo, Japan) ,  Ito H. (Astrophysical Big Bang Laboratory, RIKEN, Wako, Saitama, Japan) ,  Ivanov D. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, Utah, USA) ,  Jeong H. M. (Department of Physics, Sungkyunkwan University, Jang-an-gu, Suwon, Korea) ,  Jeong S. (Department of Physics, Sungkyunkwan University, Jang-an-gu, Suwon, Korea) ,  Jui C. C. H. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, Utah, USA) ,  Kadota K. (Department of Physics, Tokyo City University, Setagaya-ku, Tokyo, Japan) ,  Kakimoto F. (Graduate School of Science and Engineering, Tokyo Institute of Technology, Meguro, Tokyo, Japan) ,  Kalashev O. (Institute for Nuclear Research of the Russian Academy of Sciences, Moscow, Russia) ,  Kasahara K. (Advanced Research Institute for Science and Engineering, Waseda University, Shinjuku-ku, Tokyo, Japan) ,  Kawai H. (Department of Physics, Chiba University, Chiba, Chiba, Japan) ,  Kawakami S. (Graduate School of Science, Osaka City University, Osaka, Osaka, Japan) ,  Kawana S. (The Graduate School of Science and Engineering, Saitama University, Saitama, Saitama, Japan) ,  Kawata K. (Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Chiba, Japan) ,  Kido E. (Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Chiba, Japan) ,  Kim H. B. (Department of Physics and The Research Institute of Natural Science, Hanyang University, Seongdong-gu, Seoul, Korea) ,  Kim J. H. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, Utah, USA) ,  Kim J. H. (Department of Physics, School of Natural Sciences, Ulsan National Institute of Science and Technology, UNIST-gil, Ulsan, Korea) ,  Kishigami S. (Graduate School of Science, Osaka City University, Osaka, Osaka, Japan) ,  Kitamura S. (Graduate School of Science and Engineering, Tokyo Institute of Technology, Meguro, Tokyo, Japan) ,  Kitamura Y. (Graduate School of Science and Engineering, Tokyo Institute of Technology, Meguro, Tokyo, Japan) ,  Kuzmin V. (Institute for Nuclear Research of the Russian Academy of Sciences, Moscow, Russia) ,  Kuznetsov M. (Institute for Nuclear Research of the Russian Academy of Sciences, Moscow, Russia) ,  Kwon Y. J. (Department of Physics, Yonsei University, Seodaemun-gu, Seoul, Korea) ,  Lee K. H. (Department of Physics, Sungkyunkwan University, Jang-an-gu, Suwon, Korea) ,  Lubsandorzhiev B. (Institute for Nuclear Research of the Russian Academy of Sciences, Moscow, Russia) ,  Lundquist J. P. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, Utah, USA) ,  Machida K. (Interdisciplinary Graduate School of Medicine and Engineering, University of Yamanashi, Kofu, Yamanashi, Japan) ,  Martens K. (Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, the University of Tokyo, Kashiwa, Chiba, Japan) ,  Matsuyama T. (Graduate School of Science, Osaka City University, Osaka, Osaka, Japan) ,  Matthews J. N. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, Utah, USA) ,  Mayta R. (Graduate School of Science, Osaka City University, Osaka, Osaka, Japan) ,  Minamino M. (Graduate School of Science, Osaka City University, Osaka, Osaka, Japan) ,  Mukai K. (Interdisciplinary Graduate School of Medicine and Engineering, University of Yamanashi, Kofu, Yamanashi, Japan) ,  Myers I. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, Utah, USA) ,  Nagasawa K. (The Graduate School of Science and Engineering, Saitama University, Saitama, Saitama, Japan) ,  Nagataki S. (Astrophysical Big Bang Laboratory, RIKEN, Wako, Saitama, Japan) ,  Nakamura R. (Academic Assembly School of Science and Technology Institute of Engineering, Shinshu University, Nagano, Nagano, Japan) ,  Nakamura T. (Faculty of Science, Kochi University, Kochi, Kochi, Japan) ,  Nonaka T. (Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Chiba, Japan) ,  Oda H. (Graduate School of Science, Osaka City University, Osaka, Osaka, Japan) ,  Ogio S. (Graduate School of Science, Osaka City University, Osaka, Osaka, Japan) ,  Ogura J. (Graduate School of Science and Engineering, Tokyo Institute of Technology, Meguro, Tokyo, Japan) ,  Ohnishi M. (Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Chiba, Japan) ,  Ohoka H. (Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Chiba, Japan) ,  Okuda T. (Department of Physical Sciences, Ritsumeikan University, Kusatsu, Shiga, Japan) ,  Omura Y. (Graduate School of Science, Osaka City University, Osaka, Osaka, Japan) ,  Ono M. (Astrophysical Big Bang Laboratory, RIKEN, Wako, Saitama, Japan) ,  Onogi R. (Graduate School of Science, Osaka City University, Osaka, Osaka, Japan) ,  Oshima A. (Graduate School of Science, Osaka City University, Osaka, Osaka, Japan) ,  Ozawa S. (Advanced Research Institute for Science and Engineering, Waseda University, Shinjuku-ku, Tokyo, Japan) ,  Park I. H. (Department of Physics, Sungkyunkwan University, Jang-an-gu, Suwon, Korea) ,  Pshirkov M. S. (Institute for Nuclear Research of the Russian Academy of Sciences, Moscow, Russia) ,  Pshirkov M. S. (Sternberg Astronomical Institute, Moscow M.V. Lomonosov State University, Moscow, Russia) ,  Remington J. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, Utah, USA) ,  Rodriguez D. C. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, Utah, USA) ,  Rubtsov G. (Institute for Nuclear Research of the Russian Academy of Sciences, Moscow, Russia) ,  Ryu D. (Department of Physics, School of Natural Sciences, Ulsan National Institute of Science and Technology, UNIST-gil, Ulsan, Korea) ,  Sagawa H. (Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Chiba, Japan) ,  Sahara R. (Graduate School of Science, Osaka City University, Osaka, Osaka, Japan) ,  Saito K. (Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Chiba, Japan) ,  Saito Y. (Academic Assembly School of Science and Technology Institute of Engineering, Shinshu University, Nagano, Nagano, Japan) ,  Sakaki N. (Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Chiba, Japan) ,  Sakurai N. (Graduate School of Science, Osaka City University, Osaka, Osaka, Japan) ,  Scott L. M. (Department of Physics and Astronomy, Rutgers University-The State University of New Jersey, Piscataway, New Jersey, USA) ,  Seki T. (Academic Assembly School of Science and Technology Institute of Engineering, Shinshu University, Nagano, Nagano, Japan) ,  Sekino K. (Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Chiba, Japan) ,  Shah P. D. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, Utah, USA) ,  Shibata F. (Interdisciplinary Graduate School of Medicine and Engineering, University of Yamanashi, Kofu, Yamanashi, Japan) ,  Shibata T. (Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Chiba, Japan) ,  Shimodaira H. (Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Chiba, Japan) ,  Shin B. K. (Graduate School of Science, Osaka City University, Osaka, Osaka, Japan) ,  Shin H. S. (Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Chiba, Japan) ,  Smith J. D. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, Utah, USA) ,  Sokolsky P. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, Utah, USA) ,  Stokes B. T. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, Utah, USA) ,  Stratton S. R. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, Utah, USA) ,  Stratton S. R. (Department of Physics and Astronomy, Rutgers University-The State University of New Jersey, Piscataway, New Jersey, USA) ,  Stroman T. A. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, Utah, USA) ,  Suzawa T. (The Graduate School of Science and Engineering, Saitama University, Saitama, Saitama, Japan) ,  Takagi Y. (Graduate School of Science, Osaka City University, Osaka, Osaka, Japan) ,  Takahashi Y. (Graduate School of Science, Osaka City University, Osaka, Osaka, Japan) ,  Takamura M. (Department of Physics, Tokyo University of Science, Noda, Chiba, Japan) ,  Takeda M. (Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Chiba, Japan) ,  Takeishi R. (Department of Physics, Sungkyunkwan University, Jang-an-gu, Suwon, Korea) ,  Taketa A. (Earthquake Research Institute, University of Tokyo, Bunkyo-ku, Tokyo, Japan) ,  Takita M. (Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Chiba, Japan) ,  Tameda Y. (Department of Engineering Science, Faculty of Engineering, Osaka Electro-Communication University, Neyagawa-shi, Osaka, Japan) ,  Tanaka H. (Graduate School of Science, Osaka City University, Osaka, Osaka, Japan) ,  Tanaka K. (Graduate School of Information Sciences, Hiroshima City University, Hiroshima, Hiroshima, Japan) ,  Tanaka M. (Institute of Particle and Nuclear Studies, KEK, Tsukuba, Ibaraki, Japan)
資料名： Physical Review. D  (Physical Review. D)
巻： 98  号： 2  ページ： 022002  発行年： 2018年 
JST資料番号： D0748A  ISSN： 2470-0010  CODEN： PRVDAQ  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： 超高エネルギー宇宙線データの解釈における不確実性の一つは,空気シャワーモンテカルロ(MC)シミュレーションに使用されるハドロン相互作用モデルに由来する。超高エネルギー宇宙線誘起空気シャワーから地上で観測されたミュオンの数はハドロン相互作用モデルに依存すると期待される。したがって,1つは,測定されたミュオン数をMC予測と比較することにより,ハドロン相互作用モデルをテストすることができる。本論文では,高いμ粒子純度を持つ表面検出器ステーションの信号を分析することによって得られた超高エネルギー大規模空気シャワーにおけるミュー粒子密度の研究結果を示した。観測所のミュオン純度はシャワーの傾斜とステーションの相対位置の両方に依存する。望遠鏡アレイ実験からの7年間のデータにおいて,シャワーコアから2000mの横距離で[数式:原文を参照]の期待μ粒子純度を持つ信号に対して観測された粒子数は,陽子誘起シャワーに対するQGSJET II-03モデルを用いたMC予測値よりも[数式:原文を参照]倍大きいことを見出した。同様の効果は,QGSJET II-04のような他のハドロンモデルとの比較でも見られ,[数式:原文を参照]過剰を示した。また,これらの過剰の横方向距離への依存性を研究し,MCと比較して,データ中のμ粒子の横方向分布のより遅い減少を見出し,より大きな横方向距離においてより大きな不一致を引き起こした。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： *望遠鏡 ,  シミュレーション ,  モンテカルロ法 ,  ハドロン ,  検出器 ,  *シャワー ,  純度 ,  陽子 ,  *空気シャワー ,  *μ粒子 ,  不確実性 ,  予測 ,  相互作用
準シソーラス用語： *高エネルギー ,  *超高エネルギー宇宙線 , 【Automatic Indexing@JST】

分類 (5件)： エキゾチック原子・分子  (BH09010S) ,  電磁場と統一ゲージ場  (BF02020A) ,  ハドロンによって引き起されるその他の反応  (BF03100U) ,  ミュー粒子とニュートリノ  (DB02080E) ,  レプトンの電磁相互作用・弱い相互作用  (BF03020H)

タイトルに関連する用語 (7件)： 望遠鏡 ,  アレイ ,  実験 ,  高エネルギー宇宙線 ,  空気シャワー ,  ミューオン ,  研究