文献

J-GLOBAL ID：202002259487127607   整理番号：20A2335515

ハイブリッドモードにおける望遠鏡アレイ黒岩メサおよび長リッジ蛍光検出器および表面アレイによる陽子-空気断面積の測定【JST・京大機械翻訳】

Measurement of the proton-air cross section with Telescope Array’s Black Rock Mesa and Long Ridge fluorescence detectors, and surface array in hybrid mode

著者 (120件)： Abbasi R. U. (Department of Physics, Loyola University Chicago, Chicago, Illinois, 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. (Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Chiba, Japan) ,  di Matteo A. (Service de Physique Thorique, Universit Libre de Bruxelles, Brussels, Belgium) ,  Fujii T. (The Hakubi Center for Advanced Research and Graduate School of Science, Kyoto University, Kitashirakawa-Oiwakecho, Sakyo-ku, Kyoto, Japan) ,  Fujisue K. (Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Chiba, Japan) ,  Fujita K. (Graduate School of Science, Osaka City University, Osaka, Osaka, Japan) ,  Fujiwara R. (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, 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) ,  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) ,  Hayashida N. (Faculty of Engineering, Kanagawa University, Yokohama, Kanagawa, Japan) ,  Hibino K. (Faculty of Engineering, Kanagawa University, Yokohama, Kanagawa, Japan) ,  Higuchi R. (Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Chiba, Japan) ,  Honda K. (Interdisciplinary Graduate School of Medicine and Engineering, University of Yamanashi, Kofu, Yamanashi, Japan) ,  Ikeda D. (Earthquake Research Institute, University of Tokyo, Bunkyo-ku, Tokyo, Japan) ,  Inadomi T. (Academic Assembly School of Science and Technology Institute of Engineering, Shinshu University, Nagano, Nagano, 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) ,  Iwakura H. (Academic Assembly School of Science and Technology Institute of Engineering, Shinshu University, Nagano, Nagano, Japan) ,  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. (Faculty of Engineering, Kanagawa University, Yokohama, Kanagawa, Japan) ,  Kalashev O. (Institute for Nuclear Research of the Russian Academy of Sciences, Moscow, Russia) ,  Kasahara K. (Faculty of Systems Engineering and Science, Shibaura Institute of Technology, Minato-ku, Tokyo, Japan) ,  Kasami S. (Department of Engineering Science, Faculty of Engineering, Osaka Electro-Communication University, Neyagawa-shi, Osaka, 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. (Graduate School of Science, Osaka City University, Osaka, Osaka, Japan) ,  Kim J. H. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, Utah, USA) ,  Kim M. H. (Department of Physics, Sungkyunkwan University, Jang-an-gu, Suwon, Korea) ,  Kim S. W. (Department of Physics, Sungkyunkwan University, Jang-an-gu, Suwon, Korea) ,  Kishigami S. (Graduate School of Science, Osaka City University, Osaka, Osaka, 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) ,  Kuznetsov M. (Service de Physique Thorique, Universit Libre de Bruxelles, Brussels, Belgium) ,  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) ,  Matsumiya H. (Graduate School of Science, Osaka City University, Osaka, Osaka, 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) ,  Nagataki S. (Astrophysical Big Bang Laboratory, RIKEN, Wako, Saitama, Japan) ,  Nakai K. (Graduate School of Science, Osaka City University, Osaka, Osaka, 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) ,  Nakamura Y. (Academic Assembly School of Science and Technology Institute of Engineering, Shinshu University, Nagano, Nagano, Japan) ,  Nakamura Y. (Academic Assembly School of Science and Technology Institute of Engineering, Shinshu University, Nagano, Nagano, 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) ,  Ogio S. (Nambu Yoichiro Institute of Theoretical and Experimental Physics, Osaka City University, Osaka, Osaka, 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) ,  Oku Y. (Department of Engineering Science, Faculty of Engineering, Osaka Electro-Communication University, Neyagawa-shi, Osaka, 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. (Quantum ICT Advanced Development Center, National Institute for Information and Communications Technology, Koganei, 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 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) ,  Sako T. (Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Chiba, Japan) ,  Sakurai N. (Graduate School of Science, Osaka City University, Osaka, Osaka, Japan) ,  Sano K. (Academic Assembly School of Science and Technology Institute of Engineering, Shinshu University, Nagano, Nagano, Japan) ,  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. (Department of Physics, School of Natural Sciences, Ulsan National Institute of Science and Technology, UNIST-gil, Ulsan, Korea) ,  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) ,  Sone N. (Academic Assembly School of Science and Technology Institute of Engineering, Shinshu University, Nagano, Nagano, Japan) ,  Stokes B. T. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, Utah, 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)
資料名： Physical Review. D  (Physical Review. D)
巻： 102  号： 6  ページ： 062004  発行年： 2020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は,陽子断面積を測定するために,Universeで最も高い既知のエネルギー源を提供する。そのようなデータを収集する条件は加速器環境より制御されていないが,現在の発電宇宙線観測器は,実験室において達成できるエネルギーに対する信頼できる測定に対して,大きな統計を収集するための十分な曝露を有する。断面積の宇宙線測定は,一次粒子のエネルギーと質量に関係する空気シャワーの最大([数式:原文を参照])の深さを測定するために大気熱量測定を用いる。[数式:原文を参照]分布の尾部は,陽子によって発生するシャワーによって支配され,非弾性プロトン-空気断面積の測定を可能にした。本研究では,陽子-空気非弾性断面積測定([数式:原文を参照])を,望遠鏡アレイのブラックロックメサとLong Ridge蛍光検出器およびハイブリッドモードにおける表面検出器アレイによって観測したデータを用いて,提示した。[数式:原文を参照]は[数式:原文を参照]であることが観察された。全プロトン-プロトン断面積は,その後Glauber形式から推論され,[数式:原文を参照]であることが分かった。Copyright 2020 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 ,  加速器 ,  空気シャワー ,  *断面積 ,  *望遠鏡 ,  *陽子 ,  熱量測定 ,  観測装置 ,  発電 ,  検出器 ,  *蛍光検出器 ,  非弾性
準シソーラス用語： 超高エネルギー宇宙線 , 【Automatic Indexing@JST】

分類 (2件)： ハドロンによって引き起されるその他の反応  (BF03100U) ,  強い相互作用の模型  (BF02040W)

タイトルに関連する用語 (6件)： 望遠鏡 ,  アレイ ,  リッジ ,  蛍光検出器 ,  陽子 ,  断面積