文献

J-GLOBAL ID：202002216844463783   整理番号：20A2217859

望遠鏡アレイ表面検出器による超高エネルギーニュートリノの探索【JST・京大機械翻訳】

Search for Ultra-High-Energy Neutrinos with the Telescope Array Surface Detector

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, 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, 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, Seoul, Korea) ,  Chiba J. (Department of Physics, Tokyo University of Science, Chiba, Japan) ,  Chikawa M. (Department of Physics, Kindai University, Osaka, Japan) ,  di Matteo A. (Service de Physique Theorique, Universite Libre de Bruxelles, Brussels, Belgium) ,  Fujii T. (Hakubi Center for Advanced Research and Graduate School of Science, Kyoto University, Kyoto, Japan) ,  Fujii T. (Graduate School of Science, Osaka City University, Osaka, Japan) ,  Fujita K. (Graduate School of Science, Osaka City University, Osaka, Japan) ,  Fujiwara R. (Graduate School of Science, Osaka City University, Osaka, Japan) ,  Fukushima M. (Institute for Cosmic Ray Research, University of Tokyo, Chiba, Japan) ,  Fukushima M. (Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, University of Tokyo, 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, Japan) ,  Hayashi Y. (Graduate School of Science, Osaka City University, Osaka, Japan) ,  Hayashida N. (Faculty of Engineering, Kanagawa University, Kanagawa, Japan) ,  Hibino K. (Faculty of Engineering, Kanagawa University, Kanagawa, Japan) ,  Honda K. (Interdisciplinary Graduate School of Medicine and Engineering, University of Yamanashi, Yamanashi, Japan) ,  Ikeda D. (Institute for Cosmic Ray Research, University of Tokyo, Chiba, Japan) ,  Inoue N. (The Graduate School of Science and Engineering, Saitama University, Saitama, Japan) ,  Ishii T. (Interdisciplinary Graduate School of Medicine and Engineering, University of Yamanashi, Yamanashi, Japan) ,  Ishimori R. (Graduate School of Science and Engineering, Tokyo Institute of Technology, Tokyo, Japan) ,  Ito H. (Astrophysical Big Bang Laboratory, RIKEN, 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, Suwon, Korea) ,  Jeong S. (Department of Physics, Sungkyunkwan University, 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, Tokyo, Japan) ,  Kakimoto F. (Graduate School of Science and Engineering, Tokyo Institute of Technology, 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, Tokyo, Japan) ,  Kawai H. (Department of Physics, Chiba University, Chiba, Japan) ,  Kawakami S. (Graduate School of Science, Osaka City University, Osaka, Japan) ,  Kawana S. (The Graduate School of Science and Engineering, Saitama University, Saitama, Japan) ,  Kawata K. (Institute for Cosmic Ray Research, University of Tokyo, Chiba, Japan) ,  Kido E. (Institute for Cosmic Ray Research, University of Tokyo, Chiba, Japan) ,  Kim H. B. (Department of Physics and The Research Institute of Natural Science, Hanyang University, Seoul, Korea) ,  Kim J. H. (Department of Physics, School of Natural Sciences, Ulsan National Institute of Science and Technology, Ulsan, Korea) ,  Kim J. H. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, Utah, USA) ,  Kishigami S. (Graduate School of Science, Osaka City University, Osaka, Japan) ,  Kitamura S. (Graduate School of Science and Engineering, Tokyo Institute of Technology, Tokyo, Japan) ,  Kitamura Y. (Graduate School of Science and Engineering, Tokyo Institute of Technology, 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, Seoul, Korea) ,  Lee K. H. (Department of Physics, Sungkyunkwan University, 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, Yamanashi, Japan) ,  Martens K. (Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, University of Tokyo, Chiba, Japan) ,  Matsuyama T. (Graduate School of Science, Osaka City University, 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, Japan) ,  Minamino M. (Graduate School of Science, Osaka City University, Osaka, Japan) ,  Mukai K. (Interdisciplinary Graduate School of Medicine and Engineering, University of Yamanashi, 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, Japan) ,  Nagataki S. (Astrophysical Big Bang Laboratory, RIKEN, Saitama, Japan) ,  Nakai K. (Graduate School of Science, Osaka City University, Osaka, Japan) ,  Nakamura R. (Academic Assembly School of Science and Technology Institute of Engineering, Shinshu University, Nagano, Japan) ,  Nakamura T. (Faculty of Science, Kochi University, Kochi, Japan) ,  Nonaka T. (Institute for Cosmic Ray Research, University of Tokyo, Chiba, Japan) ,  Oda H. (Graduate School of Science, Osaka City University, Osaka, Japan) ,  Ogio S. (Graduate School of Science, Osaka City University, Osaka, Japan) ,  Ogio S. (Nambu Yoichiro Institute of Theoretical and Experimental Physics, Osaka City University, Osaka, Japan) ,  Ogura J. (Graduate School of Science and Engineering, Tokyo Institute of Technology, Tokyo, Japan) ,  Ohnishi M. (Institute for Cosmic Ray Research, University of Tokyo, Chiba, Japan) ,  Ohoka H. (Institute for Cosmic Ray Research, University of Tokyo, Chiba, Japan) ,  Okuda T. (Department of Physical Sciences, Ritsumeikan University, Shiga, Japan) ,  Omura Y. (Graduate School of Science, Osaka City University, Osaka, Japan) ,  Ono M. (Astrophysical Big Bang Laboratory, RIKEN, Saitama, Japan) ,  Onogi R. (Graduate School of Science, Osaka City University, Osaka, Japan) ,  Oshima A. (Graduate School of Science, Osaka City University, Osaka, Japan) ,  Ozawa S. (Advanced Research Institute for Science and Engineering, Waseda University, Tokyo, Japan) ,  Park I. H. (Department of Physics, Sungkyunkwan University, Suwon, Korea) ,  Pshirkov M. S. (Institute for Nuclear Research of the Russian Academy of Sciences, Moscow, Russia) ,  Pshirkov M. S. (Sternberg Astronomical Institute, Moscow 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, Ulsan, Korea) ,  Sagawa H. (Institute for Cosmic Ray Research, University of Tokyo, Chiba, Japan) ,  Sahara R. (Graduate School of Science, Osaka City University, Osaka, Japan) ,  Saito K. (Institute for Cosmic Ray Research, University of Tokyo, Chiba, Japan) ,  Saito Y. (Academic Assembly School of Science and Technology Institute of Engineering, Shinshu University, Nagano, Japan) ,  Sakaki N. (Institute for Cosmic Ray Research, University of Tokyo, Chiba, Japan) ,  Sako T. (Institute for Cosmic Ray Research, University of Tokyo, Chiba, Japan) ,  Sakurai N. (Graduate School of Science, Osaka City University, 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, Japan) ,  Sekino K. (Institute for Cosmic Ray Research, University of Tokyo, 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, Yamanashi, Japan) ,  Shibata T. (Institute for Cosmic Ray Research, University of Tokyo, Chiba, Japan) ,  Shimodaira H. (Institute for Cosmic Ray Research, University of Tokyo, Chiba, Japan) ,  Shin B. K. (Graduate School of Science, Osaka City University, Osaka, Japan) ,  Shin H. S. (Institute for Cosmic Ray Research, University of Tokyo, 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, Japan) ,  Takagi Y. (Graduate School of Science, Osaka City University, Osaka, Japan) ,  Takahashi Y. (Graduate School of Science, Osaka City University, Osaka, Japan) ,  Takamura M. (Department of Physics, Tokyo University of Science, Chiba, Japan) ,  Takeda M. (Institute for Cosmic Ray Research, University of Tokyo, Chiba, Japan) ,  Takeishi R. (Department of Physics, Sungkyunkwan University, Suwon, Korea) ,  Taketa A. (Earthquake Research Institute, University of Tokyo, Tokyo, Japan) ,  Takita M. (Institute for Cosmic Ray Research, University of Tokyo, Chiba, Japan)
資料名： Journal of Experimental and Theoretical Physics  (Journal of Experimental and Theoretical Physics)
巻： 131  号： 2  ページ： 255-264  発行年： 2020年 
JST資料番号： A1014A  ISSN： 1063-7761  資料種別： 逐次刊行物 (A)
記事区分： 原著論文  発行国： ドイツ (DEU)  言語： 英語 (EN)

抄録/ポイント： 望遠鏡アレイ表面検出器(2008年11月5日から2017年10月5日)で収集された9年間のデータで導出されたE>1018eVの超高エネルギー下降ニュートリノのフラックスに関する上限を示した。この方法は,多変量解析技術,いわゆるブーステッドディシジョンツリー(BDT)に基づいている。陽子-ニュートリノ分類器は,シャワーフロントの性質と横方向分布関数の両方に関連する16の観測可能に構築される。Copyright Pleiades Publishing, Inc. 2020 Translated from English into Japanese by JST.【JST・京大機械翻訳】

シソーラス用語： 分布関数 ,  *望遠鏡 ,  陽子 ,  多変量解析 ,  *ニュートリノ ,  検出器
準シソーラス用語： シャワー ,  高エネルギー , 【Automatic Indexing@JST】

分類 (2件)： ミュー粒子とニュートリノ  (DB02080E) ,  空気シャワー  (DB02070T)

タイトルに関連する用語 (6件)： 望遠鏡 ,  アレイ ,  検出器 ,  高エネルギー ,  ニュートリノ ,  探索