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J-GLOBAL ID：201802244807361187   整理番号：18A0287182

銀河起源のEeV陽子の探索【Powered by NICT】

Search for EeV protons of galactic origin

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, Kinki University, Higashi Osaka, Osaka, Japan) ,  Fujii T. (Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Chiba, 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) ,  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 Y. (Graduate School of Science, Osaka City University, Osaka, Osaka, Japan) ,  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) ,  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) ,  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) ,  Kwon Y.J. (Department of Physics, Yonsei University, Seodaemun-gu, Seoul, Korea) ,  Lan J. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, Utah, USA) ,  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) ,  Matsuda T. (Institute of Particle and Nuclear Studies, KEK, Tsukuba, Ibaraki, 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) ,  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 T. (Faculty of Science, Kochi University, Kochi, Kochi, Japan) ,  Nonaka T. (Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Chiba, Japan) ,  Nozato A. (Department of Physics, Kinki University, Higashi 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) ,  Oki K. (Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Chiba, Japan) ,  Okuda T. (Department of Physical Sciences, Ritsumeikan University, Kusatsu, Shiga, 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. (Service de Physique Theorique, Universite Libre de Bruxelles, Brussels, Belgium) ,  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) ,  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) ,  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 T. (Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Chiba, Japan) ,  Shibata F. (Interdisciplinary Graduate School of Medicine and Engineering, University of Yamanashi, Kofu, Yamanashi, 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) ,  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. (Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Chiba, Japan) ,  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. (Faculty of Engineering, Kanagawa University, Yokohama, Kanagawa, Japan) ,  Tanaka M. (Institute of Particle and Nuclear Studies, KEK, Tsukuba, Ibaraki, Japan) ,  Tanaka K. (Graduate School of Information Sciences, Hiroshima City University, Hiroshima, Hiroshima, Japan) ,  Tanaka H. (Graduate School of Science, Osaka City University, Osaka, Osaka, Japan) ,  Thomas S.B. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, Utah, USA) ,  Thomson G.B. (High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, Utah, USA) ,  Tinyakov P. (Institute for Nuclear Research of the Russian Academy of Sciences, Moscow, Russia) ,  Tinyakov P. (Service de Physique Theorique, Universite Libre de Bruxelles, Brussels, Belgium) ,  Tirone A.H. (White Station High School, Memphis, Tennessee, USA) ,  Tkachev I. (Institute for Nuclear Research of the Russian Academy of Sciences, Moscow, Russia) ,  Tokuno H. (Graduate School of Science and Engineering, Tokyo Institute of Technology, Meguro, Tokyo, Japan) ,  Tomida T. (Academic Assembly School of Science and Technology Institute of Engineering, Shinshu University, Nagano, Nagano, Japan) ,  Troitsky S. (Institute for Nuclear Research of the Russian Academy of Sciences, Moscow, Russia) ,  Tsunesada Y. (Graduate School of Science and Engineering, Tokyo Institute of Technology, Meguro, Tokyo, Japan) ,  Uchihori Y. (National Institute of Radiological Science, Chiba, Chiba, Japan)
資料名： Astroparticle Physics  (Astroparticle Physics)
巻： 86  ページ： 21-26  発行年： 2017年 
JST資料番号： W0658A  ISSN： 0927-6505  資料種別： 逐次刊行物 (A)
記事区分： 原著論文  発行国： オランダ (NLD)  言語： 英語 (EN)

抄録/ポイント： エネルギー範囲10~18.0 10~18.5eVにおける宇宙線は光,おそらくプロトン,組成を持つと考えられている。それらの起源を研究するために,それらの到来方向における異方性の探索することができる。銀河系外宇宙線は等方性であるべきであるが,このタイプの銀河宇宙線は銀河面に沿って見られるべきである,銀河反中心方向の近くの方向からの事象の不足すべきである。これは,銀河磁場の影響下での拡散挙動から弾道転移はよく進んでいる事実によるものであり,この定性的な描像は,全エネルギー範囲にわたって持続した。銀河面に沿った増強は,銀河緯度約20°の標準偏差を持つべきであると,銀河反中心方向の方向の不足は銀河経度方向に約50°の標準偏差を持つべきであることを示す銀河磁場のモデルに導かれて,著者らはこれらの効果を探索するためにエネルギー範囲を10~18.5eV~10~18.0における望遠鏡アレイ表面検出器のデータを用いた。データは等方的であった。銀河面に沿った増強と銀河反中心方向の方向の欠損は認められなかった。これらのデータを用いて,95%で1.3%の信頼水準で銀河起源のEeV宇宙線の分率の上限値を設定した。Copyright 2018 Elsevier B.V., Amsterdam. All rights reserved. Translated from English into Japanese by JST.【Powered by NICT】

シソーラス用語： *陽子 ,  経度 ,  宇宙線 ,  等方性 ,  望遠鏡 ,  検出器 ,  信頼度 ,  異方性 ,  銀河宇宙線 ,  わが銀河 ,  標準偏差 ,  緯度 ,  銀河磁場 ,  銀河面 ,  到来方向 ,  度 ,  渦状銀河 ,  天体

著者キーワード (4件)： 宇宙線 ,  銀河陽子 ,  望遠鏡アレイ ,  表面検出器

分類 (1件)： 宇宙線起源  (DB02020Q)

タイトルに関連する用語 (4件)： 銀河 ,  起源 ,  陽子 ,  探索