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J-GLOBAL ID：201802262284992495   Reference number：18A0287205

Detectability of galactic supernova neutrinos coherently scattered on xenon nuclei in XMASS

XMASSにおけるキセノン核の散乱されたコヒーレント銀河超新星ニュートリノの検出可能性【Powered by NICT】

Author (59)： Abe K. (Kamioka Observatory, Institute for Cosmic Ray Research, University of Tokyo, Higashi-Mozumi, Kamioka, Hida, Gifu, 506-1205, Japan) ,  Abe K. (Kavli Institute for the Physics and Mathematics of the Universe (WPI), University of Tokyo, Kashiwa, Chiba, 277-8582, Japan) ,  Hiraide K. (Kamioka Observatory, Institute for Cosmic Ray Research, University of Tokyo, Higashi-Mozumi, Kamioka, Hida, Gifu, 506-1205, Japan) ,  Hiraide K. (Kavli Institute for the Physics and Mathematics of the Universe (WPI), University of Tokyo, Kashiwa, Chiba, 277-8582, Japan) ,  Ichimura K. (Kamioka Observatory, Institute for Cosmic Ray Research, University of Tokyo, Higashi-Mozumi, Kamioka, Hida, Gifu, 506-1205, Japan) ,  Ichimura K. (Kavli Institute for the Physics and Mathematics of the Universe (WPI), University of Tokyo, Kashiwa, Chiba, 277-8582, Japan) ,  Kishimoto Y. (Kamioka Observatory, Institute for Cosmic Ray Research, University of Tokyo, Higashi-Mozumi, Kamioka, Hida, Gifu, 506-1205, Japan) ,  Kishimoto Y. (Kavli Institute for the Physics and Mathematics of the Universe (WPI), University of Tokyo, Kashiwa, Chiba, 277-8582, Japan) ,  Kobayashi K. (Kamioka Observatory, Institute for Cosmic Ray Research, University of Tokyo, Higashi-Mozumi, Kamioka, Hida, Gifu, 506-1205, Japan) ,  Kobayashi K. (Kavli Institute for the Physics and Mathematics of the Universe (WPI), University of Tokyo, Kashiwa, Chiba, 277-8582, Japan) ,  Kobayashi M. (Kamioka Observatory, Institute for Cosmic Ray Research, University of Tokyo, Higashi-Mozumi, Kamioka, Hida, Gifu, 506-1205, Japan) ,  Moriyama S. (Kamioka Observatory, Institute for Cosmic Ray Research, University of Tokyo, Higashi-Mozumi, Kamioka, Hida, Gifu, 506-1205, Japan) ,  Moriyama S. (Kavli Institute for the Physics and Mathematics of the Universe (WPI), University of Tokyo, Kashiwa, Chiba, 277-8582, Japan) ,  Nakagawa K. (Kamioka Observatory, Institute for Cosmic Ray Research, University of Tokyo, Higashi-Mozumi, Kamioka, Hida, Gifu, 506-1205, Japan) ,  Nakahata M. (Kamioka Observatory, Institute for Cosmic Ray Research, University of Tokyo, Higashi-Mozumi, Kamioka, Hida, Gifu, 506-1205, Japan) ,  Nakahata M. (Kavli Institute for the Physics and Mathematics of the Universe (WPI), University of Tokyo, Kashiwa, Chiba, 277-8582, Japan) ,  Norita T. (Kamioka Observatory, Institute for Cosmic Ray Research, University of Tokyo, Higashi-Mozumi, Kamioka, Hida, Gifu, 506-1205, Japan) ,  Ogawa H. (Kamioka Observatory, Institute for Cosmic Ray Research, University of Tokyo, Higashi-Mozumi, Kamioka, Hida, Gifu, 506-1205, Japan) ,  Ogawa H. (Kavli Institute for the Physics and Mathematics of the Universe (WPI), University of Tokyo, Kashiwa, Chiba, 277-8582, Japan) ,  Sekiya H. (Kamioka Observatory, Institute for Cosmic Ray Research, University of Tokyo, Higashi-Mozumi, Kamioka, Hida, Gifu, 506-1205, Japan) ,  Sekiya H. (Kavli Institute for the Physics and Mathematics of the Universe (WPI), University of Tokyo, Kashiwa, Chiba, 277-8582, Japan) ,  Takachio O. (Kamioka Observatory, Institute for Cosmic Ray Research, University of Tokyo, Higashi-Mozumi, Kamioka, Hida, Gifu, 506-1205, Japan) ,  Takeda A. (Kamioka Observatory, Institute for Cosmic Ray Research, University of Tokyo, Higashi-Mozumi, Kamioka, Hida, Gifu, 506-1205, Japan) ,  Takeda A. (Kavli Institute for the Physics and Mathematics of the Universe (WPI), University of Tokyo, Kashiwa, Chiba, 277-8582, Japan) ,  Yamashita M. (Kamioka Observatory, Institute for Cosmic Ray Research, University of Tokyo, Higashi-Mozumi, Kamioka, Hida, Gifu, 506-1205, Japan) ,  Yamashita M. (Kavli Institute for the Physics and Mathematics of the Universe (WPI), University of Tokyo, Kashiwa, Chiba, 277-8582, Japan) ,  Yang B.S. (Kamioka Observatory, Institute for Cosmic Ray Research, University of Tokyo, Higashi-Mozumi, Kamioka, Hida, Gifu, 506-1205, Japan) ,  Yang B.S. (Kavli Institute for the Physics and Mathematics of the Universe (WPI), University of Tokyo, Kashiwa, Chiba, 277-8582, Japan) ,  Kim N.Y. (Center of Underground Physics, Institute for Basic Science, 70 Yuseong-daero 1689-gil, Yuseong-gu, Daejeon, 305-811, South Korea) ,  Kim Y.D. (Center of Underground Physics, Institute for Basic Science, 70 Yuseong-daero 1689-gil, Yuseong-gu, Daejeon, 305-811, South Korea) ,  Tasaka S. (Information and multimedia center, Gifu University, Gifu 501-1193, Japan) ,  Liu J. (Kavli Institute for the Physics and Mathematics of the Universe (WPI), University of Tokyo, Kashiwa, Chiba, 277-8582, Japan) ,  Martens K. (Kavli Institute for the Physics and Mathematics of the Universe (WPI), University of Tokyo, Kashiwa, Chiba, 277-8582, Japan) ,  Suzuki Y. (Kavli Institute for the Physics and Mathematics of the Universe (WPI), University of Tokyo, Kashiwa, Chiba, 277-8582, Japan) ,  Fujita R. (Department of Physics, Kobe University, Kobe, Hyogo 657-8501, Japan) ,  Hosokawa K. (Department of Physics, Kobe University, Kobe, Hyogo 657-8501, Japan) ,  Miuchi K. (Department of Physics, Kobe University, Kobe, Hyogo 657-8501, Japan) ,  Oka N. (Department of Physics, Kobe University, Kobe, Hyogo 657-8501, Japan) ,  Onishi Y. (Department of Physics, Kobe University, Kobe, Hyogo 657-8501, Japan) ,  Takeuchi Y. (Department of Physics, Kobe University, Kobe, Hyogo 657-8501, Japan) ,  Takeuchi Y. (Kavli Institute for the Physics and Mathematics of the Universe (WPI), University of Tokyo, Kashiwa, Chiba, 277-8582, Japan) ,  Kim Y.H. (Korea Research Institute of Standards and Science, Daejeon 305-340, South Korea) ,  Kim Y.H. (Center of Underground Physics, Institute for Basic Science, 70 Yuseong-daero 1689-gil, Yuseong-gu, Daejeon, 305-811, South Korea) ,  Lee J.S. (Korea Research Institute of Standards and Science, Daejeon 305-340, South Korea) ,  Lee K.B. (Korea Research Institute of Standards and Science, Daejeon 305-340, South Korea) ,  Lee M.K. (Korea Research Institute of Standards and Science, Daejeon 305-340, South Korea) ,  Fukuda Y. (Department of Physics, Miyagi University of Education, Sendai, Miyagi 980-0845, Japan) ,  Itow Y. (Institute for Space-Earth Environmental Research, Nagoya University, Nagoya, Aichi 464-8602, Japan) ,  Itow Y. (Kobayashi-Maskawa Institute for the Origin of Particles and the Universe, Nagoya University, Furo-cho, Chikusa-ku, Nagoya, Aichi, 464-8602, Japan) ,  Kegasa R. (Institute for Space-Earth Environmental Research, Nagoya University, Nagoya, Aichi 464-8602, Japan) ,  Kobayashi K. (Institute for Space-Earth Environmental Research, Nagoya University, Nagoya, Aichi 464-8602, Japan) ,  Masuda K. (Institute for Space-Earth Environmental Research, Nagoya University, Nagoya, Aichi 464-8602, Japan) ,  Takiya H. (Institute for Space-Earth Environmental Research, Nagoya University, Nagoya, Aichi 464-8602, Japan) ,  Uchida H. (Institute for Space-Earth Environmental Research, Nagoya University, Nagoya, Aichi 464-8602, Japan) ,  Nishijima K. (Department of Physics, Tokai University, Hiratsuka, Kanagawa 259-1292, Japan) ,  Fujii K. (Department of Physics, Faculty of Engineering, Yokohama National University, Yokohama, Kanagawa 240-8501, Japan) ,  Murayama I. (Department of Physics, Faculty of Engineering, Yokohama National University, Yokohama, Kanagawa 240-8501, Japan) ,  Nakamura S. (Department of Physics, Faculty of Engineering, Yokohama National University, Yokohama, Kanagawa 240-8501, Japan) ,  XMASS Collaboration
Material： Astroparticle Physics  (Astroparticle Phys)
Volume： 89  Page： 51-56  Publication year： 2017 
JST Material Number： W0658A  ISSN： 0927-6505  Document type： Article
Article type： 原著論文  Country of issue： Netherlands (NLD)  Language： ENGLISH (EN)

Abstract/Point： The coherent elastic neutrino-...

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Thesaurus term： *Xenon ,  dark matter ,  earth(the globe) ,  *supernova ,  time evolution ,  *coherence ,  *neutrino ,  model ,  supernova explosion ,  elasticity (mechanical property) ,  electric current ,  detector ,  neutrino source ,  *supernova neutrino ,  planet ,  mechanical property

Author keywords (4)： Supernova ,  Neutrino ,  Coherent scattering ,  Liquid xenon

JST classification (5)： Muon and neutrino  (DB02080E) ,  Cosmic ray and astrophysical observing technology  (DB01000N) ,  Nebulae  (DB06000W) ,  Leptons  (BF04040K) ,  Neutrino interactions  (BF03030S)

Terms in the title (6)： キセノン ,  核 ,  散乱 ,  コヒーレント ,  銀河 ,  超新星ニュートリノ