文献

J-GLOBAL ID：201902236025660574   整理番号：19A1470933

Super-Kamiokandeにおける大気ニュートリノを用いたニュートリノ-酸素中性カレント準弾性断面積の測定【JST・京大機械翻訳】

Measurement of the neutrino-oxygen neutral-current quasielastic cross section using atmospheric neutrinos at Super-Kamiokande

著者 (120件)： Wan L. (Department of Engineering Physics, Tsinghua University, Beijing, 100084, China) ,  Abe K. (Kamioka Observatory, Institute for Cosmic Ray Research, University of Tokyo, Kamioka, Gifu 506-1205, Japan) ,  Abe K. (Kavli Institute for the Physics and Mathematics of the Universe (WPI), The University of Tokyo Institutes for Advanced Study, University of Tokyo, Kashiwa, Chiba 277-8583, Japan) ,  Bronner C. (Kamioka Observatory, Institute for Cosmic Ray Research, University of Tokyo, Kamioka, Gifu 506-1205, Japan) ,  Hayato Y. (Kamioka Observatory, Institute for Cosmic Ray Research, University of Tokyo, Kamioka, Gifu 506-1205, Japan) ,  Hayato Y. (Kavli Institute for the Physics and Mathematics of the Universe (WPI), The University of Tokyo Institutes for Advanced Study, University of Tokyo, Kashiwa, Chiba 277-8583, Japan) ,  Ikeda M. (Kamioka Observatory, Institute for Cosmic Ray Research, University of Tokyo, Kamioka, Gifu 506-1205, Japan) ,  Iyogi K. (Kamioka Observatory, Institute for Cosmic Ray Research, University of Tokyo, Kamioka, Gifu 506-1205, Japan) ,  Kameda J. (Kamioka Observatory, Institute for Cosmic Ray Research, University of Tokyo, Kamioka, Gifu 506-1205, Japan) ,  Kameda J. (Kavli Institute for the Physics and Mathematics of the Universe (WPI), The University of Tokyo Institutes for Advanced Study, University of Tokyo, Kashiwa, Chiba 277-8583, Japan) ,  Kato Y. (Kamioka Observatory, Institute for Cosmic Ray Research, University of Tokyo, Kamioka, Gifu 506-1205, Japan) ,  Kishimoto Y. (Kamioka Observatory, Institute for Cosmic Ray Research, University of Tokyo, Kamioka, Gifu 506-1205, Japan) ,  Kishimoto Y. (Kavli Institute for the Physics and Mathematics of the Universe (WPI), The University of Tokyo Institutes for Advanced Study, University of Tokyo, Kashiwa, Chiba 277-8583, Japan) ,  Marti Ll. (Kamioka Observatory, Institute for Cosmic Ray Research, University of Tokyo, Kamioka, Gifu 506-1205, Japan) ,  Miura M. (Kamioka Observatory, Institute for Cosmic Ray Research, University of Tokyo, Kamioka, Gifu 506-1205, Japan) ,  Miura M. (Kavli Institute for the Physics and Mathematics of the Universe (WPI), The University of Tokyo Institutes for Advanced Study, University of Tokyo, Kashiwa, Chiba 277-8583, Japan) ,  Moriyama S. (Kamioka Observatory, Institute for Cosmic Ray Research, University of Tokyo, Kamioka, Gifu 506-1205, Japan) ,  Moriyama S. (Kavli Institute for the Physics and Mathematics of the Universe (WPI), The University of Tokyo Institutes for Advanced Study, University of Tokyo, Kashiwa, Chiba 277-8583, Japan) ,  Mochizuki T. (Kamioka Observatory, Institute for Cosmic Ray Research, University of Tokyo, Kamioka, Gifu 506-1205, Japan) ,  Nakahata M. (Kamioka Observatory, Institute for Cosmic Ray Research, University of Tokyo, Kamioka, Gifu 506-1205, Japan) ,  Nakahata M. (Kavli Institute for the Physics and Mathematics of the Universe (WPI), The University of Tokyo Institutes for Advanced Study, University of Tokyo, Kashiwa, Chiba 277-8583, Japan) ,  Nakajima Y. (Kamioka Observatory, Institute for Cosmic Ray Research, University of Tokyo, Kamioka, Gifu 506-1205, Japan) ,  Nakajima Y. (Kavli Institute for the Physics and Mathematics of the Universe (WPI), The University of Tokyo Institutes for Advanced Study, University of Tokyo, Kashiwa, Chiba 277-8583, Japan) ,  Nakano Y. (Kamioka Observatory, Institute for Cosmic Ray Research, University of Tokyo, Kamioka, Gifu 506-1205, Japan) ,  Nakayama S. (Kamioka Observatory, Institute for Cosmic Ray Research, University of Tokyo, Kamioka, Gifu 506-1205, Japan) ,  Nakayama S. (Kavli Institute for the Physics and Mathematics of the Universe (WPI), The University of Tokyo Institutes for Advanced Study, University of Tokyo, Kashiwa, Chiba 277-8583, Japan) ,  Okada T. (Kamioka Observatory, Institute for Cosmic Ray Research, University of Tokyo, Kamioka, Gifu 506-1205, Japan) ,  Okamoto K. (Kamioka Observatory, Institute for Cosmic Ray Research, University of Tokyo, Kamioka, Gifu 506-1205, Japan) ,  Orii A. (Kamioka Observatory, Institute for Cosmic Ray Research, University of Tokyo, Kamioka, Gifu 506-1205, Japan) ,  Pronost G. (Kamioka Observatory, Institute for Cosmic Ray Research, University of Tokyo, Kamioka, Gifu 506-1205, Japan) ,  Sekiya H. (Kamioka Observatory, Institute for Cosmic Ray Research, University of Tokyo, Kamioka, Gifu 506-1205, Japan) ,  Sekiya H. (Kavli Institute for the Physics and Mathematics of the Universe (WPI), The University of Tokyo Institutes for Advanced Study, University of Tokyo, Kashiwa, Chiba 277-8583, Japan) ,  Shiozawa M. (Kamioka Observatory, Institute for Cosmic Ray Research, University of Tokyo, Kamioka, Gifu 506-1205, Japan) ,  Shiozawa M. (Kavli Institute for the Physics and Mathematics of the Universe (WPI), The University of Tokyo Institutes for Advanced Study, University of Tokyo, Kashiwa, Chiba 277-8583, Japan) ,  Sonoda Y. (Kamioka Observatory, Institute for Cosmic Ray Research, University of Tokyo, Kamioka, Gifu 506-1205, Japan) ,  Takeda A. (Kamioka Observatory, Institute for Cosmic Ray Research, University of Tokyo, Kamioka, Gifu 506-1205, Japan) ,  Takeda A. (Kavli Institute for the Physics and Mathematics of the Universe (WPI), The University of Tokyo Institutes for Advanced Study, University of Tokyo, Kashiwa, Chiba 277-8583, Japan) ,  Takenaka A. (Kamioka Observatory, Institute for Cosmic Ray Research, University of Tokyo, Kamioka, Gifu 506-1205, Japan) ,  Tanaka H. (Kamioka Observatory, Institute for Cosmic Ray Research, University of Tokyo, Kamioka, Gifu 506-1205, Japan) ,  Yano T. (Kamioka Observatory, Institute for Cosmic Ray Research, University of Tokyo, Kamioka, Gifu 506-1205, Japan) ,  Akutsu R. (Research Center for Cosmic Neutrinos, Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Chiba 277-8582, Japan) ,  Kajita T. (Research Center for Cosmic Neutrinos, Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Chiba 277-8582, Japan) ,  Kajita T. (Kavli Institute for the Physics and Mathematics of the Universe (WPI), The University of Tokyo Institutes for Advanced Study, University of Tokyo, Kashiwa, Chiba 277-8583, Japan) ,  Nishimura Y. (Research Center for Cosmic Neutrinos, Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Chiba 277-8582, Japan) ,  Okumura K. (Research Center for Cosmic Neutrinos, Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Chiba 277-8582, Japan) ,  Okumura K. (Kavli Institute for the Physics and Mathematics of the Universe (WPI), The University of Tokyo Institutes for Advanced Study, University of Tokyo, Kashiwa, Chiba 277-8583, Japan) ,  Wang R. (Research Center for Cosmic Neutrinos, Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Chiba 277-8582, Japan) ,  Xia J. (Research Center for Cosmic Neutrinos, Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Chiba 277-8582, Japan) ,  Labarga L. (Department of Theoretical Physics, University Autonoma Madrid, 28049 Madrid, Spain) ,  Fernandez P. (Department of Theoretical Physics, University Autonoma Madrid, 28049 Madrid, Spain) ,  Blaszczyk F. d. M. (Department of Physics, Boston University, Boston, Massachusetts 02215, USA) ,  Kachulis C. (Department of Physics, Boston University, Boston, Massachusetts 02215, USA) ,  Kearns E. (Department of Physics, Boston University, Boston, Massachusetts 02215, USA) ,  Kearns E. (Kavli Institute for the Physics and Mathematics of the Universe (WPI), The University of Tokyo Institutes for Advanced Study, University of Tokyo, Kashiwa, Chiba 277-8583, Japan) ,  Raaf J. L. (Department of Physics, Boston University, Boston, Massachusetts 02215, USA) ,  Stone J. L. (Department of Physics, Boston University, Boston, Massachusetts 02215, USA) ,  Stone J. L. (Kavli Institute for the Physics and Mathematics of the Universe (WPI), The University of Tokyo Institutes for Advanced Study, University of Tokyo, Kashiwa, Chiba 277-8583, Japan) ,  Sussman S. (Department of Physics, Boston University, Boston, Massachusetts 02215, USA) ,  Berkman S. (Department of Physics and Astronomy, University of British Columbia, Vancouver, British Columbia, V6T1Z4, Canada) ,  Bian J. (Department of Physics and Astronomy, University of California, Irvine, Irvine, California 92697-4575, USA) ,  Griskevich N. J. (Department of Physics and Astronomy, University of California, Irvine, Irvine, California 92697-4575, USA) ,  Kropp W. R. (Department of Physics and Astronomy, University of California, Irvine, Irvine, California 92697-4575, USA) ,  Locke S. (Department of Physics and Astronomy, University of California, Irvine, Irvine, California 92697-4575, USA) ,  Mine S. (Department of Physics and Astronomy, University of California, Irvine, Irvine, California 92697-4575, USA) ,  Weatherly P. (Department of Physics and Astronomy, University of California, Irvine, Irvine, California 92697-4575, USA) ,  Smy M. B. (Department of Physics and Astronomy, University of California, Irvine, Irvine, California 92697-4575, USA) ,  Smy M. B. (Kavli Institute for the Physics and Mathematics of the Universe (WPI), The University of Tokyo Institutes for Advanced Study, University of Tokyo, Kashiwa, Chiba 277-8583, Japan) ,  Sobel H. W. (Department of Physics and Astronomy, University of California, Irvine, Irvine, California 92697-4575, USA) ,  Sobel H. W. (Kavli Institute for the Physics and Mathematics of the Universe (WPI), The University of Tokyo Institutes for Advanced Study, University of Tokyo, Kashiwa, Chiba 277-8583, Japan) ,  Takhistov V. (Department of Physics and Astronomy, University of California, Irvine, Irvine, California 92697-4575, USA) ,  Ganezer K. S. (Department of Physics, California State University, Dominguez Hills, Carson, California 90747, USA) ,  Hill J. (Department of Physics, California State University, Dominguez Hills, Carson, California 90747, USA) ,  Kim J. Y. (Department of Physics, Chonnam National University, Kwangju 500-757, Korea) ,  Lim I. T. (Department of Physics, Chonnam National University, Kwangju 500-757, Korea) ,  Park R. G. (Department of Physics, Chonnam National University, Kwangju 500-757, Korea) ,  Bodur B. (Department of Physics, Duke University, Durham North Carolina 27708, USA) ,  Scholberg K. (Department of Physics, Duke University, Durham North Carolina 27708, USA) ,  Scholberg K. (Kavli Institute for the Physics and Mathematics of the Universe (WPI), The University of Tokyo Institutes for Advanced Study, University of Tokyo, Kashiwa, Chiba 277-8583, Japan) ,  Walter C. W. (Department of Physics, Duke University, Durham North Carolina 27708, USA) ,  Walter C. W. (Kavli Institute for the Physics and Mathematics of the Universe (WPI), The University of Tokyo Institutes for Advanced Study, University of Tokyo, Kashiwa, Chiba 277-8583, Japan) ,  Gonin M. (Ecole Polytechnique, IN2P3-CNRS, Laboratoire Leprince-Ringuet, F-91120 Palaiseau, France) ,  Imber J. (Ecole Polytechnique, IN2P3-CNRS, Laboratoire Leprince-Ringuet, F-91120 Palaiseau, France) ,  Mueller Th. A. (Ecole Polytechnique, IN2P3-CNRS, Laboratoire Leprince-Ringuet, F-91120 Palaiseau, France) ,  Ishizuka T. (Junior College, Fukuoka Institute of Technology, Fukuoka, Fukuoka 811-0295, Japan) ,  Nakamura T. (Department of Physics, Gifu University, Gifu, Gifu 501-1193, Japan) ,  Jang J. S. (GIST College, Gwangju Institute of Science and Technology, Gwangju 500-712, Korea) ,  Choi K. (Department of Physics and Astronomy, University of Hawaii, Honolulu, Hawaii 96822, USA) ,  Learned J. G. (Department of Physics and Astronomy, University of Hawaii, Honolulu, Hawaii 96822, USA) ,  Matsuno S. (Department of Physics and Astronomy, University of Hawaii, Honolulu, Hawaii 96822, USA) ,  Litchfield R. P. (Department of Physics, Imperial College London, London, SW7 2AZ, United Kingdom) ,  Uchida Y. (Department of Physics, Imperial College London, London, SW7 2AZ, United Kingdom) ,  Wascko M. O. (Department of Physics, Imperial College London, London, SW7 2AZ, United Kingdom) ,  Calabria N. F. (Dipartimento Interuniversitario di Fisica, INFN Sezione di Bari and Universita e Politecnico di Bari, I-70125, Bari, Italy) ,  Catanesi M. G. (Dipartimento Interuniversitario di Fisica, INFN Sezione di Bari and Universita e Politecnico di Bari, I-70125, Bari, Italy) ,  Intonti R. A. (Dipartimento Interuniversitario di Fisica, INFN Sezione di Bari and Universita e Politecnico di Bari, I-70125, Bari, Italy) ,  Radicioni E. (Dipartimento Interuniversitario di Fisica, INFN Sezione di Bari and Universita e Politecnico di Bari, I-70125, Bari, Italy) ,  De Rosa G. (Dipartimento di Fisica, INFN Sezione di Napoli and Universita di Napoli, I-80126, Napoli, Italy) ,  Ali A. (Dipartimento di Fisica, INFN Sezione di Padova and Universita di Padova, I-35131, Padova, Italy) ,  Collazuol G. (Dipartimento di Fisica, INFN Sezione di Padova and Universita di Padova, I-35131, Padova, Italy) ,  Iacob F. (Dipartimento di Fisica, INFN Sezione di Padova and Universita di Padova, I-35131, Padova, Italy) ,  Ludovici L. (INFN Sezione di Roma and Universita di Roma “La Sapienza”, I-00185, Roma, Italy) ,  Cao S. (High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki 305-0801, Japan) ,  Friend M. (High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki 305-0801, Japan) ,  Hasegawa T. (High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki 305-0801, Japan) ,  Ishida T. (High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki 305-0801, Japan) ,  Kobayashi T. (High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki 305-0801, Japan) ,  Nakadaira T. (High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki 305-0801, Japan) ,  Nakamura K. (High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki 305-0801, Japan) ,  Nakamura K. (Kavli Institute for the Physics and Mathematics of the Universe (WPI), The University of Tokyo Institutes for Advanced Study, University of Tokyo, Kashiwa, Chiba 277-8583, Japan) ,  Oyama Y. (High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki 305-0801, Japan) ,  Sakashita K. (High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki 305-0801, Japan) ,  Sekiguchi T. (High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki 305-0801, Japan) ,  Tsukamoto T. (High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki 305-0801, Japan) ,  Abe KE. (Department of Physics, Kobe University, Kobe, Hyogo 657-8501, Japan) ,  Hasegawa M. (Department of Physics, Kobe University, Kobe, Hyogo 657-8501, Japan) ,  Isobe Y. (Department of Physics, Kobe University, Kobe, Hyogo 657-8501, Japan) ,  Miyabe H. (Department of Physics, Kobe University, Kobe, Hyogo 657-8501, Japan) ,  Sugimoto T. (Department of Physics, Kobe University, Kobe, Hyogo 657-8501, Japan) ,  Suzuki A. T. (Department of Physics, Kobe University, Kobe, Hyogo 657-8501, Japan) ,  Takeuchi Y. (Department of Physics, Kobe University, Kobe, Hyogo 657-8501, Japan)
資料名： Physical Review. D  (Physical Review. D)
巻： 99  号： 3  ページ： 032005  発行年： 2019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： 酸素に対する大気ニュートリノの中性電流(NC)相互作用は,水性Cherenkov検出器を用いた超新星レリックニュートリノの探索における主要な背景の一つである。NCチャネルは,[数式:原文を参照]核内の核子からのニュートリノ準弾性(NCQE)散乱により支配される。本論文では,Super-Kamiokande(SK)における大気ニュートリノを用いたNCQE断面積の最初の測定について報告する。測定は,22.5kitton水の基準体積を有するSK-IVデータの2,778生日を用いた。7.5~29.5MeVの可視エネルギー窓内で,予想される71.9NCQE信号と53.1背景事象に比べて117事象を観測した。160MeVから10GeVまでの大気ニュートリノスペクトルにより重み付けし,フラックス平均NCQE断面積を[数式:原文を参照]として測定した。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： *酸素 ,  スペクトル ,  散乱 ,  中性カレント ,  *断面積 ,  チャネル ,  *ニュートリノ ,  *大気ニュートリノ ,  Cherenkov計数管 ,  超新星 ,  核子 ,  電流 ,  相互作用 ,  *弾性
準シソーラス用語： *Super-Kamiokande , 【Automatic Indexing@JST】

分類 (2件)： ニュートリノ相互作用  (BF03030S) ,  レプトン  (BF04040K)

タイトルに関連する用語 (7件)： Super-Kamiokande ,  大気ニュートリノ ,  ニュートリノ ,  酸素 ,  中性カレント ,  弾性 ,  断面積