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Atmospheric neutrino oscillation analysis with neutron tagging and an expanded fiducial volume in Super-Kamiokande I–V

T. Wester4,*, K. Abe1,44, C. Bronner1, Y. Hayato1,44, K. Hiraide1,44, K. Hosokawa1, K. Ieki1,44, M. Ikeda1,44, J. Kameda1,44 et al. (The Super-Kamiokande Collaboration)

J. Kameda1,44, Y. Kanemura1, R. Kaneshima1, Y. Kashiwagi1, Y. Kataoka1,44, S. Miki1, S. Mine1,6, M. Miura1,44, S. Moriyama1,44, Y. Nakano1, M. Nakahata1,44, S. Nakayama1,44, Y. Noguchi1, K. Sato1, H. Sekiya1,44, H. Shiba1, K. Shimizu1, M. Shiozawa1,44, Y. Sonoda1, Y. Suzuki1, A. Takeda1,44, Y. Takemoto1,44, H. Tanaka1,44, T. Yano1, S. Han2, T. Kajita2,44,22, K. Okumura2,44, T. Tashiro2, T. Tomiya2, X. Wang2, S. Yoshida2, P. Fernandez3, L. Labarga3, N. Ospina3, B. Zaldivar3, B. W. Pointon5,47, E. Kearns4,44, J. L. Raaf4, L. Wan4, J. Bian6, N. J. Griskevich6, S. Locke6, M. B. Smy6,44, H. W. Sobel6,44, V. Takhistov6,24, A. Yankelevich6, J. Hill7, S. H. Lee8, D. H. Moon8, R. G. Park8, B. Bodur9, K. Scholberg9,44, C. W. Walter9,44, A. Beauchêne10, O. Drapier10, A. Giampaolo10, Th. A. Mueller10, A. D. Santos10, P. Paganini10, B. Quilain10, T. Nakamura11, J. S. Jang12, L. N. Machado13, J. G. Learned14, K. Choi15, N. Iovine15, S. Cao16, L. H. V. Anthony17, D. Martin17, N. W. Prouse17, M. Scott17, A. A. Sztuc17, Y. Uchida17, V. Berardi18, M. G. Catanesi18, E. Radicioni18, N. F. Calabria19, A. Langella19, G. De Rosa19, G. Collazuol20, F. Iacob20, M. Mattiazzi20, L. Ludovici21, M. Gonin22, G. Pronost22, C. Fujisawa23, Y. Maekawa23, Y. Nishimura23, R. Okazaki23, R. Akutsu24, M. Friend24, T. Hasegawa24, T. Ishida24, T. Kobayashi24, M. Jakkapu24, T. Matsubara24, T. Nakadaira24, K. Nakamura24,44, Y. Oyama24, K. Sakashita24, T. Sekiguchi24, T. Tsukamoto24, N. Bhuiyan25, G. T. Burton25, F. Di Lodovico25, J. Gao25, A. Goldsack25, T. Katori25, J. Migenda25, R. Ramsden25, Z. Xie25, S. Zsoldos25,44, A. T. Suzuki26, Y. Takagi26, Y. Takeuchi26,44, H. Zhong26, J. Feng27, L. Feng27, J. R. Hu27, Z. Hu27, M. Kawaue27, T. Kikawa27, M. Mori27, T. Nakaya27,44, R. A. Wendell27,44, K. Yasutome27, S. J. Jenkins28, N. McCauley28, P. Mehta28, A. Tarrant28, Y. Fukuda29, Y. Itow30,31, H. Menjo30, K. Ninomiya30, J. Lagoda32, S. M. Lakshmi32, M. Mandal32, P. Mijakowski32, Y. S. Prabhu32, J. Zalipska32, M. Jia33, J. Jiang33, C. K. Jung33, W. Shi33, M. J. Wilking33, C. Yanagisawa33,†, M. Harada34, Y. Hino34, H. Ishino34, Y. Koshio34,44, F. Nakanishi34, S. Sakai34, T. Tada34, T. Tano34, T. Ishizuka35, G. Barr36, D. Barrow36, L. Cook36,44, A. Holin36, F. Nova36, S. Samani36, D. Wark36, S. Jung37, B. S. Yang37, J. Y. Yang37, J. Yoo37, J. E. P. Fannon38, L. Kneale38, M. Malek38, J. M. McElwee38, M. D. Thiesse38, L. F. Thompson38, S. T. Wilson38, H. Okazawa39, S. B. Kim40, E. Kwon40, J. W. Seo40, I. Yu40, A. K. Ichikawa41, K. D. Nakamura41, S. Tairafune41, K. Nishijima42, A. Eguchi43, K. Nakagiri43, Y. Nakajima43,44, S. Shima43, N. Taniuchi43, E. Watanabe43, M. Yokoyama43,44, P. de Perio44, S. Fujita44, K. Martens44, K. M. Tsui44, M. R. Vagins44,6, J. Xia44, S. Izumiyama45, M. Kuze45, R. Matsumoto45, M. Ishitsuka46, H. Ito46, Y. Ommura46, N. Shigeta46, M. Shinoki46, K. Yamauchi46, T. Yoshida46, R. Gaur47, V. Gousy-Leblanc47,‡, M. Hartz47, A. Konaka47, X. Li47, S. Chen48, B. D. Xu48, B. Zhang48, M. Posiadala-Zezula49, S. B. Boyd50, R. Edwards50, D. Hadley50, M. Nicholson50, M. O’Flaherty50, B. Richards50, A. Ali51,47, B. Jamieson51, S. Amanai52, Ll. Marti52, A. Minamino52, and S. Suzuki52 (The Super-Kamiokande Collaboration)

  • 1Kamioka Observatory, Institute for Cosmic Ray Research, University of Tokyo, Kamioka, Gifu 506-1205, Japan
  • 2Research Center for Cosmic Neutrinos, Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Chiba 277-8582, Japan
  • 3Department of Theoretical Physics, University Autonoma Madrid, 28049 Madrid, Spain
  • 4Department of Physics, Boston University, Boston, Massachusetts 02215, USA
  • 5Department of Physics, British Columbia Institute of Technology, Burnaby, British Columbia V5G 3H2, Canada
  • 6Department of Physics and Astronomy, University of California, Irvine, Irvine, California 92697-4575, USA
  • 7Department of Physics, California State University, Dominguez Hills, Carson, California 90747, USA
  • 8Institute for Universe and Elementary Particles, Chonnam National University, Gwangju 61186, Korea
  • 9Department of Physics, Duke University, Durham, North Carolina 27708, USA
  • 10Ecole Polytechnique, IN2P3-CNRS, Laboratoire Leprince-Ringuet, F-91120 Palaiseau, France
  • 11Department of Physics, Gifu University, Gifu, Gifu 501-1193, Japan
  • 12GIST College, Gwangju Institute of Science and Technology, Gwangju 500-712, Korea
  • 13School of Physics and Astronomy, University of Glasgow, Glasgow G12 8QQ, United Kingdom
  • 14Department of Physics and Astronomy, University of Hawaii, Honolulu, Hawaii 96822, USA
  • 15Center for Underground Physics, Institute for Basic Science (IBS), Daejeon 34126, Korea
  • 16Institute For Interdisciplinary Research in Science and Education, ICISE, Quy Nhon 55121, Vietnam
  • 17Department of Physics, Imperial College London, London SW7 2AZ, United Kingdom
  • 18Dipartimento Interuniversitario di Fisica, INFN Sezione di Bari and Università e Politecnico di Bari, I-70125, Bari, Italy
  • 19Dipartimento di Fisica, INFN Sezione di Napoli and Università di Napoli, I-80126, Napoli, Italy
  • 20Dipartimento di Fisica, INFN Sezione di Padova and Università di Padova, I-35131, Padova, Italy
  • 21INFN Sezione di Roma and Università di Roma “La Sapienza,” I-00185, Roma, Italy
  • 22ILANCE, CNRS—University of Tokyo International Research Laboratory, Kashiwa, Chiba 277-8582, Japan
  • 23Department of Physics, Keio University, Yokohama, Kanagawa 223-8522, Japan
  • 24High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki 305-0801, Japan
  • 25Department of Physics, King’s College London, London WC2R 2LS, United Kingdom
  • 26Department of Physics, Kobe University, Kobe, Hyogo 657-8501, Japan
  • 27Department of Physics, Kyoto University, Kyoto, Kyoto 606-8502, Japan
  • 28Department of Physics, University of Liverpool, Liverpool L69 7ZE, United Kingdom
  • 29Department of Physics, Miyagi University of Education, Sendai, Miyagi 980-0845, Japan
  • 30Institute for Space-Earth Environmental Research, Nagoya University, Nagoya, Aichi 464-8602, Japan
  • 31Kobayashi-Maskawa Institute for the Origin of Particles and the Universe, Nagoya University, Nagoya, Aichi 464-8602, Japan
  • 32National Centre for Nuclear Research, 02-093 Warsaw, Poland
  • 33Department of Physics and Astronomy, State University of New York at Stony Brook, New York 11794-3800, USA
  • 34Department of Physics, Okayama University, Okayama, Okayama 700-8530, Japan
  • 35Media Communication Center, Osaka Electro-Communication University, Neyagawa, Osaka 572-8530, Japan
  • 36STFC Rutherford Appleton Laboratory, Harwell, Oxford OX11 0QX, United Kingdom
  • 37Department of Physics, Seoul National University, Seoul 151-742, Korea
  • 38Department of Physics and Astronomy, University of Sheffield, Sheffield S3 7RH, United Kingdom
  • 39Department of Informatics in Social Welfare, Shizuoka University of Welfare, Yaizu, Shizuoka 425-8611, Japan
  • 40Department of Physics, Sungkyunkwan University, Suwon 440-746, Korea
  • 41Department of Physics, Faculty of Science, Tohoku University, Sendai, Miyagi 980-8578, Japan
  • 42Department of Physics, Tokai University, Hiratsuka, Kanagawa 259-1292, Japan
  • 43Department of Physics, University of Tokyo, Bunkyo, Tokyo 113-0033, Japan
  • 44Kavli 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
  • 45Department of Physics, Tokyo Institute of Technology, Meguro, Tokyo 152-8551, Japan
  • 46Department of Physics, Faculty of Science and Technology, Tokyo University of Science, Noda, Chiba 278-8510, Japan
  • 47TRIUMF, 4004 Wesbrook Mall, Vancouver, British Columbia V6T2A3, Canada
  • 48Department of Engineering Physics, Tsinghua University, Beijing 100084, China
  • 49Faculty of Physics, University of Warsaw, Warsaw 02-093, Poland
  • 50Department of Physics, University of Warwick, Coventry CV4 7AL, United Kingdom
  • 51Department of Physics, University of Winnipeg, Manitoba R3J 3L8, Canada
  • 52Department of Physics, Yokohama National University, Yokohama, Kanagawa 240-8501, Japan

  • *Corresponding author: twester@bu.edu
  • Also at BMCC/CUNY, Science Department, New York, New York, 1007, USA.
  • Also at University of Victoria, Department of Physics and Astronomy, P.O. Box 1700 STN CSC, Victoria, British Columbia V8W 2Y2, Canada.

Phys. Rev. D 109, 072014 – Published 24 April, 2024

DOI: https://doi.org/10.1103/PhysRevD.109.072014

Abstract

We present a measurement of neutrino oscillation parameters with the Super-Kamiokande detector using atmospheric neutrinos from the complete pure-water SK I–V (April 1996–July 2020) dataset, including events from an expanded fiducial volume. The dataset corresponds to 6511.3 live days and an exposure of 484.2 kiloton-years. Measurements of the neutrino oscillation parameters Δm322, sin2θ23, sin2θ13, δCP, and the preference for the neutrino mass ordering are presented with atmospheric neutrino data alone, and with constraints on sin2θ13 from reactor neutrino experiments. Our analysis including constraints on sin2θ13 favors the normal mass ordering at the 92.3% level.

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