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Search for proton decay into a single charged antilepton and a massless invisible particle using the full pure water data set of Super-Kamiokande

Y. M. Liu25, K. Terada52, K. Abe1,51, Y. Asaoka1,51, M. Harada1, Y. Hayato1,51, K. Hiraide1,51, T. H. Hung1, K. Ieki1,51 et al. (Super-Kamiokande Collaboration)

K. Ieki1,51, M. Ikeda1,51, J. Kameda1,51, Y. Kataoka1,51, S. Mine1,7, M. Miura1,51, S. Moriyama1,51, K. Nakagiri1, M. Nakahata1,51, S. Nakayama1,51, Y. Noguchi1, G. Pronost1, K. Sato1, H. Sekiya1,51, R. Shinoda1, M. Shiozawa1,51, Y. Suzuki1, A. Takeda1,51, Y. Takemoto1,51, H. Tanaka1,51, S. Chen2, Y. Itow2,33,34, T. Kajita2,51,24, R. Nishijima2, K. Okumura2,51, T. Tashiro2, T. Tomiya2, X. Wang2, F. J. de Garay Arcones3, P. Fernandez3, L. Labarga3, D. Samudio3, C. Yanagisawa4,38, B. Jargowsky5, E. Kearns5,51, J. Mirabito5, L. Wan5, T. Wester5, B. W. Pointon6,55, J. Bian7, B. Cortez7, N. J. Griskevich7, Y. Jiang7, M. B. Smy7,51, H. W. Sobel7,51, V. Takhistov7,26, J. Hill8, B. D. Xu9, D. Jung10, D. H. Moon10, R. G. Park10, B. S. Yang10, K. Scholberg11,51, C. W. Walter11,51, O. Drapier12, A. Ershova12, M. Ferey12, Z. Hu12, E. Le Blévec12, T. Leplumey12, Th. A. Mueller12, P. Paganini12, C. Quach12, R. Rogly12, T. Nakamura13, J. S. Jang14, R. P. Litchfield15, L. N. Machado15, F. J. P. Soler15, J. G. Learned16, K. Choi17, S. Cao18, T. V. Ngoc18, L. H. V. Anthony19, N. W. Prouse19, M. Scott19, Y. Uchida19, V. Berardi20, N. F. Calabria20, M. G. Catanesi20, N. Ospina20, E. Radicioni20, A. Langella21, G. De Rosa21, G. T. Burton22, G. Collazuol22, M. Feltre22, M. Mattiazzi22, L. Ludovici23, M. Gonin24, L. Périssé24, B. Quilain24, M. Fukazawa25, S. Horiuchi25, A. Kawabata25, Y. Maekawa25, Y. Nishimura25, A. Oka25, H. Tanigawa25, R. Akutsu26, M. Friend26, T. Hasegawa26, Y. Hino26, T. Ishida26, T. Kobayashi26, T. Matsubara26, T. Nakadaira26, Y. Oyama26, A. Portocarrero Yrey26, K. Sakashita26, T. Sekiguchi26, N. Bhuiyan27, F. Di Lodovico27, T. Katori27, R. Kralik27, N. Latham27, R. M. Ramsden27, V. Siccardi27, S. Aoyama28, H. Bambara28, Y. Inaba28, H. Ito28, M. Nishigami28, T. Sone28, A. T. Suzuki28, Y. Takeuchi28,51, S. Wada28, H. Zhong28, J. Feng29, L. Feng29, N. Fujimoto29, S. Han29, J. Hikida29, M. Kawaue29, T. Kikawa29, F. Nakanishi29, T. Nakaya29,51, R. A. Wendell29,51, S. J. Jenkins30, N. McCauley30, M. Fanì31, M. J. Wilking31, Z. Xie31, Y. Fukuda32, H. Menjo33,34, Y. Yoshioka33, J. Lagoda35, J. Zalipska35, T. Yano36, M. Mori37, J. Jiang38, Y. Asano39, K. Hamaguchi39, H. Ishino39, Y. Koshio39,51, S. Ohshita39, T. Tada39, T. Ishizuka40, G. Barr41, D. Barrow41, D. Wark41,47, A. Holin42, F. Nova42, M. Jo43, S. Jung43, J. Yoo43, L. Kneale44, T. Peacock44, P. Stowell44, H. Okazawa45, S. M. Lakshmi46, S. Hong48, E. Kwon48, M. W. Lee48, J. W. Seo48, I. Yu48, Y. Ashida49, A. K. Ichikawa49, S. Kobayashi49, K. D. Nakamura49, S. Abe50, W. Cai50, Y. Endo50, S. Goto50, S. Kodama50, Y. Kong50, H. Hayasaki50, Y. Masaki50, Y. Mizuno50, T. Muro50, K. Nakagiri50, Y. Nakajima50,51, M. Sekiyama50, N. Taniuchi50, T. Yamazumi50, M. Yokoyama50,51, P. de Perio51, S. Fujita51, C. Jesús-Valls51, K. Martens51, Ll. Marti51, A. D. Santos51, K. M. Tsui51, M. R. Vagins51,7, S. Izumiyama52, M. Kuze52, R. Matsumoto52, C. Ise53, M. Ishitsuka53, M. Sugo53, M. Wako53, K. Yamauchi53, Y. Nakano54, A. Yankelevich54, F. Cormier55, R. Gaur55, M. Hartz55, A. Konaka55, X. Li55, B. R. Smithers55, S. Chen56, Y. Wu56, A. Q. Zhang56, B. Zhang56, H. Adhikary57, M. Girgus57, P. Govindaraj57, M. Posiadala-Zezula57, Y. S. Prabhu57, S. B. Boyd58, R. Edwards58, D. Hadley58, M. O’Flaherty58, B. Richards58, A. Ali59,55, B. Jamieson59, C. Bronner60, D. Horiguchi60, A. Minamino60, and Y. Sasaki60 (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
  • 4Science Department, Borough of Manhattan Community College/City University of New York, New York, New York, 1007, USA
  • 5Department of Physics, Boston University, Boston, Massachusetts 02215, USA
  • 6Department of Physics, British Columbia Institute of Technology, Burnaby, British Columbia, V5G 3H2, Canada
  • 7Department of Physics and Astronomy, University of California, Irvine, Irvine, California 92697-4575, USA
  • 8Department of Physics, California State University, Dominguez Hills, Carson, California 90747, USA
  • 9School of Physical Sciences, University of Chinese Academy of Sciences, Beijing 101408, China
  • 10Institute for Universe and Elementary Particles, Chonnam National University, Gwangju 61186, Korea
  • 11Department of Physics, Duke University, Durham, North Carolina 27708, USA
  • 12Ecole Polytechnique, IN2P3-CNRS, Laboratoire Leprince-Ringuet, F-91120 Palaiseau, France
  • 13Department of Physics, Gifu University, Gifu City, Gifu 501-1193, Japan
  • 14GIST College, Gwangju Institute of Science and Technology, Gwangju 500-712, Korea
  • 15School of Physics and Astronomy, University of Glasgow, Glasgow, G12 8QQ, United Kingdom
  • 16Department of Physics and Astronomy, University of Hawaii, Honolulu, Hawaii 96822, USA
  • 17Center for Underground Physics, Institute for Basic Science (IBS), Daejeon, 34126, Korea
  • 18Institute For Interdisciplinary Research in Science and Education, ICISE, Quy Nhon, 55121, Vietnam
  • 19Department of Physics, Imperial College London, London, SW7 2AZ, United Kingdom
  • 20Dipartimento Interuniversitario di Fisica, INFN Sezione di Bari and Università e Politecnico di Bari, I-70125, Bari, Italy
  • 21Dipartimento di Fisica, INFN Sezione di Napoli and Università di Napoli, I-80126, Napoli, Italy
  • 22Dipartimento di Fisica, INFN Sezione di Padova and Università di Padova, I-35131, Padova, Italy
  • 23INFN Sezione di Roma and Università di Roma “La Sapienza,” I-00185, Roma, Italy
  • 24ILANCE, CNRS—University of Tokyo International Research Laboratory, Kashiwa, Chiba 277-8582, Japan
  • 25Department of Physics, Keio University, Yokohama, Kanagawa, 223-8522, Japan
  • 26High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki 305-0801, Japan
  • 27Department of Physics, King’s College London, London, WC2R 2LS, United Kingdom
  • 28Department of Physics, Kobe University, Kobe, Hyogo 657-8501, Japan
  • 29Department of Physics, Kyoto University, Kyoto, Kyoto 606-8502, Japan
  • 30Department of Physics, University of Liverpool, Liverpool, L69 7ZE, United Kingdom
  • 31School of Physics and Astronomy, University of Minnesota, Minneapolis, Minnesota 55455, USA
  • 32Department of Physics, Miyagi University of Education, Sendai, Miyagi 980-0845, Japan
  • 33Institute for Space-Earth Environmental Research, Nagoya University, Nagoya, Aichi 464-8602, Japan
  • 34Kobayashi-Maskawa Institute for the Origin of Particles and the Universe, Nagoya University, Nagoya, Aichi 464-8602, Japan
  • 35National Centre For Nuclear Research, 02-093 Warsaw, Poland
  • 36National Institute of Technology, Niihama College, Niihama, Ehime 792-8580, Japan
  • 37National Institute of Technology, Numazu College, Numazu, Shizuoka 410-8501, Japan
  • 38Department of Physics and Astronomy, State University of New York at Stony Brook, Stony Brook, New York 11794-3800, USA
  • 39Department of Physics, Okayama University, Okayama, Okayama 700-8530, Japan
  • 40Media Communication Center, Osaka Electro-Communication University, Neyagawa, Osaka, 572-8530, Japan
  • 41Department of Physics, Oxford University, Oxford, OX1 3PU, United Kingdom
  • 42Rutherford Appleton Laboratory, Harwell, Oxford, OX11 0QX, United Kingdom
  • 43Department of Physics and Astronomy, Seoul National University, Seoul 151-742, Korea
  • 44School of Mathematical and Physical Sciences, University of Sheffield, S3 7RH, Sheffield, United Kingdom
  • 45Department of Informatics in Social Welfare, Shizuoka University of Welfare, Yaizu, Shizuoka, 425-8611, Japan
  • 46August Chełkowski Institute of Physics, University of Silesia in Katowice, 75 Pułku Piechoty 1, 41-500 Chorzów, Poland
  • 47STFC, Rutherford Appleton Laboratory, Harwell Oxford, and Daresbury Laboratory, Warrington, OX11 0QX, United Kingdom
  • 48Department of Physics, Sungkyunkwan University, Suwon 440-746, Korea
  • 49Department of Physics, Faculty of Science, Tohoku University, Sendai, Miyagi, 980-8578, Japan
  • 50Department of Physics, University of Tokyo, Bunkyo, Tokyo 113-0033, Japan
  • 51Kavli 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
  • 52Department of Physics, Institute of Science Tokyo, Meguro, Tokyo 152-8551, Japan
  • 53Department of Physics and Astronomy, Faculty of Science and Technology, Tokyo University of Science, Noda, Chiba 278-8510, Japan
  • 54Faculty of Science, University of Toyama, Toyama City, Toyama 930-8555, Japan
  • 55TRIUMF, 4004 Wesbrook Mall, Vancouver, British Columbia, V6T2A3, Canada
  • 56Department of Engineering Physics, Tsinghua University, Beijing, 100084, China
  • 57Faculty of Physics, University of Warsaw, Warsaw, 02-093, Poland
  • 58Department of Physics, University of Warwick, Coventry, CV4 7AL, United Kingdom
  • 59Department of Physics, University of Winnipeg, Winnipeg, Manitoba MB R3J 3L8, Canada
  • 60Department of Physics, Yokohama National University, Yokohama, Kanagawa, 240-8501, Japan

Phys. Rev. D 114, 072005 – Published 13 October, 2026

DOI: https://doi.org/10.1103/rsr5-d3x2

Abstract

A search for proton decay via p→l++X, where l+ is a positively charged lepton and X is an invisible, massless, neutral particle, was performed using a 401  kton·years exposure representing the entire pure water phase of Super-Kamiokande. No significant indication of a proton decay was observed beyond the expected atmospheric neutrino background. Lower limits on the partial lifetime of the proton were set to 1.72×1033  years for p→e++X and 0.61×1033  years for p→μ++X at the 90% confidence level. These results improve on previous limits by factors of 2 and 1.5, respectively.

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