Physics potentials with the second Hyper-Kamiokande detector in Korea

Abe, K (University of Tokyo, Institute for Cosmic Ray Research, Kamioka Observatory, Kamioka, Japan) (University of Tokyo, Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, Kashiwa, Chiba, Japan) ; Abe, Ke (Kobe University, Department of Physics, Kobe, Japan) ; Ahn, S H (Korea Astronomy and Space Science Institute, Daejeon 34055, Korea) ; Aihara, H (University of Tokyo, Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, Kashiwa, Chiba, Japan) (University of Tokyo, Department of Physics, Tokyo, Japan) ; Aimi, A (INFN Sezione di Padova and Università di Padova, Dipartimento di Fisica, Padova, Italy) ; Akutsu, R (University of Tokyo, Institute for Cosmic Ray Research, Research Center for Cosmic Neutrinos, Kashiwa, Japan) ; Andreopoulos, C (University of Liverpool, Department of Physics, Liverpool, United Kingdom) (STFC, Rutherford Appleton Laboratory, Harwell Oxford, and Daresbury Laboratory, Warrington, United Kingdom) ; Anghel, I (Iowa State University, Department of Physics and Astronomy, Ames, Iowa, U.S.A.) ; Anthony, L H V (University of Liverpool, Department of Physics, Liverpool, United Kingdom) ; Antonova, M (Institute for Nuclear Research of the Russian Academy of Sciences, Moscow, Russia) ; Ashida, Y (Kyoto University, Department of Physics, Kyoto, Japan) ; Aushev, V (Kyiv National University, Department of Nuclear Physics, Kyiv, Ukraine) ; Barbi, M (University of Regina, Department of Physics, Regina, Saskatchewan, Canada) ; Barker, G J (University of Warwick, Department of Physics, Coventry, United Kingdom) ; Barr, G (Oxford University, Department of Physics, Oxford, United Kingdom) ; Beltrame, P (University of Edinburgh, School of Physics and Astronomy, Edinburgh, United Kingdom) ; Berardi, V (INFN Sezione di Bari and Università e Politecnico di Bari, Dipartimento Interuniversitario di Fisica, Bari, Italy) ; Bergevin, M (University of California, Davis, Department of Physics, Davis, California, U.S.A.) ; Berkman, S (University of British Columbia, Department of Physics and Astronomy, Vancouver, British Columbia, Canada) ; Berns, L (Tokyo Institute of Technology, Department of Physics, Tokyo, Japan) ; Berry, T (Royal Holloway University of London, Department of Physics, Egham, Surrey, United Kingdom) ; Bhadra, S (York University, Department of Physics and Astronomy, Toronto, Ontario, Canada) ; Blaszczyk, F d M (Boston University, Department of Physics, Boston, Massachusetts, U.S.A.) ; Blondel, A (University of Geneva, Section de Physique, DPNC, Geneva, Switzerland) ; Bolognesi, S (IRFU, CEA Saclay, Gif-sur-Yvette, France) ; Boyd, S B (University of Warwick, Department of Physics, Coventry, United Kingdom) ; Bravar, A (University of Geneva, Section de Physique, DPNC, Geneva, Switzerland) ; Bronner, C (University of Tokyo, Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, Kashiwa, Chiba, Japan) ; Buizza Avanzini, M (Ecole Polytechnique, IN2P3-CNRS, Laboratoire Leprince-Ringuet, Palaiseau, France) ; Cafagna, F S (INFN Sezione di Bari and Università e Politecnico di Bari, Dipartimento Interuniversitario di Fisica, Bari, Italy) ; Calland, R (University of Tokyo, Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, Kashiwa, Chiba, Japan) ; Cao, S (High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki, Japan) ; Cartwright, S L (University of Sheffield, Department of Physics and Astronomy, Sheffield, United Kingdom) ; Catanesi, M G (INFN Sezione di Bari and Università e Politecnico di Bari, Dipartimento Interuniversitario di Fisica, Bari, Italy) ; Checchia, C (INFN Sezione di Padova and Università di Padova, Dipartimento di Fisica, Padova, Italy) ; Chen-Wishart, Z (Royal Holloway University of London, Department of Physics, Egham, Surrey, United Kingdom) ; Cheon, B G (Hanyang University, Department of Physics, Seoul 04763, Korea) ; Cheoun, M K (Soongsil University, Origin of Matter and Evolution of Galaxy (OMEG) Institute and Department of Physics, Seoul 156-743, Korea) ; Cho, K (Korea Institute of Science and Technology Information, Daejeon 34141, Korea) ; Choi, J H (Dongshin University, Department of Physics, Naju, Korea) ; Choi, K (University of Hawaii, Department of Physics and Astronomy, Honolulu, Hawaii, U.S.A.) ; Choi, K Y (Sungkyunkwan University, Department of Physics,Suwon 16419, Korea) ; Chun, E J (Korean Institute for Advanced Studies, Seoul, Korea) ; Cole, A (University of Sheffield, Department of Physics and Astronomy, Sheffield, United Kingdom) ; Coleman, J (University of Liverpool, Department of Physics, Liverpool, United Kingdom) ; Collazuol, G (INFN Sezione di Padova and Università di Padova, Dipartimento di Fisica, Padova, Italy) ; Cowan, G (University of Edinburgh, School of Physics and Astronomy, Edinburgh, United Kingdom) ; Cremonesi, L (Queen Mary University of London, School of Physics and Astronomy, London, United Kingdom) ; Dealtry, T (Lancaster University, Physics Department, Lancaster, United Kingdom) ; De Rosa, G (INFN Sezione di Napoli and Università di Napoli, Dipartimento di Fisica, Napoli, Italy) ; Densham, C (STFC, Rutherford Appleton Laboratory, Harwell Oxford, and Daresbury Laboratory, Warrington, United Kingdom) ; Dewhurst, D (Oxford University, Department of Physics, Oxford, United Kingdom) ; Drakopoulou, E (University of Edinburgh, School of Physics and Astronomy, Edinburgh, United Kingdom) ; Di Lodovico, F (Queen Mary University of London, School of Physics and Astronomy, London, United Kingdom) ; Drapier, O (Ecole Polytechnique, IN2P3-CNRS, Laboratoire Leprince-Ringuet, Palaiseau, France) ; Dumarchez, J (Laboratoire de Physique Nucleaire et de Hautes Energies, UPMC and Universite Paris-Diderot and CNRS/IN2P3, Paris, France) ; Dunne, P (Imperial College London, Department of Physics, London, United Kingdom) ; Dziewiecki, M (Warsaw University of Technology, Institute of Radioelectronics and Multimedia Technology, Warsaw, Poland) ; Emery, S (IRFU, CEA Saclay, Gif-sur-Yvette, France) ; Esmaili, A (Pontifícia Universidade Católica do Rio de Janeiro, Departamento de Física, Rio de Janeiro, Brazil) ; Evangelisti, A (INFN Sezione di Napoli and Università di Napoli, Dipartimento di Fisica, Napoli, Italy) ; Fernández-Martinez, E (University Autonoma Madrid, Department of Theoretical Physics, Madrid, Spain) (Instituto de Física Teórica, UAM/CSIC, Madrid, Spain) ; Feusels, T (University of British Columbia, Department of Physics and Astronomy, Vancouver, British Columbia, Canada) ; Finch, A (Lancaster University, Physics Department, Lancaster, United Kingdom) ; Fiorentini, G A (York University, Department of Physics and Astronomy, Toronto, Ontario, Canada) ; Fiorillo, G (INFN Sezione di Napoli and Università di Napoli, Dipartimento di Fisica, Napoli, Italy) ; Fitton, M (STFC, Rutherford Appleton Laboratory, Harwell Oxford, and Daresbury Laboratory, Warrington, United Kingdom) ; Frankiewicz, K (National Centre for Nuclear Research, Warsaw, Poland) ; Friend, M (High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki, Japan) ; Fujii, Y (High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki, Japan) ; Fukuda, Y (Miyagi University of Education, Department of Physics, Sendai, Japan) ; Fukuda, D (Okayama University, Department of Physics, Okayama, Japan) ; Ganezer, K (California State University, Department of Physics, Carson, California, U.S.A.) ; Ghosh, M (Tokyo Metropolitan University, Department of Physics, Tokyo, Japan) ; Giganti, C (Laboratoire de Physique Nucleaire et de Hautes Energies, UPMC and Universite Paris-Diderot and CNRS/IN2P3, Paris, France) ; Gonin, M (Ecole Polytechnique, IN2P3-CNRS, Laboratoire Leprince-Ringuet, Palaiseau, France) ; Grant, N (University of Warwick, Department of Physics, Coventry, United Kingdom) ; Gumplinger, P (TRIUMF, Vancouver, British Columbia, Canada) ; Hadley, D R (University of Warwick, Department of Physics, Coventry, United Kingdom) ; Hartfiel, B (California State University, Department of Physics, Carson, California, U.S.A.) ; Hartz, M (University of Tokyo, Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, Kashiwa, Chiba, Japan) (TRIUMF, Vancouver, British Columbia, Canada) ; Hayato, Y (University of Tokyo, Institute for Cosmic Ray Research, Kamioka Observatory, Kamioka, Japan) (University of Tokyo, Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, Kashiwa, Chiba, Japan) ; Hayrapetyan, K (Queen Mary University of London, School of Physics and Astronomy, London, United Kingdom) ; Hill, J (California State University, Department of Physics, Carson, California, U.S.A.) ; Hirota, S (Kyoto University, Department of Physics, Kyoto, Japan) ; Horiuchi, S (Virginia Tech, Center for Neutrino Physics, Blacksburg, Virginia, U.S.A.) ; Ichikawa, A K (Kyoto University, Department of Physics, Kyoto, Japan) ; Iijima, T (Nagoya University, Graduate School of Science, Nagoya, Japan) (Nagoya University, Kobayashi-Maskawa Institute for the Origin of Particles and the Universe, Nagoya, Japan) ; Ikeda, M (University of Tokyo, Institute for Cosmic Ray Research, Kamioka Observatory, Kamioka, Japan) ; Imber, J (Ecole Polytechnique, IN2P3-CNRS, Laboratoire Leprince-Ringuet, Palaiseau, France) ; Inoue, K (Research Center for Neutrino Science, Tohoku University, Sendai, Japan) (University of Tokyo, Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, Kashiwa, Chiba, Japan) ; Insler, J (Louisiana State University, Department of Physics and Astronomy, Baton Rouge, Louisiana, U.S.A.) ; Intonti, R A (INFN Sezione di Bari and Università e Politecnico di Bari, Dipartimento Interuniversitario di Fisica, Bari, Italy) ; Ioannisian, A (Yerevan Institute for Theoretical Physics and Modeling, Halabian Str. 34; Yerevan 0036, Armenia) ; Ishida, T (High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki, Japan) ; Ishino, H (Okayama University, Department of Physics, Okayama, Japan) ; Ishitsuka, M (Tokyo University of Science, Department of Physics, Chiba, Japan) ; Itow, Y (Nagoya University, Kobayashi-Maskawa Institute for the Origin of Particles and the Universe, Nagoya, Japan) (Nagoya University, Solar-Terrestrial Environment Laboratory, Nagoya, Japan) ; Iwamoto, K (University of Tokyo, Department of Physics, Tokyo, Japan) ; Izmaylov, A (Institute for Nuclear Research of the Russian Academy of Sciences, Moscow, Russia) ; Jamieson, B (University of Winnipeg, Department of Physics, Winnipeg, Manitoba, Canada) ; Jang, H I (Seoyeong University, Department of Fire Safety, Gwangju, Korea) ; Jang, J S (GIST College, Gwangju Institute of Science and Technology, Gwangju 500-712, Korea) ; Jeon, S H (Sungkyunkwan University, Department of Physics,Suwon 16419, Korea) ; Jeong, K S (Pusan National University, Department of Physics, Busan 46241, Korea) ; Jiang, M (Kyoto University, Department of Physics, Kyoto, Japan) ; Jonsson, P (Imperial College London, Department of Physics, London, United Kingdom) ; Joo, K K (Chonnam National University, Department of Physics, Gwangju, Korea) ; Kaboth, A (STFC, Rutherford Appleton Laboratory, Harwell Oxford, and Daresbury Laboratory, Warrington, United Kingdom) (Royal Holloway University of London, Department of Physics, Egham, Surrey, United Kingdom) ; Kachulis, C (Boston University, Department of Physics, Boston, Massachusetts, U.S.A.) ; Kajita, T (University of Tokyo, Institute for Cosmic Ray Research, Research Center for Cosmic Neutrinos, Kashiwa, Japan) (University of Tokyo, Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, Kashiwa, Chiba, Japan) ; Kang, S K (Seoul National University of Science and Technology, School of Liberal Arts, Seoul 01811, Korea) ; Kameda, J (University of Tokyo, Institute for Cosmic Ray Research, Kamioka Observatory, Kamioka, Japan) (University of Tokyo, Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, Kashiwa, Chiba, Japan) ; Kataoka, Y (University of Tokyo, Department of Physics, Tokyo, Japan) ; Katori, T (Queen Mary University of London, School of Physics and Astronomy, London, United Kingdom) ; Kayrapetyan, K (Queen Mary University of London, School of Physics and Astronomy, London, United Kingdom) ; Kearns, E (Boston University, Department of Physics, Boston, Massachusetts, U.S.A.) (University of Tokyo, Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, Kashiwa, Chiba, Japan) ; Khabibullin, M (Institute for Nuclear Research of the Russian Academy of Sciences, Moscow, Russia) ; Khotjantsev, A (Institute for Nuclear Research of the Russian Academy of Sciences, Moscow, Russia) ; Kim, C S (Yonsei University, Department of Physics and IPAP, Seoul 03722, Korea) ; Kim, H B (Hanyang University, Department of Physics, Seoul 04763, Korea) ; Kim, H J (Kyungpook National University, Department of Physics, Daegu 41566, Korea) ; Kim, J H (Sungkyunkwan University, Department of Physics,Suwon 16419, Korea) ; Kim, J-S (Korea Astronomy and Space Science Institute, Daejeon 34055, Korea) ; Kim, J Y (Chonnam National University, Department of Physics, Gwangju, Korea) ; Kim, S B (Seoul National University, Department of Physics and Astronomy, Seoul 08826, Korea) ; Kim, S C (Korea Astronomy and Space Science Institute, Daejeon 34055, Korea) (Korea University of Science and Technology, Daejeon 34113, Korea) ; Kim, S-W (Korea Astronomy and Space Science Institute, Daejeon 34055, Korea) (Korea University of Science and Technology, Daejeon 34113, Korea) ; Kim, S Y (Seoul National University, Department of Physics and Astronomy, Seoul 08826, Korea) ; Kim, T J (Hanyang University, Department of Physics, Seoul 04763, Korea) ; Kim, W (Kyungpook National University, Department of Physics, Daegu 41566, Korea) ; King, S (Queen Mary University of London, School of Physics and Astronomy, London, United Kingdom) ; Kishimoto, Y (University of Tokyo, Institute for Cosmic Ray Research, Kamioka Observatory, Kamioka, Japan) (University of Tokyo, Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, Kashiwa, Chiba, Japan) ; Ko, P (Korean Institute for Advanced Studies, Seoul, Korea) ; Kobayashi, T (High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki, Japan) ; Koga, M (Research Center for Neutrino Science, Tohoku University, Sendai, Japan) (University of Tokyo, Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, Kashiwa, Chiba, Japan) ; Konaka, A (TRIUMF, Vancouver, British Columbia, Canada) ; Kormos, L L (Lancaster University, Physics Department, Lancaster, United Kingdom) ; Koshio, Y (Okayama University, Department of Physics, Okayama, Japan) (University of Tokyo, Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, Kashiwa, Chiba, Japan) ; Korzenev, A (University of Geneva, Section de Physique, DPNC, Geneva, Switzerland) ; Kowalik, K L (National Centre for Nuclear Research, Warsaw, Poland) ; Kropp, W R (University of California, Irvine, Department of Physics and Astronomy, Irvine, California, U.S.A.) ; Kudenko, Y (Institute for Nuclear Research of the Russian Academy of Sciences, Moscow, Russia) (National Research Nuclear University (MEPhI), Moscow, Russia) (Moscow Institute of Physics and Technology, Moscow region, Russia) ; Kurjata, R (Warsaw University of Technology, Institute of Radioelectronics and Multimedia Technology, Warsaw, Poland) ; Kutter, T (Louisiana State University, Department of Physics and Astronomy, Baton Rouge, Louisiana, U.S.A.) ; Kuze, M (Tokyo Institute of Technology, Department of Physics, Tokyo, Japan) ; Kwak, K (UNIST, Department of Physics, Ulsan, Korea) ; Kwon, E H (Seoul National University, Department of Physics and Astronomy, Seoul 08826, Korea) ; Labarga, L (University Autonoma Madrid, Department of Theoretical Physics, Madrid, Spain) ; Lagoda, J (National Centre for Nuclear Research, Warsaw, Poland) ; Lasorak, P J J (Queen Mary University of London, School of Physics and Astronomy, London, United Kingdom) ; Laveder, M (INFN Sezione di Padova and Università di Padova, Dipartimento di Fisica, Padova, Italy) ; Lawe, M (Lancaster University, Physics Department, Lancaster, United Kingdom) ; Learned, J G (University of Hawaii, Department of Physics and Astronomy, Honolulu, Hawaii, U.S.A.) ; Lee, C H (Pusan National University, Department of Physics, Busan 46241, Korea) ; Lee, S J (Korea University, Department of Physics, Seoul 02841, Korea) ; Lee, W J (Seoul National University, Department of Physics and Astronomy, Seoul 08826, Korea) ; Lim, I T (Chonnam National University, Department of Physics, Gwangju, Korea) ; Lindner, T (TRIUMF, Vancouver, British Columbia, Canada) ; Litchfield, R P (Imperial College London, Department of Physics, London, United Kingdom) ; Longhin, A (INFN Sezione di Padova and Università di Padova, Dipartimento di Fisica, Padova, Italy) ; Loverre, P (INFN Sezione di Roma, Roma, Italy) ; Lou, T (University of Tokyo, Department of Physics, Tokyo, Japan) ; Ludovici, L (INFN Sezione di Roma, Roma, Italy) ; Ma, W (Imperial College London, Department of Physics, London, United Kingdom) ; Magaletti, L (INFN Sezione di Bari and Università e Politecnico di Bari, Dipartimento Interuniversitario di Fisica, Bari, Italy) ; Mahn, K (Michigan State University, Department of Physics and Astronomy, East Lansing, Michigan, U.S.A.) ; Malek, M (University of Sheffield, Department of Physics and Astronomy, Sheffield, United Kingdom) ; Maret, L (University of Geneva, Section de Physique, DPNC, Geneva, Switzerland) ; Mariani, C (Virginia Tech, Center for Neutrino Physics, Blacksburg, Virginia, U.S.A.) ; Martens, K (University of Tokyo, Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, Kashiwa, Chiba, Japan) ; Marti, Ll (University of Tokyo, Institute for Cosmic Ray Research, Kamioka Observatory, Kamioka, Japan) ; Martin, J F (University of Toronto, Department of Physics, Toronto, Ontario, Canada) ; Marzec, J (Warsaw University of Technology, Institute of Radioelectronics and Multimedia Technology, Warsaw, Poland) ; Matsuno, S (University of Hawaii, Department of Physics and Astronomy, Honolulu, Hawaii, U.S.A.) ; Mazzucato, E (IRFU, CEA Saclay, Gif-sur-Yvette, France) ; McCarthy, M (York University, Department of Physics and Astronomy, Toronto, Ontario, Canada) ; McCauley, N (University of Liverpool, Department of Physics, Liverpool, United Kingdom) ; McFarland, K S (University of Rochester, Department of Physics and Astronomy, Rochester, New York, U.S.A.) ; McGrew, C (State University of New York at Stony Brook, Department of Physics and Astronomy, Stony Brook, New York, U.S.A.) ; Mefodiev, A (Institute for Nuclear Research of the Russian Academy of Sciences, Moscow, Russia) ; Mermod, P (University of Geneva, Section de Physique, DPNC, Geneva, Switzerland) ; Metelko, C (University of Liverpool, Department of Physics, Liverpool, United Kingdom) ; Mezzetto, M (INFN Sezione di Padova and Università di Padova, Dipartimento di Fisica, Padova, Italy) ; Migenda, J (University of Sheffield, Department of Physics and Astronomy, Sheffield, United Kingdom) ; Mijakowski, P (National Centre for Nuclear Research, Warsaw, Poland) ; Minakata, H (University of Tokyo, Institute for Cosmic Ray Research, Research Center for Cosmic Neutrinos, Kashiwa, Japan) (Instituto de Física Teórica, UAM/CSIC, Madrid, Spain) ; Minamino, A (Yokohama National University, Faculty of Engineering, Yokohama, Japan) ; Mine, S (University of California, Irvine, Department of Physics and Astronomy, Irvine, California, U.S.A.) ; Mineev, O (Institute for Nuclear Research of the Russian Academy of Sciences, Moscow, Russia) ; Mitra, A (University of Warwick, Department of Physics, Coventry, United Kingdom) ; Miura, M (University of Tokyo, Institute for Cosmic Ray Research, Kamioka Observatory, Kamioka, Japan) (University of Tokyo, Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, Kashiwa, Chiba, Japan) ; Mochizuki, T (University of Tokyo, Institute for Cosmic Ray Research, Kamioka Observatory, Kamioka, Japan) ; Monroe, J (Royal Holloway University of London, Department of Physics, Egham, Surrey, United Kingdom) ; Moon, C S (Kyungpook National University, Department of Physics, Daegu 41566, Korea) ; Moon, D H (Chonnam National University, Department of Physics, Gwangju, Korea) ; Moriyama, S (University of Tokyo, Institute for Cosmic Ray Research, Kamioka Observatory, Kamioka, Japan) (University of Tokyo, Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, Kashiwa, Chiba, Japan) ; Mueller, T (Ecole Polytechnique, IN2P3-CNRS, Laboratoire Leprince-Ringuet, Palaiseau, France) ; Muheim, F (University of Edinburgh, School of Physics and Astronomy, Edinburgh, United Kingdom) ; Murase, K (Pennsylvania State University, Department of Physics, University Park, PA 16802, U.S.A.) ; Muto, F (Nagoya University, Graduate School of Science, Nagoya, Japan) ; Nakahata, M (University of Tokyo, Institute for Cosmic Ray Research, Kamioka Observatory, Kamioka, Japan) (University of Tokyo, Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, Kashiwa, Chiba, Japan) ; Nakajima, Y (University of Tokyo, Institute for Cosmic Ray Research, Kamioka Observatory, Kamioka, Japan) ; Nakamura, K (High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki, Japan) (University of Tokyo, Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, Kashiwa, Chiba, Japan) ; Nakaya, T (Kyoto University, Department of Physics, Kyoto, Japan) (University of Tokyo, Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, Kashiwa, Chiba, Japan) ; Nakayama, S (University of Tokyo, Institute for Cosmic Ray Research, Kamioka Observatory, Kamioka, Japan) (University of Tokyo, Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, Kashiwa, Chiba, Japan) ; Nantais, C (University of Toronto, Department of Physics, Toronto, Ontario, Canada) ; Needham, M (University of Edinburgh, School of Physics and Astronomy, Edinburgh, United Kingdom) ; Nicholls, T (STFC, Rutherford Appleton Laboratory, Harwell Oxford, and Daresbury Laboratory, Warrington, United Kingdom) ; Nishimura, Y (University of Tokyo, Institute for Cosmic Ray Research, Research Center for Cosmic Neutrinos, Kashiwa, Japan) ; Noah, E (University of Geneva, Section de Physique, DPNC, Geneva, Switzerland) ; Nova, F (STFC, Rutherford Appleton Laboratory, Harwell Oxford, and Daresbury Laboratory, Warrington, United Kingdom) ; Nowak, J (Lancaster University, Physics Department, Lancaster, United Kingdom) ; Nunokawa, H (Pontifícia Universidade Católica do Rio de Janeiro, Departamento de Física, Rio de Janeiro, Brazil) ; Obayashi, Y (University of Tokyo, Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, Kashiwa, Chiba, Japan) ; Oh, Y D (Kyungpook National University, Department of Physics, Daegu 41566, Korea) ; Oh, Y (Kyungpook National University, Department of Physics, Daegu 41566, Korea) ; O’Keeffe, H M (Lancaster University, Physics Department, Lancaster, United Kingdom) ; Okajima, Y (Tokyo Institute of Technology, Department of Physics, Tokyo, Japan) ; Okumura, K (University of Tokyo, Institute for Cosmic Ray Research, Research Center for Cosmic Neutrinos, Kashiwa, Japan) (University of Tokyo, Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, Kashiwa, Chiba, Japan) ; Onishchuk, Yu (Kyiv National University, Department of Nuclear Physics, Kyiv, Ukraine) ; O’Sullivan, E (Stockholm University, Oskar Klein Centre and Department of Physics, Stockholm, Sweden) ; O’Sullivan, L (University of Sheffield, Department of Physics and Astronomy, Sheffield, United Kingdom) ; Ovsiannikova, T (Institute for Nuclear Research of the Russian Academy of Sciences, Moscow, Russia) ; Owen, R A (Queen Mary University of London, School of Physics and Astronomy, London, United Kingdom) ; Oyama, Y (High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki, Japan) ; Pérez, J (University Autonoma Madrid, Department of Theoretical Physics, Madrid, Spain) ; Pac, M Y (Dongshin University, Department of Physics, Naju, Korea) ; Palladino, V (INFN Sezione di Napoli and Università di Napoli, Dipartimento di Fisica, Napoli, Italy) ; Palomino, J L (State University of New York at Stony Brook, Department of Physics and Astronomy, Stony Brook, New York, U.S.A.) ; Paolone, V (University of Pittsburgh, Department of Physics and Astronomy, Pittsburgh, Pennsylvania, U.S.A.) ; Park, H S (Korea Astronomy and Space Science Institute, Daejeon 34055, Korea) ; Park, J C (Chungnam National University, Department of Physics, Daejeon 34134, Korea) ; Park, M G (Kyungpook National University, Department of Astronomy and Atmospheric Sciences, Daegu 41566, Korea) ; Park, S C (Yonsei University, Department of Physics and IPAP, Seoul 03722, Korea) ; Parker, W (Royal Holloway University of London, Department of Physics, Egham, Surrey, United Kingdom) ; Parsa, S (University of Geneva, Section de Physique, DPNC, Geneva, Switzerland) ; Payne, D (University of Liverpool, Department of Physics, Liverpool, United Kingdom) ; Perkin, J D (University of Sheffield, Department of Physics and Astronomy, Sheffield, United Kingdom) ; Pidcott, C (University of Sheffield, Department of Physics and Astronomy, Sheffield, United Kingdom) ; Pinzon Guerra, E (York University, Department of Physics and Astronomy, Toronto, Ontario, Canada) ; Playfer, S (University of Edinburgh, School of Physics and Astronomy, Edinburgh, United Kingdom) ; Popov, B (Laboratoire de Physique Nucleaire et de Hautes Energies, UPMC and Universite Paris-Diderot and CNRS/IN2P3, Paris, France) ; Posiadala-Zezula, M (University of Warsaw, Faculty of Physics, Warsaw, Poland) ; Poutissou, J-M (TRIUMF, Vancouver, British Columbia, Canada) ; Pritchard, A (University of Liverpool, Department of Physics, Liverpool, United Kingdom) ; Prouse, N W (Queen Mary University of London, School of Physics and Astronomy, London, United Kingdom) ; Pronost, G (University of Tokyo, Institute for Cosmic Ray Research, Kamioka Observatory, Kamioka, Japan) ; Przewlocki, P (National Centre for Nuclear Research, Warsaw, Poland) ; Quilain, B (Kyoto University, Department of Physics, Kyoto, Japan) ; Quinto, M (INFN Sezione di Bari and Università e Politecnico di Bari, Dipartimento Interuniversitario di Fisica, Bari, Italy) ; Radicioni, E (INFN Sezione di Bari and Università e Politecnico di Bari, Dipartimento Interuniversitario di Fisica, Bari, Italy) ; Ratoff, P N (Lancaster University, Physics Department, Lancaster, United Kingdom) ; Retiere, F (TRIUMF, Vancouver, British Columbia, Canada) ; Riccio, C (INFN Sezione di Napoli and Università di Napoli, Dipartimento di Fisica, Napoli, Italy) ; Richards, B (Queen Mary University of London, School of Physics and Astronomy, London, United Kingdom) ; Rondio, E (National Centre for Nuclear Research, Warsaw, Poland) ; Rose, H J (University of Liverpool, Department of Physics, Liverpool, United Kingdom) ; Rott, C (Sungkyunkwan University, Department of Physics,Suwon 16419, Korea) ; Rountree, S D (Virginia Tech, Center for Neutrino Physics, Blacksburg, Virginia, U.S.A.) ; Ruggeri, A C (INFN Sezione di Napoli and Università di Napoli, Dipartimento di Fisica, Napoli, Italy) ; Rychter, A (Warsaw University of Technology, Institute of Radioelectronics and Multimedia Technology, Warsaw, Poland) ; Ryu, D (UNIST, Department of Physics, Ulsan, Korea) ; Sacco, R (Queen Mary University of London, School of Physics and Astronomy, London, United Kingdom) ; Sakuda, M (Okayama University, Department of Physics, Okayama, Japan) ; Sanchez, M C (Iowa State University, Department of Physics and Astronomy, Ames, Iowa, U.S.A.) ; Scantamburlo, E (University of Geneva, Section de Physique, DPNC, Geneva, Switzerland) ; Scott, M (TRIUMF, Vancouver, British Columbia, Canada) ; Molina Sedgwick, S (Queen Mary University of London, School of Physics and Astronomy, London, United Kingdom) ; Seiya, Y (Osaka City University, Department of Physics, Osaka, Japan) ; Sekiguchi, T (High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki, Japan) ; Sekiya, H (University of Tokyo, Institute for Cosmic Ray Research, Kamioka Observatory, Kamioka, Japan) (University of Tokyo, Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, Kashiwa, Chiba, Japan) ; Seo, H (Seoul National University, Department of Physics and Astronomy, Seoul 08826, Korea) ; Seo, S H (Seoul National University, Department of Physics and Astronomy, Seoul 08826, Korea) ; Sgalaberna, D (University of Geneva, Section de Physique, DPNC, Geneva, Switzerland) ; Shah, R (Oxford University, Department of Physics, Oxford, United Kingdom) ; Shaikhiev, A (Institute for Nuclear Research of the Russian Academy of Sciences, Moscow, Russia) ; Shimizu, I (Research Center for Neutrino Science, Tohoku University, Sendai, Japan) ; Shiozawa, M (University of Tokyo, Institute for Cosmic Ray Research, Kamioka Observatory, Kamioka, Japan) (University of Tokyo, Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, Kashiwa, Chiba, Japan) ; Shitov, Y (Imperial College London, Department of Physics, London, United Kingdom) (Royal Holloway University of London, Department of Physics, Egham, Surrey, United Kingdom) ; Short, S (Queen Mary University of London, School of Physics and Astronomy, London, United Kingdom) ; Simpson, C (Oxford University, Department of Physics, Oxford, United Kingdom) (University of Tokyo, Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, Kashiwa, Chiba, Japan) ; Sinnis, G (Los Alamos National Laboratory, New Mexico, U.S.A.) ; Smy, M B (University of California, Irvine, Department of Physics and Astronomy, Irvine, California, U.S.A.) (University of Tokyo, Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, Kashiwa, Chiba, Japan) ; Snow, S (University of Warwick, Department of Physics, Coventry, United Kingdom) ; Sobczyk, J (Wroclaw University, Faculty of Physics and Astronomy, Wroclaw, Poland) ; Sobel, H W (University of California, Irvine, Department of Physics and Astronomy, Irvine, California, U.S.A.) (University of Tokyo, Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, Kashiwa, Chiba, Japan) ; Son, D C (Kyungpook National University, Department of Physics, Daegu 41566, Korea) ; Sonoda, Y (University of Tokyo, Institute for Cosmic Ray Research, Kamioka Observatory, Kamioka, Japan) ; Spina, R (INFN Sezione di Bari and Università e Politecnico di Bari, Dipartimento Interuniversitario di Fisica, Bari, Italy) ; Stewart, T (STFC, Rutherford Appleton Laboratory, Harwell Oxford, and Daresbury Laboratory, Warrington, United Kingdom) ; Stone, J L (Boston University, Department of Physics, Boston, Massachusetts, U.S.A.) (University of Tokyo, Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, Kashiwa, Chiba, Japan) ; Suda, Y (University of Tokyo, Department of Physics, Tokyo, Japan) ; Suwa, Y (Kyoto University, Yukawa Institute for Theoretical Physics, Kyoto, Japan) ; Suzuki, Y (University of Tokyo, Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, Kashiwa, Chiba, Japan) ; Suzuki, A T (Kobe University, Department of Physics, Kobe, Japan) ; Svoboda, R (University of California, Davis, Department of Physics, Davis, California, U.S.A.) ; Taani, M (University of Edinburgh, School of Physics and Astronomy, Edinburgh, United Kingdom) (Nagoya University, Graduate School of Science, Nagoya, Japan) ; Tacik, R (University of Regina, Department of Physics, Regina, Saskatchewan, Canada) ; Takeda, A (University of Tokyo, Institute for Cosmic Ray Research, Kamioka Observatory, Kamioka, Japan) ; Takenaka, A (University of Tokyo, Institute for Cosmic Ray Research, Kamioka Observatory, Kamioka, Japan) ; Taketa, A (University of Tokyo, Earthquake Research Institute, Tokyo, Japan) ; Takeuchi, Y (Kobe University, Department of Physics, Kobe, Japan) (University of Tokyo, Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, Kashiwa, Chiba, Japan) ; Takhistov, V (University of California, Irvine, Department of Physics and Astronomy, Irvine, California, U.S.A.) ; Tanaka, H A (University of Toronto, Department of Physics, Toronto, Ontario, Canada) ; Tanaka, H K M (University of Tokyo, Earthquake Research Institute, Tokyo, Japan) ; Tanaka, H (University of Tokyo, Institute for Cosmic Ray Research, Kamioka Observatory, Kamioka, Japan) (University of Tokyo, Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, Kashiwa, Chiba, Japan) ; Terri, R (Queen Mary University of London, School of Physics and Astronomy, London, United Kingdom) ; Thiesse, M (University of Sheffield, Department of Physics and Astronomy, Sheffield, United Kingdom) ; Thompson, L F (University of Sheffield, Department of Physics and Astronomy, Sheffield, United Kingdom) ; Thorpe, M (STFC, Rutherford Appleton Laboratory, Harwell Oxford, and Daresbury Laboratory, Warrington, United Kingdom) ; Tobayama, S (University of British Columbia, Department of Physics and Astronomy, Vancouver, British Columbia, Canada) ; Touramanis, C (University of Liverpool, Department of Physics, Liverpool, United Kingdom) ; Towstego, T (University of Toronto, Department of Physics, Toronto, Ontario, Canada) ; Tsukamoto, T (High Energy Accelerator Research Organization (KEK), Tsukuba, Ibaraki, Japan) ; Tsui, K M (University of Tokyo, Institute for Cosmic Ray Research, Research Center for Cosmic Neutrinos, Kashiwa, Japan) ; Tzanov, M (Louisiana State University, Department of Physics and Astronomy, Baton Rouge, Louisiana, U.S.A.) ; Uchida, Y (Imperial College London, Department of Physics, London, United Kingdom) ; Vagins, M R (University of California, Irvine, Department of Physics and Astronomy, Irvine, California, U.S.A.) (University of Tokyo, Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, Kashiwa, Chiba, Japan) ; Vasseur, G (IRFU, CEA Saclay, Gif-sur-Yvette, France) ; Vilela, C (State University of New York at Stony Brook, Department of Physics and Astronomy, Stony Brook, New York, U.S.A.) ; Vogelaar, R B (Virginia Tech, Center for Neutrino Physics, Blacksburg, Virginia, U.S.A.) ; Walding, J (Royal Holloway University of London, Department of Physics, Egham, Surrey, United Kingdom) ; Walker, J (University of Winnipeg, Department of Physics, Winnipeg, Manitoba, Canada) ; Ward, M (STFC, Rutherford Appleton Laboratory, Harwell Oxford, and Daresbury Laboratory, Warrington, United Kingdom) ; Wark, D (Oxford University, Department of Physics, Oxford, United Kingdom) (STFC, Rutherford Appleton Laboratory, Harwell Oxford, and Daresbury Laboratory, Warrington, United Kingdom) ; Wascko, M O (Imperial College London, Department of Physics, London, United Kingdom) ; Weber, A (STFC, Rutherford Appleton Laboratory, Harwell Oxford, and Daresbury Laboratory, Warrington, United Kingdom) ; Wendell, R (Kyoto University, Department of Physics, Kyoto, Japan) (University of Tokyo, Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, Kashiwa, Chiba, Japan) ; Wilkes, R J (University of Washington, Department of Physics, Seattle, Washington, U.S.A.) ; Wilking, M J (State University of New York at Stony Brook, Department of Physics and Astronomy, Stony Brook, New York, U.S.A.) ; Wilson, J R (Queen Mary University of London, School of Physics and Astronomy, London, United Kingdom) ; Won, E (Korea University, Department of Physics, Seoul 02841, Korea) ; Xin, T (Iowa State University, Department of Physics and Astronomy, Ames, Iowa, U.S.A.) ; Yamamoto, K (Osaka City University, Department of Physics, Osaka, Japan) ; Yanagisawa, C (State University of New York at Stony Brook, Department of Physics and Astronomy, Stony Brook, New York, U.S.A.) ; Yano, T (Kobe University, Department of Physics, Kobe, Japan) ; Yasuda, O (Tokyo Metropolitan University, Department of Physics, Tokyo, Japan) ; Yen, S (TRIUMF, Vancouver, British Columbia, Canada) ; Yershov, N (Institute for Nuclear Research of the Russian Academy of Sciences, Moscow, Russia) ; Yeum, D N (Seoul National University, Department of Physics and Astronomy, Seoul 08826, Korea) ; Yokoyama, M (University of Tokyo, Kavli Institute for the Physics and Mathematics of the Universe (WPI), Todai Institutes for Advanced Study, Kashiwa, Chiba, Japan) (University of Tokyo, Department of Physics, Tokyo, Japan) ; Yoo, H D (Seoul National University, Department of Physics and Astronomy, Seoul 08826, Korea) ; Yoo, J (Korea Advanced Institute of Science and Technology (KAIST), Department of Physics, Daejeon 34141, Korea) ; Yoon, S C (Seoul National University, Department of Physics and Astronomy, Seoul 08826, Korea) ; Yoon, T S (Kyungpook National University, Department of Astronomy and Atmospheric Sciences, Daegu 41566, Korea) ; Yoshida, T (Tokyo Institute of Technology, Department of Physics, Tokyo, Japan) ; Yu, I (Sungkyunkwan University, Department of Physics,Suwon 16419, Korea) ; Yu, M (York University, Department of Physics and Astronomy, Toronto, Ontario, Canada) ; Zalipska, J (National Centre for Nuclear Research, Warsaw, Poland) ; Zaremba, K (Warsaw University of Technology, Institute of Radioelectronics and Multimedia Technology, Warsaw, Poland) ; Ziembicki, M (Warsaw University of Technology, Institute of Radioelectronics and Multimedia Technology, Warsaw, Poland) ; Zito, M (IRFU, CEA Saclay, Gif-sur-Yvette, France) ; Zsoldos, S (Queen Mary University of London, School of Physics and Astronomy, London, United Kingdom)

30 January 2019

Abstract: Hyper-Kamiokande consists of two identical water-Cherenkov detectors of total 520 kt, with the first one in Japan at 295 km from the J-PARC neutrino beam with 2.5 off-axis angles (OAAs), and the second one possibly in Korea at a later stage. Having the second detector in Korea would benefit almost all areas of neutrino oscillation physics, mainly due to longer baselines. There are several candidate sites in Korea with baselines of 1000–1300 km and OAAs of 1 –3 . We conducted sensitivity studies on neutrino oscillation physics for a second detector, either in Japan (JD 2) or Korea (JD + KD), and compared the results with a single detector in Japan. Leptonic charge–parity (CP) symmetry violation sensitivity is improved, especially when the CP is non-maximally violated. The larger matter effect at Korean candidate sites significantly enhances sensitivities to non-standard interactions of neutrinos and mass ordering determination. Current studies indicate the best sensitivity is obtained at Mt. Bisul (1088 km baseline, OAA). Thanks to a larger (1000 m) overburden than the first detector site, clear improvements to sensitivities for solar and supernova relic neutrino searches are expected.


Published in: PTEP 2018 (2018) 063C01
Published by: Oxford University Press/Physical Society of Japan
DOI: 10.1093/ptep/pty044
arXiv: 1611.06118
License: CC-BY-3.0



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