Skip to main navigation Skip to search Skip to main content

Physics potentials with the second Hyper-Kamiokande detector in Korea

  • K. Abe
  • , Ke Abe
  • , S. H. Ahn
  • , H. Aihara
  • , A. Aimi
  • , R. Akutsu
  • , C. Andreopoulos
  • , I. Anghel
  • , L. H.V. Anthony
  • , M. Antonova
  • , Y. Ashida
  • , V. Aushev
  • , M. Barbi
  • , G. J. Barker
  • , G. Barr
  • , P. Beltrame
  • , V. Berardi
  • , M. Bergevin
  • , S. Berkman
  • , L. Berns
  • T. Berry, S. Bhadra, F. D.M. Blaszczyk, A. Blondel, S. Bolognesi, S. B. Boyd, A. Bravar, C. Bronner, M. Buizza Avanzini, F. S. Cafagna, R. Calland, S. Cao, S. L. Cartwright, M. G. Catanesi, C. Checchia, Z. Chen-Wishart, B. G. Cheon, M. K. Cheoun, K. Cho, J. H. Choi, K. Choi, K. Y. Choi, E. J. Chun, A. Cole, J. Coleman, G. Collazuol, G. Cowan, L. Cremonesi, T. Dealtry, G. De Rosa, C. Densham, D. Dewhurst, E. Drakopoulou, F. Di Lodovico, O. Drapier, J. Dumarchez, P. Dunne, M. Dziewiecki, S. Emery, A. Esmaili, A. Evangelisti, E. Fernández-Martinez, T. Feusels, A. Finch, G. A. Fiorentini, G. Fiorillo, M. Fitton, K. Frankiewicz, M. Friend, Y. Fujii, Y. Fukuda, D. Fukuda, K. Ganezer, M. Ghosh, C. Giganti, M. Gonin, N. Grant, P. Gumplinger, D. R. Hadley, B. Hartfiel, M. Hartz, Y. Hayato, K. Hayrapetyan, J. Hill, S. Hirota, S. Horiuchi, A. K. Ichikawa, T. Iijima, M. Ikeda, J. Imber, K. Inoue, J. Insler, R. A. Intonti, A. Ioannisian, T. Ishida, H. Ishino, M. Ishitsuka, Y. Itow, K. Iwamoto, A. Izmaylov, B. Jamieson, H. I. Jang, J. S. Jang, S. H. Jeon, K. S. Jeong, M. Jiang, P. Jonsson, K. K. Joo, A. Kaboth, C. Kachulis, T. Kajita, S. K. Kang, J. Kameda, Y. Kataoka, T. Katori, K. Kayrapetyan, E. Kearns, M. Khabibullin, A. Khotjantsev, C. S. Kim, H. B. Kim, H. J. Kim, J. H. Kim, J. S. Kim, J. Y. Kim, S. B. Kim, S. C. Kim, S. W. Kim, S. Y. Kim, T. J. Kim, W. Kim, S. King, Y. Kishimoto, P. Ko, T. Kobayashi, M. Koga, A. Konaka, L. L. Kormos, Y. Koshio, A. Korzenev, K. L. Kowalik, W. R. Kropp, Y. Kudenko, R. Kurjata, T. Kutter, M. Kuze, K. Kwak, E. H. Kwon, L. Labarga, J. Lagoda, P. J.J. Lasorak, M. Laveder, M. Lawe, J. G. Learned, C. H. Lee, S. J. Lee, W. J. Lee, I. T. Lim, T. Lindner, R. P. Litchfield, A. Longhin, P. Loverre, T. Lou, L. Ludovici, W. Ma, L. Magaletti, K. Mahn, M. Malek, L. Maret, C. Mariani, K. Martens, L. Marti, J. F. Martin, J. Marzec, S. Matsuno, E. Mazzucato, M. McCarthy, N. McCauley, K. S. McFarland, C. McGrew, A. Mefodiev, P. Mermod, C. Metelko, M. Mezzetto, J. Migenda, P. Mijakowski, H. Minakata, A. Minamino, S. Mine, O. Mineev, A. Mitra, M. Miura, T. Mochizuki, J. Monroe, C. S. Moon, D. H. Moon, S. Moriyama, T. Mueller, F. Muheim, K. Murase, F. Muto, M. Nakahata, Y. Nakajima, K. Nakamura, T. Nakaya, S. Nakayama, C. Nantais, M. Needham, T. Nicholls, Y. Nishimura, E. Noah, F. Nova, J. Nowak, H. Nunokawa, Y. Obayashi, Y. D. Oh, Y. Oh, H. M. O'Keeffe, Y. Okajima, K. Okumura, Yu Onishchuk, E. O'Sullivan, L. O'Sullivan, T. Ovsiannikova, R. A. Owen, Y. Oyama, J. Pérez, M. Y. Pac, V. Palladino, J. L. Palomino, V. Paolone, H. S. Park, J. C. Park, M. G. Park, W. Parker, S. C. Park, S. Parsa, D. Payne, J. D. Perkin, C. Pidcott, E. Pinzon Guerra, S. Playfer, B. Popov, M. Posiadala-Zezula, J. M. Poutissou, A. Pritchard, N. W. Prouse, G. Pronost, P. Przewlocki, B. Quilain, M. Quinto, E. Radicioni, P. N. Ratoff, F. Retiere, C. Riccio, B. Richards, E. Rondio, H. J. Rose, C. Rott, S. D. Rountree, A. C. Ruggeri, A. Rychter, D. Ryu, R. Sacco, M. Sakuda, M. C. Sanchez, E. Scantamburlo, M. Scott, S. Molina Sedgwick, Y. Seiya, T. Sekiguchi, H. Sekiya, H. Seo, S. H. Seo, D. Sgalaberna, R. Shah, A. Shaikhiev, I. Shimizu, M. Shiozawa, Y. Shitov, S. Short, C. Simpson, G. Sinnis, M. B. Smy, S. Snow, J. Sobczyk, H. W. Sobel, D. C. Son, Y. Sonoda, R. Spina, T. Stewart, J. L. Stone, Y. Suda, Y. Suwa, Y. Suzuki, A. T. Suzuki, R. Svoboda, M. Taani, R. Tacik, A. Takeda, A. Takenaka, A. Taketa, Y. Takeuchi, V. Takhistov, H. A. Tanaka, H. K.M. Tanaka, H. Tanaka, R. Terri, M. Thiesse, L. F. Thompson, M. Thorpe, S. Tobayama, C. Touramanis, T. Towstego, T. Tsukamoto, K. M. Tsui, M. Tzanov, Y. Uchida, M. R. Vagins, G. Vasseur, C. Vilela, R. B. Vogelaar, J. Walding, J. Walker, M. Ward, D. Wark, M. O. Wascko, A. Weber, R. Wendell, R. J. Wilkes, M. J. Wilking, J. R. Wilson, E. Won, T. Xin, K. Yamamoto, C. Yanagisawa, T. Yano, O. Yasuda, S. Yen, N. Yershov, D. N. Yeum, M. Yokoyama, H. D. Yoo, J. Yoo, S. C. Yoon, T. S. Yoon, T. Yoshida, I. Yu, M. Yu, J. Zalipska, K. Zaremba, M. Ziembicki, M. Zito, S. Zsoldos
  • University of Tokyo
  • Kobe University
  • Korea Astronomy and Space Science Institute
  • INFN
  • University of Liverpool
  • CCLRC Rutherford Appleton Laboratory
  • Iowa State University
  • Institute for Nuclear Research of the Russian Academy of Sciences
  • Kyoto University
  • National University of Kyiv
  • University of Regina
  • University of Warwick
  • University of Oxford
  • University of Edinburgh
  • Politecnico di Bari
  • University of California, Davis
  • University of British Columbia
  • Tokyo Institute of Technology
  • Royal Holloway University of London
  • York University
  • Boston University
  • University of Geneva
  • Universite Paris-Saclay
  • High Energy Accelerator Research Organization (KEK)
  • The University of Sheffield
  • Hanyang University
  • Soongsil University
  • Korea Institute of Science and Technology Information
  • Dongshin University
  • University of Hawaii
  • Sungkyunkwan University
  • Korean Institute for Advanced Studies
  • Queen Mary University of London
  • Lancaster University
  • University of Naples Federico II
  • Universités Paris VI and VII
  • Imperial College London
  • Warsaw University of Technology
  • Pontifícia Universidade Católica do Rio de Janeiro
  • Universidad Autónoma de Madrid
  • University of Sheffield
  • National Centre for Nuclear Research (NCBJ)
  • Miyagi University of Education
  • Okayama University
  • California State University, Dominguez Hills
  • Tokyo Metropolitan University
  • TRIUMF
  • Virginia Polytechnic Institute and State University
  • Nagoya University
  • Ip Paris
  • Tohoku University
  • Louisiana State University
  • Yerevan Institute for Theoretical Physics and Modeling
  • Tokyo University of Science
  • University of Winnipeg
  • Seoyeong University
  • Gwangju Institute of Science and Technology
  • Pusan National University
  • Chonnam National University
  • Seoul National University of Science and Technology
  • Yonsei University
  • Kyungpook National University
  • Seoul National University
  • Korea University of Science and Technology
  • Long Beach VA and University of California
  • National Research Nuclear University MEPhI
  • Moscow Institute of Physics and Technology
  • Ulsan National Institute of Science and Technology
  • Korea University
  • Sezione di Roma
  • Michigan State University
  • University of Toronto
  • University of Rochester
  • Stony Brook University
  • Yokohama National University
  • Pennsylvania State University
  • Stockholm University
  • University of Pittsburgh
  • Chungnam National University
  • University of Warsaw
  • Osaka City University
  • MST-8, Los Alamos National Laboratory
  • Wroclaw University
  • Yukawa Institute for Theoretical Physics
  • University of Washington
  • Korea Advanced Institute of Science and Technology

Research output: Contribution to journalArticlepeer-review

185 Citations (Scopus)

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, 1.3° 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.

Original languageEnglish
Article number063C01
JournalProgress of Theoretical and Experimental Physics
Volume2018
Issue number6
DOIs
Publication statusPublished - 1 Jun 2018

Keywords

  • C03
  • C04
  • C12
  • C32
  • C43

Fingerprint

Dive into the research topics of 'Physics potentials with the second Hyper-Kamiokande detector in Korea'. Together they form a unique fingerprint.

Cite this