T
Takaaki Mori
Researcher at Okayama University
Publications - 60
Citations - 3552
Takaaki Mori is an academic researcher from Okayama University. The author has contributed to research in topics: Neutrino & Super-Kamiokande. The author has an hindex of 27, co-authored 59 publications receiving 2992 citations.
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Journal ArticleDOI
Solar neutrino results in Super-Kamiokande-III
K. Abe,Y. Hayato,T. Iida,M. Ikeda,M. Ikeda,C. Ishihara,K. Iyogi,J. Kameda,Ken-ichiro Kobayashi,Yusuke Koshio,Y. Kozuma,M. Miura,S. Moriyama,Masayuki Nakahata,S. Nakayama,Y. Obayashi,H. Ogawa,Hiroyuki Sekiya,Masato Shiozawa,Yasunari Suzuki,Atsushi Takeda,Y. Takenaga,Koh Ueno,K. Ueshima,Hiroshi Watanabe,S. Yamada,T. Yokozawa,S. Hazama,H. Kaji,Takaaki Kajita,K. Kaneyuki,T. McLachlan,Ko Okumura,Y. Shimizu,N. Tanimoto,M. R. Vagins,M. R. Vagins,L. Labarga,L. M. Magro,Frédéric Dufour,E. Kearns,E. Kearns,Michael Litos,J. L. Raaf,J. L. Stone,J. L. Stone,L. R. Sulak,W. Wang,W. Wang,M. Goldhaber,K. Bays,David William Casper,J. P. Cravens,W. R. Kropp,S. Mine,C. Regis,A. L. Renshaw,M. B. Smy,M. B. Smy,H. W. Sobel,H. W. Sobel,K. S. Ganezer,John Hill,W. E. Keig,J. S. Jang,J. Y. Kim,I. T. Lim,Justin Albert,R. A. Wendell,T. Wongjirad,Kate Scholberg,Kate Scholberg,C. W. Walter,C. W. Walter,T. Ishizuka,S. Tasaka,John G. Learned,S. Matsuno,Y. Watanabe,Takehisa Hasegawa,T. Ishida,T. Ishii,T. Kobayashi,T. Nakadaira,Koji Nakamura,K. Nishikawa,H. Nishino,Yuichi Oyama,Ken Sakashita,T. Sekiguchi,T. Tsukamoto,A. T. Suzuki,Y. Takeuchi,Y. Takeuchi,A. Minamino,Tsuyoshi Nakaya,Tsuyoshi Nakaya,Y. Fukuda,Yoshitaka Itow,G. Mitsuka,T. Tanaka,C. K. Jung,G. D. Lopez,C. McGrew,R. Terri,C. Yanagisawa,N. Tamura,Hirokazu Ishino,A. Kibayashi,S. Mino,Takaaki Mori,Makoto Sakuda,H. Toyota,Y. Kuno,Minoru Yoshida,S. B. Kim,B. S. Yang,H. Okazawa,Y. Choi,K. Nishijima,Y. Yokosawa,M. Koshiba,Y. Totsuka,Masashi Yokoyama,Song Chen,Y. Heng,Zishuo Yang,Haoxiong Zhang,D. Kielczewska,P. Mijakowski,K. Connolly,M. Dziomba,E. Thrane,E. Thrane,R. J. Wilkes +134 more
TL;DR: The results of the third phase of the Super-Kamiokande solar neutrino measurement are presented and compared to the first and second phase results in this article, where improved detector calibrations, a full detector simulation, and improved analysis methods are estimated to be approximately 2.1%, which is about two thirds of the systematic uncertainty for the first phase.
Journal ArticleDOI
Physics potential of a long-baseline neutrino oscillation experiment using a J-PARC neutrino beam and Hyper-Kamiokande
K. Abe,K. Abe,Hiroaki Aihara,Hiroaki Aihara,C. Andreopoulos,I. Anghel,Akitaka Ariga,Tomoko Ariga,R. Asfandiyarov,M. Askins,J. J. Back,P. Ballett,M. Barbi,Gareth J. Barker,G.D. Barr,F. Bay,P. Beltrame,Vincenzo Berardi,M. Bergevin,S. Berkman,Tracey Berry,S. Bhadra,F. d. M. Blaszczyk,A. Blondel,S. Bolognesi,S. B. Boyd,A. Bravar,C. Bronner,F. Cafagna,G. Carminati,S. L. Cartwright,M. G. Catanesi,K. Choi,J. H. Choi,G. Collazuol,G. A. Cowan,L. Cremonesi,GS Davies,G. De Rosa,C. Densham,J. A. Detwiler,D. Dewhurst,F. Di Lodovico,S. Di Luise,O. Drapier,S. W. K. Emery,Antonio Ereditato,Pablo Fernandez,T. Feusels,Alexander Finch,M. Fitton,M. Friend,Y. Fujii,Y. Fukuda,D. Fukuda,V. Galymov,K. S. Ganezer,M. Gonin,P. Gumplinger,D. R. Hadley,Leïla Haegel,A. Haesler,Yoshinori Haga,B. L. Hartfiel,M. Hartz,M. Hartz,Yoshinari Hayato,Yoshinari Hayato,M. Hierholzer,J. Hill,A. Himmel,Seiko Hirota,Shunsaku Horiuchi,K. Huang,A. K. Ichikawa,T. Iijima,M. Ikeda,J. Imber,Kunio Inoue,Kunio Inoue,J. Insler,R. A. Intonti,T. J. Irvine,T. Ishida,Hirokazu Ishino,Masaki Ishitsuka,Yoshitaka Itow,A. Izmaylov,B. Jamieson,H. I. Jang,M. Jiang,K. K. Joo,C. K. Jung,C. K. Jung,A. C. Kaboth,Takaaki Kajita,Takaaki Kajita,J. Kameda,J. Kameda,Y. Karadhzov,Teppei Katori,E. Kearns,E. Kearns,M. M. Khabibullin,A. N. Khotjantsev,Jy Kim,Soo-Bong Kim,Yasuhiro Kishimoto,Yasuhiro Kishimoto,Takashi Kobayashi,M. Koga,M. Koga,A. Konaka,L. L. Kormos,A. Korzenev,Yusuke Koshio,Yusuke Koshio,W. R. Kropp,Yu. G. Kudenko,T. Kutter,M. Kuze,L. Labarga,J. Lagoda,Marco Laveder,M. Lawe,J. G. Learned,I. T. Lim,T. Lindner,A. Longhin,L. Ludovici,W. Y. Ma,L. Magaletti,Kendall Mahn,M. Malek,C. Mariani,Ll. Marti,J. F. Martin,C. Martin,P. Martins,E. Mazzucato,N. McCauley,Kevin Scott McFarland,C. McGrew,M. Mezzetto,Hisakazu Minakata,A. Minamino,S. Mine,Oleg Mineev,M. Miura,M. Miura,Jocelyn Monroe,Takaaki Mori,S. Moriyama,S. Moriyama,Th. A. Mueller,F. Muheim,Masayuki Nakahata,Masayuki Nakahata,Koji Nakamura,Koji Nakamura,Tsuyoshi Nakaya,Tsuyoshi Nakaya,S. Nakayama,S. Nakayama,M. Needham,T. Nicholls,M. Nirkko,Y. Nishimura,Etam Noah,J. A. Nowak,Hiroshi Nunokawa,H. M. O'Keeffe,Y. Okajima,Kimihiro Okumura,Kimihiro Okumura,S. M. Oser,Erin O'Sullivan,T. Ovsiannikova,R. A. Owen,Yuichi Oyama,Jose L. Perez,M. Y. Pac,V. Palladino,J. L. Palomino,V. Paolone,D. Payne,O. Perevozchikov,J. D. Perkin,C. Pistillo,S. Playfer,M. Posiadala-Zezula,J. M. Poutissou,B. Quilain,M. Quinto,E. Radicioni,P. N. Ratoff,M. Ravonel,M. A.M. Rayner,A. Redij,F. Retiere,C. Riccio,E. Richard,E. Rondio,H. J. Rose,M. Ross-Lonergan,Carsten Rott,S. D. Rountree,André Rubbia,R. Sacco,Makoto Sakuda,M. C. Sanchez,E. Scantamburlo,Kate Scholberg,Kate Scholberg,Mark Scott,Y. Seiya,T. Sekiguchi,Hiroyuki Sekiya,Hiroyuki Sekiya,A. Shaikhiev,I. Shimizu,Masato Shiozawa,Masato Shiozawa,S. Short,G. Sinnis,M. B. Smy,M. B. Smy,Jan T. Sobczyk,Henry W. Sobel,Henry W. Sobel,T. Stewart,J. L. Stone,J. L. Stone,Yusuke Suda,Yoshihiro Suzuki,A. Suzuki,Robert Svoboda,R. Tacik,Atsushi Takeda,Akimichi Taketa,Y. Takeuchi,Y. Takeuchi,H.A. Tanaka,H. K. Tanaka,Hajime Tanaka,Hajime Tanaka,R. Terri,Lester D.R. Thompson,M. Thorpe,S. Tobayama,N. Tolich,T. Tomura,T. Tomura,C. Touramanis,T. Tsukamoto,M. Tzanov,Y. Uchida,M. R. Vagins,M. R. Vagins,G. Vasseur,R. B. Vogelaar,C. W. Walter,C. W. Walter,D. L. Wark,D. L. Wark,M. O. Wascko,A. C. Weber,A. C. Weber,R. A. Wendell,R. A. Wendell,R. J. Wilkes,M. J. Wilking,J. R. Wilson,T. Xin,Kazuhiro Yamamoto,C. Yanagisawa,T. Yano,S. Yen,N. Yershov,Masashi Yokoyama,Masashi Yokoyama,M. Zito +281 more
TL;DR: In this article, the physics potential of a long baseline neutrino experiment using the Hyper-Kamiokande detector and neutrinos from the J-PARC proton synchrotron is presented.
Journal ArticleDOI
Search for neutrinos from annihilation of captured low-mass dark matter particles in the Sun by Super-Kamiokande
K. Choi,K. Abe,K. Abe,Yoshinori Haga,Y. Hayato,Y. Hayato,K. Iyogi,J. Kameda,J. Kameda,Yasuhiro Kishimoto,Yasuhiro Kishimoto,M. Miura,M. Miura,S. Moriyama,S. Moriyama,Masayuki Nakahata,Masayuki Nakahata,Yuuki Nakano,S. Nakayama,S. Nakayama,Hiroyuki Sekiya,Hiroyuki Sekiya,Masato Shiozawa,Masato Shiozawa,Yasunari Suzuki,Yasunari Suzuki,Atsushi Takeda,Atsushi Takeda,T. Tomura,T. Tomura,R. A. Wendell,R. A. Wendell,T. J. Irvine,Takaaki Kajita,Takaaki Kajita,I. Kametani,K. Kaneyuki,K. Kaneyuki,K. P. Lee,Y. Nishimura,Kimihiro Okumura,Kimihiro Okumura,T. McLachlan,L. Labarga,E. Kearns,E. Kearns,J. L. Raaf,J. L. Stone,J. L. Stone,L. R. Sulak,S. Berkman,H.A. Tanaka,S. Tobayama,M. Goldhaber,G. Carminati,W. R. Kropp,S. Mine,A. L. Renshaw,M. B. Smy,M. B. Smy,H. W. Sobel,H. W. Sobel,K. S. Ganezer,John Hill,N. Hong,J. Y. Kim,I. T. Lim,T. Akiri,A. Himmel,Kate Scholberg,Kate Scholberg,C. W. Walter,C. W. Walter,T. Wongjirad,T. Ishizuka,Shigeki Tasaka,J. S. Jang,J. G. Learned,S. Matsuno,S. N. Smith,T. Hasegawa,T. Ishida,T. Ishii,T. Kobayashi,T. Nakadaira,K. Nakamura,K. Nakamura,Yuichi Oyama,K. Sakashita,T. Sekiguchi,T. Tsukamoto,A. T. Suzuki,Y. Takeuchi,C. Bronner,Seiko Hirota,K. Huang,K. Ieki,M. Ikeda,T. Kikawa,A. Minamino,Tsuyoshi Nakaya,Tsuyoshi Nakaya,Kazuhiro Suzuki,Susumu Takahashi,Y. Fukuda,Yoshitaka Itow,G. Mitsuka,P. Mijakowski,Joshua Hignight,J. Imber,C. K. Jung,C. Yanagisawa,Hirokazu Ishino,A. Kibayashi,Yusuke Koshio,Takaaki Mori,Makoto Sakuda,T. Yano,Y. Kuno,R. Tacik,R. Tacik,S. B. Kim,H. Okazawa,Y. Choi,K. Nishijima,M. Koshiba,Y. Totsuka,Masashi Yokoyama,Masashi Yokoyama,K. Martens,Ll. Marti,M. R. Vagins,M. R. Vagins,J. F. Martin,P. de Perio,A. Konaka,M. J. Wilking,Song Chen,Yejin Zhang,R. J. Wilkes +139 more
TL;DR: In this article, the authors considered neutrino events with interaction vertices in the SK detector in addition to upward-going muons produced in the surrounding rock and found no significant excess over expected atmospheric-neutrino background and interpreted the result in terms of upper limits on WIMP-nucleon elastic scattering cross sections under different assumptions about the annihilation channel.
Journal ArticleDOI
Supernova Relic Neutrino Search at Super-Kamiokande
K. Bays,T. Iida,K. Abe,Y. Hayato,K. Iyogi,J. Kameda,Yusuke Koshio,L. Marti,M. Miura,S. Moriyama,Masayuki Nakahata,S. Nakayama,Y. Obayashi,Hiroyuki Sekiya,Masato Shiozawa,Yoshihiro Suzuki,Atsushi Takeda,Y. Takenaga,Koh Ueno,K. Ueshima,S. Yamada,T. Yokozawa,H. Kaji,Takaaki Kajita,K. Kaneyuki,T. McLachlan,Ko Okumura,K. P. Lee,K. Martens,M. R. Vagins,M. R. Vagins,L. Labarga,E. Kearns,E. Kearns,Michael Litos,J. L. Raaf,J. L. Stone,J. L. Stone,L. R. Sulak,W. R. Kropp,S. Mine,C. Regis,A. L. Renshaw,M. B. Smy,M. B. Smy,H. W. Sobel,H. W. Sobel,K. S. Ganezer,John Hill,W. E. Keig,Sunghoon Cho,J. S. Jang,J. Y. Kim,I. T. Lim,Justin Albert,Kate Scholberg,Kate Scholberg,C. W. Walter,C. W. Walter,R. A. Wendell,T. Wongjirad,T. Ishizuka,Shigeki Tasaka,J. G. Learned,S. Matsuno,S. N. Smith,Takehisa Hasegawa,T. Ishida,T. Ishii,T. Kobayashi,T. Nakadaira,Koji Nakamura,K. Nishikawa,Yuichi Oyama,K. Sakashita,T. Sekiguchi,T. Tsukamoto,A. T. Suzuki,Y. Takeuchi,Y. Takeuchi,M. Ikeda,Kodai Matsuoka,A. Minamino,A. Murakami,Tsuyoshi Nakaya,Tsuyoshi Nakaya,Y. Fukuda,Yoshitaka Itow,G. Mitsuka,M. Miyake,T. Tanaka,Joshua Hignight,J. Imber,C. K. Jung,I. Taylor,C. Yanagisawa,A. Kibayashi,Hirokazu Ishino,S. Mino,Makoto Sakuda,Takaaki Mori,H. Toyota,Y. Kuno,S. B. Kim,B. S. Yang,H. Okazawa,Y. Choi,K. Nishijima,M. Koshiba,Y. Totsuka,Masashi Yokoyama,Y. Heng,Song Chen,Haoxiong Zhang,Zishuo Yang,P. Mijakowski,K. Connolly,M. Dziomba,R. J. Wilkes +118 more
TL;DR: A new Super-Kamiokande search for supernova relic neutrinos was conducted using 2853 live days of data as mentioned in this paper, and the results showed that the neutrino flux was between 2.8 and 3.3 MeV.
Journal ArticleDOI
Atmospheric neutrino oscillation analysis with external constraints in Super-Kamiokande I-IV
Ke. Abe,C. Bronner,Y. Haga,Y. Hayato,M. Ikeda,K. Iyogi,J. Kameda,Yuta Kato,Yuji Kishimoto,L. Marti,M. Miura,S. Moriyama,Masayuki Nakahata,Tomohiko Nakajima,Yuuki Nakano,S. Nakayama,Y. Okajima,A. Orii,G. Pronost,Hiroyuki Sekiya,Masato Shiozawa,Y. Sonoda,Atsushi Takeda,A. Takenaka,H. K. Tanaka,Shigeki Tasaka,T. Tomura,R. Akutsu,T. J. Irvine,Takaaki Kajita,I. Kametani,K. Kaneyuki,Y. Nishimura,Kimihiro Okumura,E. Richard,K. M. Tsui,L. Labarga,Pablo Fernandez,F. d. M. Blaszczyk,J. Gustafson,C. Kachulis,E. Kearns,J. L. Raaf,J. L. Stone,Lawrence Sulak,S. Berkman,S. Tobayama,M. Goldhaber,G. Carminati,M. Elnimr,W. R. Kropp,S. Mine,S. Locke,A. L. Renshaw,M. B. Smy,Henry W. Sobel,V. Takhistov,P. Weatherly,K. S. Ganezer,Brandon L. Hartfiel,J. Hill,N. Hong,J. Y. Kim,I. T. Lim,R. G. Park,T. Akiri,A. Himmel,Z. Li,Erin O'Sullivan,Kate Scholberg,C. W. Walter,T. Wongjirad,T. Ishizuka,T. Nakamura,J. S. Jang,K. Choi,J. G. Learned,S. Matsuno,S. N. Smith,J. Amey,R. P. Litchfield,W. Y. Ma,Y. Uchida,M. O. Wascko,S. V. Cao,M. Friend,T. Hasegawa,T. Ishida,T. Ishii,Takashi Kobayashi,T. Nakadaira,K. Nakamura,Y. Oyama,K. Sakashita,T. Sekiguchi,T. Tsukamoto,K. Abe,Makoto Hasegawa,A. T. Suzuki,Y. Takeuchi,T. Yano,T. Hayashino,Seiko Hirota,K. Huang,K. Ieki,M. Jiang,T. Kikawa,K. E. Nakamura,Tsuyoshi Nakaya,N. D. Patel,Kazuhiro Suzuki,Susumu Takahashi,R. A. Wendell,L. H. V. Anthony,N. McCauley,A. Pritchard,Y. Fukuda,Yoshitaka Itow,G. Mitsuka,M. Murase,Francesco Muto,T. Suzuki,P. Mijakowski,K. Frankiewicz,Joshua Hignight,J. Imber,C. K. Jung,Xiaoning Li,J. L. Palomino,G. Santucci,C. Vilela,M. J. Wilking,C. Yanagisawa,Shintaro Ito,D. Fukuda,Hirokazu Ishino,T. Kayano,A. Kibayashi,Yusuke Koshio,Takaaki Mori,H. Nagata,Makoto Sakuda,C. Xu,Yoshitaka Kuno,D. L. Wark,F. Di Lodovico,B. Richards,R. Tacik,Soo-Bong Kim,A. Cole,Lester D.R. Thompson,H. Okazawa,Y. Choi,K. Ito,K. Nishijima,M. Koshiba,Y. Totsuka,Yusuke Suda,Masashi Yokoyama,R. G. Calland,M. Hartz,K. Martens,B. Quilain,C. Simpson,Yoshihiro Suzuki,M. R. Vagins,D. Hamabe,Masahiro Kuze,T. Yoshida,Masaki Ishitsuka,J. F. Martin,C. M. Nantais,P. de Perio,H.A. Tanaka,A. Konaka,Song Chen,L. Wan,Y. M. Zhang,R. J. Wilkes,A. Minamino +179 more
TL;DR: In this article, an analysis of atmospheric neutrino data from all four run periods of Super-Kamiokande optimized for the sensitivity of neutrinos to the mass hierarchy is presented.