S
S. Mino
Researcher at Okayama University
Publications - 8
Citations - 1201
S. Mino is an academic researcher from Okayama University. The author has contributed to research in topics: Neutrino & Super-Kamiokande. The author has an hindex of 8, co-authored 8 publications receiving 1078 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
Atmospheric neutrino oscillation analysis with subleading effects in Super-Kamiokande I, II, and III
R. A. Wendell,C. Ishihara,K. Abe,Y. Hayato,T. Iida,M. Ikeda,K. Iyogi,J. Kameda,Ken-ichiro Kobayashi,Yusuke Koshio,Y. Kozuma,M. Miura,Shigetaka Moriyama,Masayuki Nakahata,Shoei Nakayama,Y. Obayashi,H. Ogawa,Hiroyuki Sekiya,Masato Shiozawa,Yasunari Suzuki,Atsushi Takeda,Y. Takenaga,Y. Takeuchi,Koh Ueno,K. Ueshima,Hiroshi Watanabe,S. Yamada,Tsutomu Yokozawa,S. Hazama,H. Kaji,Takaaki Kajita,K. Kaneyuki,T. McLachlan,Ko Okumura,Yasuhiro Shimizu,N. Tanimoto,Mark R. Vagins,Mark R. Vagins,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,Michael B. Smy,Michael 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,M. Fechner,Kate Scholberg,Kate Scholberg,C. W. Walter,C. W. Walter,S. Tasaka,J. G. Learned,S. Matsuno,Y. Watanabe,Takehisa Hasegawa,T. Ishida,T. Ishii,T. Kobayashi,T. Nakadaira,K. Nakamura,K. Nishikawa,H. Nishino,Yuichi Oyama,K. Sakashita,T. Sekiguchi,T. Tsukamoto,Atsumu Suzuki,A. Minamino,Tsuyoshi Nakaya,Tsuyoshi Nakaya,Y. Fukuda,Yoshitaka Itow,G. Mitsuka,Toshiyuki Tanaka,C. K. Jung,G. D. Lopez,C. McGrew,C. Yanagisawa,N. Tamura,Hirokazu Ishino,A. Kibayashi,S. Mino,T. Mori,Makoto Sakuda,H. Toyota,Y. Kuno,Minoru Yoshida,S. B. Kim,B. S. Yang,T. Ishizuka,H. Okazawa,Y. Choi,Kyoshi Nishijima,Y. Yokosawa,Masatoshi Koshiba,Masashi Yokoyama,Y. Totsuka,Song Chen,Y. Heng,Zishuo Yang,Huaqiao Zhang,D. Kielczewska,P. Mijakowski,K. Connolly,M. Dziomba,E. Thrane,E. Thrane,R. J. Wilkes +128 more
TL;DR: In this article, a search for nonzero {theta}{sub 13} and deviations of sin{sup 2{theta}}{sub 23} from 0.04(0.09) and 1.9(1.5) was conducted.
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
Evidence for the appearance of atmospheric tau neutrinos in super-Kamiokande
K. Abe,Y. Hayato,T. Iida,K. Iyogi,J. Kameda,Yusuke Koshio,Y. Kozuma,Ll. Marti,M. Miura,S. Moriyama,Masayuki Nakahata,S. Nakayama,Y. Obayashi,Hiroyuki Sekiya,Masato Shiozawa,Yasunari Suzuki,Atsushi Takeda,Y. Takenaga,Koh Ueno,K. Ueshima,S. Yamada,T. Yokozawa,C. Ishihara,H. Kaji,Takaaki Kajita,K. Kaneyuki,K. P. Lee,T. McLachlan,Ko Okumura,Y. Shimizu,N. Tanimoto,L. Labarga,E. Kearns,E. Kearns,Michael Litos,J. L. Raaf,J. L. Stone,J. L. Stone,L. R. Sulak,M. Goldhaber,K. Bays,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,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,K. Nakamura,K. Nishikawa,Yuichi Oyama,K. Sakashita,T. Sekiguchi,T. Tsukamoto,A. T. Suzuki,Y. Takeuchi,Y. Takeuchi,M. Ikeda,A. Minamino,Tsuyoshi Nakaya,Tsuyoshi Nakaya,Y. Fukuda,Yoshitaka Itow,G. Mitsuka,Tetsuya S. Tanaka,C. K. Jung,G. D. Lopez,I. Taylor,C. Yanagisawa,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,M. Koshiba,Masashi Yokoyama,Y. Totsuka,K. Martens,Jan Schuemann,M. R. Vagins,M. R. Vagins,Song Chen,Y. Heng,Zishuo Yang,Haoxiong Zhang,D. Kielczewska,P. Mijakowski,K. Connolly,M. Dziomba,E. Thrane,R. J. Wilkes +122 more
TL;DR: Super-Kamiokande atmospheric neutrino data were fit with an unbinned maximum likelihood method to search for the appearance of tau leptons resulting from the interactions of oscillation-generated tau neutrinos in the detector, finding a low tau normalization.
Journal ArticleDOI
Search for differences in oscillation parameters for atmospheric neutrinos and antineutrinos at Super-Kamiokande.
K. Abe,Yoshinari Hayato,T. Iida,M. Ikeda,K. Iyogi,J. Kameda,Yusuke Koshio,Y. Kozuma,M. Miura,S. Moriyama,Masayuki Nakahata,S. Nakayama,Y. Obayashi,Hiroyuki Sekiya,Masato Shiozawa,Yoshihiro Suzuki,Atsushi Takeda,Y. Takenaga,Y. Takeuchi,Y. Takeuchi,Koh Ueno,K. Ueshima,Hiroshi Watanabe,S. Yamada,T. Yokozawa,C. Ishihara,H. Kaji,K. P. Lee,Takaaki Kajita,K. Kaneyuki,T. McLachlan,Kimihiro Okumura,Y. Shimizu,N. Tanimoto,K. Martens,M. Vagins,M. 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,M. Goldhaber,K. Bays,W. R. Kropp,S. Mine,C. Regis,M. B. Smy,M. B. Smy,Henry W. Sobel,Henry W. Sobel,K. S. Ganezer,John Hill,W. E. Keig,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,Shigeki Tasaka,J. G. Learned,S. Matsuno,T. Hasegawa,T. Ishida,T. Ishii,Takashi Kobayashi,T. Nakadaira,Koji Nakamura,K. Nishikawa,H. Nishino,Yuichi Oyama,K. Sakashita,T. Sekiguchi,T. Tsukamoto,A. Suzuki,A. Minamino,Tsuyoshi Nakaya,Tsuyoshi Nakaya,Y. Fukuda,Yoshitaka Itow,G. Mitsuka,T. Tanaka,C. K. Jung,I. Taylor,C. Yanagisawa,Hirokazu Ishino,A. Kibayashi,S. Mino,Takaaki Mori,Makoto Sakuda,H. Toyota,Y. Kuno,Soo-Bong Kim,B. S. Yang,T. Ishizuka,H. Okazawa,Y. Choi,K. Nishijima,M. Koshiba,Masashi Yokoyama,Y. Totsuka,Song Chen,Y. Heng,Zishuo Yang,Haoxiong Zhang,D. Kielczewska,P. Mijakowski,K. Connolly,M. Dziomba,R. J. Wilkes +119 more
TL;DR: Best-fit antineutrino mixing is found to be at (Δm2,sin2 2θ)=(2.0×10(-3) eV2, 1.0) and is consistent with the overall Super-K measurement.