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Showing papers by "Tsuyoshi Nakaya published in 2012"


Journal ArticleDOI
K. Bays1, T. Iida2, K. Abe2, Y. Hayato2, K. Iyogi2, J. Kameda2, Yusuke Koshio2, L. Marti2, M. Miura2, S. Moriyama2, Masayuki Nakahata2, S. Nakayama2, Y. Obayashi2, Hiroyuki Sekiya2, Masato Shiozawa2, Yoshihiro Suzuki2, Atsushi Takeda2, Y. Takenaga2, Koh Ueno2, K. Ueshima2, S. Yamada2, T. Yokozawa2, H. Kaji2, Takaaki Kajita2, K. Kaneyuki2, T. McLachlan2, Ko Okumura2, K. P. Lee2, K. Martens2, M. R. Vagins2, M. R. Vagins1, L. Labarga3, E. Kearns4, E. Kearns2, Michael Litos4, J. L. Raaf4, J. L. Stone2, J. L. Stone4, L. R. Sulak4, W. R. Kropp1, S. Mine1, C. Regis1, A. L. Renshaw1, M. B. Smy2, M. B. Smy1, H. W. Sobel1, H. W. Sobel2, K. S. Ganezer5, John Hill5, W. E. Keig5, Sunghoon Cho6, J. S. Jang6, J. Y. Kim6, I. T. Lim6, Justin Albert7, Kate Scholberg2, Kate Scholberg7, C. W. Walter7, C. W. Walter2, R. A. Wendell7, T. Wongjirad7, T. Ishizuka8, Shigeki Tasaka9, J. G. Learned, S. Matsuno, S. N. Smith, Takehisa Hasegawa, T. Ishida, T. Ishii, T. Kobayashi, T. Nakadaira, Koji Nakamura2, K. Nishikawa, Yuichi Oyama, K. Sakashita, T. Sekiguchi, T. Tsukamoto, A. T. Suzuki10, Y. Takeuchi10, Y. Takeuchi2, M. Ikeda11, Kodai Matsuoka11, A. Minamino11, A. Murakami11, Tsuyoshi Nakaya11, Tsuyoshi Nakaya2, Y. Fukuda12, Yoshitaka Itow13, G. Mitsuka13, M. Miyake13, T. Tanaka13, Joshua Hignight14, J. Imber14, C. K. Jung14, I. Taylor14, C. Yanagisawa14, A. Kibayashi15, Hirokazu Ishino, S. Mino15, Makoto Sakuda15, Takaaki Mori15, H. Toyota15, Y. Kuno16, S. B. Kim17, B. S. Yang17, H. Okazawa18, Y. Choi19, K. Nishijima20, M. Koshiba2, Y. Totsuka2, Masashi Yokoyama2, Y. Heng21, Song Chen21, Haoxiong Zhang21, Zishuo Yang21, P. Mijakowski22, K. Connolly23, M. Dziomba23, R. J. Wilkes23 
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.
Abstract: A new Super-Kamiokande search for supernova relic neutrinos was conducted using 2853 live days of data. Sensitivity is now greatly improved compared to the 2003 Super-Kamiokande result, which placed a flux limit near many theoretical predictions. This more detailed analysis includes a variety of improvements such as increased efficiency, a lower energy threshold, and an expanded data set. New combined upper limits on supernova relic neutrino flux are between 2.8 and $3.1{\overline{\ensuremath{ u}}}_{e}\text{ }\text{ }{\mathrm{cm}}^{\ensuremath{-}2}\text{ }{\mathrm{s}}^{\ensuremath{-}1}g16\text{ }\text{ }\mathrm{MeV}$ total positron energy (17.3 MeV ${\mathrm{E}}_{\ensuremath{ u}}$).

203 citations


Journal ArticleDOI
K. Abe1, N. Abgrall2, Yasuo Ajima, Hiroaki Aihara1  +457 moreInstitutions (57)
TL;DR: In this article, the authors reported a measurement of muon-neutrino disappearance in the T2K experiment, which is the first implementation of the off-axis technique in a long-baseline neutrino oscillation experiment.
Abstract: We report a measurement of muon-neutrino disappearance in the T2K experiment. The 295-km muon-neutrino beam from Tokai to Kamioka is the first implementation of the off-axis technique in a long-baseline neutrino oscillation experiment. With data corresponding to 1.43 x 10(20) protons on target, we observe 31 fully-contained single mu-like ring events in Super-Kamiokande, compared with an expectation of 104 +/- 14 (syst) events without neutrino oscillations. The best-fit point for two-flavor nu(mu) -> nu(tau) oscillations is sin(2)(2 theta(23)) = 0.98 and vertical bar Delta m(32)(2)vertical bar = 2.65 x 10(-3) eV(2). The boundary of the 90% confidence region includes the points sin(2)(2 theta(23)), vertical bar Delta m(32)(2)vertical bar = (1.0, 3.1 x 10(-3) eV(2)), (0.84, 2.65 x 10(-3) eV(2)) and (1.0, 2.2 x 10(-3) eV(2)).

112 citations


Journal ArticleDOI
Kendall Mahn1, Yasuhiro Nakajima2, Alexis A. Aguilar-Arevalo3, J. L. Alcaraz-Aunion4, C. E. Anderson5, A. O. Bazarko6, S. J. Brice7, B. C. Brown7, L. Bugel8, Jun Cao9, J. Catala-Perez10, G. Cheng1, L. Coney1, Janet Conrad8, D. C. Cox11, A. Curioni5, R. Dharmapalan12, Zelimir Djurcic13, U. Dore14, D. A. Finley7, B. T. Fleming5, R. Ford7, A. J. Franke1, F. G. Garcia7, G. T. Garvey15, C. Giganti14, J.J. Gómez-Cadenas10, J. Grange16, C. Green15, C. Green11, J. A. Green15, P. Guzowski17, Andrew J. Hanson11, T. L. Hart18, E. Hawker15, Y. Hayato19, Katsuki Hiraide2, W. Huelsnitz15, R. Imlay20, R. A. Johnson21, B. J. P. Jones8, G. Jover-Manas4, G. Karagiorgi1, P. H. Kasper7, Teppei Katori8, Teppei Katori11, Y. Kobayashi22, T. Kobilarcik7, I. Kourbanis7, S. Koutsoliotas23, Hidetoshi Kubo2, Y. Kurimoto2, E. M. Laird6, S. K. Linden5, J. M. Link24, Y. L. Liu9, W. C. Louis15, P. F. Loverre14, L. Ludovici14, C. Mariani1, W. Marsh7, S. Masuike22, Kodai Matsuoka2, C. Mauger15, V. T. McGary8, G. McGregor15, W. Metcalf20, P. D. Meyers6, F. Mills7, G. B. Mills15, G. Mitsuka19, Y. Miyachi22, S. Mizugashira22, Jocelyn Monroe1, C. D. Moore7, J. Mousseau16, Tsuyoshi Nakaya2, R. Napora25, R. H. Nelson18, P. Nienaber26, J. A. Nowak20, D. Orme2, B. Osmanov16, Minoru Otani2, S. Ouedraogo20, R. B. Patterson6, Z. Pavlovic15, D. Perevalov12, C. C. Polly7, E.J. Prebys7, J. L. Raaf21, H. Ray16, H. Ray15, B. P. Roe9, A. D. Russell7, Federico Sanchez4, V. D. Sandberg15, R. Schirato15, D. W. Schmitz1, M. H. Shaevitz1, T. A. Shibata22, F. C. Shoemaker6, David Smith27, M. Soderberg5, M. Sorel10, Panagiotis Spentzouris7, J. Spitz5, I. Stancu12, R. J. Stefanski7, M. Sung20, H. Takei22, H. A. Tanaka6, H. K. Tanaka8, M. Tanaka, Rex Tayloe11, I. J. Taylor17, R. J. Tesarek7, M. Tzanov18, Y. Uchida17, R. G. Van de Water15, J. J. Walding17, M. O. Wascko17, D. H. White15, H. B. White7, M. J. Wilking18, Masashi Yokoyama2, H. J. Yang9, G. P. Zeller7, E. D. Zimmerman18 
TL;DR: In this paper, the results of a νμ disappearance search in the Δ am2 region of 0.5-40 eV2 Δm2 were reported, with an improvement over previous experimental constraints between 10 and 30 eV 2.
Abstract: The SciBooNE and MiniBooNE collaborations report the results of a νμ disappearance search in the Δ'm2 region of 0.5-40 eV2. The neutrino rate as measured by the SciBooNE tracking detectors is used to constrain the rate at the MiniBooNE Cherenkov detector in the first joint analysis of data from both collaborations. Two separate analyses of the combined data samples set 90% confidence level (CL) limits on νμ disappearance in the 0.5-40 eV2 Δm2 region, with an improvement over previous experimental constraints between 10 and 30 eV2

104 citations


Journal ArticleDOI
K. Abe1, N. Abgrall2, Yasuo Ajima, Hiroaki Aihara1  +435 moreInstitutions (54)
TL;DR: The Interactive Neutrino GRID (INGRID) is an on-axis near detector for the T2K long baseline neutrino oscillation experiment.
Abstract: Precise measurement of neutrino beam direction and intensity was achieved based on a new concept with modularized neutrino detectors. INGRID (Interactive Neutrino GRID) is an on-axis near detector for the T2K long baseline neutrino oscillation experiment. INGRID consists of 16 identical modules arranged in horizontal and vertical arrays around the beam center. The module has a sandwich structure of iron target plates and scintillator trackers. INGRID directly monitors the muon neutrino beam profile center and intensity using the number of observed neutrino events in each module. The neutrino beam direction is measured with accuracy better than 0.4 mrad from the measured profile center. The normalized event rate is measured with 4% precision.

104 citations


Journal ArticleDOI
H. Nishino1, H. Nishino2, K. Abe2, Y. Hayato2, T. Iida2, M. Ikeda2, J. Kameda2, Yusuke Koshio2, M. Miura2, S. Moriyama2, Masayuki Nakahata2, S. Nakayama2, Y. Obayashi2, Hiroyuki Sekiya2, Masato Shiozawa2, Yasunari Suzuki2, Atsushi Takeda2, Y. Takenaga2, Y. Takeuchi2, Koh Ueno2, K. Ueshima, Hiroshi Watanabe, S. Yamada2, S. Hazama2, I. Higuchi2, C. Ishihara2, H. Kaji2, Takaaki Kajita2, K. Kaneyuki2, G. Mitsuka2, Ko Okumura2, N. Tanimoto2, Frédéric Dufour3, E. Kearns3, E. Kearns2, Michael Litos3, J. L. Raaf3, J. L. Stone2, J. L. Stone3, L. R. Sulak3, M. Goldhaber4, K. Bays5, J. P. Cravens5, W. R. Kropp5, S. Mine5, C. Regis5, M. B. Smy5, M. B. Smy2, H. W. Sobel5, H. W. Sobel2, K. S. Ganezer6, John Hill6, W. E. Keig6, J. S. Jang7, J. Y. Kim7, I. T. Lim7, Justin Albert8, Kate Scholberg8, Kate Scholberg2, C. W. Walter8, C. W. Walter2, R. A. Wendell8, T. Ishizuka9, Shigeki Tasaka10, J. G. Learned, S. Matsuno, Y. Watanabe11, Takehisa Hasegawa, T. Ishida, T. Ishii, T. Kobayashi, T. Nakadaira, K. Nakamura2, K. Nishikawa, Yuichi Oyama, K. Sakashita, T. Sekiguchi, T. Tsukamoto, A. T. Suzuki12, A. Minamino13, Tsuyoshi Nakaya2, Tsuyoshi Nakaya13, Masashi Yokoyama13, Y. Fukuda14, Yoshitaka Itow15, Tetsuya S. Tanaka15, C. K. Jung16, G. D. Lopez16, C. McGrew16, C. Yanagisawa16, N. Tamura17, Y. Idehara18, Makoto Sakuda18, Y. Kuno19, Minoru Yoshida19, S. B. Kim20, B. S. Yang20, H. Okazawa21, Y. Choi22, H. Seo22, Y. Furuse23, K. Nishijima23, Y. Yokosawa23, M. Koshiba2, Y. Totsuka2, M. R. Vagins5, M. R. Vagins2, Shaomin Chen24, Y. Heng24, J. Liu24, Zishuo Yang24, Haoxiong Zhang24, D. Kielczewska25, K. Connolly26, E. Thrane26, R. J. Wilkes26 
TL;DR: In this paper, lower limits on the nucleon partial lifetime at 90% confidence level were obtained, ranging from $3.6 to $8.2, depending on the decay modes.
Abstract: Searches for a nucleon decay into a charged antilepton (${e}^{+}$ or ${\ensuremath{\mu}}^{+}$) plus a light meson (${\ensuremath{\pi}}^{0}$, ${\ensuremath{\pi}}^{\ensuremath{-}}$, $\ensuremath{\eta}$, ${\ensuremath{\rho}}^{0}$, ${\ensuremath{\rho}}^{\ensuremath{-}}$, $\ensuremath{\omega}$) were performed using the Super-Kamiokande I and II data. Twelve nucleon decay modes were searched for. The total exposure is $140.9\text{ }\text{ }\mathrm{kiloton}\ifmmode\cdot\else\textperiodcentered\fi{}\mathrm{years}$, which includes a $91.7\text{ }\text{ }\mathrm{kiloton}\ifmmode\cdot\else\textperiodcentered\fi{}\mathrm{year}$ exposure (1489.2 live days) of Super-Kamiokande-I and a $49.2\text{ }\text{ }\mathrm{kiloton}\ifmmode\cdot\else\textperiodcentered\fi{}\mathrm{year}$ exposure (798.6 live days) of Super-Kamiokande II. The number of candidate events in the data was consistent with the atmospheric neutrino background expectation. No significant evidence for a nucleon decay was observed in the data. Thus, lower limits on the nucleon partial lifetime at 90% confidence level were obtained. The limits range from $3.6\ifmmode\times\else\texttimes\fi{}{10}^{31}$ to $8.2\ifmmode\times\else\texttimes\fi{}{10}^{33}\text{ }\text{ }\mathrm{years}$, depending on the decay modes.

76 citations


Journal ArticleDOI
C. Regis1, K. Abe2, Y. Hayato2, K. Iyogi2, J. Kameda2, Yusuke Koshio2, Ll. Marti2, M. Miura2, S. Moriyama2, Masayuki Nakahata2, S. Nakayama2, Y. Obayashi2, Hiroyuki Sekiya2, Masato Shiozawa2, Yasunari Suzuki2, Atsushi Takeda2, Y. Takenaga2, Koh Ueno2, T. Yokozawa2, H. Kaji2, Takaaki Kajita2, K. Kaneyuki2, K. P. Lee2, Ko Okumura2, T. McLachlan2, L. Labarga3, E. Kearns2, E. Kearns4, J. L. Raaf4, J. L. Stone4, J. L. Stone2, L. R. Sulak4, M. Goldhaber5, K. Bays1, G. Carminati1, W. R. Kropp1, S. Mine1, A. L. Renshaw1, M. B. Smy2, M. B. Smy1, H. W. Sobel2, H. W. Sobel1, K. S. Ganezer6, John Hill6, W. E. Keig6, J. S. Jang7, J. S. Jang8, J. Y. Kim7, I. T. Lim7, Justin Albert9, Kate Scholberg2, Kate Scholberg9, C. W. Walter2, C. W. Walter9, R. A. Wendell9, T. Wongjirad9, T. Ishizuka10, Shigeki Tasaka11, J. G. Learned, S. Matsuno, S. N. Smith, Takehisa Hasegawa, T. Ishida, T. Ishii, T. Kobayashi, T. Nakadaira, K. Nakamura2, K. Nishikawa, Yuichi Oyama, K. Sakashita, T. Sekiguchi, T. Tsukamoto, A. T. Suzuki12, Y. Takeuchi12, Y. Takeuchi2, K. Ieki13, M. Ikeda13, Hidetoshi Kubo13, A. Minamino13, A. Murakami13, Tsuyoshi Nakaya2, Tsuyoshi Nakaya13, Y. Fukuda14, K. Choi15, Yoshitaka Itow15, G. Mitsuka15, M. Miyake15, P. Mijakowski, Joshua Hignight16, J. Imber16, C. K. Jung16, I. Taylor16, C. Yanagisawa16, Hirokazu Ishino17, A. Kibayashi17, Takaaki Mori17, Makoto Sakuda17, J. Takeuchi17, Y. Kuno18, S. B. Kim19, H. Okazawa20, Y. Choi21, K. Nishijima22, M. Koshiba2, Y. Totsuka2, Masashi Yokoyama2, K. Martens2, M. R. Vagins2, M. R. Vagins1, Song Chen23, H. Sui23, Zishuo Yang23, Haoxiong Zhang23, K. Connolly24, M. Dziomba24, R. J. Wilkes24 
TL;DR: In this article, a lower bound of $1.6 was established for the probability of proton decay in this mode at the 90% confidence level, and the number of candidate events in the data was consistent with the atmospheric neutrino background expectation.
Abstract: We have searched for proton decay via $p\ensuremath{\rightarrow}{\ensuremath{\mu}}^{+}{K}^{0}$ using data from a $91.7\text{ }\text{ }\mathrm{kiloton}\ifmmode\cdot\else\textperiodcentered\fi{}\mathrm{year}$ exposure of Super-Kamiokande- I, a $49.2\text{ }\text{ }\mathrm{kiloton}\ifmmode\cdot\else\textperiodcentered\fi{}\mathrm{year}$ exposure of Super-Kamiokande II, and a $31.9\text{ }\text{ }\mathrm{kiloton}\ifmmode\cdot\else\textperiodcentered\fi{}\mathrm{year}$ exposure of Super-Kamiokande III. The number of candidate events in the data was consistent with the atmospheric neutrino background expectation and no evidence for proton decay in this mode was found. We set a partial lifetime lower limit of $1.6\ifmmode\times\else\texttimes\fi{}{10}^{33}\text{ }\text{ }\mathrm{years}$ at the 90% confidence level.

40 citations


Journal ArticleDOI
Koh Ueno1, K. Abe1, Y. Hayato1, T. Iida1, K. Iyogi1, J. Kameda1, Yusuke Koshio1, Y. Kozuma1, M. Miura1, S. Moriyama1, Masayuki Nakahata1, S. Nakayama1, Y. Obayashi1, Hiroyuki Sekiya1, Masato Shiozawa1, Yasunari Suzuki1, Atsushi Takeda1, Y. Takenaga1, K. Ueshima1, S. Yamada1, T. Yokozawa1, K. Martens2, J. Schuemann2, M. Vagins2, C. Ishihara1, H. Kaji1, Takaaki Kajita1, K. Kaneyuki1, T. McLachlan1, Ko Okumura1, Y. Shimizu1, N. Tanimoto1, E. Kearns3, Michael Litos3, J. L. Raaf3, J. L. Stone3, L. R. Sulak3, K. Bays4, W. R. Kropp4, S. Mine4, C. Regis4, A. L. Renshaw4, M. B. Smy4, H. W. Sobel4, K. S. Ganezer5, John Hill5, W. E. Keig5, J. S. Jang6, J. Y. Kim6, I. T. Lim6, Justin Albert7, Kate Scholberg7, C. W. Walter7, R. A. Wendell7, T. Wongjirad7, T. Ishizuka8, Shigeki Tasaka9, J. G. Learned10, S. Matsuno10, T. Hasegawa11, T. Ishida11, T. Ishii11, T. Kobayashi11, T. Nakadaira11, K. Nakamura11, K. Nishikawa11, Yuichi Oyama11, K. Sakashita11, T. Sekiguchi11, T. Tsukamoto11, A. T. Suzuki12, Y. Takeuchi12, M. Ikeda13, A. Minamino13, Tsuyoshi Nakaya13, L. Labarga, Ll. Marti, Y. Fukuda14, Yoshitaka Itow15, G. Mitsuka15, T. Tanaka15, C. K. Jung16, G. Lopez16, I. Taylor16, C. Yanagisawa16, Hirokazu Ishino17, A. Kibayashi17, S. Mino17, Takaaki Mori17, Makoto Sakuda17, H. Toyota17, Y. Kuno18, Minoru Yoshida18, S. B. Kim19, B. S. Yang19, H. Okazawa20, Y. Choi21, K. Nishijima22, M. Koshiba1, Y. Totsuka1, Masashi Yokoyama1, Song Chen23, Y. Heng23, Zishuo Yang23, Haoxiong Zhang23, D. Kielczewska24, P. Mijakowski24, K. Connolly25, M. Dziomba25, E. Thrane25, R. J. Wilkes25 
TL;DR: In this article, a search for low energy neutrinos in the electron total energy range from 19 to 55 MeV was carried out with SK and gave a monopole flux limit of F M ( σ 0 / 1 mb ) 6.3 × 10 - 24 ( β M / 10 - 3 ) 2 cm - 2 s - 1 sr - 1 at 90% C.L.

35 citations


Journal ArticleDOI
TL;DR: In this paper, the authors search for proton decay in muon plus neutral kaon using data from a 917 kiloton-year exposure of Super-Kamiokande-I, a 492 kiloton year exposure of Kamiokende-II, and a 319 kiloton years exposure of SKI-III and set a partial lifetime lower limit of 16x10^33 years at the 90% confidence level.
Abstract: We have searched for proton into muon plus neutral kaon using data from a 917 kiloton-year exposure of Super-Kamiokande-I, a 492 kiloton-year exposure of Super-Kamiokande-II, and a 319 kiloton-year exposure of Super-Kamiokande-III The number of candidate events in the data was consistent with the atmospheric neutrino background expectation and no evidence for proton decay in this mode was found We set a partial lifetime lower limit of 16x10^33 years at the 90% confidence level

16 citations