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Showing papers by "K. Nishikawa 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. Smy1, M. B. Smy2, H. W. Sobel2, H. W. Sobel1, K. S. Ganezer5, John Hill5, W. E. Keig5, Sunghoon Cho6, J. S. Jang6, J. Y. Kim6, I. T. Lim6, Justin Albert7, Kate Scholberg7, Kate Scholberg2, C. W. Walter2, C. W. Walter7, 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 Nakaya2, Tsuyoshi Nakaya11, 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
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
N. Abgrall1, Antoni Aduszkiewicz2, T. Antičić, N. G. Antoniou3, J. Argyriades1, B. Baatar4, A. Blondel1, J. Blümer5, M. Bogusz6, Laszlo Boldizsar7, A. Bravar1, William Brooks8, J. Brzychczyk9, A. Bubak10, S.A. Bunyatov4, O. Busygina, T. Cetner6, K. U. Choi11, P. Christakoglou3, T. Czopowicz6, N. Davis3, Fotis K. Diakonos3, S. Di Luise12, W. Dominik2, J. Dumarchez13, Ralph Engel5, Antonio Ereditato14, Luigi Salvatore Esposito12, G. A. Feofilov15, Z. Fodor16, A. Ferrero1, Ágnes Fülöp7, X. Garrido5, Marek Gaździcki17, Marek Gaździcki18, M.B. Golubeva, Katarzyna Grebieszkow6, A. Grzeszczuk10, F.F. Guber, A. Haesler1, H. Hakobyan8, T. Hasegawa, R. Idczak19, Y. Ivanov8, A. Ivashkin, Kreso Kadija, A. Kapoyannis3, N. Katrynska19, D. Kielczewska2, D. P. Kikola6, J. H. Kim11, M. Kirejczyk2, J. Kisiel10, Takashi Kobayashi, O. Kochebina15, V. I. Kolesnikov4, D. Kolev2, V. P. Kondratiev15, A. Korzenev1, S. Kowalski10, Alexey Krasnoperov4, Sergey Kuleshov8, Alexey Kurepin, R. Lacey20, J. Lagoda, Andras Laszlo7, V. V. Lyubushkin4, M. Maćkowiak-Pawłowska6, Z. Majka9, Alexander Malakhov4, A. Marchionni12, A. Marcinek9, Ioana Codrina Maris5, Vincent Marin, T. Matulewicz2, Viktor Matveev4, G. L. Melkumov4, A. Meregaglia12, M. Messina14, St Mrówczyński18, S. Murphy1, T. Nakadaira, K. Nishikawa, T. Palczewski, G. Pálla7, Apostolos Panagiotou3, T. Paul5, W. Peryt6, O. Petukhov, R. Płaneta9, J. Pluta6, B. A. Popov4, M. Posiadala2, S. Puławski10, W. Rauch21, M. Ravonel1, Rainer Arno Ernst Renfordt17, Arnaud Robert13, Dieter Røhrich22, E. Rondio, Biagio Rossi14, M. Roth5, André Rubbia12, Maciej Rybczyński18, A. Sadovsky, Ken Sakashita, T. Sekiguchi, P. Seyboth18, M. Shibata, E. Skrzypczak2, M. Słodkowski6, P. Staszel9, G. Stefanek18, J. Stepaniak, C. Strabel12, H. Ströbele17, T. Susa, P. Szaflik10, M. Szuba5, M. Tada, A. Taranenko20, V. Tereshchenko4, R. Tsenov2, Ludwik Turko19, R. Ulrich5, M. Unger5, M. Vassiliou3, Darko Veberič5, Vladimir Vechernin15, Gyorgy Vesztergombi7, A. Wilczek10, Zbigniew Wlodarczyk18, A. Wojtaszek-Szwarc18, J. Yi11, I. K. Yoo11, L. Zambelli13, W. Zipper10 
TL;DR: In this paper, a graphite target with a thickness of 4% of a nuclear interaction length was used to measure positively charged kaons in p+C interactions at 31 GeV/c.
Abstract: Spectra of positively charged kaons in p+C interactions at 31 GeV/c were measured with the NA61/SHINE spectrometer at the CERN SPS. The analysis is based on the full set of data collected in 2007 with a graphite target with a thickness of 4% of a nuclear interaction length. Interaction cross sections and charged pion spectra were already measured using the same set of data. These new measurements in combination with the published ones are required to improve predictions of the neutrino flux for the T2K long baseline neutrino oscillation experiment in Japan. In particular, the knowledge of kaon production is crucial for precisely predicting the intrinsic electron neutrino component and the high energy tail of the T2K beam. The results are presented as a function of laboratory momentum in 2 intervals of the laboratory polar angle covering the range from 20 up to 240 mrad. The kaon spectra are compared with predictions of several hadron production models. Using the published pion results and the new kaon data, the K+/\pi+ ratios are computed.

98 citations


Journal ArticleDOI
H. Nishino1, H. Nishino2, K. Abe1, Y. Hayato1, T. Iida1, M. Ikeda1, J. Kameda1, Yusuke Koshio1, M. Miura1, S. Moriyama1, Masayuki Nakahata1, S. Nakayama1, Y. Obayashi1, Hiroyuki Sekiya1, Masato Shiozawa1, Yasunari Suzuki1, Atsushi Takeda1, Y. Takenaga1, Y. Takeuchi1, Koh Ueno1, K. Ueshima, Hiroshi Watanabe, S. Yamada1, S. Hazama1, I. Higuchi1, C. Ishihara1, H. Kaji1, Takaaki Kajita1, K. Kaneyuki1, G. Mitsuka1, Ko Okumura1, N. Tanimoto1, Frédéric Dufour3, E. Kearns3, E. Kearns1, Michael Litos3, J. L. Raaf3, J. L. Stone3, J. L. Stone1, L. R. Sulak3, M. Goldhaber4, K. Bays5, J. P. Cravens5, W. R. Kropp5, S. Mine5, C. Regis5, M. B. Smy1, M. B. Smy5, H. W. Sobel5, H. W. Sobel1, K. S. Ganezer6, John Hill6, W. E. Keig6, J. S. Jang7, J. Y. Kim7, I. T. Lim7, Justin Albert8, Kate Scholberg1, Kate Scholberg8, C. W. Walter8, C. W. Walter1, 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. Nakamura1, K. Nishikawa, Yuichi Oyama, K. Sakashita, T. Sekiguchi, T. Tsukamoto, A. T. Suzuki12, A. Minamino13, Tsuyoshi Nakaya1, 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. Koshiba1, Y. Totsuka1, M. R. Vagins1, M. R. Vagins5, 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. Smy1, M. B. Smy2, H. W. Sobel1, H. W. Sobel2, K. S. Ganezer6, John Hill6, W. E. Keig6, J. S. Jang7, J. S. Jang8, J. Y. Kim8, I. T. Lim8, 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. Takeuchi2, Y. Takeuchi12, 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. Vagins1, M. R. Vagins2, 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


ReportDOI
25 Jun 2012
TL;DR: Within the three-flavor mixing framework, there are three mixing angles (!!",!!",!!"), two independent mass splittings characterized by Δ!!"! and Δ!"!.
Abstract: Neutrino oscillations have been firmly established by experiments that measure solar neutrinos, atmospheric neutrinos, reactor antineutrinos, and accelerator-produced neutrinos and antineutrinos. To a first approximation, three-flavor mixing provides a good description of the neutrino oscillation phenomenology. Within the three-flavor mixing framework there are three mixing angles (!!", !!", !!"), two independent mass splittings characterized by Δ!!" ! and Δ!!" !

3 citations


Posted Content
TL;DR: In this article, a liquid Argon TPC detector with fiducial mass of 150 kg was constructed as part of the R&D program of the next generation neutrino and nucleon decay detector.
Abstract: We have constructed a liquid Argon TPC detector with fiducial mass of 150 kg as a part of the R&D program of the next generation neutrino and nucleon decay detector. This paper describes a study of particle identification performance of the detector using well-defined charged particles (pions, kaons, and protons) with momentum of ~800 MeV/$c$ obtained at J-PARC K1.1BR beamline.

1 citations