Search

Your search keyword '"M. Dziomba"' showing total 4 results
Start Over Author "M. Dziomba" Journal physical review d
4 results on '"M. Dziomba"'

1. Search for proton decay viap→νK+using260 kiloton·yeardata of Super-Kamiokande

Author

Shigeki Tasaka, E. Kearns, Y. Takeuchi, Masashi Yokoyama, K. Martens, S. Moriyama, M. Miyake, Yuichi Oyama, Masayuki Nakahata, T. Ishizuka, Tsuyoshi Nakaya, C. W. Walter, Takaaki Mori, Takaaki Kajita, K. Abe, A. T. Suzuki, K. P. Lee, K. S. Ganezer, J. L. Stone, L. Labarga, T. Kobayashi, T. Nakadaira, Makoto Sakuda, K. Sakashita, M. Dziomba, K. Choi, K. Ieki, T. Tsukamoto, Joshua Hignight, Yoshihiro Suzuki, Hiroyuki Sekiya, R. J. Wilkes, K. Iyogi, H. Kaji, H. W. Sobel, Y. Totsuka, J. Takeuchi, T. Wongjirad, I. Taylor, Y. Fukuda, H. Okazawa, T. Ishida, M. Goldhaber, C. Yanagisawa, S. B. Kim, J. Y. Kim, Song Chen, H. Sui, A. L. Renshaw, C. K. Jung, M. Ikeda, Masato Shiozawa, Y. Choi, Yoshitaka Itow, K. Nishijima, J. Kameda, J. Imber, T. Ishii, K. Connolly, Y. Hayato, Atsushi Takeda, P. Mijakowski, S. N. Smith, H. Zhang, S. Matsuno, R. A. Wendell, T. McLachlan, A. Kibayashi, Ll. Marti, John Hill, Yusuke Koshio, S. Nakayama, W. E. Keig, K. Kaneyuki, T. Sekiguchi, K. Bays, Justin Albert, Y. Kuno, J. S. Jang, T. Yokozawa, Y. Takenaga, M. Miura, J. L. Raaf, J. G. Learned, L. R. Sulak, M. B. Smy, Koh Ueno, Y. Obayashi, M. R. Vagins, W. R. Kropp, K. Nakamura, A. Murakami, G. Mitsuka, I. T. Lim, A. Minamino, K. Nishikawa, M. Koshiba, Ko Okumura, S. Mine, Takehisa Hasegawa, Hidetoshi Kubo, Hirokazu Ishino, Zishuo Yang, Kate Scholberg, and G. Carminati

Subjects
Physics, Nuclear physics, Nuclear and High Energy Physics, Particle physics, Proton, Proton decay, Super-Kamiokande, Lower limit
Abstract

We have searched for proton decay via p→νK+ using Super-Kamiokande data from April 1996 to February 2013, 260 kiloton•year exposure in total. No evidence for this proton decay mode is found. A lower limit of the proton lifetime is set to τ/B(p→νK+)>5.9×1033 years at 90% confidence level.

Published
2014
Full Text
View/download PDF

2. Publisher’s Note: T2K neutrino flux prediction [Phys. Rev. D87, 012001 (2013)]

Author

C. Bojechko, R. J. Wilson, R. Ohta, D. Ruterbories, M. Ieva, A. Himmel, R. Tacik, R. G. Calland, D. Gudin, C. Hearty, V. Galymov, A. Konaka, S. Short, W. H. Toki, A. K. Ichikawa, J. P. A. M. de André, P. Plonski, S. Roth, J. Kameda, E. S. Pinzon Guerra, Th. A. Mueller, Matthew T. Reeves, P. Mijakowski, T. Sekiguchi, J. Åmuda, B. E. Berger, D. Naples, P. Guzowski, K. Nishikawa, A. Hillairet, H. M. O'Keeffe, Kazuhiro Suzuki, C. W. Walter, E. Kearns, Masashi Yokoyama, E. Poplawska, M. Dziomba, H. Kakuno, L. Zambelli, Jan T. Sobczyk, K. Laihem, J. Caravaca Rodríguez, H.A. Tanaka, M. Ziembicki, J. Insler, E. Mazzucato, G. F. Pearce, K. Sakashita, S. M. Oser, M. Sorel, A. T. Suzuki, T. Tomura, P. Kitching, M. O. Wascko, M. Posiadala, M. G. Catanesi, Artur F. Izmaylov, M. Zito, K. Koseki, S. Mine, F. d. M. Blaszczyk, M. Murdoch, Y. Kanazawa, J. D. Perkin, Tsuyoshi Nakaya, J. M. Poutissou, C. Bronner, J. F. Martin, D. Autiero, S. Nakayama, R. A. Wendell, S. Yen, P. de Perio, T. Yano, Yoshikazu Yamada, B. Kirby, M. M. Tanaka, T. Nakadaira, S. Emery, F. Di Lodovico, M. Tada, I. Kreslo, D. J. Payne, K. Kowalik, Richard J.H. Smith, Koji Nakamura, André Rubbia, M. D. Haigh, Vincenzo Berardi, Tomoko Ariga, A. N. Khotjantsev, Akitaka Ariga, Ko Okumura, M. Y. Pac, Y. Seiya, E. L. Mathie, Yu. G. Kudenko, N. C. Hastings, Jan Kisiel, L. Monfregola, S. Manly, A. Cervera, Shigeki Aoki, Hiroyuki Sekiya, T. Akiri, T. Hasegawa, M. Ravonel, F. Bay, A. Clifton, S. Kumaratunga, T. Szeglowski, Hidetoshi Kubo, S. Giffin, Y. Fukuda, G. Vasseur, Ian Taylor, D. Cherdack, K. Nakajima, A. J. Finch, Kendall Mahn, P. Jonsson, L. Magaletti, C. Giganti, S. B. Boyd, M. M. Khabibullin, R. Sacco, Ke. Abe, E.D. Frank, R. A. Johnson, V. Matveev, T. Tsukamoto, G. Christodoulou, C. McGrew, M. J. Wilking, T. Ishida, O. Perevozchikov, Y. Hayato, C. Andreopoulos, P. Sinclair, B. Still, S. Moriyama, T. McLachlan, S. Murphy, T. Nakai, K. Mavrokoridis, D. R. Hadley, Masayuki Nakahata, B. Rossi, Masashi Tanaka, Jing Wang, E. Reinherz-Aronis, V. Paolone, Y. Uchida, M. Szeptycka, F. Retiere, V. Palladino, K. P. Lee, M. Day, A. Longhin, J. Marteau, C. Yanagisawa, Z. Williamson, E. Rondio, Michal Dziewiecki, Kazuhiro Yamamoto, E. Scantamburlo, K. Iyogi, L. Southwell, J. Myslik, Y. Takeuchi, R.P. Kurjata, S. W. Bentham, N. McCauley, T. Kajita, Minoru Otani, T. Kikawa, M. Gonin, L. Escudero, M. Lawe, E. D. Zimmerman, I. Z. Danko, T. Golan, M. B. Smy, H. W. Sobel, W. Oryszczak, S. A. Dytman, Koh Ueno, B. A. Popov, A. Curioni, Hiroaki Aihara, P. N. Ratoff, R. Terri, T. Kutter, K. Huang, C. Licciardi, R. Castillo, Yuichi Oyama, R. P. Litchfield, M. Friend, Yuki Fujii, Magdalena Malek, S. Di Luise, S. Assylbekov, B. Quilain, P. Stamoulis, E. Radicioni, S. J. Coleman, Marco Laveder, D. L. Wark, Kate Scholberg, P. Przewlocki, J. Steinmann, C. Touramanis, O. V. Mineev, A. Gaudin, Antonio Ereditato, N. Yershov, T. Hara, A. D. Marino, A. Blondel, J. Dumarchez, A. C. Weber, C. Nielsen, G. Kogan, Takashi Kobayashi, M. Barbi, J. Schwehr, G. De Rosa, M. Messina, Y. Nishimura, H. Kaji, Lester D.R. Thompson, R. A. Owen, C. A. Miller, A. Minamino, N. Grant, M. R. Vagins, G. Collazuol, Mark Scott, Scott Davis, J.J. Gómez-Cadenas, M. Macaire, D. Hansen, G. D. Lopez, Y. Shustrov, Justin Albert, N. Abgrall, C. Lister, M. Miura, S. J. Ives, T. Yuan, Jung-Hyun Kim, A. V. Waldron, T. Nagasaki, A. Zalewska, Federico Sanchez, A. Murakami, A. Bravar, C. Matsumura, I. T. Lim, J. Dobson, S. L. Cartwright, K. Connolly, Joshua Hignight, D. Terhorst, Yoshihiro Suzuki, Y. Totsuka, Susumu Takahashi, T. Wongjirad, T. Maruyama, M. Bass, J. H. Jo, F. Khanam, G.D. Barr, I. Karpikov, T. Ishii, D. Kielczewska, M. Batkiewicz, A. Dabrowska, M. Hartz, K. Ieki, D. Karlen, R. J. Wilkes, T. Lindner, Y. Obayashi, Janusz Marzec, M. A. M. Rayner, P. A. Rodrigues, T. Duboyski, Gareth J. Barker, Takahiro Hiraki, Dmitriy Beznosko, W. R. Kropp, James R. Wilson, S. Tobayama, J. P. Coleman, A. Laing, Kodai Matsuoka, G. Jover-Manas, S. Horikawa, T. Dealtry, A. Missert, J. Holeczek, K. Nakayoshi, N. Buchanan, R. L. Helmer, D. I. Scully, A. Thorley, A. Korzenev, Rhiju Das, B. Jamieson, C. J. Densham, K. Zaremba, D. G. Brook-Roberge, Atsushi Takeda, K. K. Joo, T. Wachala, T. Nicholls, B. C. Smith, Yusuke Koshio, M. Mezzetto, L. L. Kormos, C. Wilkinson, F. Dufour, Antonin Vacheret, K. S. McFarland, M. Tzanov, C. J. Metelko, R. Poutissou, P. Masliah, K. Gilje, A. Marchionni, S. B. Kim, J. Y. Kim, R. Sulej, Iain Alexander Bertram, J. Imber, M. Shibata, A. Hyndman, S. Berkman, C. K. Jung, M. Ikeda, Masato Shiozawa, L. Ludovici, A. Kilinski, A. Haesler, G. Wikström, S. Bhadra, S. Y. Suzuki, Luigi Salvatore Esposito, and J. Lagoda

Subjects
Nuclear physics, Physics, Nuclear and High Energy Physics, 010308 nuclear & particles physics, 0103 physical sciences, Monte Carlo method, Flux, Neutrino, Solar neutrino problem, 010306 general physics, 01 natural sciences
Published
2013
Full Text
View/download PDF

3. Search for proton decay viap→μ+K0in Super-Kamiokande I, II, and III

Author

M. Koshiba, J. S. Jang, Takaaki Mori, Ko Okumura, E. Kearns, K. Connolly, J. L. Stone, K. Choi, Y. Totsuka, K. P. Lee, J. G. Learned, Masashi Yokoyama, Yusuke Koshio, T. Wongjirad, Ke. Abe, H. W. Sobel, A. T. Suzuki, K. Iyogi, T. Tsukamoto, L. Labarga, H. Sui, T. Nakadaira, T. Ishizuka, Tsuyoshi Nakaya, W. R. Kropp, K. Nishijima, S. Mine, T. Kobayashi, Makoto Sakuda, T. Ishii, Shigeki Tasaka, K. Nishikawa, Song Chen, J. C. Hill, H. Zhang, C. K. Jung, T. Ishida, Y. Takenaga, M. Miura, M. Ikeda, K. Kaneyuki, Masato Shiozawa, Y. Choi, K. S. Ganezer, Takehisa Hasegawa, W. E. Keig, C. Regis, Hidetoshi Kubo, T. Sekiguchi, A. Kibayashi, S. B. Kim, J. L. Raaf, Hirokazu Ishino, Yoshitaka Itow, K. Bays, J. Y. Kim, G. Carminati, S. N. Smith, H. Okazawa, Atsushi Takeda, K. Nakamura, H. Kaji, Joshua Hignight, A. Minamino, Yasunari Suzuki, C. W. Walter, T. McLachlan, Y. Obayashi, Ian Taylor, K. Ieki, R. J. Wilkes, S. Moriyama, Masayuki Nakahata, S. Matsuno, J. Takeuchi, Y. Hayato, K. Sakashita, Zishuo Yang, Justin Albert, Kate Scholberg, Y. Kuno, Hiroyuki Sekiya, Y. Fukuda, C. Yanagisawa, M. Goldhaber, M. Dziomba, Y. Takeuchi, T. Kajita, M. R. Vagins, A. Murakami, S. Nakayama, G. Mitsuka, I. T. Lim, R. A. Wendell, J. Kameda, P. Mijakowski, Kalen Martens, L. R. Sulak, M. B. Smy, Koh Ueno, T. Yokozawa, J. Imber, Ll. Marti, M. Miyake, Yuichi Oyama, and A. L. Renshaw

Subjects
Physics, Nuclear and High Energy Physics, Particle physics, Muon, Proton, Proton decay, Atmospheric neutrino, Super-Kamiokande, Lower limit
Abstract

We have searched for proton into muon plus neutral kaon using data from a 91.7 kiloton-year exposure of Super-Kamiokande-I, a 49.2 kiloton-year exposure of Super-Kamiokande-II, and a 31.9 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 1.6x10^33 years at the 90% confidence level.

Published
2012
Full Text
View/download PDF

4. Solar neutrino results in Super-Kamiokande-III

Author

C. K. Jung, J. L. Raaf, Y. Takeuchi, D. Kielczewska, Y. Watanabe, G. Mitsuka, J. S. Jang, Y. Yokosawa, N. Tanimoto, Y. Obayashi, K. S. Ganezer, Song Chen, Hiroshi Watanabe, John G. Learned, K. Connolly, W. R. Kropp, H. Nishino, S. Yamada, M. Dziomba, Minoru Yoshida, C. W. Walter, C. McGrew, Masato Shiozawa, Y. Choi, T. Iida, T. Tsukamoto, J. Kameda, H. Toyota, Y. Hayato, B. S. Yang, Ken-ichiro Kobayashi, P. Mijakowski, M. Koshiba, T. Ishida, Y. Takenaga, M. Goldhaber, Yuichi Oyama, K. Ueshima, R. J. Wilkes, John Hill, T. Tanaka, S. Moriyama, Haoxiong Zhang, S. Hazama, M. Miura, R. Terri, Masayuki Nakahata, Ko Okumura, A. Kibayashi, Michael Litos, W. Wang, A. T. Suzuki, Hiroyuki Sekiya, Y. Fukuda, S. B. Kim, H. W. Sobel, J. Y. Kim, N. Tamura, S. Nakayama, Y. Heng, Takaaki Mori, Frédéric Dufour, Atsushi Takeda, L. M. Magro, K. Abe, S. Tasaka, J. L. Stone, R. A. Wendell, M. Ikeda, M. R. Vagins, T. Nakadaira, W. E. Keig, K. Nishikawa, H. Kaji, K. Kaneyuki, Koji Nakamura, Ken Sakashita, L. Labarga, T. Sekiguchi, K. Bays, T. Ishii, T. Kobayashi, Makoto Sakuda, C. Yanagisawa, Yasunari Suzuki, Justin Albert, A. Minamino, I. T. Lim, Y. Shimizu, Y. Kuno, Yoshitaka Itow, K. Nishijima, Takaaki Kajita, G. D. Lopez, S. Mino, A. L. Renshaw, E. Kearns, Masashi Yokoyama, Yusuke Koshio, T. Ishizuka, T. McLachlan, Tsuyoshi Nakaya, H. Okazawa, S. Matsuno, K. Iyogi, J. P. Cravens, T. Yokozawa, David William Casper, H. Ogawa, C. Ishihara, L. R. Sulak, M. B. Smy, Koh Ueno, Hirokazu Ishino, Y. Totsuka, T. Wongjirad, Y. Kozuma, E. Thrane, Zishuo Yang, Kate Scholberg, S. Mine, Takehisa Hasegawa, C. Regis, and UAM. Departamento de Física Teórica

Subjects
Physics, Systematic error, Nuclear and High Energy Physics, Particle physics, Solar neutrino, Física, FOS: Physical sciences, Elementary particle, High Energy Physics - Experiment, High Energy Physics - Experiment (hep-ex), Content (measure theory), Neutrino, Super-Kamiokande, Analysis method, Lepton
Abstract

Artículo escrito por un elevado número de autores, solo se referencian el que aparece en primer lugar, el nombre del grupo de colaboración, si le hubiere, y los autores pertenecientes a la UAM, The results of the third phase of the Super-Kamiokande solar neutrino measurement are presented and compared to the first and second phase results. With improved detector calibrations, a full detector simulation, and improved analysis methods, the systematic uncertainty on the total neutrino flux is estimated to be ± 2.1%, which is about two thirds of the systematic uncertainty for the first phase of Super-Kamiokande. The observed 8B solar flux in the 5.0 to 20 MeV total electron energy region is 2.32 ± 0.04 (stat.) ± 0.05 (sys.) x 10^6 cm^-2sec^-1, under the assumption of pure electron-flavor content, in agreement with previous measurements. A combined oscillation analysis is carried out using SK-I, II, and III data, and the results are also combined with the results of other solar neutrino experiments. The best-fit oscillation parameters are obtained to be sin^2 {\theta}12 = 0.30+0.02-0.01(tan^2 {\theta}12 = 0.42+0.04 -0.02) and {\Delta}m2_21 = 6.2+1.1-1.9 *10^-5eV^2. Combined with KamLAND results, the best-fit oscillation parameters are found to be sin^2 {\theta}12 = 0.31±0.01 (tan^2 {\theta}12 = 0.44±0.03) and {\Delta}m2_21 = 7.6 ± 0.2 x 10^-5 eV^2. The 8B neutrino flux obtained from global solar neutrino experiments is 5.3 ± 0.2 (stat + sys) x 10^6cm^-2s^-1, while the 8B flux becomes 5.1 ± 0.1 (stat +sys ) x 10^6cm^-2s^-1 by adding KamLAND result. In a three-flavor analysis combining all solar neutrino experiments, the upper limit of sin^2 {\theta}13 is 0.060 at 95% C.L.. After combination with KamLAND results, the upper limit of sin^2 {\theta}13 is found to be 0.059 at 95% C.L., The authors gratefully acknowledge the cooperation of the Kamioka Mining and Smelting Company. Super-K has been built and operated from funds provided by the Japanese Ministry of Education, Culture, Sports, Science and Technology, the U.S. Department of Energy, and the U.S. National Science Foundation. This work was partially supported by the Research Foundation of Korea (BK21 and KNRC), the Korean Ministry of Science and Technology, the National Science Foundation of China, and the Spanish Ministry of Science and Innovation (Grants No. FPA2009- 13697-C04-02 and No. Consolider-Ingenio-2010/CPAN)

Published
2011
Full Text
View/download PDF

Catalog

Books, media, physical & digital resources
See catalog results