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249 results on '"Mino, S."'

4. A Search for Nucleon Decay via $n \rightarrow \bar{\nu} \pi^{0}$ and $p \rightarrow \bar{\nu} \pi^{+}$ in Super-Kamiokande

Author

Collaboration, Super-Kamiokande, Abe, K., Hayato, Y., Iida, T., Iyogi, K., Kameda, J., Koshio, Y., Kozuma, Y., Marti, Ll., Miura, M., Moriyama, S., Nakahata, M., Nakayama, S., Obayashi, Y., Sekiya, H., Shiozawa, M., Suzuki, Y., Takeda, A., Takenaga, Y., Ueno, K., Ueshima, K., Yamada, S., Yokozawa, T., Ishihara, C., Kaji, H., Kajita, T., Kaneyuki, K., Lee, K. P., McLachlan, T., Okumura, K., Shimizu, Y., Tanimoto, N., Kearns, E., Litos, M., Raaf, J. L., Stone, J. L., Sulak, L. R., Goldhaber, M., Bays, K., Kropp, W. R., Mine, S., Regis, C., Renshaw, A., Smy, M. B., Sobel, H. W., Ganezer, K. S., Hill, J., Keig, W. E., Jang, J. S., Kim, J. Y., Lim, I. T., Albert, J. B., Scholberg, K., Walter, C. W., Wendell, R., Wongjirad, T. M., Ishizuka, T., Tasaka, S., Learned, J. G., Matsuno, S., Smith, S. N., Hasegawa, T., Ishida, T., Ishii, T., Kobayashi, T., Nakadaira, T., Nakamura, K., Nishikawa, K., Oyama, Y., Sakashita, K., Sekiguchi, T., Tsukamoto, T., Suzuki, A. T., Takeuchi, Y., Ikeda, M., Minamino, A., Nakaya, T., Fukuda, Y., Itow, Y., Mitsuka, G., Tanaka, T., Jung, C. K., Lopez, G. D., Taylor, I., Yanagisawa, C., Ishino, H., Kibayashi, A., Mino, S., Mori, T., Sakuda, M., Toyota, H., Kuno, Y., Yoshida, M., Kim, S. B., Yang, B. S., Okazawa, H., Choi, Y., Nishijima, K., Koshiba, M., Yokoyama, M., Totsuka, Y., Martens, K., Schuemann, J., Vagins, M. R., Chen, S., Heng, Y., Yang, Z., Zhang, H., Kielczewska, D., Mijakowski, P., Connolly, K., Dziomba, M., Thrane, E., and Wilkes, R. J.

Subjects
High Energy Physics - Experiment
Abstract

We present the results of searches for nucleon decay via bound neutron to antineutrino plus pizero and proton to antineutrino plus piplus using data from a combined 172.8 kiloton-years exposure of Super-Kamiokande-I, -II, and -III. We set lower limits on the partial lifetime for each of these modes. For antineutrino pizero, the partial lifetime is >1.1x10^{33} years; for antineutrino piplus, the partial lifetime is >3.9x10^{32} years at 90% confidence level., Comment: 6 pages, 5 figures, submitted to Physical Review Letters

Published
2013
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5. Search for GUT Monopoles at Super-Kamiokande

Author

Collaboration, The Super-Kamiokande, Ueno, K., Abe, K., Hayato, Y., Iida, T., Iyogi, K., Kameda, J., Koshio, Y., Kozuma, Y., Miura, M., Moriyama, S., Nakahata, M., Nakayama, S., Obayashi, Y., Sekiya, H., Shiozawa, M., Suzuki, Y., Takeda, A., Takenaga, Y., Ueshima, K., Yamada, S., Yokozawa, T., Martens, K., Schuemann, J., Vagins, M., Ishihara, C., Kaji, H., Kajita, T., Kaneyuki, K., McLachlan, T., Okumura, K., Shimizu, Y., Tanimoto, N., Kearns, E., Litos, M., Raaf, J. L., Stone, J. L., Sulak, L. R., Bays, K., Kropp, W. R., Mine, S., Regis, C., Renshaw, A., Smy, M. B., Sobel, H. W., Ganezer, K. S., Hill, J., Keig, W. E., Jang, J. S., Kim, J. Y., Lim, I. T., Albert, J. B., Scholberg, K., Walter, C. W., Wendell, R., Wongjirad, T., Ishizuka, T., Tasaka, S., Learned, J. G., Matsuno, S., Hasegawa, T., Ishida, T., Ishii, T., Kobayashi, T., Nakadaira, T., Nakamura, K., Nishikawa, K., Oyama, Y., Sakashita, K., Sekiguchi, T., Tsukamoto, T., Suzuki, A. T., Takeuchi, Y., Ikeda, M., Minamino, A., Nakaya, T., Labarga, L., Marti, Ll., Fukuda, Y., Itow, Y., Mitsuka, G., Tanaka, T., Jung, C. K., Lopez, G., Taylor, I., Yanagisawa, C., Ishino, H., Kibayashi, A., Mino, S., Mori, T., Sakuda, M., Toyota, H., Kuno, Y., Yoshida, M., Kim, S. B., Yang, B. S., Okazawa, H., Choi, Y., Nishijima, K., Koshiba, M., Totsuka, Y., Yokoyama, M., Chen, S., Heng, Y., Yang, Z., Zhang, H., Kielczewska, D., Mijakowski, P., Connolly, K., Dziomba, M., Thrane, E., and Wilkes, R. J.

Subjects
High Energy Physics - Experiment, Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Solar and Stellar Astrophysics
Abstract

GUT monopoles captured by the Sun's gravitation are expected to catalyze proton decays via the Callan-Rubakov process. In this scenario, protons, which initially decay into pions, will ultimately produce \nu_{e}, \nu_{\mu} and \bar{\nu}_{\mu}. After undergoing neutrino oscillation, all neutrino species appear when they arrive at the Earth, and can be detected by a 50,000 metric ton water Cherenkov detector, Super-Kamiokande (SK). A search for low energy neutrinos in the electron total energy range from 19 to 55 MeV was carried out with SK and gives a monopole flux limit of F_M(\sigma_0/1 mb) < 6.3 \times 10^{-24} (\beta_M/10^{-3})^2 cm^{-2} s^{-1} sr^{-1} at 90% C.L., where \beta_M is the monopole velocity in units of the speed of light and \sigma_0 is the catalysis cross section at \beta_M=1. The obtained limit is more than eight orders of magnitude more stringent than the current best cosmic-ray supermassive monopole flux limit, F_M < 1 \times 10^{-15} cm^{-2} s^{-1} sr^{-1} for \beta_M < 10^{-3} and also two orders of magnitude lower than the result of the Kamiokande experiment, which used a similar detection method., Comment: 15 pages, 6 figures

Published
2012
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6. Supernova Relic Neutrino Search at Super-Kamiokande

Author

Collaboration, The Super-Kamiokande, Bays, K., Iida, T., Abe, K., Hayato, Y., Iyogi, K., Kameda, J., Koshio, Y., Marti, L., Miura, M., Moriyama, S., Nakahata, M., Nakayama, S., Obayashi, Y., Sekiya, H., Shiozawa, M., Suzuki, Y., Takeda, A., Takenaga, Y., Ueno, K., Kajita, K. Ueshima S. Yamada T. Yokozawa H. Kaji T., Kaneyuki, K., McLachlan, T., Okumura, K., Pik, L. K., Martens, K., Vagins, M., Labarga, L., Kearns, E., Litos, M., Raaf, J. L., Stone, J. L., Sulak, L. R., Kropp, W. R., Mine, S., Regis, C., Renshaw, A., Smy, M. B., Sobel, H. W., Ganezer, K. S., Hill, J., Keig, W. E., Cho, S., Jang, J. S., Kim, J. Y., Lim, I. T., Albert, J., Scholberg, K., Walter, C. W., Wendell, R., Wongjirad, T., Ishizuka, T., Tasaka, S., Learned, J. G., Matsuno, S., Smith, S., Hasegawa, T., Ishida, T., Ishii, T., Kobayashi, T., Nakadaira, T., Nakamura, K., Nishikawa, K., Oyama, Y., Sakashita, K., Sekiguchi, T., Tsukamoto, T., Suzuki, A. T., Takeuchi, Y., Ikeda, M., Matsuoka, K., Minamino, A., Murakami, A., Nakaya, T., Fukuda, Y., Itow, Y., Mitsuka, G., Miyake, M., Tanaka, T., Hignight, J., Imber, J., Jung, C. K., Taylor, I., Yanagisawa, C., Kibayashi, A., Ishino, H., Mino, S., Sakuda, M., Mori, T., Toyota, H., Kuno, Y., Kim, S. B., Yang, B. S., Okazawa, H., Choi, Y., Nishijima, K., Koshiba, M., Totsuka, Y., Yokoyama, M., Heng, Y., Chen, S., Zhang, H., Yang, Z., Mijakowski, P., Connolly, K., Dziomba, M., and Wilkes, R. J.

Subjects
High Energy Physics - Experiment
Abstract

A new Super-Kamiokande (SK) search for Supernova Relic Neutrinos (SRNs) was conducted using 2853 live days of data. Sensitivity is now greatly improved compared to the 2003 SK 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 SRN flux are between 2.8 and 3.0 nu_e cm^-2 s^-1 > 16 MeV total positron energy (17.3 MeV E_nu).

Published
2011
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7. Search for Differences in Oscillation Parameters for Atmospheric Neutrinos and Antineutrinos at Super-Kamiokande

Author

Collaboration, Super-Kamiokande, Abe, K., Hayato, Y., Iida, T., Ikeda, M., Iyogi, K., Kameda, J., Koshio, Y., Kozuma, Y., Miura, M., Moriyama, S., Nakahata, M., Nakayama, S., Obayashi, Y., Sekiya, H., Shiozawa, M., Suzuki, Y., Takeda, A., Takenaga, Y., Takeuchi, Y., Ueno, K., Ueshima, K., Watanabe, H., Yamada, S., Yokozawa, T., Ishihara, C., Kaji, H., Lee, K. P., Kajita, T., Kaneyuki, K., McLachlan, T., Okumura, K., Shimizu, Y., Tanimoto, N., Martens, K., Vagins, M. R., Labarga, L., Magro, L. M., Dufour, F., Kearns, E., Litos, M., Raaf, J. L., Stone, J. L., Sulak, L. R., Goldhaber, M., Bays, K., Kropp, W. R., Mine, S., Regis, C., Smy, M. B., Sobel, H. W., Ganezer, K. S., Hill, J., Keig, W. E., Jang, J. S., Kim, J. Y., Lim, I. T., Albert, J. B., Scholberg, K., Walter, C. W., Wendell, R., Wongjirad, T. M., Tasaka, S., Learned, J. G., Matsuno, S., Hasegawa, T., Ishida, T., Ishii, T., Kobayashi, T., Nakadaira, T., Nakamura, K., Nishikawa, K., Nishino, H., Oyama, Y., Sakashita, K., Sekiguchi, T., Tsukamoto, T., Suzuki, A. T., Minamino, A., Nakaya, T., Fukuda, Y., Itow, Y., Mitsuka, G., Tanaka, T., Jung, C. K., Taylor, I., Yanagisawa, C., Ishino, H., Kibayashi, A., Mino, S., Mori, T., Sakuda, M., Toyota, H., Kuno, Y., Kim, S. B., Yang, B. S., Ishizuka, T., Okazawa, H., Choi, Y., Nishijima, K., Koshiba, M., Yokoyama, M., Totsuka, Y., Chen, S., Heng, Y., Yang, Z., Zhang, H., Kielczewska, D., Mijakowski, P., Connolly, K., Dziomba, M., and Wilkes, R. J.

Subjects
High Energy Physics - Experiment
Abstract

We present a search for differences in the oscillations of antineutrinos and neutrinos in the Super-Kamiokande -I, -II, and -III atmospheric neutrino sample. Under a two-flavor disappearance model with separate mixing parameters between neutrinos and antineutrinos, we find no evidence for a difference in oscillation parameters. Best fit antineutrino mixing is found to be at (dm2bar, sin2 2 thetabar) = (2.0x10^-3 eV^2, 1.0) and is consistent with the overall Super-K measurement., Comment: 6 pages, 4 figures. Figure updated

Published
2011
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8. Solar neutrino results in Super-Kamiokande-III

Author

Abe, K., Hayato, Y., Iida, T., Ikeda, M., Ishihara, C., Iyogi, K., Kameda, J., Kobayashi, K., Koshio, Y., Kozuma, Y., Miura, M., Moriyama, S., Nakahata, M., Nakayama, S., Obayashi, Y., Ogawa, H., Sekiya, H., Shiozawa, M., Suzuki, Y., Takeda, A., Takenaga, Y., Ueno, K., Ueshima, K., Watanabe, H., Yamada, S., Yokozawa, T., Hazama, S., Kaji, H., Kajita, T., Kaneyuki, K., McLachlan, T., Okumura, K., Shimizu, Y., Tanimoto, N., Vagins, M. R., Labarga, L., Magro, L. M, Dufour, F., Kearns, E., Litos, M., Raaf, J. L., Stone, J. L., Sulak, L. R., Wang, W., Goldhaber, M., Bays, K., Casper, D., Cravens, J. P., Kropp, W. R., Mine, S., Regis, C., Renshaw, A., Smy, M. B., Sobel, H. W., Ganezer, K. S., Hill, J., Keig, W. E., Jang, J. S., Kim, J. Y., Lim, I. T., Albert, J., Wendell, R., Wongjirad, T., Scholberg, K., Walter, C. W., Ishizuka, T., Tasaka, S., Learned, J. G., Matsuno, S., Watanabe, Y., Hasegawa, T., Ishida, T., Ishii, T., Kobayashi, T., Nakadaira, T., Nakamura, K., Nishikawa, K., Nishino, H., Oyama, Y., Sakashita, K., Sekiguchi, T., Tsukamoto, T., Suzuki, A. T., Takeuchi, Y., Minamino, A., Nakaya, T., Fukuda, Y., Itow, Y., Mitsuka, G., Tanaka, T., Jung, C. K., Lopez, G., McGrew, C., Terri, R., Yanagisawa, C., Tamura, N., Ishino, H., Kibayashi, A., Mino, S., Mori, T., Sakuda, M., Toyota, H., Kuno, Y., Yoshida, M., Kim, S. B., Yang, B. S., Okazawa, H., Choi, Y., Nishijima, K., Yokosawa, Y., Koshiba, M., Totsuka, Y., Yokoyama, M., Chen, S., Heng, Y., Yang, Z., Zhang, H., Kielczewska, D., Mijakowski, P., Connolly, K., Dziomba, M., Thrane, E., and Wilkes, R. J.

Subjects
High Energy Physics - Experiment
Abstract

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.) *10^6 cm^-2sec^-1, 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*10^-5eV^2 . The 8B neutrino flux obtained from global solar neutrino experiments is 5.3+/-0.2(stat.+sys.)*10^6cm^-2s^-1, while the 8B flux becomes 5.1+/-0.1(stat.+sys.)*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.., Comment: 19 pages, 33 figures in the main text. The appendix section on errata is added in v3

Published
2010
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9. Atmospheric neutrino oscillation analysis with sub-leading effects in Super-Kamiokande I, II, and III

Author

Collaboration, Super-Kamiokande, Wendell, R., Ishihara, C., Abe, K., Hayato, Y., Iida, T., Ikeda, M., Iyogi, K., Kameda, J., Kobayashi, K., Koshio, Y., Kozuma, Y., Miura, M., Moriyama, S., Nakahata, M., Nakayama, S., Obayashi, Y., Ogawa, H., Sekiya, H., Shiozawa, M., Suzuki, Y., Takeda, A., Takenaga, Y., Takeuchi, Y., Ueno, K., Ueshima, K., Watanabe, H., Yamada, S., Yokozawa, T., Hazama, S., Kaji, H., Kajita, T., Kaneyuki, K., McLachlan, T., Okumura, K., Shimizu, Y., Tanimoto, N., Vagins, M. R., Dufour, F., Kearns, E., Litos, M., Raaf, J. L., Stone, J. L., Sulak, L. R., Wang, W., Goldhaber, M., Bays, K., Casper, D., Cravens, J. P., Kropp, W. R., Mine, S., Regis, C., Smy, M. B., Sobel, H. W., Ganezer, K. S., Hill, J., Keig, W. E., Jang, J. S., Kim, J. Y., Lim, I. T., Albert, J., Fechner, M., Scholberg, K., Walter, C. W., Tasaka, S., Learned, J. G., Matsuno, S., Watanabe, Y., Hasegawa, T., Ishida, T., Ishii, T., Kobayashi, T., Nakadaira, T., Nakamura, K., Nishikawa, K., Nishino, H., Oyama, Y., Sakashita, K., Sekiguchi, T., Tsukamoto, T., Suzuki, A. T., Minamino, A., Nakaya, T., Fukuda, Y., Itow, Y., Mitsuka, G., Tanaka, T., Jung, C. K., Lopez, G., McGrew, C., Yanagisawa, C., Tamura, N., Ishino, H., Kibayashi, A., Mino, S., Mori, T., Sakuda, M., Toyota, H., Kuno, Y., Yoshida, M., Kim, S. B., Yang, B. S., Ishizuka, T., Okazawa, H., Choi, Y., Nishijima, K., Yokosawa, Y., Koshiba, M., Yokoyama, M., Totsuka, Y., Chen, S., Heng, Y., Yang, Z., Zhang, H., Kielczewska, D., Mijakowski, P., Connolly, K., Dziomba, M., Thrane, E., and Wilkes, R. J.

Subjects
High Energy Physics - Experiment
Abstract

We present a search for non-zero theta_{13} and deviations of sin^2 theta_{23} from 0.5 in the oscillations of atmospheric neutrino data from Super-Kamiokande -I, -II, and -III. No distortions of the neutrino flux consistent with non-zero theta_{13} are found and both neutrino mass hierarchy hypotheses are in agreement with the data. The data are best fit at Delta m^2 = 2.1 x 10^-3 eV^2, sin^2 theta_{13} = 0.0, and sin^2 theta_{23} =0.5. In the normal (inverted) hierarchy theta_{13} and Delta m^2 are constrained at the one-dimensional 90% C.L. to sin^2 theta_{13} < 0.04 (0.09) and 1.9 (1.7) x 10^-3 < Delta m^2 < 2.6 (2.7) x 10^-3 eV^2. The atmospheric mixing angle is within 0.407 <= sin^2 theta_{23} <= 0.583 at 90% C.L., Comment: 17 Pages, 14 figures. To be submitted to Phys. Rev. D Minor update to text after referee comments. Figures modified for better grayscale printing.

Published
2010
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17. Search for GUT monopoles at Super–Kamiokande

Author

Ueno, K., Abe, K., Hayato, Y., Iida, T., Iyogi, K., Kameda, J., Koshio, Y., Kozuma, Y., Miura, M., Moriyama, S., Nakahata, M., Nakayama, S., Obayashi, Y., Sekiya, H., Shiozawa, M., Suzuki, Y., Takeda, A., Takenaga, Y., Ueshima, K., Yamada, S., Yokozawa, T., Martens, K., Schuemann, J., Vagins, M., Ishihara, C., Kaji, H., Kajita, T., Kaneyuki, K., McLachlan, T., Okumura, K., Shimizu, Y., Tanimoto, N., Kearns, E., Litos, M., Raaf, J.L., Stone, J.L., Sulak, L.R., Bays, K., Kropp, W.R., Mine, S., Regis, C., Renshaw, A., Smy, M.B., Sobel, H.W., Ganezer, K.S., Hill, J., Keig, W.E., Jang, J.S., Kim, J.Y., Lim, I.T., Albert, J.B., Scholberg, K., Walter, C.W., Wendell, R., Wongjirad, T., Ishizuka, T., Tasaka, S., Learned, J.G., Matsuno, S., Hasegawa, T., Ishida, T., Ishii, T., Kobayashi, T., Nakadaira, T., Nakamura, K., Nishikawa, K., Oyama, Y., Sakashita, K., Sekiguchi, T., Tsukamoto, T., Suzuki, A.T., Takeuchi, Y., Ikeda, M., Minamino, A., Nakaya, T., Labarga, L., Marti, Ll., Fukuda, Y., Itow, Y., Mitsuka, G., Tanaka, T., Jung, C.K., Lopez, G., Taylor, I., Yanagisawa, C., Ishino, H., Kibayashi, A., Mino, S., Mori, T., Sakuda, M., Toyota, H., Kuno, Y., Yoshida, M., Kim, S.B., Yang, B.S., Okazawa, H., Choi, Y., Nishijima, K., Koshiba, M., Totsuka, Y., Yokoyama, M., Chen, S., Heng, Y., Yang, Z., Zhang, H., Kielczewska, D., Mijakowski, P., Connolly, K., Dziomba, M., Thrane, E., and Wilkes, R.J.

Published
2012
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18. Ecogenomics of the Marine Benthic Filamentous Cyanobacterium Adonisia

Author

Walter, J.M., Coutinho, F.H., Leomil, L., Hargreaves, P.I., Campeão, M.E., Vieira, V.V., Silva, B.S. da, Fistarol, G.O., Salomon, P.S., Sawabe, T., Mino, S., Hosokawa, M., Miyashita, H., Maruyama, F., Verk, M.C. van, Dutilh, B.E., Thompson, C.C., Thompson, F.L., Walter, J.M., Coutinho, F.H., Leomil, L., Hargreaves, P.I., Campeão, M.E., Vieira, V.V., Silva, B.S. da, Fistarol, G.O., Salomon, P.S., Sawabe, T., Mino, S., Hosokawa, M., Miyashita, H., Maruyama, F., Verk, M.C. van, Dutilh, B.E., Thompson, C.C., and Thompson, F.L.

Abstract

Contains fulltext : 224856.pdf (publisher's version ) (Closed access), Turfs are among the major benthic components of reef systems worldwide. The nearly complete genome sequences, basic physiological characteristics, and phylogenomic reconstruction of two phycobiliprotein-rich filamentous cyanobacteria strains isolated from turf assemblages from the Abrolhos Bank (Brazil) are investigated. Both Adonisia turfae CCMR0081(T) (= CBAS 745(T)) and CCMR0082 contain approximately 8 Mbp in genome size and experiments identified that both strains exhibit chromatic acclimation. Whereas CCMR0081(T) exhibits chromatic acclimation type 3 (CA3) regulating both phycocyanin (PC) and phycoerythrin (PE), CCMR0082 strain exhibits chromatic acclimation type 2 (CA2), in correspondence with genes encoding specific photosensors and regulators for PC and PE. Furthermore, a high number and diversity of secondary metabolite synthesis gene clusters were identified in both genomes, and they were able to grow at high temperatures (28 °C, with scant growth at 30 °C). These characteristics provide insights into their widespread distribution in reef systems.

Published
2020

22. Insertion of cyclic prefix for all-optical fractional OFDM

Author

Nagashima, T., Murakawa, T., Shimizu, S., Hasegawa, M., Hattori, K., Okuno, M., Mino, S., Himeno, A., Wada, N., Uenohara, H., Konishi, T., CINCOTTI, GABRIELLA, Photonics in Switching (PS), Florence, Italy 2015, Nagashima, T., Cincotti, Gabriella, Murakawa, T., Shimizu, S., Hasegawa, M., Hattori, K., Okuno, M., Mino, S., Himeno, A., Wada, N., Uenohara, H., and Konishi, T.

Published
2015

24. Cost effective fractional OFDM receiver using arrayed waveguide grating

Author

Nagashima, T., Gabriella CINCOTTI, Murakawa, T., Shimizu, S., Hasegawa, M., Hattori, K., Okuno, M., Mino, S., Himeno, A., Wada, N., Uenohara, H., Konishi, T., Optoelectronics and Communications Conference/International Conference on Photonics in Switching (OECC/PS), Toki Messe, Niigata, Japan, T., Nagashima, Cincotti, Gabriella, T., Murakawa, S., Shimizu, M., Hasegawa, K., Hattori, M., Okuno, S., Mino, A., Himeno, N., Wada, H., Uenohara, and T., Konishi

Published
2016

25. A Search for Nucleon Decay via $n \rightarrow \bar�� ��^{0}$ and $p \rightarrow \bar�� ��^{+}$ in Super-Kamiokande

Author

Kamiokande Collaboration, Abe, K., Hayato, Y., Iida, T., Iyogi, K., Kameda, J., Koshio, Y., Kozuma, Y., Marti, Ll., Miura, M., Moriyama, S., Nakahata, M., Nakayama, S., Obayashi, Y., Sekiya, H., Shiozawa, M., Suzuki, Y., Takeda, A., Takenaga, Y., Ueno, K., Ueshima, K., Yamada, S., Yokozawa, T., Ishihara, C., Kaji, H., Kajita, T., Kaneyuki, K., Lee, K. P., McLachlan, T., Okumura, K., Shimizu, Y., Tanimoto, N., Kearns, E., Litos, M., Raaf, J. L., Stone, J. L., Sulak, L. R., Goldhaber, M., Bays, K., Kropp, W. R., Mine, S., Regis, C., Renshaw, A., Smy, M. B., Sobel, H. W., Ganezer, K. S., Hill, J., Keig, W. E., Jang, J. S., Kim, J. Y., Lim, I. T., Albert, J. B., Scholberg, K., Walter, C. W., Wendell, R., Wongjirad, T. M., Ishizuka, T., Tasaka, S., Learned, J. G., Matsuno, S., Smith, S. N., Hasegawa, T., Ishida, T., Ishii, T., Kobayashi, T., Nakadaira, T., Nakamura, K., Nishikawa, K., Oyama, Y., Sakashita, K., Sekiguchi, T., Tsukamoto, T., Suzuki, A. T., Takeuchi, Y., Ikeda, M., Minamino, A., Nakaya, T., Fukuda, Y., Itow, Y., Mitsuka, G., Tanaka, T., Jung, C. K., Lopez, G. D., Taylor, I., Yanagisawa, C., Ishino, H., Kibayashi, A., Mino, S., Mori, T., Sakuda, M., Toyota, H., Kuno, Y., Yoshida, M., Kim, S. B., Yang, B. S., Okazawa, H., Choi, Y., Nishijima, K., Koshiba, M., Yokoyama, M., Totsuka, Y., Martens, K., Schuemann, J., Vagins, M. R., Chen, S., Heng, Y., Yang, Z., Zhang, H., Kielczewska, D., Mijakowski, P., Connolly, K., Dziomba, M., Thrane, E., and Wilkes, R. J.

Subjects
High Energy Physics - Experiment (hep-ex), FOS: Physical sciences
Abstract

We present the results of searches for nucleon decay via bound neutron to antineutrino plus pizero and proton to antineutrino plus piplus using data from a combined 172.8 kiloton-years exposure of Super-Kamiokande-I, -II, and -III. We set lower limits on the partial lifetime for each of these modes. For antineutrino pizero, the partial lifetime is >1.1x10^{33} years; for antineutrino piplus, the partial lifetime is >3.9x10^{32} years at 90% confidence level., 6 pages, 5 figures, submitted to Physical Review Letters

Published
2013
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26. Cyclic prefix insertion for all-optical fractional OFDM

Author

Nagashima, T., primary, Murakawa, T., additional, Hasegawa, M., additional, Konishi, T., additional, Cincotti, G., additional, Shimizu, S., additional, Wada, N., additional, Uenohara, H., additional, Hattori, K., additional, Okuno, M., additional, Mino, S., additional, and Himeno, A., additional

Published
2015
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38. Atmospheric neutrino oscillation analysis with subleading effects in Super-Kamiokande I, II, and III

Author

Wendell, R., primary, Ishihara, C., additional, Abe, K., additional, Hayato, Y., additional, Iida, T., additional, Ikeda, M., additional, Iyogi, K., additional, Kameda, J., additional, Kobayashi, K., additional, Koshio, Y., additional, Kozuma, Y., additional, Miura, M., additional, Moriyama, S., additional, Nakahata, M., additional, Nakayama, S., additional, Obayashi, Y., additional, Ogawa, H., additional, Sekiya, H., additional, Shiozawa, M., additional, Suzuki, Y., additional, Takeda, A., additional, Takenaga, Y., additional, Takeuchi, Y., additional, Ueno, K., additional, Ueshima, K., additional, Watanabe, H., additional, Yamada, S., additional, Yokozawa, T., additional, Hazama, S., additional, Kaji, H., additional, Kajita, T., additional, Kaneyuki, K., additional, McLachlan, T., additional, Okumura, K., additional, Shimizu, Y., additional, Tanimoto, N., additional, Vagins, M. R., additional, Dufour, F., additional, Kearns, E., additional, Litos, M., additional, Raaf, J. L., additional, Stone, J. L., additional, Sulak, L. R., additional, Wang, W., additional, Goldhaber, M., additional, Bays, K., additional, Casper, D., additional, Cravens, J. P., additional, Kropp, W. R., additional, Mine, S., additional, Regis, C., additional, Smy, M. B., additional, Sobel, H. W., additional, Ganezer, K. S., additional, Hill, J., additional, Keig, W. E., additional, Jang, J. S., additional, Kim, J. Y., additional, Lim, I. T., additional, Albert, J., additional, Fechner, M., additional, Scholberg, K., additional, Walter, C. W., additional, Tasaka, S., additional, Learned, J. G., additional, Matsuno, S., additional, Watanabe, Y., additional, Hasegawa, T., additional, Ishida, T., additional, Ishii, T., additional, Kobayashi, T., additional, Nakadaira, T., additional, Nakamura, K., additional, Nishikawa, K., additional, Nishino, H., additional, Oyama, Y., additional, Sakashita, K., additional, Sekiguchi, T., additional, Tsukamoto, T., additional, Suzuki, A. T., additional, Minamino, A., additional, Nakaya, T., additional, Fukuda, Y., additional, Itow, Y., additional, Mitsuka, G., additional, Tanaka, T., additional, Jung, C. K., additional, Lopez, G., additional, McGrew, C., additional, Yanagisawa, C., additional, Tamura, N., additional, Ishino, H., additional, Kibayashi, A., additional, Mino, S., additional, Mori, T., additional, Sakuda, M., additional, Toyota, H., additional, Kuno, Y., additional, Yoshida, M., additional, Kim, S. B., additional, Yang, B. S., additional, Ishizuka, T., additional, Okazawa, H., additional, Choi, Y., additional, Nishijima, K., additional, Yokosawa, Y., additional, Koshiba, M., additional, Yokoyama, M., additional, Totsuka, Y., additional, Chen, S., additional, Heng, Y., additional, Yang, Z., additional, Zhang, H., additional, Kielczewska, D., additional, Mijakowski, P., additional, Connolly, K., additional, Dziomba, M., additional, Thrane, E., additional, and Wilkes, R. J., additional

Published
2010
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41. 160-Gb/s OTDM Transmission Using Integrated All-Optical MUX/DEMUX With All-Channel Modulation and Demultiplexing

Author

Ohara, T., primary, Takara, H., additional, Shake, I., additional, Mori, K., additional, Sato, K., additional, Kawanishi, S., additional, Mino, S., additional, Yamada, T., additional, Ishii, M., additional, Ogawa, I., additional, Kitoh, T., additional, Magari, K., additional, Okamoto, M., additional, Roussev, R.V., additional, Kurz, J.R., additional, Parameswaran, K.R., additional, and Fejer, M.M., additional

Published
2004
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45. Time-frequency photonic signal processing.

Author

Cincotti, G., Konishi, T., Murakawa, T., Nagashima, T., Shimizu, S., Hasegawa, M., Hattori, K., Okuno, M., Mino, S., Himeno, A., Wada, N., and Uenohara, H.

Published
2016

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