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29 March 2024
 
  » arxiv » 1109.1621

 Article overview


Search for Differences in Oscillation Parameters for Atmospheric Neutrinos and Antineutrinos at Super-Kamiokande
Super-Kamiokande Collaboration ; K. Abe ; Y. Hayato ; T. Iida ; M. Ikeda ; K. Iyogi ; J. Kameda ; Y. Koshio ; Y. Kozuma ; M. Miura ; S. Moriyama ; M. Nakahata ; S. Nakayama ; Y. Obayashi ; H. Sekiya ; M. Shiozawa ; Y. Suzuki ; A. Takeda ; Y. Takenaga ; Y. Takeuchi ; K. Ueno ; K. Ueshima ; H. Watanabe ; S. Yamada ; T. Yokozawa ; C. Ishihara ; H. Kaji ; K. P. Lee ; T. Kajita ; K. Kaneyuki ; T. McLachlan ; K. Okumura ; Y. Shimizu ; N. Tanimoto ; K. Martens ; M. R. Vagins ; L. Labarga ; L. M. Magro ; F. Dufour ; E. Kearns ; M. Litos ; J.L. Raaf ; J.L. Stone ; L.R. Sulak ; M. Goldhaber ; K. Bays ; W.R. Kropp ; S. Mine ; C. Regis ; M. B. Smy ; H. W. Sobel ; K. S. Ganezer ; J. Hill ; W. E. Keig ; J. S. Jang ; J. Y. Kim ; I. T. Lim ; J. B. Albert ; K. Scholberg ; C. W. Walter ; R. Wendell ; T. M. Wongjirad ; S. Tasaka ; J. G. Learned ; S. Matsuno ; T. Hasegawa ; T. Ishida ; T. Ishii ; T. Kobayashi ; T. Nakadaira ; K. Nakamura ; K. Nishikawa ; H. Nishino ; Y. Oyama ; K. Sakashita ; T. Sekiguchi ; T. Tsukamoto ; A. T. Suzuki ; A. Minamino ; T. Nakaya ; Y. Fukuda ; Y. Itow ; G. Mitsuka ; T. Tanaka ; C. K. Jung ; I. Taylor ; C. Yanagisawa ; H. Ishino ; A. Kibayashi ; S. Mino ; T. Mori ; M. Sakuda ; H. Toyota ; Y. Kuno ; S. B. Kim ; B. S. Yang ; T. Ishizuka ; H. Okazawa ; Y. Choi ; K. Nishijima ; M. Koshiba ; M. Yokoyama ; Y. Totsuka ; S. Chen ; Y. Heng ; Z. Yang ; H. Zhang ; D. Kielczewska ; P. Mijakowski ; K. Connolly ; M. Dziomba ; R. J. Wilkes ;
Date 8 Sep 2011
AbstractWe 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.
Source arXiv, 1109.1621
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