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Related papers: Solutions to the Atmospheric Neutrino Problem

200 papers

We propose simple phenomenological lepton mass matrices which describe the three neutrinos almost degenerate in mass, leading to a very large mixing angle between $\nu_\mu$ and $\nu_\tau$, as consistent with a recent report on atmospheric…

High Energy Physics - Phenomenology · Physics 2009-10-30 M. Fukugita , M. Tanimoto , T. Yanagida

We develop a general theoretical framework to analytically disentangle the contributions of the neutrino mass hierarchy, the atmospheric mixing angle, and the CP phase, in neutrino oscillations. To illustrate the usefulness of this…

High Energy Physics - Phenomenology · Physics 2015-06-17 Shao-Feng Ge , Kaoru Hagiwara , Carsten Rott

A model of neutrino oscillation experiments is constructed. The experiments incorporated are: solar neutrinos (Chlorine, Gallium, Super-K, and SNO), reactor neutrinos (Bugey and CHOOZ), beam stop neutrinos (LSND decay at rest and decay in…

Nuclear Theory · Physics 2007-05-23 D. C. Latimer , D. J. Ernst

In these two lectures I describe first the theory of neutrino mass and then discuss the implications of recent data (including 708--day data Super--Kamiokande data) which strongly indicate the need for neutrino conversions to account for…

High Energy Physics - Phenomenology · Physics 2007-05-23 J. W. F. Valle

We show that if the solar and atmospheric data are both described by maximal vacuum oscillations at the relevant mass scales then there exists a unique mixing matrix for three neutrino flavors. The solution necessarily conserves CP and…

High Energy Physics - Phenomenology · Physics 2009-09-15 V. Barger , S. Pakvasa , T. J. Weiler , K. Whisnant

We study properties of the oscillation effects in the matter of the Earth on antineutrino fluxes from supernovae. We show that these effects can provide explanation of the difference in the energy spectra of the events detected by…

High Energy Physics - Phenomenology · Physics 2009-10-31 C. Lunardini , A. Yu. Smirnov

We show how a unified description of the various two-flavor neutrino oscillation solutions, allowed by the atmospheric and solar neutrino experiments, are naturally realized within the framework of $\nu$MSSM (MSSM augmented with the seesaw…

High Energy Physics - Phenomenology · Physics 2011-05-12 Qaisar Shafi , Zurab Tavartkiladze

We present a four-neutrino model with three active neutrinos and one sterile neutrino which naturally has maximal $\nu_\mu\to\nu_\tau$ oscillations of atmospheric neutrinos and can explain the solar neutrino and LSND results. The model…

High Energy Physics - Phenomenology · Physics 2009-09-15 V. Barger , T. J. Weiler , K. Whisnant

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…

High Energy Physics - Experiment · Physics 2012-08-27 Kamiokande Collaboration , R. Wendell , C. Ishihara , K. Abe , Y. Hayato , T. Iida , M. Ikeda , K. Iyogi , J. Kameda , K. Kobayashi , Y. Koshio , Y. Kozuma , M. Miura , S. Moriyama , M. Nakahata , S. Nakayama , Y. Obayashi , H. Ogawa , H. Sekiya , M. Shiozawa , Y. Suzuki , A. Takeda , Y. Takenaga , Y. Takeuchi , K. Ueno , K. Ueshima , H. Watanabe , S. Yamada , T. Yokozawa , S. Hazama , H. Kaji , T. Kajita , K. Kaneyuki , T. McLachlan , K. Okumura , Y. Shimizu , N. Tanimoto , M. R. Vagins , F. Dufour , E. Kearns , M. Litos , J. L. Raaf , J. L. Stone , L. R. Sulak , W. Wang , M. Goldhaber , K. Bays , D. Casper , J. P. Cravens , 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. Albert , M. Fechner , K. Scholberg , C. W. Walter , S. Tasaka , J. G. Learned , S. Matsuno , Y. Watanabe , 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 , G. Lopez , C. McGrew , C. Yanagisawa , N. Tamura , H. Ishino , A. Kibayashi , S. Mino , T. Mori , M. Sakuda , H. Toyota , Y. Kuno , M. Yoshida , S. B. Kim , B. S. Yang , T. Ishizuka , H. Okazawa , Y. Choi , K. Nishijima , Y. Yokosawa , M. Koshiba , M. Yokoyama , Y. Totsuka , S. Chen , Y. Heng , Z. Yang , H. Zhang , D. Kielczewska , P. Mijakowski , K. Connolly , M. Dziomba , E. Thrane , R. J. Wilkes

The minimal interpretation of the atmospheric neutrino data suggests that the muon neutrino oscillates into another species with a mixing angle close to the maximal $\pi/4$. In the Exact Parity Symmetric Model, both the muon and electron…

High Energy Physics - Phenomenology · Physics 2011-03-10 J. Bunn , R. Foot , R. R. Volkas

In the previous paper (Part~1), we have verified that the SK assumption on the direction does not hold in the analysis of neutrino events occurred inside the SK detector. We have made four possible L/E analyses, L_nu/E_nu, L_nu/E_mu,…

High Energy Physics - Experiment · Physics 2010-07-29 E. Konishi , Y. Minorikawa , V. I. Galkin , M. Ishiwata , I. Nakamura , N. Takahashi , M. Kato , A. Misaki

A search for day-night variations in the solar neutrino flux resulting from neutrino oscillations has been carried out using the 504 day sample of solar neutrino data obtained at Super-Kamiokande. The absence of a significant day-night…

High Energy Physics - Experiment · Physics 2012-08-27 Kamiokande Collaboration , Y. Fukuda , T. Hayakawa , E. Ichihara , K. Inoue

We perform an updated model-independent analysis using the latest solar neutrino data obtained by $^{37}$Cl and $^{71}$Ga radiochemical experiments, and most notably by a large water-Cherenkov detector SuperKamiokande with their 504 days of…

High Energy Physics - Phenomenology · Physics 2009-10-31 Hisakazu Minakata , Hiroshi Nunokawa

The atmospheric neutrino oscillations and the vacuum oscillation solution of the solar neutrino problem can be consistently described by a doubly or triply degenerate neutrino spectrum as long as the high level of degeneracy required is not…

High Energy Physics - Phenomenology · Physics 2009-10-31 R. Barbieri , G. Ross , A. Strumia

Solar and atmospheric neutrino data require physics beyond the Standard Model of particle physics. The simplest, most generic, but not yet unique, interpretation of the data is in terms of neutrino oscillations. I summarize the results of…

Astrophysics · Physics 2007-05-23 J. W. F. Valle

The available upward-going muon data from the Kamiokande, Baksan, MACRO, IMB, and SuperKamiokande experiments are reviewed and combined. Bounds on the neutrino mass and mixing parameters are derived for oscillations in two and three…

High Energy Physics - Phenomenology · Physics 2009-10-07 G. L. Fogli , E. Lisi , A. Marrone

Some of the hot topics in neutrino physics are discussed, with particular emphasis on neutrino oscillations. After proposing credibility criteria for assessing various claimed effects, particular stress is laid on the solar neutrino…

High Energy Physics - Phenomenology · Physics 2007-05-23 John Ellis

It was suggested that a tension between the mass-squared differences obtained from the solar neutrino and KamLAND experiments can be solved by introducing the non-standard flavor-dependent interaction in neutrino propagation. In this paper…

High Energy Physics - Phenomenology · Physics 2017-01-04 Shinya Fukasawa , Osamu Yasuda

A search for a non-zero neutrino magnetic moment has been conducted using 1496 live days of solar neutrino data from {\SK}. Specifically, we searched for distortions to the energy spectrum of recoil electrons arising from magnetic…

High Energy Physics - Experiment · Physics 2012-08-27 Kamiokande Collaboration , D. W. Liu

The $^8$B solar neutrino flux predicted by the standard solar model (SSM) is consistent within the theoretical and experimental uncertainties with that observed at Kamiokande. The Gallium and Chlorine solar neutrino experiments, however,…

Astrophysics · Physics 2007-05-23 Arnon Dar
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