English
Related papers

Related papers: Solutions to the Atmospheric Neutrino Problem

200 papers

We study the interplay of neutrino oscillation and invisible decay in atmospheric and long-baseline neutrinos experiments. We perform a global analysis of the full atmospheric data from Super-Kamiokande together with long-baseline K2K and…

High Energy Physics - Phenomenology · Physics 2008-11-26 M. C. Gonzalez-Garcia , Michele Maltoni

Recent solar & atmospheric nu-data strongly indicate need for physics beyond the Standard Model. I review the ways of reconciling them in terms of 3-nu oscillations. Though not implied by data, bi-maximal nu-mixing models emerge as a…

High Energy Physics - Phenomenology · Physics 2009-09-17 J. W. F. Valle

We point out that the measurement of the $L/E$ distribution of atmospheric neutrino events with sufficient resolution in order to observe the characteristic modulations of neutrino oscillations would provide a unique way to test the…

High Energy Physics - Phenomenology · Physics 2007-05-23 G. Mannocchi , L. Periale , P. Picchi , F. Pietropaolo , S. Ragazzi , A. Rubbia

In this Letter we show that the evidence for neutrino oscillations from the Super-Kamiokande atmospheric neutrino data fully determines the 3x3 neutrino-oscillations mixing matrix and predicts an energy independent solar neutrino deficit at…

High Energy Physics - Phenomenology · Physics 2011-02-07 Ion Stancu

Using data from both solar and atmospheric neutrinos, Super-Kamiokande has provided fundamental information on neutrino flavor mixing and neutrino mass square differences.

High Energy Physics - Experiment · Physics 2007-05-23 M. B. Smy

New results from Super-Kamiokande, K2K and SNO not only have spurred on the interest in neutrino oscillation physics, but also have started to shift the interest from discovery to precision measurements. Future projects focusing on…

High Energy Physics - Experiment · Physics 2007-05-23 T. Tabarelli de Fatis

If Nature has chosen the vacuum oscillation solution to the Solar neutrino puzzle, a key theoretical challenge is to understand the extreme smallness of the $\Delta m^2_{\nu_e-\nu_X}$ ($\sim 10^{-10} eV^2$) required for the purpose. We find…

High Energy Physics - Phenomenology · Physics 2009-10-31 Z. Chacko , R. N. Mohapatra

Long length vacuum oscillations solution of the solar neutrino problem is discussed. We show that there is a strict correlation between a distortion of the neutrino energy spectrum and an amplitude of seasonal variations of the neutrino…

High Energy Physics - Phenomenology · Physics 2009-10-30 S. P. Mikheyev , A. Yu. Smirnov

Recent observations of variability in the ``atmospheric neutrino'' rate place constraints on possible explanations of the atmospheric neutrino anomaly. Many proposed solutions to the problem are static and can not be adapted to the temporal…

High Energy Physics - Phenomenology · Physics 2007-05-23 J. M. LoSecco

It is shown that recent results from the Super-Kamiokande detector constrain the tau neutrino diagonal magnetic moment to $\mu_{\nu_{\tau}} < 1.3\times 10^{-7} \mu_{B}$ for the case of $\nu_{\mu}\to \nu_{\tau}$ interpretation of the…

High Energy Physics - Phenomenology · Physics 2009-10-31 S. N. Gninenko

Neutrino oscillations with parameters relevant for the large mixing solution of the solar neutrino problem ($\Delta m^2_{21} = (2 - 20) \cdot 10^{-5}$ eV$^2$, $\sin^2 2\theta_{12} > 0.65$) can lead to observable (up to 10 - 12 %) excess of…

High Energy Physics - Phenomenology · Physics 2009-10-31 O. L. G. Peres , A. Y. Smirnov

We present measurements of total neutron production from atmospheric neutrino interactions in water, analyzed as a function of electron-equivalent visible energy over a range of 30 MeV to 10 GeV. These results are based on 4,270 days of…

High Energy Physics - Experiment · Physics 2025-06-23 Kamiokande collaboration , S. Han , K. Abe , S. Abe , Y. Asaoka , C. Bronner , M. Harada , Y. Hayato , K. Hiraide , K. Hosokawa , K. Ieki , M. Ikeda , J. Kameda , Y. Kanemura , R. Kaneshima , Y. Kashiwagi , Y. Kataoka , S. Miki , S. Mine , M. Miura , S. Moriyama , M. Nakahata , S. Nakayama , Y. Noguchi , G. Pronost , K. Sato , K. Okamoto , H. Sekiya , H. Shiba , K. Shimizu , R. Shinoda , M. Shiozawa , Y. Sonoda , Y. Suzuki , A. Takeda , Y. Takemoto , A. Takenaka , H. Tanaka , T. Yano , T. Kajita , K. Okumura , R. Nishijima , T. Tashiro , T. Tomiya , X. Wang , S. Yoshida , P. Fernandez , L. Labarga , N. Ospina , D. Samudio , B. Zaldivar , B. W. Pointon , C. Yanagisawa , E. Kearns , J. L. Raaf , L. Wan , T. Wester , J. Bian , B. Cortez , N. J. Griskevich , M. B. Smy , H. W. Sobel , V. Takhistov , A. Yankelevich , J. Hill , M. C. Jang , S. H. Lee , D. H. Moon , R. G. Park , B. S. Yang , B. Bodur , K. Scholberg , C. W. Walter , A. Beauchêne , O. Drapier , A. Giampaolo , A. Ershova , Th. A. Mueller , A. D. Santos , P. Paganini , C. Quach , R. Rogly , T. Nakamura , J. S. Jang , L. N. Machado , F. P. Soler , J. G. Learned , K. Choi , N. Iovine , S. Cao , L. H. V. Anthony , D. Martin , N. W. Prouse , M. Scott , Y. Uchida , A. A. Sztuc , V. Berardi , N. F. Calabria , M. G. Catanesi , E. Radicioni , A. Langella , G. De Rosa , G. Collazuol , M. Feltre , F. Iacob , M. Mattiazzi , L. Ludovici , M. Gonin , L. Périssé , 23 B. Quilain , C. Fujisawa , S. Horiuchi , A. Kawabata , M. Kobayashi , Y. M. Liu , Y. Maekawa , Y. Nishimura , R. Okazaki , R. Akutsu , M. Friend , T. Hasegawa , T. Ishida , T. Kobayashi , M. Jakkapu , T. Matsubara , T. Nakadaira , K. Nakamura , Y. Oyama , A. Portocarrero Yrey , K. Sakashita , T. Sekiguchi , T. Tsukamoto , N. Bhuiyan , G. T. Burton , F. Di Lodovico , J. Gao , A. Goldsack , T. Katori , J. Migenda , R. M. Ramsden , Z. Xie , S. Zsoldos , T. Sone , A. T. Suzuki , Y. Takagi , Y. Takeuchi , S. Wada , H. Zhong , J. Feng , L. Feng , J. Hikida , J. R. Hu , Z. Hu , M. Kawaue , T. Kikawa , M. Mori , T. Nakaya , T. V. Ngoc , R. A. Wendell , K. Yasutome , S. J. Jenkins , N. McCauley , A. Tarrant , P. Mehta , M. Fanì , M. J. Wilking , Y. Fukuda , Y. Itow , H. Menjo , Y. Yoshioka , K. Ninomiya , J. Lagoda , S. M. Lakshmi , M. Mandal , P. Mijakowski , Y. S. Prabhu , J. Zalipska , M. Jia , J. Jiang , C. K. Jung , W. Shi , K. Hamaguchi , Y. Hino , H. Ishino , Y. Koshio , F. Nakanishi , S. Sakai , T. Tada , T. Tano , T. Ishizuka , G. Barr , D. Barrow , L. Cook , S. Samani , D. Wark , A. Holin , F. Nova , S. Jung , J. Y. Yang , J. Yoo , J. E. P. Fannon , L. Kneale , M. Malek , J. M. McElwee , T. Peacock , P. Stowell , M. D. Thiesse , L. F. Thompson , S. T. Wilson , H. Okazawa , S. M. Lakshmi , S. B. Kim , E. Kwon , M. W. Lee , J. W. Seo , I. Yu , A. K. Ichikawa , K. D. Nakamura , S. Tairafune , K. Nishijima , A. Eguchi , S. Goto , S. Kodama , Y. Mizuno , T. Muro , K. Nakagiri , Y. Nakajima , S. Shima , N. Taniuchi , E. Watanabe , M. Yokoyama , P. de Perio , S. Fujita , C. Jesús-Valls , K. Martens , Ll. Marti , K. M. Tsui , M. R. Vagins , J. Xia , M. Kuze , S. Izumiyama , R. Matsumoto , K. Terada , R. Asaka , M. Ishitsuka , H. Ito , Y. Ommura , N. Shigeta , M. Shinoki , M. Sugo , M. Wako , K. Yamauchi , T. Yoshida , Y. Nakano , F. Cormier , R. Gaur , V. Gousy-Leblanc , M. Hartz , A. Konaka , X. Li , B. R. Smithers , S. Chen , Y. Wu , B. D. Xu , A. Q. Zhang , B. Zhang , M. Girgus , P. Govindaraj , M. Posiadala-Zezula , S. B. Boyd , R. Edwards , D. Hadley , M. Nicholson , M. O'Flaherty , B. Richards , A. Ali , B. Jamieson , S. Amanai , D. Hamaguchi , A. Minamino , Y. Sasaki , R. Shibayama , R. Shimamura , S. Suzuki

Flavour changing (FC) neutrino-matter interactions have been proposed as a solution to the atmospheric neutrino anomaly. Here we perform the analysis of the full set of the recent 52 kTy Super-Kamiokande atmospheric neutrino data, including…

High Energy Physics - Phenomenology · Physics 2009-10-31 N. Fornengo , M. C. Gonzalez-Garcia , J. W. F. Valle

The previously published atmospheric neutrino data did not distinguish whether muon neutrinos were oscillating into tau neutrinos or sterile neutrinos, as both hypotheses fit the data. Using data recorded in 1100 live-days of the…

High Energy Physics - Experiment · Physics 2008-11-26 Kamiokande Collaboration

In the minimal standard model it is possible to gauge any one of the following global symmetries in an anomaly free way: (i)$L_{e}-L_{\mu}$, (ii) $L_{e}-L_{\tau}$ or (iii) $L_{\mu}-L_{\tau}$. If the gauge boson corresponding to (i) or (ii)…

High Energy Physics - Phenomenology · Physics 2009-11-10 Anjan S. Joshipura , Subhendra Mohanty

We consider the upscattering of atmospheric neutrinos in the interior of the Earth producing heavy neutral leptons (HNLs) which subsequently decay inside large volume detectors (e.g. Super-Kamiokande or DUNE). We compute the flux of…

High Energy Physics - Phenomenology · Physics 2024-09-04 R. Andrew Gustafson , Ryan Plestid , Ian M. Shoemaker

Neutrino oscillation experiments provide a unique tool for probing neutrino-matter interactions, especially those involving the tau neutrino. We describe the sensitivity of the present atmospheric neutrino data to these interactions in the…

High Energy Physics - Phenomenology · Physics 2007-05-23 Alexander Friedland , Cecilia Lunardini , Michele Maltoni

The current status of oscillation solutions to the Solar Neutrino Problem is reviewed. Four oscillation solutions are discussed in the light of 708d Superkamiokande data: MSW, Just-So VO, VO with Energy-Independent Suppression (EIS) and…

High Energy Physics - Phenomenology · Physics 2011-08-17 V. Berezinsky

The results of solar neutrino data from the first phase of Super-Kamiokande are presented. Super-Kamiokande can measure not only the solar neutrino flux but also its energy spectrum and its time variations such as day vs night and seasonal…

High Energy Physics - Experiment · Physics 2007-05-23 Y. Koshio

A short review of the status of neutrino mixing and neutrino oscillations is given. The basics of neutrino mixing and oscillations is discussed. The latest evidences of neutrino oscillations obtained in the Super-Kamiokande and the SNO…

High Energy Physics - Phenomenology · Physics 2009-11-07 S. M. Bilenky