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In this talk we present our results on the sensitivity to the neutrino mass hierarchy, the octant of the mixing angle and the CP phase in the future long baseline experiments T2HK and DUNE as well as in the atmospheric neutrino observation…

High Energy Physics - Phenomenology · Physics 2016-11-01 Osamu Yasuda , Shinya Fukasawa , Monojit Ghosh

Seesaw-type and low-scale models of neutrino masses are reviewed, along with the corresponding structure of the lepton mixing matrix. The status of neutrino oscillation parameters as of June 2006 is given, including recent fluxes, as well…

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

A problem, whether a neutrino-antineutrino transition could be responsible for the muon neutrino deficit found in underground experiments (Super-Kamiokande, MACRO, Soudan 2) and in the accelerator long-baseline K2K experiment, is discussed…

High Energy Physics - Phenomenology · Physics 2007-05-23 E. N. Alexeyev , L. V. Volkova

We perform a global analysis of neutrino oscillation data in the framework of three neutrinos, including the recent improved measurement of the neutral current events at SNO. In addition to all current solar neutrino data we take into…

High Energy Physics - Phenomenology · Physics 2009-09-17 M. Maltoni , T. Schwetz , M. A. Tortola , J. W. F. Valle

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 look into the recent puzzlng results from MiniBooNE and contrast their results with that from NOMAD. A pictuire which provides consistent decscriptiobn of both is discussed here. This also points to future directions in neutrino studies.

General Physics · Physics 2011-03-24 Syed Afsar Abbas , Shakeb Ahmad

Super-Kamiokande collaboration assumes that the direction of every observed lepton coincides with the incoming direction of the incident neutrino, which is the fundamental basement throughout all their analysis on neutrino oscillation. We…

High Energy Physics - Experiment · Physics 2009-09-29 E. Konishi , Y. Minorikawa , V. I. Galkin , M. Ishiwata , I. Nakamura , N. Takahashi , M. Kato , A. Misaki

The Super-Kamiokande experiment has collected a large sample of high-energy neutrino events. These are primarily atmospheric neutrinos, but a bright enough astrophysical source could also be visible. The data have been examined for possible…

Astrophysics · Physics 2007-05-23 A. Habig

We study the robustness of the determination of the neutrino masses and mixing from the analysis of atmospheric and K2K data under the presence of different forms of phenomenologically allowed new physics in the nu_mu--nu_tau sector. We…

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

The latest results from K2K experiment are reported, with focus on muon neutrino oscillation. The results are based on data taken from June 1999 to February 2004, corresponding to 8.9 x 10^19 protons on target.

High Energy Physics - Experiment · Physics 2007-05-23 C. Mariani , for K2K Collaboration

Various statistical issues relevant to searches for new physics or to parameter determination in analyses of data in neutrino experiments are briefly discussed.

High Energy Physics - Experiment · Physics 2016-07-14 Louis Lyons

I review the current status of neutrino astrophysics, including solar neutrinos; atmospheric neutrinos; neutrino mass and oscillations; supernova neutrinos; neutrino nucleosynthesis (Big Bang nucleosynthesis, the neutrino process, the…

Nuclear Theory · Physics 2008-08-07 W. C. Haxton

Cosmology provides an excellent laboratory for testing various aspects of neutrino physics. Here, I review the current status of cosmological searches for neutrino mass, as well as other properties of neutrinos. Future cosmological probes…

High Energy Physics - Phenomenology · Physics 2010-10-27 Steen Hannestad

The theoretical motivations, experimental searches/hints, and implications of neutrino mass are surveyed.

High Energy Physics - Phenomenology · Physics 2016-09-01 Paul Langacker

In this talk I review measurements and calculations of the flux of neutrinos produced by interactions of cosmic rays in the atmosphere. The main reason for interest in this subject is the apparent anomaly between the predicted and the…

High Energy Physics - Phenomenology · Physics 2007-05-23 T. K. Gaisser

This article reviews the many new results from neutrino oscillation searches which were presented at ICHEP '98. Exciting indications of neutrino oscillations have been seen in the solar neutrino deficit, atmospheric neutrino deficit and…

High Energy Physics - Experiment · Physics 2007-05-23 J. M. Conrad

The T2K collaboration: reports evidence for electron neutrino appearance at the atmospheric mass splitting, |\Delta m_{32}^2|=2.4x10^{-3} eV^2. An excess of electron neutrino interactions over background is observed from a muon neutrino…

High Energy Physics - Experiment · Physics 2019-08-17 T2K Collaboration , K. Abe , N. Abgrall , H. Aihara , T. Akiri , J. B. Albert , C. Andreopoulos , S. Aoki , A. Ariga , T. Ariga , S. Assylbekov , D. Autiero , M. Barbi , G. J. Barker , G. Barr , M. Bass , M. Batkiewicz , F. Bay , S. W. Bentham , V. Berardi , B. E. Berger , S. Berkman , I. Bertram , D. Beznosko , S. Bhadra , F. d. M. Blaszczyk , A. Blondel , C. Bojechko , S. Boyd , D. Brailsford , A. Bravar , C. Bronner , D. G. Brook-Roberge , N. Buchanan , R. G. Calland , J. Caravaca Rodriguez , S. L. Cartwright , R. Castillo , M. G. Catanesi , A. Cervera , D. Cherdack , G. Christodoulou , A. Clifton , J. Coleman , S. J. Coleman , G. Collazuol , K. Connolly , L. Cremonesi , A. Curioni , A. Dabrowska , I. Danko , R. Das , S. Davis , M. Day , J. P. A. M. de Andre , P. de Perio , G. De Rosa , T. Dealtry , S. Dennis , C. Densham , F. Di Lodovico , S. Di Luise , J. Dobson , O. Drapier , T. Duboyski , F. Dufour , J. Dumarchez , S. Dytman , M. Dziewiecki , M. Dziomba , S. Emery , A. Ereditato , L. Escudero , A. J. Finch , E. Frank , M. Friend , Y. Fujii , Y. Fukuda , A. Furmanski , V. Galymov , A. Gaudin , S. Giffin , C. Giganti , K. Gilje , T. Golan , J. J. Gomez-Cadenas , M. Gonin , N. Grant , D. Gudin , D. R. Hadley , A. Haesler , M. D. Haigh , P. Hamilton , D. Hansen , T. Hara , M. Hartz , T. Hasegawa , N. C. Hastings , Y. Hayato , C. Hearty , R. L. Helmer , M. Hierholzer , J. Hignight , A. Hillairet , A. Himmel , T. Hiraki , S. Hirota , J. Holeczek , S. Horikawa , K. Huang , A. K. Ichikawa , K. Ieki , M. Ieva , M. Ikeda , J. Imber , J. Insler , T. J. Irvine , T. Ishida , T. Ishii , S. J. Ives , K. Iyogi , A. Izmaylov , A. Jacob , B. Jamieson , R. A. Johnson , J. H. Jo , P. Jonsson , K. K. Joo , C. K. Jung , A. Kaboth , H. Kaji , T. Kajita , H. Kakuno , J. Kameda , Y. Kanazawa , D. Karlen , I. Karpikov , E. Kearns , M. Khabibullin , F. Khanam , A. Khotjantsev , D. Kielczewska , T. Kikawa , A. Kilinski , J. Y. Kim , J. Kim , S. B. Kim , B. Kirby , J. Kisiel , P. Kitching , T. Kobayashi , G. Kogan , A. Kolaceke , A. Konaka , L. L. Kormos , A. Korzenev , K. Koseki , Y. Koshio , K. Kowalik , I. Kreslo , W. Kropp , H. Kubo , Y. Kudenko , S. Kumaratunga , R. Kurjata , T. Kutter , J. Lagoda , K. Laihem , A. Laing , M. Laveder , M. Lawe , M. Lazos , K. P. Lee , C. Licciardi , I. T. Lim , T. Lindner , C. Lister , R. P. Litchfield , A. Longhin , G. D. Lopez , L. Ludovici , M. Macaire , L. Magaletti , K. Mahn , M. Malek , S. Manly , A. Marchionni , A. D. Marino , J. Marteau , J. F. Martin , T. Maruyama , J. Marzec , P. Masliah , E. L. Mathie , V. Matveev , K. Mavrokoridis , E. Mazzucato , N. McCauley , K. S. McFarland , C. McGrew , T. McLachlan , M. Messina , C. Metelko , M. Mezzetto , P. Mijakowski , C. A. Miller , A. Minamino , O. Mineev , S. Mine , A. Missert , M. Miura , L. Monfregola , S. Moriyama , Th. A. Mueller , A. Murakami , M. Murdoch , S. Murphy , J. Myslik , T. Nagasaki , T. Nakadaira , M. Nakahata , T. Nakai , K. Nakajima , K. Nakamura , S. Nakayama , T. Nakaya , K. Nakayoshi , D. Naples , T. C. Nicholls , C. Nielsen , M. Nirkko , K. Nishikawa , Y. Nishimura , H. M. O'Keeffe , Y. Obayashi , R. Ohta , K. Okumura , T. Okusawa , W. Oryszczak , S. M. Oser , M. Otani , R. A. Owen , Y. Oyama , M. Y. Pac , V. Palladino , V. Paolone , D. Payne , G. F. Pearce , O. Perevozchikov , J. D. Perkin , Y. Petrov , E. S. Pinzon Guerra , P. Plonski , E. Poplawska , B. Popov , M. Posiadala , J. -M. Poutissou , R. Poutissou , P. Przewlocki , B. Quilain , E. Radicioni , P. N. Ratoff , M. Ravonel , M. A. M. Rayner , M. Reeves , E. Reinherz-Aronis , F. Retiere , A. Robert , P. A. Rodrigues , E. Rondio , S. Roth , A. Rubbia , D. Ruterbories , R. Sacco , K. Sakashita , F. Sanchez , E. Scantamburlo , K. Scholberg , J. Schwehr , M. Scott , D. I. Scully , Y. Seiya , T. Sekiguchi , H. Sekiya , D. Sgalaberna , M. Shibata , M. Shiozawa , S. Short , Y. Shustrov , P. Sinclair , B. Smith , R. J. Smith , M. Smy , J. T. Sobczyk , H. Sobel , M. Sorel , L. Southwell , P. Stamoulis , J. Steinmann , B. Still , A. Suzuki , K. Suzuki , S. Y. Suzuki , Y. Suzuki , T. Szeglowski , M. Szeptycka , R. Tacik , M. Tada , S. Takahashi , A. Takeda , Y. Takeuchi , H. A. Tanaka , M. M. Tanaka , M. Tanaka , I. J. Taylor , D. Terhorst , R. Terri , L. F. Thompson , A. Thorley , S. Tobayama , W. Toki , T. Tomura , Y. Totsuka , C. Touramanis , T. Tsukamoto , M. Tzanov , Y. Uchida , K. Ueno , A. Vacheret , M. Vagins , G. Vasseur , T. Wachala , A. V. Waldron , C. W. Walter , D. Wark , M. O. Wascko , A. Weber , R. Wendell , R. J. Wilkes , M. J. Wilking , C. Wilkinson , Z. Williamson , J. R. Wilson , R. J. Wilson , T. Wongjirad , Y. Yamada , K. Yamamoto , C. Yanagisawa , S. Yen , N. Yershov , M. Yokoyama , T. Yuan , A. Zalewska , L. Zambelli , K. Zaremba , M. Ziembicki , E. D. Zimmerman , M. Zito , J. Zmuda

Neutrinos from a future Galactic supernova will be detected by several large underground detectors, in particular by SuperKamiokande (SK) and the Sudbury Neutrino Observatory (SNO). If, as expected, the $\nu_{\mu}$ and $\nu_{\tau}$…

Astrophysics · Physics 2007-05-23 Petr Vogel

Recent experimental results and developments in the theoretical treatment of neutrino-nucleus interactions in the energy range of 1-10 GeV are discussed. Difficulties in extracting neutrino-nucleon cross sections from neutrino-nucleus…

High Energy Physics - Experiment · Physics 2012-10-01 Jorge G. Morfin , Juan Nieves , Jan T. Sobczyk

Interference phenomena of neutrinos are studied. High energy neutrino in T2K near detector and low energy neutrino in KamLAND are possible experiments that could show macroscopic interferences of neutrino waves. In both experiments…

High Energy Physics - Phenomenology · Physics 2010-03-10 K. Ishikawa , Y. Tobita