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The T2K (Tokai to Kamioka) experiment is a second generation long baseline neutrino oscillation experiment located in Japan. The main goal is to probe the $\theta_{13}$ neutrino mixing parameter by looking for $\nu_{\mu}\to\nu_e$…

High Energy Physics - Experiment · Physics 2019-08-14 Alexander Izmaylov

Recent results of atmospheric neutrino experiments are reviewed and their possible interpretations are discussed, main emphasis being put on the neutrino oscillation hypothesis.

High Energy Physics - Phenomenology · Physics 2009-09-25 E. Kh. Akhmedov

In the context of neutrino scenarios characterized by four (three active plus one sterile) neutrino species and by mass spectra with two separated doublets, we analyze solutions to the atmospheric neutrino anomaly which smoothly interpolate…

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

Neutrino oscillation scenarios involving large angle $\nu_{\mu} \to \nu_e$ oscillations are disfavoured in the parameter range $\Delta m^2/eV^2 >~ 10^{-3}$ by recent results from the CHOOZ reactor-based $\bar{\nu}_e$ disappearance…

High Energy Physics - Phenomenology · Physics 2007-05-23 R. Foot , R. R. Volkas , O. Yasuda

We present a formalism for precise description of oscillation phenomena in matter at high energies or high densities, V > \Delta m^2/2E, where V is the matter-induced potential of neutrinos. The accuracy of the approximation is determined…

High Energy Physics - Phenomenology · Physics 2008-11-26 E. Kh. Akhmedov , M. Maltoni , A. Yu. Smirnov

The final results of the MACRO experiment on atmospheric neutrino oscillations are presented and discussed. The data concern different event topologies with average neutrino energies of ~3 and ~50 GeV. Multiple Coulomb Scattering of the…

High Energy Physics - Experiment · Physics 2009-11-10 G. Giacomelli , A. Margiotta

The Kamiokande II and IMB data on contained events induced by atmospheric neutrinos exhibit too low a ratio of muons to electrons, which has been interpreted as a possible indication of neutrino oscillations. At the same time, the recent…

High Energy Physics - Phenomenology · Physics 2008-11-26 E. Akhmedov , P. Lipari , M. Lusignoli

Hyper-Kamiokande will be a next generation underground water Cherenkov detector with a total (fiducial) mass of 0.99 (0.56) million metric tons, approximately 20 (25) times larger than that of Super-Kamiokande. One of the main goals of…

High Energy Physics - Experiment · Physics 2015-05-20 Hyper-Kamiokande Proto-Collaboraion , : , K. Abe , H. Aihara , C. Andreopoulos , I. Anghel , A. Ariga , T. Ariga , R. Asfandiyarov , M. Askins , J. J. Back , P. Ballett , M. Barbi , G. J. Barker , G. Barr , F. Bay , P. Beltrame , V. Berardi , M. Bergevin , S. Berkman , T. Berry , S. Bhadra , F. d. M. Blaszczyk , A. Blondel , S. Bolognesi , S. B. Boyd , A. Bravar , C. Bronner , F. S. Cafagna , G. Carminati , S. L. Cartwright , M. G. Catanesi , K. Choi , J. H. Choi , G. Collazuol , G. Cowan , L. Cremonesi , G. Davies , G. De Rosa , C. Densham , J. Detwiler , D. Dewhurst , F. Di Lodovico , S. Di Luise , O. Drapier , S. Emery , A. Ereditato , P. Fernández , T. Feusels , A. Finch , M. Fitton , M. Friend , Y. Fujii , Y. Fukuda , D. Fukuda , V. Galymov , K. Ganezer , M. Gonin , P. Gumplinger , D. R. Hadley , L. Haegel , A. Haesler , Y. Haga , B. Hartfiel , M. Hartz , Y. Hayato , M. Hierholzer , J. Hill , A. Himmel , S. Hirota , S. Horiuchi , K. Huang , A. K. Ichikawa , T. Iijima , M. Ikeda , J. Imber , K. Inoue , J. Insler , R. A. Intonti , T. Irvine , T. Ishida , H. Ishino , M. Ishitsuka , Y. Itow , A. Izmaylov , B. Jamieson , H. I. Jang , M. Jiang , K. K. Joo , C. K. Jung , A. Kaboth , T. Kajita , J. Kameda , Y. Karadhzov , T. Katori , E. Kearns , M. Khabibullin , A. Khotjantsev , J. Y. Kim , S. B. Kim , Y. Kishimoto , T. Kobayashi , M. Koga , A. Konaka , L. L. Kormos , A. Korzenev , Y. Koshio , W. R. Kropp , Y. Kudenko , T. Kutter , M. Kuze , L. Labarga , J. Lagoda , M. Laveder , M. Lawe , J. G. Learned , I. T. Lim , T. Lindner , A. Longhin , L. Ludovici , W. Ma , L. Magaletti , K. Mahn , M. Malek , C. Mariani , L. Marti , J. F. Martin , C. Martin , P. P. J. Martins , E. Mazzucato , N. McCauley , K. S. McFarland , C. McGrew , M. Mezzetto , H. Minakata , A. Minamino , S. Mine , O. Mineev , M. Miura , J. Monroe , T. Mori , S. Moriyama , T. Mueller , F. Muheim , M. Nakahata , K. Nakamura , T. Nakaya , S. Nakayama , M. Needham , T. Nicholls , M. Nirkko , Y. Nishimura , E. Noah , J. Nowak , H. Nunokawa , H. M. O'Keeffe , Y. Okajima , K. Okumura , S. M. Oser , E. O'Sullivan , T. Ovsiannikova , R. A. Owen , Y. Oyama , J. Pérez , M. Y. Pac , V. Palladino , J. L. Palomino , V. Paolone , D. Payne , O. Perevozchikov , J. D. Perkin , C. Pistillo , S. Playfer , M. Posiadala-Zezula , J. -M. Poutissou , B. Quilain , M. Quinto , E. Radicioni , P. N. Ratoff , M. Ravonel , M. A. Rayner , A. Redij , F. Retiere , C. Riccio , E. Richard , E. Rondio , H. J. Rose , M. Ross-Lonergan , C. Rott , S. D. Rountree , A. Rubbia , R. Sacco , M. Sakuda , M. C. Sanchez , E. Scantamburlo , K. Scholberg , M. Scott , Y. Seiya , T. Sekiguchi , H. Sekiya , A. Shaikhiev , I. Shimizu , M. Shiozawa , S. Short , G. Sinnis , M. B. Smy , J. Sobczyk , H. W. Sobel , T. Stewart , J. L. Stone , Y. Suda , Y. Suzuki , A. T. Suzuki , R. Svoboda , R. Tacik , A. Takeda , A. Taketa , Y. Takeuchi , H. A. Tanaka , H. K. M. Tanaka , H. Tanaka , R. Terri , L. F. Thompson , M. Thorpe , S. Tobayama , N. Tolich , T. Tomura , C. Touramanis , T. Tsukamoto , M. Tzanov , Y. Uchida , M. R. Vagins , G. Vasseur , R. B. Vogelaar , C. W. Walter , D. Wark , M. O. Wascko , A. Weber , R. Wendell , R. J. Wilkes , M. J. Wilking , J. R. Wilson , T. Xin , K. Yamamoto , C. Yanagisawa , T. Yano , S. Yen , N. Yershov , M. Yokoyama , M. Zito

The predictions of the atmospheric nu event rates are affected by significant uncertainties, however the evidence for the `disappearance' of nu_mu's and nubar_mu's obtained by SK (and other underground detectors) is robust and cannot be…

High Energy Physics - Phenomenology · Physics 2007-05-23 Paolo Lipari

The muon and anti-muon neutrino energy spectrum is determined from 2000-2003 AMANDA telescope data using regularised unfolding. This is the first measurement of atmospheric neutrinos in the energy range 2 - 200 TeV. The result is compared…

High Energy Astrophysical Phenomena · Physics 2014-11-20 IceCube Collaboration , R. Abbasi

Using 5,326 days of atmospheric neutrino data, a search for atmospheric tau neutrino appearance has been performed in the Super-Kamiokande experiment. Super-Kamiokande measures the tau normalization to be 1.47$\pm$0.32 under the assumption…

High Energy Physics - Experiment · Physics 2018-09-19 Kamiokande Collaboration , Z. Li , K. Abe , C. Bronner , Y. Hayato , M. Ikeda , K. Iyogi , J. Kameda , Y. Kato , Y. Kishimoto , Ll. Marti , M. Miura , S. Moriyama , M. Nakahata , Y. Nakajima , Y. Nakano , S. Nakayama , A. Orii , G. Pronost , H. Sekiya , M. Shiozawa , Y. Sonoda , A. Takeda , A. Takenaka , H. Tanaka , S. Tasaka , T. Tomura , R. Akutsu , T. Kajita , Y. Nishimura , K. Okumura , K. M. Tsui , P. Fernandez , L. Labarga , F. d. M. Blaszczyk , J. Gustafson , C. Kachulis , E. Kearns , J. L. Raaf , J. L. Stone , L. R. Sulak , S. Berkman , S. Tobayama , M. Elnimr , W. R. Kropp , S. Locke , S. Mine , P. Weatherly , M. B. Smy , H. W. Sobel , V. Takhistov , K. S. Ganezer , J. Hill , J. Y. Kim , I. T. Lim , R. G. Park , A. Himmel , E. O'Sullivan , K. Scholberg , C. W. Walter , T. Ishizuka , T. Nakamura , J. S. Jang , K. Choi , J. G. Learned , S. Matsuno , S. N. Smith , J. Amey , R. P. Litchfield , W. Y. Ma , Y. Uchida , M. O. Wascko , S. Cao , M. Friend , T. Hasegawa , T. Ishida , T. Ishii , T. Kobayashi , T. Nakadaira , K. Nakamura , Y. Oyama , K. Sakashita , T. Sekiguchi , T. Tsukamoto , KE. Abe , M. Hasegawa , A. T. Suzuki , Y. Takeuchi , T. Yano , T. Hayashino , T. Hiraki , S. Hirota , K. Huang , M. Jiang , M. Mori , KE. Nakamura , T. Nakaya , N. D. Patel , R. A. Wendell , L. H. V. Anthony , N. McCauley , A. Pritchard , Y. Fukuda , Y. Itow , M. Murase , F. Muto , P. Mijakowski , K. Frankiewicz , C. K. Jung , X. Li , J. L. Palomino , G. Santucci , C. Vilela , M. J. Wilking , C. Yanagisawa , G. Yang , S. Ito , D. Fukuda , H. Ishino , A. Kibayashi , Y. Koshio , H. Nagata , M. Sakuda , C. Xu , Y. Kuno , D. Wark , F. Di Lodovico , B. Richards , S. M. Sedgwick , R. Tacik , S. B. Kim , A. Cole , L. Thompson , H. Okazawa , Y. Choi , K. Ito , K. Nishijima , M. Koshiba , Y. Suda , M. Yokoyama , R. G. Calland , M. Hartz , K. Martens , M. Murdoch , B. Quilain , C. Simpson , Y. Suzuki , M. R. Vagins , D. Hamabe , M. Kuze , Y. Okajima , T. Yoshida , M. Ishitsuka , J. F. Martin , C. M. Nantais , H. A. Tanaka , T. Towstego , A. Konaka , S. Chen , L. Wan , Y. Zhang , A. Minamino , R. J. Wilkes

Current status of the K2K (KEK to Kamioka) long-baseline neutrino-oscillation experiment is presented.

High Energy Physics - Experiment · Physics 2007-05-23 Yuichi Oyama

Using the published Kamiokande data of the multi-GeV atmospheric neutrinos, we have searched the optimum set of the neutrino oscillation parameters among three flavors. It is found that $\chi^2$ is minimized for ($\Delta m_{21}^2$, $\Delta…

High Energy Physics - Phenomenology · Physics 2007-05-23 Osamu Yasuda

The recent results from Super-Kamiokande (SK) are reported. On atmospheric neutrino analysis, we have performed a full 3-flavor oscillation analysis with SK-I+II+III data. A CPT violation study on atmospheric neutrino is also done with…

High Energy Physics - Experiment · Physics 2019-08-14 Yasuo Takeuchi

The history and recent progress of atmospheric neutrinos are reviewed. An emphasis is placed on results from experiments other than Super-Kamiokande.

High Energy Physics - Experiment · Physics 2009-11-07 Maury Goodman

We have reconsidered the atmospheric neutrino anomaly in light of the laetst data from Super-Kamiokande contained events and from Super-Kamiokande and MACRO up-going muons. We have reanalysed the proposed solution to the atmospheric…

High Energy Physics - Phenomenology · Physics 2010-05-28 N. Fornengo , M. Maltoni , R. Tomas , J. W. F. Valle

The SuperKamiokande group assert that they have found an oscillatory signature in atmospheric neutrinos through the analysis of \textit{Fully Contained Events} and \textit{Partially Contained Events}. We have performed an $L/E$…

High Energy Physics - Experiment · Physics 2007-05-23 N. Takahashi , A. Misaki

Vacuum oscillations are considered for the combined solar neutrino observations, including the Kamiokande II spectrum data and incorporating theoretical uncertainties and their correlations. Despite the conceptual difficulty of the fine…

High Energy Physics - Phenomenology · Physics 2007-05-23 Naoya Hata

A search for the appearance of tau neutrinos from \mutau oscillations in the atmospheric neutrinos has been performed using 1489.2 days of atmospheric neutrino data from the Super-Kamiokande-I experiment. A best fit tau neutrino appearance…

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

I review the history on neutrino magnetic moments and apply the neurino magnetic moment idea to constrain its bound from Super-Kamiokande neutrino oscillation data.

High Energy Physics - Phenomenology · Physics 2007-05-23 Jihn E. Kim