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Related papers: Hyper-Kamiokande

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A variety of new physics scenarios allow for neutrinos to up-scatter into a heavy neutral lepton state. For a range of couplings and neutrino energies, the heavy neutrino may travel some distance before decaying to visible final states.…

High Energy Physics - Phenomenology · Physics 2022-10-31 Mack Atkinson , Pilar Coloma , Ivan Martinez-Soler , Noemi Rocco , Ian M. Shoemaker

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

The atmospheric neutrino background for proton decay to positron and neutral pion in ring imaging water Cherenkov detectors is studied with an artificial accelerator neutrino beam for the first time. In total, about 314,000 neutrino events…

High Energy Physics - Experiment · Physics 2008-11-26 K2K Collaboration , S. Mine

The largest Solar flare have been recorded in gamma flash and hard spectra up to tens GeV energy. The present building and upgrade of Hyper-Kamiokande (HK) and IceCube (as well as Deep Core, PINGU) neutrino detectors do offer a novel way to…

High Energy Astrophysical Phenomena · Physics 2017-07-10 Daniele Fargion , Pietro Oliva

A set of quantitative predictions for the day-night asymmetry in the Super - Kamiokande detector is presented. For these predictions, neutrino events are collected in ``samples'' defined by the trajectories in the Earth of the corresponding…

High Energy Physics - Phenomenology · Physics 2007-05-23 Michele Maris

Neutrino physics is an experimentally driven field. So, we investigate the different detection techniques available in the literature and study the various neutrino oscillation experiments in a chronological manner. Our primary focus is on…

High Energy Physics - Phenomenology · Physics 2021-06-01 Ankur Nath , Ng. K. Francis

The discrepancy of the measured solar neutrino flux compared to the predictions of the standard solar model may be explained by the neutrino flavor oscillation hypothesis. A more direct and less model-dependent test of this hypothesis is a…

High Energy Physics - Experiment · Physics 2007-05-23 Michael B Smy

In Japan, as the first experiment utilizes J-PARC (Japan Proton Accelerator Research Complex) neutrino facility, T2K (Tokai to Kamioka Long Baseline Neutrino Experiment) starts operation. T2K is supposed to give critical information, which…

High Energy Physics - Experiment · Physics 2010-01-05 Takuya Hasegawa

The physics potential of high intensity conventional beams is explored. We consider a low energy super beam which could be produced by a proposed new accelerator at CERN, the Super Proton Linac. Water Cherenkov and liquid oil scintillator…

High Energy Physics - Phenomenology · Physics 2007-05-23 J. J. Gomez-Cadenas , A. Blondel , J. Burguet-Castell , D. Casper , M. DOnega , S. Gilardoni , P. Hernandez , M. Mezzetto

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

Atmospheric neutrino and solar neutrino data from the first phase of Super-Kamiokande (SK-I) are presented. The observed data are used to study atmospheric and solar neutrino oscillations. Zenith angle distributions from various atmospheric…

High Energy Physics - Experiment · Physics 2019-08-14 M. Ishitsuka

Testing, in a non-trivial, model-independent way, the hypothesis that the three-massive-neutrinos paradigm properly describes nature is among the main goals of the current and the next generation of neutrino oscillation experiments. In the…

High Energy Physics - Phenomenology · Physics 2017-11-22 André de Gouvêa , Kevin J. Kelly

Tokai-to-Kamioka T2K is a long baseline neutrino oscillation experiment, looking for sub-dominant muon neutrino to electron neutrino oscillations. One of the primary aims of the T2K experiment is to narrow down the current limit on the…

High Energy Physics - Experiment · Physics 2010-06-08 Melissa George

The NEMO project aims at the search, development and validation of key technologies for the construction, deployment and mantainance of an underwater Cherenkov km3 neutrino telescope in the Mediterranean Sea. Moreover, the NEMO…

Astrophysics · Physics 2007-05-23 Piera Sapienza

Recent Super-Kamiokande data on the atmospheric neutrino anomaly are used to test various mechanisms for neutrino oscillations. It is found that the current atmospheric neutrino data alone cannot rule out any particular mechanism. Future…

High Energy Physics - Phenomenology · Physics 2008-11-26 R. Foot , C. N. Leung , O. Yasuda

Hyper-Kamiokande (HK) is the world's largest water Cherenkov ring-imaging detector, planning to start data taking in 2028. The Outer Detector (OD) surrounds the Inner Detector and plays a critical role in rejecting background events…

Instrumentation and Detectors · Physics 2026-05-13 R. Shinoda

Some of the earliest work on neutrino astronomy was accomplished by a class of underground detectors primarily designed for particle physics goals . These detectors used inexpensive water to obtain the large masses needed to observe the…

High Energy Astrophysical Phenomena · Physics 2022-02-04 John M. LoSecco

T2K is a long-baseline neutrino oscillation experiment, in which a muon-neutrino beam is directed over a 295 km baseline from the J-PARC facility to the Super-Kamiokande detector. This allows neutrino oscillation to be studied in two…

High Energy Physics - Experiment · Physics 2019-08-14 Kirsty Duffy

This is a contribution paper of the XXth International Conference on Neutrino Physics and Astrophysics (Neutrino2002) and YITP workshop.

High Energy Physics - Phenomenology · Physics 2009-11-07 N. Okamura
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