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The PANDA experiment at the FAIR facility at GSI will study hadron physics using a high intensity antiproton beam of up to 15 GeV/c momentum to perform high precision spectroscopy. Two DIRC detectors with their image planes residing in an…

High energy physics community is continuously working on development of new photodetectors able to improve their experiments detection performances and so to increase the possibility of new discoveries and new important scientific results.…

Instrumentation and Detectors · Physics 2020-04-28 F. C. T. Barbato , G. Barbarino

Large-scale optical neutrino and dark-matter detectors rely on large-area photomultiplier tubes (PMTs) for cost-effective light detection. The new R14688-100 8-inch PMT developed by Hamamatsu provides state-of-the-art timing resolution of…

Many of the yet unanswered questions in neutrino physics, such as CP violation in the lepton sector or neutrino mass hierarchy, could be answered with higher sensitivity neutrino experiments. New photodetectors based on micro-channel plates…

Instrumentation and Detectors · Physics 2013-10-11 Ioana Anghel

Water Cherenkov detectors like Super-Kamiokande, and the next generation Hyper-Kamiokande are adding gadolinium to their water to improve the detection of neutrons. By detecting neutrons in addition to the leptons in neutrino interactions,…

Instrumentation and Detectors · Physics 2023-01-16 Blair Jamieson , Matt Stubbs , Sheela Ramanna , John Walker , Nick Prouse , Ryosuke Akutsu , Patrick de Perio , Wojciech Fedorko

In this talk, we show the physics impacts of putting a large Water Cerenkov detector in Korea during the T2K experimental period. The T2K experiment which will start in 2009 plans to use the high intensity conventional neutrino beam from…

High Energy Physics - Phenomenology · Physics 2007-05-23 Naotoshi Okamura

The T2K collaboration reports a precision measurement of muon neutrino disappearance with an off-axis neutrino beam with a peak energy of 0.6 GeV. Near detector measurements are used to constrain the neutrino flux and cross section…

High Energy Physics - Experiment · Physics 2013-11-25 T2K collaboration , K. Abe , N. Abgrall , H. Aihara , T. Akiri , 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 , S. Bhadra , F. d. M. Blaszczyk , A. Blondel , C. Bojechko , S. B. Boyd , D. Brailsford , A. Bravar , C. Bronner , 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 , P. de Perio , G. De Rosa , T. Dealtry , S. R. Dennis , C. Densham , F. Di Lodovico , S. Di Luise , O. Drapier , T. Duboyski , F. Dufour , J. Dumarchez , S. Dytman , M. Dziewiecki , S. Emery , A. Ereditato , L. Escudero , A. J. Finch , E. Frank , M. Friend , Y. Fujii , Y. Fukuda , A. P. 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. C. Kaboth , T. Kajita , H. Kakuno , J. Kameda , Y. Kanazawa , D. Karlen , I. Karpikov , E. Kearns , M. Khabibullin , A. Khotjantsev , D. Kielczewska , T. Kikawa , A. Kilinski , J. Kim , S. B. Kim , J. Kisiel , P. Kitching , T. Kobayashi , G. Kogan , A. Kolaceke , A. Konaka , L. L. Kormos , A. Korzenev , K. Koseki , Y. Koshio , I. Kreslo , W. Kropp , H. Kubo , Y. Kudenko , S. Kumaratunga , R. Kurjata , T. Kutter , J. Lagoda , K. Laihem , 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. 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 , C. Metelko , 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. Nakamura , S. Nakayama , T. Nakaya , K. Nakayoshi , C. Nielsen , M. Nirkko , K. Nishikawa , Y. Nishimura , H. M. O'Keeffe , 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 , C. Pistillo , 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 , A. Redij , 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 , Y. Seiya , T. Sekiguchi , H. Sekiya , D. Sgalaberna , 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 , Y. Suda , A. Suzuki , K. Suzuki , S. Y. Suzuki , Y. Suzuki , T. Szeglowski , R. Tacik , M. Tada , S. Takahashi , A. Takeda , Y. Takeuchi , H. A. Tanaka , M. 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 , J. Zalipska , L. Zambelli , K. Zaremba , M. Ziembicki , E. D. Zimmerman , M. Zito , J. Zmuda

Photomultiplier tubes (PMTs) are widely used in neutrino and other experiments for the detection of weak light. To date PMTs are the most sensitive single photon detector per unit area. In addition to the quantum efficiency for photon…

Instrumentation and Detectors · Physics 2019-09-23 Liang-Jian Wen , Miao He , Yi-Fang Wang , Jun Cao , Shu-Lin Liu , Yue-Kun Heng , Zhong-Hua Qin

The Deep Underground Neutrino Experiment (DUNE) is a long-baseline neutrino oscillation experiment aiming to measure the oscillation parameters with an unprecedented precision that will allow determining the CP violation phase in the…

High Energy Physics - Experiment · Physics 2024-12-20 J. Soto-Oton

The optical module of the KM3NeT neutrino telescope is an innovative, multi-faceted large area photodetection module. It contains 31 three-inch photomultiplier tubes in a single 0.44 m diameter pressure-resistant glass sphere. The module is…

Instrumentation and Methods for Astrophysics · Physics 2022-03-21 KM3NeT Collaboration

We have developed an accurate simulation model of the large 9 inch photomultiplier tubes (PMT) used in water-Cherenkov detectors of cosmic-ray induced extensive air-showers. This work was carried out as part of the development of the…

Instrumentation and Detectors · Physics 2014-11-20 Alexandre Creusot , Darko Veberic

This paper describes the analysis to estimate the sensitivity of the Hyper-Kamiokande experiment to long-baseline neutrino oscillation parameters using accelerator (anti)neutrinos. Results are presented for the CPV discovery sensitivity and…

High Energy Physics - Experiment · Physics 2025-05-22 Kamiokande Collaboration

The Large High Altitude Air Shower Observatory (LHAASO) project has been proposed for the survey and study of cosmic rays. In the LHAASO project, the Water Cherenkov Detector Array (WCDA) is one of major detectors for searching gamma ray…

Instrumentation and Detectors · Physics 2016-01-20 Weihao Wu , Lei Zhao , Yu Liang , Li Yu , Jianfeng Liu , Shubin Liu , Qi An

Jinping Neutrino Experiment plans to deploy a new type of 8-inch MCP-PMT with high photon detection efficiency for MeV-scale neutrino measurements. This work studies the performance of the MCP-PMTs, including the photon detection…

High Energy Physics - Experiment · Physics 2023-07-17 Aiqiang Zhang , Benda Xu , Jun Weng , Huiyou Chen , Wenhui Shao , Tong Xu , Ling Ren , Sen Qian , Zhe Wang , Shaomin Chen

In recent years, large underwater telescopes have been designed and realized to measure high energy neutrinos from astrophysical objects. Muon tracks produced by the neutrino interaction in the surrounding medium are reconstructed from the…

The Tokai to Kamioka (T2K) experiment uses a beam of muon neutrinos, produced at the J-PARC facility on the east coast of Japan, to study neutrino oscillations driven by the $\Delta m_{\textrm{atm}}^{2}$ mass splitting. A suite of near…

High Energy Physics - Experiment · Physics 2015-01-20 Martin David Haigh

The Belle-II experiment and superKEKB accelerator will form a next generation B-factory at KEK, capable of running at an instantaneous luminosity 40 times higher than the Belle detector and KEKB. This will allow for the elucidation of many…

Instrumentation and Detectors · Physics 2013-10-18 Matthew Barrett

The first prototype of a photo-detection unit of the future KM3NeT neutrino telescope has been deployed in the deep waters of the Mediterranean Sea. This digital optical module has a novel design with a very large photocathode area…

Instrumentation and Methods for Astrophysics · Physics 2015-06-19 S. Adrián-Martínez , M. Ageron , F. Aharonian , S. Aiello , A. Albert , F. Ameli , E. G. Anassontzis , M. Anghinolfi , G. Anton , S. Anvar , M. Ardid , R. de Asmundis , K. Balasi , H. Band , G. Barbarino , E. Barbarito , F. Barbato , B. Baret , S. Baron , A. Belias , E. Berbee , A. M. van den Berg , A. Berkien , V. Bertin , S. Beurthey , V. van Beveren , N. Beverini , S. Biagi , S. Bianucci , M. Billault , A. Birbas , H. Boer Rookhuizen , R. Bormuth , V. Bouche , B. Bouhadef , G. Bourlis , M. Bouwhuis , C. Bozza , R. Bruijn , J. Brunner , G. Cacopardo , L. Caillat , M. Calamai , D. Calvo , A. Capone , L. Caramete , F. Caruso , S. Cecchini , A. Ceres , R. Cereseto , C. Champion , F. Chateau , T. Chiarusi , B. Christopoulou , M. Circella , L. Classen , R. Cocimano , S. Colonges , R. Coniglione , A. Cosquer , M. Costa , P. Coyle , A. Creusot , C. Curtil , G. Cuttone , C. D'Amato , A. D'Amico , G. De Bonis , G. De Rosa , N. Deniskina , J. -J. Destelle , C. Distefano , C. Donzaud , D. Dornic , Q. Dorosti-Hasankiadeh , E. Drakopoulou7 , D. Drouhin , L. Drury , D. Durand , T. Eberl , C. Eleftheriadis , D. Elsaesser , A. Enzenhofer , P. Fermani , L. A. Fusco , D. Gajana , T. Gal , S. Galata , F. Gallo , F. Garufi , M. Gebyehu , V. Giordano , N. Gizani , R. Gracia Ruiz , K. Graf , R. Grasso , G. Grella , A. Grmek , R. Habel , H. van Haren , T. Heid , A. Heijboer , E. Heine , S. Henry , J. J. Hernandez-Rey , B. Herold , M. A. Hevinga , M. van der Hoek , J. Hofestadt , J. Hogenbirk , C. Hugon , J. Hosl , M. Imbesi , C. James , P. Jansweijer , J. Jochum , M. de Jong , M. Kadler , O. Kalekin , A. Kappes , E. Kappos , U. Katz , O. Kavatsyuk , P. Keller , G. Kieft , E. Koffeman , H. Kok , P. Kooijman , J. Koopstra , A. Korporaal , A. Kouchner , S. Koutsoukos , I. Kreykenbohm , V. Kulikovskiy , R. Lahmann , P. Lamare , G. Larosa , D. Lattuada , H. Le Provost , A. Leisos , D. Lenis , E. Leonora , M. Lindsey Clark , A. Liolios , C. D. Llorens Alvarez , H. Lohner , D. Lo Presti , F. Louis , E. Maccioni , K. Mannheim , K. Manolopoulos , A. Margiotta , O. Maris , C. Markou , J. A. Martinez-Mora , A. Martini , R. Masullo , T. Michael , P. Migliozzi , E. Migneco , A. Miraglia , C. Mollo , M. Mongelli , M. Morganti , S. Mos , Y. Moudden , P. Musico , M. Musumeci , C. Nicolaou , C. A. Nicolau , A. Orlando , A. Orzelli , K. Papageorgiou , A. Papaikonomou , R. Papaleo , G. E. Pavalas , H. Peek , C. Pellegrino , M. G. Pellegriti , C. Perrina , C. Petridou , P. Piattelli , K. Pikounis , V. Popa , Th. Pradier , M. Priede , G. Puhlhofer , S. Pulvirenti , C. Racca , F. Raffaelli , N. Randazzo , P. A. Rapidis , P. Razis , D. Real , L. Resvanis , J. Reubelt , G. Riccobene , A. Rovelli , J. Royon , M. Saldana , D. F. E. Samtleben , M. Sanguineti , A. Santangelo , P. Sapienza , I. Savvidis , J. Schmelling , J. Schnabel , M. Sedita , T. Seitz , I. Sgura , F. Simeone , I. Siotis , V. Sipala , M. Solazzo , A. Spitaleri , M. Spurio , G. Stavropoulos , J. Steijger , T. Stolarczyk , D. Stransky , M. Taiuti , G. Terreni , D. Tezier , S. Theraube , L. F. Thompson , P. Timmer , H. I. Trapierakis , L. Trasatti , A. Trovato , M. Tselengidou , A. Tsirigotis , S. Tzamarias , E. Tzamariudaki , B. Vallage , V. Van Elewyck , J. Vermeulen , P. Vernin , S. Viola , D. Vivolo , P. Werneke , L. Wiggers , J. Wilms , E. de Wolf , R. H. L. van Wooning , K. Yatkin , K. Zachariadou , E. Zonca , J. D. Zornoza , J. Zúñiga , A. Zwart

The three neutrino model has 9 physical parameters, 3 neutrino masses, 3 mixing angles and 3 CP violating phases. Among them, neutrino oscillation experiments can probe 6 parameters: 2 mass squared differences, 3 mixing angles, and 1 CP…

High Energy Physics - Phenomenology · Physics 2009-11-10 Kaoru Hagiwara

Organic photodetectors (OPDs) possess bright prospects in applications of medical imaging and wearable electronics due to the advantages such as low cost, good biocompatibility, and good flexibility. Photomultiplication OPDs (PM-OPDs)…