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XENON is a dark matter direct detection project, consisting of a time projection chamber (TPC) filled with liquid xenon as detection medium. The construction of the next generation detector, XENON1T, is presently taking place at the…

We describe the design, construction and performance of a Ring Imaging Cherenkov Detector (RICH) constructed to identify charged particles in the CLEO experiment. Cherenkov radiation occurs in LiF crystals, both planar and ones with a novel…

We consider the prospects for the detection of relatively light dark matter through direct annihilation to neutrinos. We specifically focus on the detection possibilities of water Cherenkov and liquid scintillator neutrino detection…

High Energy Physics - Phenomenology · Physics 2010-04-30 Jason Kumar , John G. Learned , Stefanie Smith

The discovery of the Higgs boson has fully confirmed the Standard Model of particles and fields. Nevertheless, there are still fundamental phenomena, like the existence of dark matter and the baryon asymmetry of the Universe, which deserve…

Instrumentation and Detectors · Physics 2019-09-04 Giovanni De Lellis

The Deep Underground Neutrino Experiment (DUNE) will be the first mega-science program on the US soil and will shade light on some of the open questions in neutrino physics. The experiment foresees the realization of an intense neutrino…

Instrumentation and Detectors · Physics 2026-02-17 H. V. Souza

We propose here a large homogeneous calorimeter as the next generation neutrino detector for $\nu$ factories and/or conventional $\nu$ beams. The active media is chosen to be water for obvious economical reasons. The \v Cerenkov light…

High Energy Physics - Experiment · Physics 2007-05-23 Yi-Fang Wang

The IceCube Neutrino Observatory features both a kilometer-cubed detector between 1.45 and 2.45 km depth and an array of ice-filled tanks, called IceTop, located at the surface. The presence of both detectors at the same location allows for…

High Energy Astrophysical Phenomena · Physics 2019-08-21 Delia Tosi , Hershal Pandya

The SciBath-768 detector is a prototype neutral particle detector offering high-precision reconstruction of neutrino and neutron events. It consists of a three dimensional grid of 768 wavelength-shifting fibers immersed in 82 liters of…

High Energy Physics - Experiment · Physics 2011-10-21 R. Cooper , L. Garrison , H. -O. Meyer , T. Mikev , L. Rebenitsch , R. Tayloe

The Jiangmen Underground Neutrino Observatory (JUNO) is proposed to determine the neutrino mass hierarchy using an underground liquid scintillator detector. It is located 53 km away from both Yangjiang and Taishan Nuclear Power Plants in…

Instrumentation and Detectors · Physics 2015-09-29 T. Adam , F. An , G. An , Q. An , N. Anfimov , V. Antonelli , G. Baccolo , M. Baldoncini , E. Baussan , M. Bellato , L. Bezrukov , D. Bick , S. Blyth , S. Boarin , A. Brigatti , T. Brugière , R. Brugnera , M. Buizza Avanzini , J. Busto , A. Cabrera , H. Cai , X. Cai , A. Cammi , D. Cao , G. Cao , J. Cao , J. Chang , Y. Chang , M. Chen , P. Chen , Q. Chen , S. Chen , S. Chen , S. Chen , X. Chen , Y. Chen , Y. Cheng , D. Chiesa , A. Chukanov , M. Clemenza , B. Clerbaux , D. D'Angelo , H. de Kerret , Z. Deng , Z. Deng , X. Ding , Y. Ding , Z. Djurcic , S. Dmitrievsky , M. Dolgareva , D. Dornic , E. Doroshkevich , M. Dracos , O. Drapier , S. Dusini , M. A. Díaz , T. Enqvist , D. Fan , C. Fang , J. Fang , X. Fang , L. Favart , D. Fedoseev , G. Fiorentini , R. Ford , A. Formozov , R. Gaigher , H. Gan , A. Garfagnini , G. Gaudiot , C. Genster , M. Giammarchi , F. Giuliani , M. Gonchar , G. Gong , H. Gong , M. Gonin , Y. Gornushkin , M. Grassi , C. Grewing , V. Gromov , M. Gu , M. Guan , V. Guarino , W. Guo , X. Guo , Y. Guo , M. Göger-Neff , P. Hackspacher , C. Hagner , R. Han , Z. Han , J. Hao , M. He , D. Hellgartner , Y. Heng , D. Hong , S. Hou , Y. Hsiung , B. Hu , J. Hu , S. Hu , T. Hu , W. Hu , H. Huang , X. Huang , X. Huang , L. Huo , W. Huo , A. Ioannisian , D. Ioannisyan , M. Jeitler , K. Jen , S. Jetter , X. Ji , X. Ji , S. Jian , D. Jiang , X. Jiang , C. Jollet , M. Kaiser , B. Kan , L. Kang , M. Karagounis , N. Kazarian , S. Kettell , D. Korablev , A. Krasnoperov , S. Krokhaleva , Z. Krumshteyn , A. Kruth , P. Kuusiniemi , T. Lachenmaier , L. Lei , R. Lei , X. Lei , R. Leitner , F. Lenz , C. Li , F. Li , F. Li , J. Li , N. Li , S. Li , T. Li , W. Li , W. Li , X. Li , X. Li , X. Li , X. Li , Y. Li , Y. Li , Z. Li , H. Liang , H. Liang , J. Liang , M. Licciardi , G. Lin , S. Lin , T. Lin , Y. Lin , I. Lippi , G. Liu , H. Liu , H. Liu , J. Liu , J. Liu , J. Liu , J. Liu , Q. Liu , Q. Liu , S. Liu , S. Liu , Y. Liu , P. Lombardi , Y. Long , S. Lorenz , C. Lu , F. Lu , H. Lu , J. Lu , J. Lu , J. Lu , B. Lubsandorzhiev , S. Lubsandorzhiev , L. Ludhova , F. Luo , S. Luo , Z. Lv , V. Lyashuk , Q. Ma , S. Ma , X. Ma , X. Ma , Y. Malyshkin , F. Mantovani , Y. Mao , S. Mari , D. Mayilyan , W. McDonough , G. Meng , A. Meregaglia , E. Meroni , M. Mezzetto , J. Min , L. Miramonti , M. Montuschi , N. Morozov , T. Mueller , P. Muralidharan , M. Nastasi , D. Naumov , E. Naumova , I. Nemchenok , Z. Ning , H. Nunokawa , L. Oberauer , J. P. Ochoa-Ricoux , A. Olshevskiy , F. Ortica , H. Pan , A. Paoloni , N. Parkalian , S. Parmeggiano , V. Pec , N. Pelliccia , H. Peng , P. Poussot , S. Pozzi , E. Previtali , S. Prummer , F. Qi , M. Qi , S. Qian , X. Qian , H. Qiao , Z. Qin , G. Ranucci , A. Re , B. Ren , J. Ren , T. Rezinko , B. Ricci , M. Robens , A. Romani , B. Roskovec , X. Ruan , X. Ruan , A. Rybnikov , A. Sadovsky , P. Saggese , G. Salamanna , J. Sawatzki , J. Schuler , A. Selyunin , G. Shi , J. Shi , Y. Shi , V. Sinev , C. Sirignano , M. Sisti , O. Smirnov , M. Soiron , A. Stahl , L. Stanco , J. Steinmann , V. Strati , G. Sun , X. Sun , Y. Sun , Y. Sun , D. Taichenachev , J. Tang , A. Tietzsch , I. Tkachev , W. H. Trzaska , Y. Tung , S. van Waasen , C. Volpe , V. Vorobel , L. Votano , C. Wang , C. Wang , C. Wang , G. Wang , H. Wang , M. Wang , R. Wang , S. Wang , W. Wang , W. Wang , Y. Wang , Y. Wang , Y. Wang , Y. Wang , Z. Wang , Z. Wang , Z. Wang , Z. Wang , Z. Wang , W. Wei , Y. Wei , M. Weifels , L. Wen , Y. Wen , C. Wiebusch , S. Wipperfurth , S. C. Wong , B. Wonsak , C. Wu , Q. Wu , Z. Wu , M. Wurm , J. Wurtz , Y. Xi , D. Xia , J. Xia , M. Xiao , Y. Xie , J. Xu , J. Xu , L. Xu , Y. Xu , B. Yan , X. Yan , C. Yang , C. Yang , H. Yang , L. Yang , M. Yang , Y. Yang , Y. Yang , Y. Yang , E. Yanovich , Y. Yao , M. Ye , X. Ye , U. Yegin , F. Yermia , Z. You , B. Yu , C. Yu , C. Yu , G. Yu , Z. Yu , Y. Yuan , Z. Yuan , M. Zanetti , P. Zeng , S. Zeng , T. Zeng , L. Zhan , C. Zhang , F. Zhang , G. Zhang , H. Zhang , J. Zhang , J. Zhang , J. Zhang , K. Zhang , P. Zhang , Q. Zhang , T. Zhang , X. Zhang , X. Zhang , Y. Zhang , Y. Zhang , Y. Zhang , Y. Zhang , Y. Zhang , Y. Zhang , Z. Zhang , Z. Zhang , J. Zhao , M. Zhao , T. Zhao , Y. Zhao , H. Zheng , M. Zheng , X. Zheng , Y. Zheng , W. Zhong , G. Zhou , J. Zhou , L. Zhou , N. Zhou , R. Zhou , S. Zhou , W. Zhou , X. Zhou , Y. Zhou , H. Zhu , K. Zhu , H. Zhuang , L. Zong , J. Zou

Many Beyond-Standard Model physics signatures are enhanced in high-energy neutrino interactions. To explore these signatures, ultra-large Cherenkov detectors such as IceCube exploit event samples with charged current muon neutrino…

High Energy Physics - Phenomenology · Physics 2021-12-15 Austin Schneider , Barbara Skrzypek , Carlos A. Argüelles , Janet M. Conrad

The Precision IceCube Next Generation Upgrade (PINGU) is a proposed low-energy in-fill array of the IceCube Neutrino Observatory. Leveraging technology proven with IceCube, PINGU will feature the world's largest effective volume for…

Instrumentation and Detectors · Physics 2017-09-07 PINGU Collaboration

The ANTARES Neutrino Telescope is a water Cherenkov detector composed of an array of approximately 900 photomultiplier tubes in 12 vertical strings, spread over an area of about 0.1 km^2 with an instrumented height of about 350 metres.…

Instrumentation and Methods for Astrophysics · Physics 2019-08-13 Francesco Simeone

In this paper we stress the idea that new, more precise neutrino cross-sections measurements at low energies will be necessary to improve the results of future big neutrino detectors, which will be dominated by the contribution of the…

High Energy Physics - Phenomenology · Physics 2008-11-26 M. Campanelli , S. Navas-Concha , A. Rubbia

Massive underground detectors can be considered as sort of observatories for rare physics phenomena like astrophysical neutrino detection and nucleon decay searches. We briefly overview the past tracking calorimeters developed for nucleon…

High Energy Physics - Phenomenology · Physics 2007-05-23 A. Rubbia

In this review we first address two questions: 1. Why do we need kilometer-scale muon and neutrino detectors? 2. What do we learn from the operating Baikal and AMANDA detectors about the construction of kilometer-scale detectors? I will…

High Energy Physics - Experiment · Physics 2009-10-31 F. Halzen

We propose the Hyper-Kamiokande (Hyper-K) detector as a next generation un- derground water Cherenkov detector. It will serve as a far detector of a long base- line neutrino oscillation experiment envisioned for the upgraded J-PARC beam,…

High Energy Physics - Experiment · Physics 2013-09-03 Kamiokande Working Group

The NO{\nu}A Experiment will construct a detector optimized for electron neutrino detection in the existing Neutrino at Main Injector (NuMI) beamline. This beamline is capable of operating at 400 kW of primary beam power and the upgrade…

Accelerator Physics · Physics 2012-07-18 C. Ader , D. W. Wildman

We discuss the Chooz experiment, a long baseline search for neutrino vacuum oscillations, which will utilize a large gadolinium-loaded liquid scintillation detector one km from a large nuclear power station in France. The 300-meter (water…

High Energy Physics - Phenomenology · Physics 2007-05-23 R. I. Steinberg

A new experiment with an intense ~2 GeV neutrino beam at CERN SPS is proposed in order to definitely clarify the possible existence of additional neutrino states, as pointed out by neutrino calibration source experiments, reactor and…

Instrumentation and Detectors · Physics 2012-10-01 M. Antonello , D. Bagliani , B. Baibussinov , H. Bilokon , F. Boffelli , M. Bonesini , E. Calligarich , N. Canci , S. Centro , A. Cesana , K. Cieslik , D. B. Cline , A. G. Cocco , D. Dequal , A. Dermenev , R. Dolfini , M. De Gerone , S. Dussoni , C. Farnese , A. Fava , A. Ferrari , G. Fiorillo , G. T. Garvey , F. Gatti , D. Gibin , S. Gninenko , F. Guber , A. Guglielmi , M. Haranczyk , J. Holeczek , A. Ivashkin , M. Kirsanov , J. Kisiel , I. Kochanek , A. Kurepin , J. Lagoda , G. Lucchini , W. C. Louis , S. Mania , G. Mannocchi , S. Marchini , V. Matveev , A. Menegolli , G. Meng , G. B. Mills , C. Montanari , M. Nicoletto , S. Otwinowski , T. J. Palczewki , G. Passardi , F. Perfetto , P. Picchi , F. Pietropaolo , P. Plonski , A. Rappoldi , G. L. Raselli , M. Rossella , C. Rubbia , P. Sala , A. Scaramelli , E. Segreto , D. Stefan , J. Stepaniak , R. Sulej , O. Suvorova , M. Terrani , D. Tlisov , R. G. Van de Water , G. Trinchero , M. Turcato , F. Varanini , S. Ventura , C. Vignoli , H. G. Wang , X. Yang , A. Zani , K Zaremba , M. Benettoni , P. Bernardini , A. Bertolin , R. Brugnera , M. Calabrese , A. Cecchetti , S. Cecchini , G. Collazuol , P. Creti , F. Dal Corso , A. Del Prete , I. De Mitri , G. De Robertis , M. De Serio , L. Degli Esposti , D. Di Ferdinando , U. Dore , S. Dusini , P. Fabbricatore , C. Fanin , R. A. Fini , G. Fiore , A. Garfagnini , G. Giacomelli , R. Giacomelli , C. Guandalini , M. Guerzoni , U. Kose , G. Laurenti , M. Laveder , I. Lippi , F. Loddo , A. Longhin , P. Loverre , G. Mancarella , G. Mandrioli , A. Margiotta , G. Marsella , N. Mauri , E. Medinaceli , A. Mengucci , M. Mezzetto , R. Michinelli , M. T. Muciaccia , D. Orecchini , A. Paoloni , G. Papadia , A. Pastore , L. Patrizii , M. Pozzato , G. Rosa , Z. Sahnounm , S. Simone , M. Sioli , G. Sirri , M. Spurio , L. Stanco , A. Surdo , M. Tenti , V. Togo , M. Ventura , M. Zago

The sensitivity of a huge underground water/ice Cherenkov detector, such as PINGU in IceCube, to the neutrino mass hierarchy, the atmospheric mixing angle and its octant, is studied in detail. Based on the event rate decomposition in the…

High Energy Physics - Phenomenology · Physics 2015-06-18 Shao-Feng Ge , Kaoru Hagiwara