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The IceCube Neutrino Observatory is a kilometer-scale detector currently under construction at the South Pole. The full detector will comprise 5,160 photomultipliers (PMTs) deployed on 86 strings from 1.45-2.45 km deep within the ice. As of…

Instrumentation and Methods for Astrophysics · Physics 2019-08-14 Juan A. Aguilar

We study the problem of determination of the sign of Delta m^2_{31}, or the neutrino mass hierarchy, through observations of atmospheric neutrinos in future detectors. We consider two proposed detector types : (a) Megaton sized water…

High Energy Physics - Phenomenology · Physics 2008-11-26 Raj Gandhi , Pomita Ghoshal , Srubabati Goswami , Poonam Mehta , S Uma Sankar , Shashank Shalgar

Jinping Neutrino Experiment (Jinping) is proposed to significantly improve measurements on solar neutrinos and geoneutrinos in China Jinping Laboratory - a lab with a number of unparalleled features, thickest overburden, lowest reactor…

A new underground lab, Yemilab, is being constructed in Handuk iron mine, Korea. The default design of Yemilab includes a space for a future neutrino experiment. We propose to build a water-based liquid scintillator (WbLS) detector of…

Instrumentation and Detectors · Physics 2019-03-14 Seon-Hee Seo

This is a preliminary version of a formal proposal by the 3M collaboration to construct a megaton, modular, multipurpose (3M) neutrino detector for a program of experiments in neutrino physics. The detector components will be located in…

High Energy Physics - Experiment · Physics 2007-05-23 M. V. Diwan , R. L. Hahn , W. Marciano , B. Viren , R. Svoboda , W. Frati , K. Lande , A. K. Mann , R. Van Berg , J. R. Klein

The ANTARES (Astronomy with a Neutrino Telescope and Abyss environmental RESearch) Collaboration constructed and deployed the world's largest operational underwater neutrino telescope, optimised for the detection of Cherenkov light produced…

Instrumentation and Methods for Astrophysics · Physics 2009-05-12 G. Carminati

Hyper-Kamiokande has been proposed as a next generation neutrino oscillation experiment capable of observing accelerator, atmospheric, solar and astrophysical neutrinos, as well as possible proton decays, providing a rich scientific…

Instrumentation and Detectors · Physics 2015-04-28 Debra Dewhurst

The Main Injector Neutrino Oscillation Search (MINOS) experiment uses an accelerator-produced neutrino beam to perform precision measurements of the neutrino oscillation parameters in the "atmospheric neutrino" sector associated with muon…

Instrumentation and Detectors · Physics 2010-05-12 MINOS Collaboration , D. G. Michael

It is proposed to complement the ESS proton linac with equipment that would enable the production, concurrently with the production of the planned ESS beam used for neutron production, of a 5 MW beam of 10$^{23}$ 2.5 GeV protons per year in…

High Energy Physics - Experiment · Physics 2013-02-12 E. Baussan , M. Dracos , T. Ekelof , E. Fernandez Martinez , H. Ohman , N. Vassilopoulos

The study of neutrino oscillation at accelerators is limited by systematic uncertainties, in particular on the neutrino flux, cross-section, and energy estimates. These systematic uncertainties could be eliminated by a novel experimental…

The IceCube neutrino observatory uses $1\,\mathrm{km}^{3}$ of the natural Antarctic ice near the geographic South Pole as optical detection medium. When charged particles, such as particles produced in neutrino interactions, pass through…

High Energy Astrophysical Phenomena · Physics 2019-08-21 Anna Pollmann

We report the results of a search for neutrino-induced particle cascades using a deep ocean water Cherenkov detector. The effective mass of the detector, a string of seven 40 cm diameter photomultipliers at 5.2 m spacing, is found through…

SNO+ is a multipurpose neutrino experiment located approximately 2 km underground in SNOLAB, Sudbury, Canada. The detector started taking physics data in May 2017 and is currently completing its first phase, as a pure water Cherenkov…

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…

Instrumentation and Detectors · Physics 2015-01-20 Kamiokande Working Group , 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. Fernandez , 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 , R. A. Owen , Y. Oyama , J. Perez , 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. 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

IceCube is a kilometer scale high-energy neutrino observatory, currently under construction at the South Pole. It is a photo-detector, using the deep Antarctic ice as detection medium for the Cherenkov photons induced by relativistic…

Astrophysics · Physics 2016-11-09 Hagar Landsman

The concept of a small, single-layer water Cherenkov detector, with three photomultiplier tubes (PMTs), placed at its bottom in a $120^{\circ}$ star configuration (\emph{Mercedes} Water Cherenkov Detector) is presented. The PMTs are placed…

Although formal proposals have not yet been made, the UNO and Hyper-Kamiokande projects are being developed to follow-up the tremendously successful program at Super-Kamiokande using a detector that is 20-50 times larger. The potential of…

Astrophysics · Physics 2009-11-10 Maury Goodman

We set constraints and future sensitivity projections on millicharged particles (MCPs) based on electron scattering data in numerous neutrino experiments, starting with MiniBooNE and the Liquid Scintillator Neutrino Detector (LSND). Both…

High Energy Physics - Phenomenology · Physics 2019-12-12 Gabriel Magill , Ryan Plestid , Maxim Pospelov , Yu-Dai Tsai

The current focus of the CERN program is the Large Hadron Collider (LHC), however, CERN is engaged in long baseline neutrino physics with the CNGS project and supports T2K as recognized CERN RE13, and for good reasons: a number of observed…

High Energy Physics - Phenomenology · Physics 2009-10-29 A. Rubbia

ANTARES is a neutrino telescope designed to search for high-energy neutrinos from astrophysical sources such as quasars, gamma-ray bursters, microquasars, supernova remnants and AGN. The objectives also include the indirect search for…

Astrophysics · Physics 2019-08-14 E. V. Korolkova
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