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A next generation water Cherenkov detector Hyper-Kamiokande to be built in Japan is described. The main goals of this project include a sensitive measurement of CP violation in neutrino oscillations, a search for proton decay and study of…

Instrumentation and Detectors · Physics 2020-08-26 Yury Kudenko

The proposed large scale Cherenkov neutrino telescope KM3NeT will carry photo-sensors on flexible structures, the detection units. The Mediterranean Sea, where KM3NeT will be installed, constitutes a highly dynamic environment in which the…

Instrumentation and Methods for Astrophysics · Physics 2019-08-14 Alexander Enzenhöfer

The KM3NeT Collaboration runs a multi-site neutrino observatory in the Mediterranean Sea. Water Cherenkov particle detectors, deep in the sea and far off the coasts of France and Italy, are already taking data while incremental construction…

Instrumentation and Methods for Astrophysics · Physics 2020-07-15 S. Aiello , F. Ameli , M. Andre , G. Androulakis , M. Anghinolfi , G. Anton , M. Ardid , J. Aublin , C. Bagatelas , G. Barbarino , B. Baret , S. Basegmez du Pree , M. Bendahman , E. Berbee , A. M. van den Berg , V. Bertin , S. Biagi , A. Biagioni , M. Bissinger , J. Boumaaza , S. Bourret , M. Bouta , G. Bouvet , M. Bouwhuis , C. Bozza , H. Branzas , M. Bruchner , R. Bruijn , J. Brunner , E. Buis , R. Buompane , J. Busto , D. Calvo , A. Capone , S. Celli , M. Chabab , N. Chau , S. Cherubini , V. Chiarella , T. Chiarusi , M. Circella , R. Cocimano , J. A. B. Coelho , A. Coleiro , M. Colomer Molla , R. Coniglione , P. Coyle , A. Creusot , G. Cuttone , A. D'Onofrio , R. Dallier , M. De Palma , I. Di Palma , A. F. Díaz , D. Diego-Tortosa , C. Distefano , A. Domi , R. Donà , C. Donzaud , D. Dornic , M. Dörr , M. Durocher , T. Eberl , I. El Bojaddaini , H. Eljarrari , D. Elsaesser , A. Enzenhöfer , P. Fermani , G. Ferrara , M. D. Filipovic , A. Franco , L. A. Fusco , T. Gal , A. Garcia Soto , F. Garufi , L. Gialanella , E. Giorgio , S. R. Gozzini , R. Gracia , K. Graf , D. Grasso , T. Grégoire , G. Grella , D. Guderian , C. Guidi , S. Hallmann , H. Hamdaoui , H. van Haren , A. Heijboer , A. Hekalo , J. J. Hernández-Rey , J. Hofestädt , F. Huang , G. Illuminati , C. W. James , M. de Jong , P. de Jong , M. Kadler , P. Kalaczynski , O. Kalekin , U. F. Katz , N. R. Khan Chowdhury , F. van der Knaap , E. N. Koffeman , P. Kooijman , A. Kouchner , V. Kulikovskiy , R. Lahmann , G. Larosa , R. Le Breton , F. Leone , E. Leonora , G. Levi , M. Lincetto , A. Lonardo , F. Longhitano , D. Lopez-Coto , G. Maggi , J. Manczak , K. Mannheim , A. Margiotta , A. Marinelli , C. Markou , G. Martignac , L. Martin , J. A. Martínez-Mora , A. Martini , F. Marzaioli , S. Mazzou , R. Mele , K. W. Melis , P. Migliozzi , E. Migneco , P. Mijakowski , L. S. Miranda , C. M. Mollo , M. Morganti , M. Moser , A. Moussa , R. Muller , M. Musumeci , L. Nauta , S. Navas , C. A. Nicolau , C. Nielsen , B. O' Fearraigh , M. Organokov , A. Orlando , V. Panagopoulos , G. Papalashvili , R. Papaleo , C. Pastore , G. E. Pavalas , C. Pellegrino , M. Perrin-Terrin , P. Piattelli , C. Pieterse , K. Pikounis , O. Pisanti , C. Poirè , G. Polydefki , V. Popa , M. Post , T. Pradier , G. Puhlhofer , S. Pulvirenti , L. Quinn , F. Raffaelli , N. Randazzo , A. Rapicavoli , S. Razzaque , D. Real , S. Reck , J. Reubelt , G. Riccobene , M. Richer , L. Rigalleau , A. Rovelli , I. Salvadori , D. F. E. Samtleben , A. Sánchez Losa , M. Sanguineti , A. Santangelo , D. Santonocito , P. Sapienza , J. Schnabel , V. Sciacca , J. Seneca , I. Sgura , R. Shanidze , A. Sharma , F. Simeone , A. Sinopoulou , B. Spisso , M. Spurio , D. Stavropoulos , J. Steijger , S. M. Stellacci , B. Strandberg , D. Stransky , M. Taiuti , Y. Tayalati , E. Tenllado , T. Thakore , S. Tingay , E. Tzamariudaki , D. Tzanetatos , V. Van Elewyck , G. Vannoye , F. Versari , S. Viola , D. Vivolo , G. de Wasseige , J. Wilms , R. Wojaczynski , E. de Wolf , D. Zaborov , A. Zegarelli , J. D. Zornoza , J. Zúñiga

The ANTARES Collaboration is completing the deployment of a 12 lines underwater detector, 2500m deep in the Mediterranean Sea, dedicated to high energy neutrino astronomy. Starting with the first line in 2006, 10 lines were continuously…

Astrophysics · Physics 2019-08-13 Thierry Pradier

The ANTARES neutrino telescope is currently being constructed in the Mediterranean Sea. The complete detector will consist of 12 strings, supplemented by an additional instrumentation line. Nine strings are at present deployed of which five…

Astrophysics · Physics 2019-08-13 Felix Fehr

The hope is that in the near future neutrino astronomy, born with the identification of thermonuclear fusion in the sun and the particle processes controlling the fate of a nearby supernova, will reach throughout and beyond our Galaxy and…

Astrophysics · Physics 2009-10-28 S. Barwick , F. Halzen , P. B. Price

The NEMO 3 experiment is located in the Modane Underground Laboratory and has been taking data since 2003 with seven isotopes. It is searching for the double beta decay process with two or zero neutrinos emitted in the final state.…

High Energy Physics - Experiment · Physics 2019-08-14 R. L. Flack

We review detector technologies which are currently considered for ultimate nucleon decay searches, new generation astrophysical neutrinos studies, and for future long-baseline neutrino experiments at new high-intensity neutrino beam…

High Energy Physics - Phenomenology · Physics 2009-11-10 A. Rubbia

The ANTARES underwater neutrino telescope is located in the Mediterranean Sea about 40 km from Toulon at a depth of 2475 m. In its 12 line configuration it has almost 900 photomultipliers in 295 floors. The performance of the detector is…

High Energy Physics - Experiment · Physics 2013-01-01 Giorgio Giacomelli

We investigate the potential of near-future neutrino telescopes like NESTOR for searches for exotic processes in ultrahigh energy neutrino-quark scattering. (NESTOR is the acronym for NEutrinos, from Supernovae and TeV sources, Ocean Range…

High Energy Physics - Phenomenology · Physics 2007-05-23 D. A. Morris , A. Ringwald

The ANTARES collaboration is building a deep sea neutrino telescope in the Mediterranean Sea. This detector will cover a sensitive area of typically 0.1 km-squared and will be equipped with about 1000 optical modules. Each of these optical…

Astrophysics · Physics 2012-08-27 The ANTARES Collaboration

NEMO 3 experiment is designed to search for neutrinoless double beta decay. It is located in the Modane Underground Laboratory (LSM) and has been taking data since February 2003. The half- lives of two neutrino beta decay have been measured…

High Energy Physics - Experiment · Physics 2010-02-25 Zornitza Daraktchieva

The AMADEUS system is an integral part of the ANTARES neutrino telescope in the Mediterranean Sea. The project aims at the investigation of techniques for acoustic neutrino detection in the deep sea. Installed at a depth of more than 2000m,…

Instrumentation and Methods for Astrophysics · Physics 2018-11-30 Robert Lahmann

The KM3NeT Collaboration is constructing two large neutrino detectors in the Mediterranean Sea: ARCA, located near Sicily and aiming at neutrino astronomy, and ORCA located near Toulon and designed for the study of intrinsic neutrino…

Instrumentation and Methods for Astrophysics · Physics 2023-08-09 Dídac D. Tortosa , Miguel Ardid , Manuel Bou-Cabo , Guillermo Lara , Juan A. Martínez-Mora

MEMPHYS (MEgaton Mass PHYSics) is a proposed large-scale water Cherenkov experiment to be performed deep underground. It is dedicated to nucleon decay searches, neutrinos from supernovae, solar and atmospheric neutrinos, as well as…

High Energy Physics - Experiment · Physics 2013-02-20 L. Agostino , M. Buizza-Avanzini , M. Dracos , D. Duchesneau , M. Marafini , M. Mezzetto , L. Mosca , T. Patzak , A. Tonazzo , N. Vassilopoulos

The aim of the NEMO 3 experiment is the search for neutrinoless double beta decay and precise measurement of two-neutrino double beta decay of several isotopes. The experiment has been taking data since 2003. Since no evidence for…

High Energy Physics - Experiment · Physics 2019-08-13 Ladislav Vala

We present the results of Monte Carlo simulation studies of the capability of the proposed NEMO km$^3$ telescope to detect TeV muon neutrinos from Galactic microquasars. In particular we determined the detector sensitivity to each known…

Astrophysics · Physics 2007-06-21 C. Distefano

Neutrino telescopes are unrivaled tools to explore the Universe at its most extreme. The current generation of telescopes has shown that very high energy neutrinos are produced in the cosmos, even with hints of their possible origin, and…

Instrumentation and Methods for Astrophysics · Physics 2021-11-29 Elisa Resconi , P-ONE Collaboration

The discovery of a high-energy cosmic neutrino flux has paved the way for the field of neutrino astronomy. For a large part of the flux, the sources remain unidentified. The KM3NeT detector, which is under construction in the Mediterranean…

Instrumentation and Methods for Astrophysics · Physics 2022-05-06 Thijs van Eeden , Jordan Seneca , Aart Heijboer

KM3NeT is a research infrastructure housing the next generation neutrino detectors in the depths of the Mediterranean Sea. The ARCA detector, which is currently under construction, is optimized for searches for neutrinos from astrophysical…

High Energy Physics - Experiment · Physics 2019-08-14 Konstantinos Pikounis , Ekaterini Tzamariudaki