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The observation of high-energy neutrinos from astrophysical sources would substantially improve our knowledge and understanding of the non-thermal processes in these sources, and would in particular pinpoint the accelerators of cosmic rays.…

Astrophysics · Physics 2019-08-14 J. Carr , D. Dornic , F. Jouvenot , U. F. Katz , S. Kuch , G. Maurin , R. Shanidze

ANTARES is a large volume neutrino telescope currently under construction off La Seyne-sur-mer, France, at 2475m depth. Neutrino telescopes aim at detecting neutrinos as a new probe for a sky study at energies greater than 1 TeV. The…

Astrophysics · Physics 2019-08-15 A. Kouchner

We explore the possibility of simultaneous determination of neutrino mass hierarchy and the CP violating phase by using two identical detectors placed at different baseline distances. We focus on a possible experimental setup using neutrino…

High Energy Physics - Phenomenology · Physics 2010-04-06 Masaki Ishitsuka , Takaaki Kajita , Hisakazu Minakata , Hiroshi Nunokawa

We consider the determination of the solar neutrino oscillation parameters $\Delta m^2_{21}$ and $\theta_{12}$ by studying oscillations of reactor anti-neutrinos emitted by nuclear power plants (located mainly in France) with a detector…

High Energy Physics - Phenomenology · Physics 2008-11-26 S. T. Petcov , T. Schwetz

Future large liquid-scintillator detectors can be implemented to observe neutrinos from a core-collapse supernova (SN) in our galaxy in various reaction channels: (1) The inverse beta decay $\overline{\nu}^{}_e + p \to n + e^+$; (2) The…

High Energy Physics - Phenomenology · Physics 2016-07-27 Jia-Shu Lu , Yu-Feng Li , Shun Zhou

The ANTARES telescope is the largest underwater neutrino telescope existing at present. It is based on the detection of Cherenkov light produced in sea water by neutrino-induced muons. The detector, consisting of a tri-dimensional array of…

High Energy Astrophysical Phenomena · Physics 2019-08-13 Salvatore Mangano

Water Cherenkov and scintillator detectors are a critical tool for neutrino physics.Their large size, low threshold, and low operational cost make them excellent detectors for long baseline neutrino oscillations, proton decay, supernova and…

Instrumentation and Detectors · Physics 2016-01-07 N. Barros , T. Kaptanoglu , B. Kimmelman , J. R. Klein , E. Moore , J. Nguyen , K. Stavreva , R. Svoboda

KM3NeT is a deep-sea research infrastructure being constructed in the Mediterranean Sea. It will host the next generation Cherenkov neutrino telescope and nodes for a deep sea multidisciplinary observatory, providing oceanographers, marine…

Instrumentation and Methods for Astrophysics · Physics 2014-08-08 Annarita Margiotta

The ANTARES Collaboration is deploying a large neutrino detector at a depth of 2475 m in the Mediterranean Sea, 40 km off shore from La Seyne-sur-Mer in South France. The construction of this 12-line detector with 75 phototubes per line…

Astrophysics · Physics 2007-10-03 ANTARES Collaboration , S. Escoffier

IceCube is a 1 km$^3$ neutrino detector now being built at the South Pole. Its 4800 optical modules will detect Cherenkov radiation from charged particles produced in neutrino interactions. IceCube will search for neutrinos of astrophysical…

Astrophysics · Physics 2019-08-13 Spencer R. Klein

The ANTARES Neutrino Telescope is a water Cherenkov detector currently under construction in the Mediterranean Sea. It is also designed to serve as a platform for investigations of the deep-sea environment. In this context, the ANTARES…

Astrophysics · Physics 2008-11-26 K Graf , G Anton , J Hoessl , A Kappes , U F Katz , R Lahmann , C Naumann , K Salomon

In this article, the potential of water Cherenkov detectors equipped with multi-PMT modules for background-free upward-going neutrino detection and improved direction reconstruction is demonstrated. By analyzing signal time traces with…

High Energy Physics - Experiment · Physics 2025-08-08 J. Alvarez-Muñiz , R. Colalillo , R. Conceição , B. S. González , V. M. Grieco , F. Guarino , M. Pimenta , B. Tomé , M. Waqas

The ANTARES neutrino telescope is presently being built in the Mediterranean Sea at a depth of 2500 m. The primary aim of the experiment is the detection of high energy cosmic muon neutrinos, which are identified by the muons that are…

Astrophysics · Physics 2019-08-13 S. Mangano

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

Extensive airshower detection is an important issue in current astrophysics endeavours. Surface arrays detectors are a common practice since they are easy to handle and have a 100% duty cycle. In this work we present an experimental study…

An economical procedure to upgrade the existing Fairport water Cherenkoff detector is described. The detector will lower its energy threshold by increased photocoverage and light yield. Furthermore, by addition of a Gd salt it will become…

Instrumentation and Detectors · Physics 2007-05-23 E. P. Bonvin , S. T. Hatamian

The ANTARES underwater neutrino telescope, at a depth of 2475 m in the Mediterranean Sea, near Toulon, is taking data in its final configuration of 12 detection lines. Each line is equipped with 75 photomultipliers (PMT) housed in glass…

Astrophysics · Physics 2019-08-13 G. Giacomelli

New low-cost, high-power proton cyclotrons open the opportunity for a novel precision search for CP violation in the neutrino sector. The accelerators can produce decay-at-rest neutrino beams located at multiple distances from a Gd-doped…

High Energy Physics - Experiment · Physics 2010-04-14 J. M. Conrad , M. H. Shaevitz

The missing mass spectroscopy of $\Xi^{-}$ hypernuclei with the $(K^{-},K^{+})$ reaction is planned to be performed at the J-PARC K1.8 beam line by using a new magnetic spectrometer, Strangeness $-2$ Spectrometer (S-2S). A $\v{C}$cerenkov…

Instrumentation and Detectors · Physics 2016-07-11 T. Gogami , N. Amano , S. Kanatsuki , T. Nagae , K. Takenaka

We study the sensitivity to neutrino masses of a Galactic supernova neutrino signal as could be measured with the detectors presently in operation and with future large volume water \v{C}erencov and scintillator detectors. The analysis uses…

Astrophysics · Physics 2007-05-23 Jorge I. Zuluaga