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The emission of neutrinos within a wide energy range is predicted from very-high-energy phenomena in the Universe. Even the current or next-generation Cherenkov neutrino telescopes might be too small to detect the faint fluxes expected for…

Instrumentation and Methods for Astrophysics · Physics 2019-08-13 K. Graf

This talk review status and results from the two presently operating underwater/ice neutrino telescopes, NT-200 in Lake Baikal and Amanda-II at the South Pole. It also gives a description of the design and the expected performance of…

Astrophysics · Physics 2009-11-10 Christian Spiering

The acoustic neutrino detection technique is a promising approach for future large-scale detectors with the aim of measuring the small expected flux of neutrinos at energies in the EeV-range and above. The technique is based on the…

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

Arrays of acoustic receivers are an integral part of present and potential future Cherenkov neutrino telescopes in the deep sea. They measure the positions of individual detector elements which vary with time as an effect of undersea…

Instrumentation and Methods for Astrophysics · Physics 2013-04-03 Robert Lahmann

Baikal-GVD is a large ($\sim$1 km$^3$) underwater neutrino telescope installed in the fresh waters of Lake Baikal. The deep lake water environment is pervaded by background light, which is detectable by Baikal-GVD's photosensors. We…

Instrumentation and Methods for Astrophysics · Physics 2023-07-11 I. Kharuk , G. Rubtsov , G. Safronov

Acoustic neutrino detection is a promising technique to instrument the large volumes required to measure the small expected flux of ultra-high energy cosmogenic neutrinos. Using ice as detection medium allows for coincident detection of…

Instrumentation and Methods for Astrophysics · Physics 2014-10-22 Timo Karg

In this paper we show that QUASAR-370 large area hybrid phototube developed for and successfully used in a number of astroparticle physics experiments, the lake Baikal deep underwater neutrino experiment among them, could be used as a…

Instrumentation and Detectors · Physics 2010-02-08 B. K. Lubsandorzhiev

High energy neutrino astronomy has seen significant progress in the past few years. This includes the detection of neutrino flux from the Galactic plane, as well as strong evidence for neutrino emission from the active galaxy NGC 1068, both…

High Energy Astrophysical Phenomena · Physics 2026-02-11 Dmitry Zaborov

Acoustic neutrino detection is a promising approach to extend the energy range of neutrino telescopes to energies beyond $10^{18}$\,eV. Currently operational and planned water-Cherenkov neutrino telescopes, most notably KM3NeT, include…

Instrumentation and Methods for Astrophysics · Physics 2017-06-27 D. Kießling , G. Anton , A. Enzenhöfer , K. Graf , J. Hößl , U. Katz , R. Lahmann , M. Neff , C. Sieger

The first optical modules of the Baikal high energy neutrino telescope have recently been deployed. Commissioning of the AMANDA, DUMAND and NESTOR detectors will follow soon. Before discussing the detectors we review the arguments that…

High Energy Physics - Phenomenology · Physics 2007-05-23 F. Halzen

Acoustic neutrino detection is a promising approach for large-scale ultra-high energy neutrino detectors in water. In this article, a Monte Carlo simulation chain for acoustic neutrino detection devices in water is presented. It is designed…

Instrumentation and Methods for Astrophysics · Physics 2013-04-03 M. Neff , G. Anton , A. Enzenhöfer , K. Graf , J. Hößl , U. Katz , R. Lahmann