Cherenkov detectors for high energy neutrino astrophysics

Ja.-A.M. Dzhilkibaev, G.V. Domogatsky, O.V. Suvorova
Institute for Nuclear Research, Russian Academy of Sciences, prosp. 60-letiya Oktyabrya 7a, Moscow, 117312, Russian Federation

This review discusses the current status of and prospects for large-scale Cherenkov detectors that operate in deep-underwater- and under-ice environments (Lake Baikal, Mediterranean sea, Antarctica) and which have, in the last decades, become the primary tool for measuring high energy neutrino fluxes.
110th anniversary of the birth of P.A. Cherenkov (Scientific session of the Physical Sciences Division of the Russian Academy of Sciences, 17 December 2014)

Keywords: Cherenkov radiation, neutrino telescopes, neutrino astrophysics
PACS: 29.40.Ka, 41.60.Bq, 95.55.Vj (all)
DOI: 10.3367/UFNe.0185.201505j.0531
URL: https://ufn.ru/en/articles/2015/5/i/
Web of Science

000360073200009
Scopus

2-s2.0-84938834012
ADS NASA

2015PhyU...58..495D
Citation: Dzhilkibaev Ja-A M, Domogatsky G V, Suvorova O V "Cherenkov detectors for high energy neutrino astrophysics" Phys. Usp. 58 495–502 (2015)

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Received: 16th, March 2015, accepted: 17th, December 2014

Оригинал: Джилкибаев Ж-А М, Домогацкий Г В, Суворова О В «Черенковские детекторы в нейтринной астрофизике высоких энергий» УФН 185 531–539 (2015); DOI: 10.3367/UFNr.0185.201505j.0531

P.A. Cerenkov is author of Physics-Uspekhi

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