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