PoS - Proceedings of Science
Volume 395 - 37th International Cosmic Ray Conference (ICRC2021) - NU - Neutrinos & Muons
Evaluation of large area photomultipliers for use in a new Baksan Large Neutrino Telescope project
Presented by N. Ushakov*  on behalf of A. Fazliakhmetov, V. Gavrin, T. Ibragimova, B. Lubsandorzhiev, A. Lukanov, A. Shikhin, A. Sidorenkov and D. Voronin
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Pre-published on: July 31, 2021
Published on: March 18, 2022
Abstract
The Baksan Large Neutrino Telescope is a liquid scintillation neutrino detector with a target mass of 10 kt, which is proposed to be constructed at the Baksan Neutrino Observatory of the Russian Academy of Sciences at a depth of 4700 m.w.e. In addition to the main full-scale detector, this project includes prototypes with target masses of 0.5, 5 and 100 t. This article evaluates photomultipliers (PMTs) Hamamatsu R7081-100 WA-S70 that are used in the first two phases of the project as the main ones. Also this article evaluates PMTs Hamamatsu R5912-100 WA-S70 used for the muon veto system for the 5-t detector prototype. To evaluate the PMTs, the quantum efficiency, single photoelectron response, timing characteristics, anode dark count rate, linearity and long afterpulses were measured.
DOI: https://doi.org/10.22323/1.395.1101
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