Baikal-GVD Document 25-v1

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[ICRC 2021] Methods for the suppression of background cascades produced along atmospheric muon tracks in the Baikal-GVD

Document #:
Baikal-GVD-doc-25-v1
Document type:
Paper
Submitted by:
Yury Malyshkin
Updated by:
Yury Malyshkin
Document Created:
11 Oct 2022, 18:33
Contents Revised:
11 Oct 2022, 18:33
Metadata Revised:
12 Nov 2022, 15:58
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Abstract:
The Baikal-GVD (Gigaton Volume Detector) is a km 3 - scale neutrino telescope located in Lake Baikal. Currently (year 2021) the Baikal-GVD is composed of 2304 optical modules divided to 8 independent detection units, called clusters. Specific neutrino interactions can cause Cherenkov light topology, referred to as a cascade. However, cascade-like events originate from discrete stochastic energy losses along muon tracks. These cascades produce the most abundant background in searching for high-energy neutrino cascade events. Several methods have been developed, optimized, and tested to suppress background cascades.
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Publication Information:
https://doi.org/10.22323/1.395.1114
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