Atmospheric muon suppression for Baikal-GVD cascade analysis

Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68407700%3A21670%2F24%3A00381646" target="_blank" >RIV/68407700:21670/24:00381646 - isvavai.cz</a>
Result on the web
<a href="https://doi.org/10.22323/1.444.0986" target="_blank" >https://doi.org/10.22323/1.444.0986</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.22323/1.444.0986" target="_blank" >10.22323/1.444.0986</a>

Result language
angličtina
Original language name
Atmospheric muon suppression for Baikal-GVD cascade analysis
Original language description
The Baikal-GVD (Gigaton Volume Detector) is a neutrino telescope installed at a depth of 1366 m in Lake Baikal. The expedition of 2023 results in the array of 3492 optical modules that detect the Cherenkov radiation from secondary charged particles coming from the neutrino interactions.. Neutrinos produce different kinds of topologically distinct light signatures. Charged current muon neutrino interactions create an elongated track in the water. Charged and neutral current interactions of other neutrino flavors yield hadronic and electromagnetic cascades. The background in the neutrino cascade channel arises mainly due to discrete stochastic energy losses produced along atmospheric muon tracks. In this paper, a developed algorithm for the cascade event selection is presented.
Czech name
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Czech description
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Project
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Continuities
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace

Publication year
2024
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

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