ÚTEFČVUT Ústav technické a experimentální fyziky ČVUT v PrazeInstitute of Experimental and Applied Physics, CTU in Prague

Selection techniques of neutrino-induced cascades in the Baikal-GVD neutrino telescope

NázevTitle
Selection techniques of neutrino-induced cascades in the Baikal-GVD neutrino telescopeSelection techniques of neutrino-induced cascades in the Baikal-GVD neutrino telescope
Druh výsledkuResult type
Příspěvek ve sborníkuProceedings paper
AutořiAuthors
Z. Bardačová
Klíčová slovaKeywords
neutrino telescope, Baikal-GVD, cascade
KonferenceConference
18th International Conference on Topics in Astroparticle and Underground Physics (Vienna, Austria, 2023-08-28)
ExperimentCollaboration
Baikal-GVD
DOIDOI
10.22323/1.441.0248
Časopis / citaceJournal / citation
In: Proceedings of XVIII International Conference on Topics in Astroparticle and Underground Physics — PoS(TAUP2023), Sissa Medialab, 2024, pp. 248 · ISSN 1824-8039
RokYear
2024
JazykLanguage
eng
ZáznamyRecords
ProjektProject
Laboratoire Souterrain de Modane - účast ČRLaboratoire Souterrain de Modane – participation of the Czech Republic
Plný text (open access)Full text (open access)
https://pos.sissa.it/441/248/pdf
Citace ke staženíDownload citation
TXT · BibTeX

AbstraktAbstract

One of the light signatures in the Baikal-GVD neutrino telescope consists of hadronic and electromagnetic cascades produced by charged interactions of electron and tau neutrinos. In the case of neutral current interactions, all flavors yield cascades. The background in the neutrino cascade channel arises mainly due to discrete stochastic energy losses produced along atmospheric muon tracks. In this contribution, a developed algorithm for the cascade event selection is presented.

One of the light signatures in the Baikal-GVD neutrino telescope consists of hadronic and electromagnetic cascades produced by charged interactions of electron and tau neutrinos. In the case of neutral current interactions, all flavors yield cascades. The background in the neutrino cascade channel arises mainly due to discrete stochastic energy losses produced along atmospheric muon tracks. In this contribution, a developed algorithm for the cascade event selection is presented.

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