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

Observations of track-like neutrino events with Baikal-GVD

NázevTitle
Observations of track-like neutrino events with Baikal-GVDObservations of track-like neutrino events with Baikal-GVD
Druh výsledkuResult type
Příspěvek ve sborníkuProceedings paper
AutořiAuthors
L. Fajt, I. Štekl, F. Šimkovic
Klíčová slovaKeywords
astrophysical neutrino, Baikal-GVD
KonferenceConference
37th International Cosmic Ray Conference (Berlin, Germany, 2021-07-15)
Časopis / citaceJournal / citation
In: 37th International Cosmic Ray Conference, Proceedings of Science, 2022, pp. 1-8 · ISSN 1824-8039
RokYear
2022
JazykLanguage
eng
ZáznamyRecords
ProjektProject
Inženýrské aplikace fyziky mikrosvětaEngineering applications of microworld physics
Citace ke staženíDownload citation
TXT · BibTeX

AbstraktAbstract

The Baikal Gigaton Volume Detector (Baikal-GVD) is a km3 -scale neutrino detector currently under construction in Lake Baikal, Russia. The detector currently consists of 2304 optical modules arranged on 64 vertical strings. Further extension of the array is planned for March 2022. The data from the partially complete array have been analyzed using a χ 2 -based track reconstruction algorithm. After suppression of the downward-going atmospheric muon background, a flux of upward-going neutrino events is observed, dominated by the atmospheric neutrinos. The observed flux is in good agreement with Monte Carlo predictions.

The Baikal Gigaton Volume Detector (Baikal-GVD) is a km3 -scale neutrino detector currently under construction in Lake Baikal, Russia. The detector currently consists of 2304 optical modules arranged on 64 vertical strings. Further extension of the array is planned for March 2022. The data from the partially complete array have been analyzed using a χ 2 -based track reconstruction algorithm. After suppression of the downward-going atmospheric muon background, a flux of upward-going neutrino events is observed, dominated by the atmospheric neutrinos. The observed flux is in good agreement with Monte Carlo predictions.

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