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

Recent Results From the Baikal-GVD Neutrino Telescope

NázevTitle
Recent Results From the Baikal-GVD Neutrino TelescopeRecent Results From the Baikal-GVD Neutrino Telescope
Druh výsledkuResult type
Článek v časopiseJournal article
AutořiAuthors
V. A. Allakhverdyan, A. D. Avrorin, A. V. Avrorin, V. M. Aynutdinov, E. Eckerová, L. Fajt, F. Šimkovic, I. Štekl, Z. Bardačová
Klíčová slovaKeywords
neutrino telescope, astrophysics, high-energy phenomenon
KonferenceConference
21st Lomonosov Conference on Elementary Particle Physics (Moscow, Russian Federation, 2023-08-24)
DOIDOI
10.3103/S0027134924701674
Časopis / citaceJournal / citation
Moscow University Physics Bulletin 79(S1), 210-219 (2024) · ISSN 0027-1349
RokYear
2024
JazykLanguage
eng
ZáznamyRecords
ProjektProject
Inženýrské aplikace fyziky mikrosvětaEngineering applications of microworld physics; Institucionální podpora na rozvoj výzkumné org.Institucionální podpora na rozvoj výzkumné org.
CitovánoCited by
1 (INSPIRE-HEP)
2025: 1
Citace ke staženíDownload citation
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AbstraktAbstract

Neutrino is considered as a superior astronomical messenger thanks to not being deflected or absorbed by interstellar medium. Detection of neutrinos from distant high-energy cosmic accelerators has been a long-standing problem emerged in the last quarter of 20th century. Only in 2013 was the diffuse cosmic neutrino flux discovered by the 1 km(3)-scale IceCube neutrino telescope at the South Pole. Nevertheless evidence for sources of cosmic neutrino remain weak up to the present day. The Baikal-GVD neutrino telescope being built in Lake Baikal is the largest detector of this kind in the Northern Hemisphere. Presently an instrumented volume of the detector is about 0.5 km(3) which allows the telescope to start contributing to the cosmic neutrino origin quest. In this report we discuss the motivation present the status and main results of the Baikal-GVD experiment.

Neutrino is considered as a superior astronomical messenger thanks to not being deflected or absorbed by interstellar medium. Detection of neutrinos from distant high-energy cosmic accelerators has been a long-standing problem emerged in the last quarter of 20th century. Only in 2013 was the diffuse cosmic neutrino flux discovered by the 1 km(3)-scale IceCube neutrino telescope at the South Pole. Nevertheless evidence for sources of cosmic neutrino remain weak up to the present day. The Baikal-GVD neutrino telescope being built in Lake Baikal is the largest detector of this kind in the Northern Hemisphere. Presently an instrumented volume of the detector is about 0.5 km(3) which allows the telescope to start contributing to the cosmic neutrino origin quest. In this report we discuss the motivation present the status and main results of the Baikal-GVD experiment.

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