Status of the Baikal-GVD Neutrino Telescope and Main Results
- NázevTitle
- Status of the Baikal-GVD Neutrino Telescope and Main ResultsStatus of the Baikal-GVD Neutrino Telescope and Main Results
- Druh výsledkuResult type
- Článek v časopiseJournal article
- AutořiAuthors
- V.A. Allakhverdyan, A.D. Avrorin, A.V. Avrorin, V.M. Aynutdinov, L. Fajt, F. Šimkovic, I. Štekl
- Klíčová slovaKeywords
- astroparticle physics, Baikal, cascade, neutrino, neutrino telescope
- ExperimentCollaboration
- Baikal-GVD
- DOIDOI
- 10.3103/S1062873823702817
- Časopis / citaceJournal / citation
- Bulletin of the Russian Academy of Sciences: Physics 87(7), 1059-1062 (2023) · ISSN 1062-8738
- RokYear
- 2023
- 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
- 6 (INSPIRE-HEP)
- Citace ke staženíDownload citation
- TXT · BibTeX
AbstraktAbstract
The status of the Baikal-GVD neutrino telescope under construction and its main scientific results are presented. The detector consists of 2916 optical sensors located at 81 vertical strings deep below the surface of Lake Baikal. Its geometric configuration is optimized for detecting neutrinos with energies above 100 TeV. Events from muon neutrinos were identified, the flux of which is consistent with the expectation for the flux of atmospheric neutrinos. The data obtained during the alerts of the ANTARES and IceCube telescopes were analyzed. Candidate events for high-energy neutrinos of astrophysical origin have been obtained
The status of the Baikal-GVD neutrino telescope under construction and its main scientific results are presented. The detector consists of 2916 optical sensors located at 81 vertical strings deep below the surface of Lake Baikal. Its geometric configuration is optimized for detecting neutrinos with energies above 100 TeV. Events from muon neutrinos were identified, the flux of which is consistent with the expectation for the flux of atmospheric neutrinos. The data obtained during the alerts of the ANTARES and IceCube telescopes were analyzed. Candidate events for high-energy neutrinos of astrophysical origin have been obtained