Diffuse neutrino flux measurements with the Baikal-GVD neutrino telescope
- NázevTitle
- Diffuse neutrino flux measurements with the Baikal-GVD neutrino telescopeDiffuse neutrino flux measurements with the Baikal-GVD neutrino telescope
- Druh výsledkuResult type
- Příspěvek ve sborníkuProceedings paper
- AutořiAuthors
- E. Eckerová
- Klíčová slovaKeywords
- Baikal-GVD, neutrino telescope
- KonferenceConference
- 38th International Cosmic Ray Conference (Nagoya, Japan, 2023-07-26)
- ExperimentCollaboration
- Baikal-GVD
- DOIDOI
- 10.22323/1.444.1015
- Časopis / citaceJournal / citation
- In: Proceedings of 38th International Cosmic Ray Conference — PoS(ICRC2023), Sissa Medialab, 2024, pp. 1015 · ISSN 1824-8039
- RokYear
- 2024
- JazykLanguage
- eng
- ZáznamyRecords
- ProjektProject
- Institucionální podpora na rozvoj výzkumné org.Institucionální podpora na rozvoj výzkumné org.
- CitovánoCited by
- 5 (INSPIRE-HEP)
- Plný text (open access)Full text (open access)
- http://dx.doi.org/10.22323/1.444.1015
- Citace ke staženíDownload citation
- TXT · BibTeX
AbstraktAbstract
Baikal-GVD is a next generation, kilometer-scale neutrino telescope currently under construction in Lake Baikal. GVD consists of multi-megaton subarrays (clusters) and is designed for the detection of astrophysical neutrino fluxes at energies from a few TeV up to 100 PeV. The large detector volume and modular design of Baikal-GVD allows for the measurements of the astrophysical diffuse neutrino flux to be performed already at early phases of the array construction. We present here recent results of the measurements on the diffuse cosmic neutrino flux obtained with the Baikal-GVD neutrino telescope using cascade-like events.
Baikal-GVD is a next generation, kilometer-scale neutrino telescope currently under construction in Lake Baikal. GVD consists of multi-megaton subarrays (clusters) and is designed for the detection of astrophysical neutrino fluxes at energies from a few TeV up to 100 PeV. The large detector volume and modular design of Baikal-GVD allows for the measurements of the astrophysical diffuse neutrino flux to be performed already at early phases of the array construction. We present here recent results of the measurements on the diffuse cosmic neutrino flux obtained with the Baikal-GVD neutrino telescope using cascade-like events.