Baikal-GVD: Status and prospects
- NázevTitle
- Baikal-GVD: Status and prospectsBaikal-GVD: Status and prospects
- Druh výsledkuResult type
- Příspěvek ve sborníkuProceedings paper
- AutořiAuthors
- A.D. Avrorin, A.V. Avrorin, V.M. Aynutdinov, R. Bannash, L. Fajt, I. Štekl, F. Šimkovic
- Klíčová slovaKeywords
- astrophysical neutrino, neutrino telescope, Baikal-GVD
- KonferenceConference
- 20th International Seminar on High Energy Physics (Valday, Russian Federation, 2018-05-27)
- ExperimentCollaboration
- Baikal-GVD
- DOIDOI
- 10.1051/epjconf/201819101006
- Časopis / citaceJournal / citation
- EPJ Web of Conferences 191, 01006 (2018) · ISSN 2101-6275
- RokYear
- 2018
- JazykLanguage
- eng
- ZáznamyRecords
- ProjektProject
- Inženýrské aplikace fyziky mikrosvětaEngineering applications of microworld physics
- CitovánoCited by
- 99 (INSPIRE-HEP)
- Plný text (open access)Full text (open access)
- https://www.epj-conferences.org/articles/epjconf/pdf/2018/26/epjconf_quarks2018…
- Citace ke staženíDownload citation
- TXT · BibTeX
AbstraktAbstract
Baikal-GVD is a next generation, kilometer-scale neutrino telescope under construction in Lake Baikal. It is designed to detect astrophysical neutrino fluxes at energies from a few TeV up to 100 PeV. GVD is formed by multi-megaton subarrays (clusters). The array construction started in 2015 by deployment of a reduced-size demonstration cluster named Dubna. The first cluster in it's baseline configuration was deployed in 2016, the second in 2017 and the third in 2018. The full-scale GVD will be an array of ~10.000 light sensors with an instrumented volume about of 2 cubic km. The first phase (GVD-1) is planned to be completed by 2020-2021. It will comprise 8 clusters with 2304 light sensors in total. We describe the design of Baikal-GVD and present selected results obtained in 2015 - 2017.
Baikal-GVD is a next generation, kilometer-scale neutrino telescope under construction in Lake Baikal. It is designed to detect astrophysical neutrino fluxes at energies from a few TeV up to 100 PeV. GVD is formed by multi-megaton subarrays (clusters). The array construction started in 2015 by deployment of a reduced-size demonstration cluster named Dubna. The first cluster in it's baseline configuration was deployed in 2016, the second in 2017 and the third in 2018. The full-scale GVD will be an array of ~10.000 light sensors with an instrumented volume about of 2 cubic km. The first phase (GVD-1) is planned to be completed by 2020-2021. It will comprise 8 clusters with 2304 light sensors in total. We describe the design of Baikal-GVD and present selected results obtained in 2015 - 2017.