Search for a diffuse astrophysical neutrino flux with KM3NeT/ARCA using data of 2021-2022
- NázevTitle
- Search for a diffuse astrophysical neutrino flux with KM3NeT/ARCA using data of 2021-2022Search for a diffuse astrophysical neutrino flux with KM3NeT/ARCA using data of 2021-2022
- Druh výsledkuResult type
- Příspěvek ve sborníkuProceedings paper
- AutořiAuthors
- V. Tsourapis, E. Drakopoulou, C. Markou, A. Sinopoulou, Z. Bardačová, E. Eckerová, F. Mamedov, Y. Shitov, I. Štekl
- DOIDOI
- 10.22323/1.444.1195
- Časopis / citaceJournal / citation
- In: 38th International Cosmic Ray Conference (ICRC2023). Trieste: PoS - Proceedings of Science, Sissa Medialab srl, 2024. p. 1-10. vol. 444. ISSN 1824-8039.
- JazykLanguage
- eng
- ScopusScopus
- 2-s2.0-85200699437
- RIVRIV
- RIV/68407700:21670/24:00389333!RIV26-MSM-21670___
- ProjektProject
- Laboratoire Souterrain de Modane - účast ČRLaboratoire Souterrain de Modane – participation of the Czech Republic; LSM-CZ III - Podzemní laboratoř LSM - účast České republiky - LM2023063 (2023–2026)LSM-CZ III - Podzemní laboratoř LSM - účast České republiky - LM2023063 (2023–2026)
AbstraktAbstract
KM3NeT is a research infrastructure hosting two neutrino detectors which are currently under construction in the Mediterranean Sea. The KM3NeT/ARCA detector focuses on the detection of high energy neutrinos (>TeV) from astrophysical sources. In this contribution, an analysis of the data obtained during 2021-2022, using machine learning techniques, is presented. The potential of KM3NeT/ARCA to detect a diffuse flux of astrophysical neutrinos at the early stages of the detector construction is reported. The results of this analysis are presented.
KM3NeT is a research infrastructure hosting two neutrino detectors which are currently under construction in the Mediterranean Sea. The KM3NeT/ARCA detector focuses on the detection of high energy neutrinos (>TeV) from astrophysical sources. In this contribution, an analysis of the data obtained during 2021-2022, using machine learning techniques, is presented. The potential of KM3NeT/ARCA to detect a diffuse flux of astrophysical neutrinos at the early stages of the detector construction is reported. The results of this analysis are presented.