All-sky diffuse astrophysical neutrino flux with KM3NeT/ARCA data
- NázevTitle
- All-sky diffuse astrophysical neutrino flux with KM3NeT/ARCA dataAll-sky diffuse astrophysical neutrino flux with KM3NeT/ARCA data
- Druh výsledkuResult type
- Příspěvek ve sborníkuProceedings paper
- AutořiAuthors
- A.B. Bouasla, R. Attallah, O. Adriani, A. Albert, Z. Beňušová, E. Eckerová, Ľ. Krupa, F. Mamedov, M. Petropavlova, Y. Shitov, I. Štekl
- Klíčová slovaKeywords
- KM3NeT, neutrino telescope, ultra-high-energy neutrino
- KonferenceConference
- 39th International Cosmic Ray Conference (Geneva, Switzerland, 2025-07-14)
- ExperimentCollaboration
- KM3NeT
- DOIDOI
- 10.22323/1.501.1196
- Časopis / citaceJournal / citation
- In: Proceedings of 39th International Cosmic Ray Conference — PoS(ICRC2025), Sissa Medialab, 2025, pp. 1196 · ISSN 1824-8039
- RokYear
- 2025
- JazykLanguage
- eng
- ZáznamyRecords
- ProjektProject
- LSM-CZ III - Podzemní laboratoř LSM - účast České republiky - LM2023063 (2023–2026)LSM-CZ III - Podzemní laboratoř LSM - účast České republiky - LM2023063 (2023–2026); Laboratoire Souterrain de Modane - účast ČRLaboratoire Souterrain de Modane – participation of the Czech Republic
- CitovánoCited by
- 1 (INSPIRE-HEP)
- Plný text (open access)Full text (open access)
- https://pos.sissa.it/501/1196/pdf
- Citace ke staženíDownload citation
- TXT · BibTeX
AbstraktAbstract
KM3NeT/ARCA is a rapidly evolving neutrino detector in the Mediterranean Sea. The capability of the detector to measure the diffuse astrophysical neutrino flux was recently demonstrated by the observation of an ultra-high-energy neutrino of astrophysical origin. In this contribution, an analysis of KM3NeT/ARCA data, employing machine learning techniques and advanced statistical methods is presented, as well as a fit to the parameters of the diffuse flux. The latest results for the diffuse cosmic neutrino flux with KM3NeT/ARCA will be reported.
KM3NeT/ARCA is a rapidly evolving neutrino detector in the Mediterranean Sea. The capability of the detector to measure the diffuse astrophysical neutrino flux was recently demonstrated by the observation of an ultra-high-energy neutrino of astrophysical origin. In this contribution, an analysis of KM3NeT/ARCA data, employing machine learning techniques and advanced statistical methods is presented, as well as a fit to the parameters of the diffuse flux. The latest results for the diffuse cosmic neutrino flux with KM3NeT/ARCA will be reported.