Hodnocení radioaktivity materiálu a vylepšené kalibrační techniky pro zvýšení výkonnosti neutrinových teleskopů KM3NET
- NázevTitle
- Hodnocení radioaktivity materiálu a vylepšené kalibrační techniky pro zvýšení výkonnosti neutrinových teleskopů KM3NETMaterial radioactivity evaluations and improved calibration techniques to advance performances of the KM3NET neutrino telescopes
- PoskytovatelProvider
- Grantová agentura České republikyCzech Science Foundation
- ProgramProgramme
- Standardní projektyStandard projects
- Kód CEPCEP code
- GA24-12702S
- Datum zahájeníStart date
- 2024-01-01
- Datum ukončeníEnd date
- 2026-12-31
- Vztah ČVUTCTU relation
- ČVUT je v pozici příjemce jako jediný účastník projektuCTU is the only beneficiary participant in the project
- Řešitel ČVUTCTU investigator
- Yury Shitov
- Řešitelský tým (ÚTEF)Team (UTEF)
- Mgr. Fadahat Mamedov, Ph.D. (člen řešitelského týmuresearch team member)
- Mgr. Zuzana Beňušová, Ph.D. (člen řešitelského týmuresearch team member)
- Mgr. Mariia Petropavlova (člen řešitelského týmuresearch team member)
- Mgr. Eliška Eckerová, Ph.D. (člen řešitelského týmuresearch team member)
- Mgr. Rastislav Dvornický, Ph.D. (člen řešitelského týmuresearch team member)
- Bc. Ondřej Jamelský (člen řešitelského týmuresearch team member)
- Mgr. Adam Smetana, Ph.D. (člen řešitelského týmuresearch team member)
AbstraktAbstract
The KM3NeT project, a leading neutrino telescope (NT), offers groundbreaking opportunities in diverse physics areas, including ultra-high-energy cosmic ray (UHECR) detection, neutrino oscillation studies, dark matter searches, supernova detection, and more. IEAP CTU, a full member of KM3NeT since 2022, collaborates with NIKHEF-CPPM-LSM to explore astrophysical neutrinos through experimental and theoretical studies. Our scientific team of 7 members (4 experts and 3 PhD students) has a broad experience in this (10+ years of work in Baikal-GVD NT) and related areas of neutrino physics. Our research focuses on UHEC-neutrino studies and their sources. Additionally, we aim to refine digital optical module (DOM) characterization and calibration, enhancing NT performance. We will also provide theoretical estimates of KM3NeT NT's sensitivity to neutrino selfinteractions.
The KM3NeT project, a leading neutrino telescope (NT), offers groundbreaking opportunities in diverse physics areas, including ultra-high-energy cosmic ray (UHECR) detection, neutrino oscillation studies, dark matter searches, supernova detection, and more. IEAP CTU, a full member of KM3NeT since 2022, collaborates with NIKHEF-CPPM-LSM to explore astrophysical neutrinos through experimental and theoretical studies. Our scientific team of 7 members (4 experts and 3 PhD students) has a broad experience in this (10+ years of work in Baikal-GVD NT) and related areas of neutrino physics. Our research focuses on UHEC-neutrino studies and their sources. Additionally, we aim to refine digital optical module (DOM) characterization and calibration, enhancing NT performance. We will also provide theoretical estimates of KM3NeT NT's sensitivity to neutrino selfinteractions.
VýsledkyResults
- Neutrino-induced polarization rotation in active galactic nuclei plasmasNeutrino-induced polarization rotation in active galactic nuclei plasmas
- Observation of an ultra-high-energy cosmic neutrino with KM3NeTObservation of an ultra-high-energy cosmic neutrino with KM3NeT
- First searches for dark matter with the KM3NeT neutrino telescopesFirst searches for dark matter with the KM3NeT neutrino telescopes
- Search for neutrino emission from GRB 221009A using the KM3NeT ARCA and ORCA detectorsSearch for neutrino emission from GRB 221009A using the KM3NeT ARCA and ORCA detectors
- Astronomy potential of KM3NeT/ARCAAstronomy potential of KM3NeT/ARCA
- Probing invisible neutrino decay with the first six detection units of KM3NeT/ORCAProbing invisible neutrino decay with the first six detection units of KM3NeT/ORCA
- Measurement of neutrino oscillation parameters with the first six detection units of KM3NeT/ORCAMeasurement of neutrino oscillation parameters with the first six detection units of KM3NeT/ORCA
- KM3NeT constraint on Lorentz-violating superluminal neutrino velocityKM3NeT constraint on Lorentz-violating superluminal neutrino velocity
- Ultrahigh-Energy Event KM3-230213A within the Global Neutrino LandscapeUltrahigh-Energy Event KM3-230213A within the Global Neutrino Landscape
- Search for non-standard neutrino interactions with the first six detection units of KM3NeT/ORCASearch for non-standard neutrino interactions with the first six detection units of KM3NeT/ORCA
- Search for quantum decoherence in neutrino oscillations with six detection units of KM3NeT/ORCASearch for quantum decoherence in neutrino oscillations with six detection units of KM3NeT/ORCA
- Study of tau neutrinos and non-unitary neutrino mixing with the first six detection units of KM3NeT/ORCAStudy of tau neutrinos and non-unitary neutrino mixing with the first six detection units of KM3NeT/ORCA
- Constraints on Neutrino Self Interactions from Multi-messenger neutrinos scattering on CνBConstraints on Neutrino Self Interactions from Multi-messenger neutrinos scattering on CνB
- gSeaGen code by KM3NeT: An efficient tool to propagate muons simulated with CORSIKAgSeaGen code by KM3NeT: An efficient tool to propagate muons simulated with CORSIKA
- On the Potential Cosmogenic Origin of the Ultra-high-energy Event KM3-230213AOn the Potential Cosmogenic Origin of the Ultra-high-energy Event KM3-230213A