ÚTEFČVUT Ústav technické a experimentální fyziky ČVUT v PrazeInstitute of Experimental and Applied Physics, CTU in Prague

Search for quantum decoherence in neutrino oscillations with six detection units of KM3NeT/ORCA

NázevTitle
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
Druh výsledkuResult type
Článek v časopiseJournal article
AutořiAuthors
S. Aiello, A. Albert, A.R. Alhebsi, M. Alshamsi, Z. Bardačova, E. Eckerová, F. Mamedov, Y. Shitov, I. Štekl
Klíčová slovaKeywords
frequentist statistics, neutrino experiments
ExperimentCollaboration
KM3NeT
DOIDOI
10.1088/1475-7516/2025/03/039
Časopis / citaceJournal / citation
Journal of Cosmology and Astroparticle Physics 2025(03), 039 (2025) · ISSN 1475-7516
RokYear
2025
JazykLanguage
eng
ZáznamyRecords
ProjektProject
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
CitovánoCited by
16 (INSPIRE-HEP)
2024: 12025: 52026: 10
Citace ke staženíDownload citation
TXT · BibTeX

AbstraktAbstract

Neutrinos described as an open quantum system may interact with the environment which introduces stochastic perturbations to their quantum phase. This mechanism leads to a loss of coherence along the propagation of the neutrino - a phenomenon commonly referred to as decoherence - and ultimately, to a modification of the oscillation probabilities. Fluctuations in space-time, as envisaged by various theories of quantum gravity, are a potential candidate for a decoherence-inducing environment. Consequently, the search for decoherence provides a rare opportunity to investigate quantum gravitational effects which are usually beyond the reach of current experiments. In this work, quantum decoherence effects are searched for in neutrino data collected by the KM3NeT/ORCA detector from January 2020 to November 2021. The analysis focuses on atmospheric neutrinos within the energy range of a few GeV to 100 GeV. Adopting the open quantum system framework, decoherence is described in a phenomenological manner with the strength of the effect given by the parameters Γ21 and Γ31. Following previous studies, a dependence of the type Γ ij ∝ (E/E 0) n on the neutrino energy is assumed and the cases n = -2,-1 are explored. No significant deviation with respect to the standard oscillation hypothesis is observed. Therefore, 90% CL upper limits are estimated as Γ21 < 4.6· 1021GeV and Γ31 < 8.4· 1021GeV for n = -2 and Γ21 < 1.9· 10-22GeV and Γ31 < 2.7· 10-22GeV for n = -1, respectively.

Neutrinos described as an open quantum system may interact with the environment which introduces stochastic perturbations to their quantum phase. This mechanism leads to a loss of coherence along the propagation of the neutrino - a phenomenon commonly referred to as decoherence - and ultimately, to a modification of the oscillation probabilities. Fluctuations in space-time, as envisaged by various theories of quantum gravity, are a potential candidate for a decoherence-inducing environment. Consequently, the search for decoherence provides a rare opportunity to investigate quantum gravitational effects which are usually beyond the reach of current experiments. In this work, quantum decoherence effects are searched for in neutrino data collected by the KM3NeT/ORCA detector from January 2020 to November 2021. The analysis focuses on atmospheric neutrinos within the energy range of a few GeV to 100 GeV. Adopting the open quantum system framework, decoherence is described in a phenomenological manner with the strength of the effect given by the parameters Γ21 and Γ31. Following previous studies, a dependence of the type Γ ij ∝ (E/E 0) n on the neutrino energy is assumed and the cases n = -2,-1 are explored. No significant deviation with respect to the standard oscillation hypothesis is observed. Therefore, 90% CL upper limits are estimated as Γ21 < 4.6· 1021GeV and Γ31 < 8.4· 1021GeV for n = -2 and Γ21 < 1.9· 10-22GeV and Γ31 < 2.7· 10-22GeV for n = -1, respectively.

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