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

  • Sezione di Catania
  • Institut de Recherches Subatomiques
  • University of Haute Alsace
  • CPPM
  • Sezione di Napoli
  • Università di Napoli 'Federico II' and Sezione INFN
  • INFN
  • Universitat Politécnica de Catalunya
  • Université de Nantes
  • Universidad Politecnica de Valencia
  • Faculte des Sciences
  • Université de Paris
  • Università degli Studi di Genova
  • Sezione di Genova
  • Ensicaen
  • Comenius University
  • Sezione di Bologna
  • University of Bologna
  • Second University of Naples
  • University of Hull
  • North-West University
  • Universite de Annaba
  • University of Salerno
  • Institute of Space Sciences
  • TNO Bldg. and Construction Research
  • Dipartimento di Fisica

Research output: Contribution to journalArticlepeer-review

5 Scopus citations

Abstract

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.

Original languageBritish English
Article number039
JournalJournal of Cosmology and Astroparticle Physics
Volume2025
Issue number3
DOIs
StatePublished - 1 Mar 2025

Keywords

  • Frequentist statistics
  • neutrino experiments

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