| dc.description | The authors acknowledge the financial support of the funding
agencies: Funds for Scientific Research (FRS-FNRS), Francqui foundation, BAEF foundation.
Czech Science Foundation (GAČR 24-12702S); Agence Nationale de la Recherche (contract
ANR-15-CE31-0020), Centre National de la Recherche Scientifique (CNRS), Commission Européenne (FEDER fund and Marie Curie Program), LabEx UnivEarthS (ANR-10-LABX-0023
and ANR-18-IDEX-0001), Paris Île-de-France Region, Normandy Region (Alpha, Blue-waves
and Neptune), France; Shota Rustaveli National Science Foundation of Georgia (SRNSFG,
FR-22-13708), Georgia; This work is part of the MuSES project which has received funding
from the European Research Council (ERC) under the European Union’s Horizon 2020 Research and Innovation Programme (grant agreement No 101142396). The General Secretariat
of Research and Innovation (GSRI), Greece; Istituto Nazionale di Fisica Nucleare (INFN) and
Ministero dell’Università e della Ricerca (MUR), through PRIN 2022 program (Grant PANTHEON 2022E2J4RK, Next Generation EU) and PON R&I program (Avviso n. 424 del 28
febbraio 2018, Progetto PACK-PIR01 00021), Italy; IDMAR project Po-Fesr Sicilian Region
az. 1.5.1; A. De Benedittis, W. Idrissi Ibnsalih, M. Bendahman, A. Nayerhoda, G. Papalashvili,
I. C. Rea, A. Simonelli have been supported by the Italian Ministero dell’Università e della
Ricerca (MUR), Progetto CIR01 00021 (Avviso n. 2595 del 24 dicembre 2019); KM3NeT4RR
MUR Project National Recovery and Resilience Plan (NRRP), Mission 4 Component 2
Investment 3.1, Funded by the European Union – NextGenerationEU,CUP I57G21000040001,
Concession Decree MUR No. n. Prot. 123 del 21/06/2022; Ministry of Higher Education,
Scientific Research and Innovation, Morocco, and the Arab Fund for Economic and Social
Development, Kuwait; Nederlandse organisatie voor Wetenschappelijk Onderzoek (NWO),
the Netherlands; Ministry of Research, Innovation and Digitalisation, Romania; Slovak Research and Development Agency under Contract No. APVV-22-0413; Ministry of Education,
Research, Development and Youth of the Slovak Republic; MCIN for PID2021-124591NB-C41,
-C42, -C43 and PDC2023-145913-I00 funded by MCIN/AEI/10.13039/501100011033 and by
“ERDF A way of making Europe”, for ASFAE/2022/014 and ASFAE/2022 /023 with funding
from the EU NextGenerationEU (PRTR-C17.I01) and Generalitat Valenciana, for Grant
AST22_6.2 with funding from Consejería de Universidad, Investigación e Innovación and Gobierno de España and European Union — NextGenerationEU, for CSIC-INFRA23013 and for
CNS2023-144099, Generalitat Valenciana for CIDEGENT/2018/034, /2019/043, /2020/049,
/2021/23, for CIDEIG/2023/20, for CIPROM/2023/51 and for GRISOLIAP/2021/192 and
EU for MSC/101025085, Spain; Khalifa University internal grants (ESIG-2023-008 and
RIG-2023-070), United Arab Emirates; The European Union’s Horizon 2020 Research and
Innovation Programme (ChETEC-INFRA — Project no. 101008324). | es_ES |
| dc.description.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 Γij ∝ (E/E0)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. | es_ES |