Probing invisible neutrino decay with the first six detection units of KM3NeT/ORCA

TL;DR

This study uses early data from KM3NeT/ORCA to search for signs of invisible neutrino decay, finding results consistent with the Standard Model and setting constraints on decay parameters.

Contribution

First analysis of invisible neutrino decay using initial six detection units of KM3NeT/ORCA with a novel likelihood approach.

Findings

Best-fit decay parameter consistent with zero within uncertainties

Results compatible with Standard Model at 2.1 sigma

Provides new constraints on neutrino decay parameters

Abstract

In the era of precision measurements of neutrino oscillation parameters, it is necessary for experiments to disentangle discrepancies that may indicate physics beyond the Standard Model in the neutrino sector. KM3NeT/ORCA is a water Cherenkov neutrino detector under construction and anchored at the bottom of the Mediterranean Sea. The detector is designed to study the oscillations of atmospheric neutrinos and determine the neutrino mass ordering. This paper focuses on the initial configuration of ORCA, referred to as ORCA6, which comprises six out of the foreseen 115 detection units of photosensors. A high-purity neutrino sample was extracted during 2020 and 2021, corresponding to an exposure of 433 kton-years. This sample is analysed following a binned log-likelihood approach to search for invisible neutrino decay, in a three-flavour neutrino oscillation scenario, where the third neutrino mass state $\nu_3$ decays into an invisible state, e.g. a sterile neutrino. The resulting best fit of the invisible neutrino decay parameter is $\alpha_3 = 0.92^{+1.08}_{-0.57}\times 10^{-4}~\mathrm{eV^2}$, corresponding to a scenario with $\theta_{23}$ in the second octant and normal neutrino mass ordering. The results are consistent with the Standard Model, within a $2.1\,\sigma$ interval.