Measurement of the atmospheric νe and νμ energy spectra with the ANTARES neutrino telescope

This letter presents a combined measurement of the energy spectra of atmospheric nu(e) and nu(mu) in the energy range between similar to 100 GeV and similar to 50 TeV with the ANTARES neutrino telescope. The analysis uses 3012 days of detector livetime in the period 2007-2017, and selects 1016 neutrinos interacting in (or close to) the instrumented volume of the detector, yielding shower-like events (mainly from nu(e) + (nu) over bar (e) charged current plus all neutrino neutral current interactions) and starting track events (mainly from nu(mu) + (nu) over bar (mu) charged current interactions). The contamination by atmospheric muons in the final sample is suppressed at the level of a few per mill by different steps in the selection analysis, including a Boosted Decision Tree classifier. The distribution of reconstructed events is unfolded in terms of electron and muon neutrino fluxes. The derived energy spectra are compared with previous measurements that, above 100 GeV, are limited to experiments in polar ice and, for nu(mu), to Super-Kamiokande. (C) 2021 The Author(s). Published by Elsevier B.V.

Automated summary

This study presents a combined measurement of the energy spectra of atmospheric nu(e) and nu(mu) using the ANTARES neutrino telescope in the high energy range. The analysis focuses on interactions of neutrinos within the detector, yielding electron and muon neutrino fluxes. The results are compared with previous measurements, revealing the energy spectra of atmospheric neutrinos.