Cosmic Ray Physics with the KM3NeT Telescopes

TL;DR

The KM3NeT telescopes detect atmospheric muons and neutrinos in seawater, enabling diverse cosmic ray physics studies, including flux measurements and detector calibration, with recent improvements in simulation accuracy.

Contribution

This paper presents the first atmospheric muon neutrino flux measurement with KM3NeT/ORCA and incorporates the Daemonflux model to improve simulation-data agreement.

Findings

Successful measurement of atmospheric muon neutrino flux.

Integration of Daemonflux reduces simulation discrepancies.

Enhanced understanding of atmospheric muons for calibration and systematic studies.

Abstract

The KM3NeT research infrastructure instruments a large volume of seawater using photomultiplier tubes, which are sensitive to the Cherenkov radiation stimulated by the products of neutrino interactions in the water, as well as that stimulated by atmospheric muons which penetrate the sea depths. The KM3NeT/ARCA and KM3NeT/ORCA detectors are situated at different depths in the Mediterranean Sea, with different extension and densities of the photo-detection elements. Although operating independently, taken as a whole the two detectors provide a wide energy coverage for the atmospheric muons flux. Through the detection and analysis of these atmospheric muons, a variety of physics studies are possible with the KM3NeT telescope. A measurement of the atmospheric muon neutrino flux has been carried out with data from the initial six detection units of the KM3NeT/ORCA detector. Relatedly to the atmospheric muon flux, the recent atmospheric lepton model `Daemonflux' has been incorporated into the KM3NeT Monte Carlo event generator for atmospheric muon bundles. This has resulted in a stark alleviation of the atmospheric muon data-Monte Carlo simulation discrepancy - a systemic issue in cosmic ray experiments referred to as the `Muon Puzzle' - and a comprehensive description of the atmospheric muon data in KM3NeT. These atmospheric muons are also used in the calibration of the detectors, as well as constraining systematic uncertainties in the detectors such as the optical properties of the instrumented seawater. An overview of these topics, and other cosmic ray analyses, is presented.