Comparison of the measured atmospheric muon rate with Monte Carlo simulations and sensitivity study for detection of prompt atmospheric muons with KM3NeT
Piotr Kalaczy\'nski (for the KM3NeT Collaboration)

TL;DR
This paper compares measured atmospheric muon rates at KM3NeT with Monte Carlo simulations and explores the potential for detecting prompt atmospheric muons, which are crucial for understanding high-energy cosmic ray interactions.
Contribution
It provides the first comparison of KM3NeT atmospheric muon data with detailed Monte Carlo simulations and assesses the sensitivity to prompt muons at different depths.
Findings
Measured muon rates agree with simulations within uncertainties
First estimates of prompt muon signals at KM3NeT depths are presented
The study enhances understanding of atmospheric muons for neutrino telescope calibration
Abstract
The KM3NeT Collaboration has successfully deployed the first detection units of the next generation undersea neutrino telescopes in the Mediterranean Sea at the two sites in Italy and in France. The data sample collected between December 2016 and January 2020 has been used to measure the atmospheric muon rate at two different depths under the sea level: 3.5 km with KM3NeT-ARCA and 2.5 km with KM3NeT-ORCA. Atmospheric muons represent an abundant signal in a neutrino telescope and can be used to test the reliability of the Monte Carlo simulation chain and to study the physics of extensive air showers caused by highly-energetic primary nuclei impinging the Earth's atmosphere. At energies above PeV the contribution from prompt muons, created right after the first interaction in the shower, is expected to become dominant, however its existence has not yet been experimentally confirmed. In…
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