Characterization of the Atmospheric Muon Flux in IceCube
IceCube Collaboration: M. G. Aartsen, K. Abraham, M. Ackermann, J., Adams, J. A. Aguilar, M. Ahlers, M. Ahrens, D. Altmann, T. Anderson, M., Archinger, C. Arguelles, T. C. Arlen, J. Auffenberg, X. Bai, S. W. Barwick,, V. Baum, R. Bay, J. J. Beatty, J. Becker Tjus, K.-H. Becker

TL;DR
This paper details how IceCube detects and analyzes atmospheric muons to understand cosmic ray interactions, revealing the muon energy spectrum and evidence of prompt decay contributions at high energies.
Contribution
It introduces new techniques for extracting physical measurements from atmospheric muon data and provides first results on muon multiplicity and energy spectra at PeV energies.
Findings
Muon multiplicity spectrum aligns with surface detector results.
Single muon energy spectrum extends to PeV energies.
Evidence of a prompt decay component in the muon flux.
Abstract
Muons produced in atmospheric cosmic ray showers account for the by far dominant part of the event yield in large-volume underground particle detectors. The IceCube detector, with an instrumented volume of about a cubic kilometer, has the potential to conduct unique investigations on atmospheric muons by exploiting the large collection area and the possibility to track particles over a long distance. Through detailed reconstruction of energy deposition along the tracks, the characteristics of muon bundles can be quantified, and individual particles of exceptionally high energy identified. The data can then be used to constrain the cosmic ray primary flux and the contribution to atmospheric lepton fluxes from prompt decays of short-lived hadrons. In this paper, techniques for the extraction of physical measurements from atmospheric muon events are described and first results are…
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