Composition from high $p_\mathrm{T}$ muons in IceCube
D. Soldin (for the IceCube Collaboration)

TL;DR
This paper explores how high transverse momentum muons detected by IceCube can reveal the composition of ultra-high-energy cosmic rays and test quantum chromodynamics predictions in high-energy particle interactions.
Contribution
It introduces a method to determine cosmic ray composition through muon separation measurements and discusses recent IceCube results using high $p_T$ muons.
Findings
Muon separation correlates with primary cosmic ray composition.
IceCube's measurements support pQCD predictions for high-energy interactions.
High $p_T$ muons can distinguish between different cosmic ray nuclei.
Abstract
Cosmic rays with energies up to enter the atmosphere and produce showers of secondary particles. Inside these showers muons with high transverse momentum () are produced from the decay of heavy hadrons, or from high pions and kaons very early in the shower development. These isolated muons can have large transverse separations from the shower core up to several hundred meters, together with the muon bundle forming a double or triple track signature in IceCube. The separation from the core is a measure of the transverse momentum of the muon's parent particle. Assuming the validity of perturbative quantum chromodynamics (pQCD) the muon lateral distribution depends on the composition of the incident nuclei, thus the composition of high energy cosmic rays can be determined from muon separation measurements. Vice…
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Taxonomy
TopicsAstrophysics and Cosmic Phenomena · Neutrino Physics Research · Dark Matter and Cosmic Phenomena
