Muon Production in Relativistic Cosmic-Ray Interactions
Spencer R. Klein

TL;DR
This paper reviews high-energy muon production in cosmic-ray interactions, highlighting how muon data can reveal cosmic-ray composition and test high-energy particle physics models, especially with upcoming detector capabilities.
Contribution
It discusses muon production data, interprets it with soft models, and projects future measurements with IceCube and Km3Net to explore high-$p_T$ regimes.
Findings
Muon spectra measured by MACRO show high-energy cosmic-ray interactions.
IceCube and Km3Net will extend muon $p_T$ measurements into perturbative QCD regimes.
Muon data can complement collider experiments in understanding cosmic-ray composition.
Abstract
Cosmic-rays with energies up to eV have been observed. The nuclear composition of these cosmic rays is unknown but if the incident nuclei are protons then the corresponding center of mass energy is TeV. High energy muons can be used to probe the composition of these incident nuclei. The energy spectra of high-energy ( 1 TeV) cosmic ray induced muons have been measured with deep underground or under-ice detectors. These muons come from pion and kaon decays and from charm production in the atmosphere. Terrestrial experiments are most sensitive to far-forward muons so the production rates are sensitive to high- partons in the incident nucleus and low- partons in the nitrogen/oxygen targets. Muon measurements can complement the central-particle data collected at colliders. This paper will review muon production data and discuss some…
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Taxonomy
TopicsAstrophysics and Cosmic Phenomena · Particle Detector Development and Performance · Dark Matter and Cosmic Phenomena
