QGSM-based prompt muon calculations match IceCube spectra above 500 TeV, while lower charm-production models require extra flux from rare decays of eta, eta', rho, omega, and phi mesons.
The IceCube Neutrino Observatory - Contributions to ICRC 2017 Part III: Cosmic Rays
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Papers on cosmic-ray measurements submitted to the 35th International Cosmic Ray Conference (ICRC 2017, Busan, South Korea) by the IceCube Collaboration
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High-energy atmospheric muon flux calculations in comparison with recent measurements
QGSM-based prompt muon calculations match IceCube spectra above 500 TeV, while lower charm-production models require extra flux from rare decays of eta, eta', rho, omega, and phi mesons.