Visible inelasticity in starting tracks can statistically separate tau and muon neutrino events, yielding competitive sensitivity to the tau-to-muon flux ratio with current IceCube exposures.
Calculation of conventional and prompt lepton fluxes at very high energy
3 Pith papers cite this work. Polarity classification is still indexing.
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Pith papers citing it
abstract
An efficient method for calculating inclusive conventional and prompt atmospheric leptons fluxes is presented. The coupled cascade equations are solved numerically by formulating them as matrix equation. The presented approach is very flexible and allows the use of different hadronic interaction models, realistic parametrizations of the primary cosmic-ray flux and the Earth's atmosphere, and a detailed treatment of particle interactions and decays. The power of the developed method is illustrated by calculating lepton flux predictions for a number of different scenarios.
verdicts
UNVERDICTED 3representative citing papers
First muography at CJPL reconstructs directional overburden opacity map in agreement with satellite terrain models and predicts muon fluxes for CJPL-II halls.
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.
citing papers explorer
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Visible inelasticity as a probe of tau flavor content of astrophysical neutrinos
Visible inelasticity in starting tracks can statistically separate tau and muon neutrino events, yielding competitive sensitivity to the tau-to-muon flux ratio with current IceCube exposures.
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Mountain Muography for China Jinping Underground Laboratory
First muography at CJPL reconstructs directional overburden opacity map in agreement with satellite terrain models and predicts muon fluxes for CJPL-II halls.
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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.