Report on Tests and Measurements of Hadronic Interaction Properties with Air Showers
arXiv:1902.08124 · doi:10.1051/epjconf/201921002004
Abstract
We present a summary of recent tests and measurements of hadronic interaction properties with air showers. This report has a special focus on muon density measurements. Several experiments reported deviations between simulated and recorded muon densities in extensive air showers, while others reported no discrepancies. We combine data from eight leading air shower experiments to cover shower energies from PeV to tens of EeV. Data are combined using the z-scale, a unified reference scale based on simulated air showers. Energy-scales of experiments are cross-calibrated. Above 10 PeV, we find a muon deficit in simulated air showers for each of the six considered hadronic interaction models. The deficit is increasing with shower energy. For the models EPOS-LHC and QGSJet-II.04, the slope is found significant at 8 sigma.
Submitted to the Proceedings of UHECR2018
References in corpus (4)
- Testing Hadronic Interactions at Ultrahigh Energies with Air Showers Measured by the Pierre Auger Observatory
- Probing the evolution of the EAS muon content in the atmosphere with KASCADE-Grande
- Development of a Machine Learning Based Analysis Chain for the Measurement of Atmospheric Muon Spectra with IceCube
- Average shape of longitudinal shower profiles measured at the Pierre Auger Observatory
Cited by in corpus (51)
- IceCube-Gen2: The Window to the Extreme Universe
- The Forward Physics Facility: Sites, Experiments, and Physics Potential
- The Muon Puzzle in cosmic-ray induced air showers and its connection to the Large Hadron Collider
- Imaging the nucleus with high-energy photons
- Forward Neutrino Fluxes at the LHC
- Ultra-High-Energy Cosmic Rays: The Intersection of the Cosmic and Energy Frontiers
- Measurements of All-Particle Energy Spectrum and Mean Logarithmic Mass of Cosmic Rays from 0.3 to 30 PeV with LHAASO-KM2A
- Glauber Monte Carlo predictions for ultra-relativistic collisions with
- An explanation of the muon puzzle of ultrahigh-energy cosmic rays and the role of the Forward Physics Facility for model improvement
- Opportunities for new physics searches with heavy ions at colliders
- Density of GeV muons in air showers measured with IceTop
- Espresso and Stochastic Acceleration of Ultra-high-energy Cosmic Rays in Relativistic Jets
- Enhancing the cosmic-ray mass sensitivity of air-shower arrays by combining radio and muon detectors
- The very forward CASTOR calorimeter of the CMS experiment
- First Measurement of the Muon Neutrino Interaction Cross Section and Flux as a Function of Energy at the LHC with FASER
- Science and Project Planning for the Forward Physics Facility in Preparation for the 2024-2026 European Particle Physics Strategy Update
- The NEVOD-EAS air-shower array
- High-Energy Galactic Cosmic Rays (Astro2020 Science White Paper)
- The rise of muon content in extensive air showers after the 3 PeV knee of the primary cosmic ray spectrum according to data of the Tien Shan mountain installation
- What is the nature and origin of the highest-energy particles in the universe?
- Determination of the Cosmic-Ray Chemical Composition: Open Issues and Prospects
- Modeling Strangeness Enhancements to resolve the Muon Excess in Cosmic Ray Extensive Air Shower Data
- Sub-TeV hadronic interaction model differences and their impact on air showers
- Air shower genealogy for muon production
- Muon puzzle in ultra-high energy EASs according to Yakutsk array and Auger experiment data
- Scaling violation in interaction of cosmic ray hadrons and the nature of the 3 PeV knee in the spectrum of primary cosmic rays
- Status of the Yakutsk air shower array and future plans
- Neutrino Experiments at the Large Hadron Collider
- Hypothetical Lorentz invariance violation and the muon content of extensive air showers
- Potential for measuring the longitudinal and lateral profile of muons in TeV air showers with IACTs
- Muons in EASs with eV according to data of the Yakutsk Array
- Deep learning method for identifying mass composition of ultra-high-energy cosmic rays
- Top pair production at ultra-high energies
- Road map for the tuning of hadronic interaction models with accelerator-based and astroparticle data
- Muon lateral distribution function of extensive air showers: results of the Sydney University Giant Air-shower Recorder versus modern Monte-Carlo simulations
- Detecting LHC Neutrinos at Surface Level
- Studying the mass sensitivity of air-shower observables using simulated cosmic rays
- A Direct Comparison of Muon Measurements at the Yakutsk Array and the Pierre Auger Observatory
- Measurements and tests of hadronic interactions at ultra-high energies with the Pierre Auger Observatory
- Bose-Einstein condensation and muon production in ultra-high energy cosmic ray particle collisions
- Measurement of the mean number of muons with energies above 500 GeV in air showers detected with the IceCube Neutrino Observatory
- Composition determination of cosmic rays from the muon content of the showers
- Cosmogenic Muon Background Characterization for the Colorado Underground Research Institute (CURIE)
- Particle physics in cosmic rays
- Probing Hadronic Interactions with Cosmic Rays
- Letter of Intent: The Forward Physics Facility
- The Forward Physics Facility at the High-Luminosity LHC
- Energy spectrum and mass composition of the primary cosmic rays based on the intensity of muon bundles detected in the NEVOD-DECOR experiment
- Using the Virasoro conditions to revise the model of a quark-gluon string fragmentation
- Calculation of rescaling factors and nuclear multiplication of muons in extensive air showers
- The puzzle of composition of cosmic rays with energies (2-12.5) EeV according to muon detectors data of the Yakutsk EAS array