Investigation of Hadronic Interactions at Ultra-High Energies with the Pierre Auger Observatory

Abstract

The aim of the Pierre Auger Observatory is the investigation of the nature of cosmic ray particles at ultra-high energies. It can simultaneously observe the longitudinal air shower development in the atmosphere as well as particle densities on the ground. While there are no dedicated muon detectors, techniques have been developed to estimate the number of muons, $N_{\mu }$, produced by air showers. Both, the longitudinal development, in particular the depth of the shower maximum, $X_{\max }$, and the muon content of air showers are highly sensitive to hadronic interactions at ultra-high energies. Currently, none of the available hadronic interaction models used for simulations of extensive air showers is able to consistently describe the observations of $X_{\max }$ and $N_{\mu }$ made by the Pierre Auger Observatory.

Prepared for the proceedings of the XLIII Rencontres de Moriond QCD and High Energy Interactions 2009

References in corpus (4)

• Cosmic Rays from the Knee to the Highest Energies
• Reconstruction of Longitudinal Profiles of Ultra-High Energy Cosmic Ray Showers from Fluorescence and Cherenkov Light Measurements
• A Model-Independent Method of Determining Energy Scale and Muon Number in Cosmic Ray Surface Detectors
• Sensitivity of Extensive Air Showers to Features of Hadronic Interactions at Ultra-High Energies

Cited by in corpus (4)

• Testing Lorentz Invariance with Neutrinos from Ultrahigh Energy Cosmic Ray Interactions
• Superbradyons and some possible dark matter signatures
• Preon models, relativity, quantum mechanics and cosmology (I)
• Test of hadronic interaction models with air shower data