Testing hadronic interaction packages at cosmic ray energies
arXiv:0903.2409 · doi:10.1103/PhysRevD.79.054006
Abstract
A comparative analysis of the secondary particles output of the main hadronic interaction packages used in simulations of extensive air showers is presented. Special attention is given to the study of events with very energetic leading secondary particles, including diffractive interactions.
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Cited by in corpus (10)
- Hadronic Multiparticle Production at Ultra-High Energies and Extensive Air Showers
- Ultra-High-Energy Cosmic Rays
- Probing the Nuclear Symmetry Energy with Heavy Ion Collisions
- Electromagnetic Structure of Few-Nucleon Ground States
- Strange fireball as an explanation of the muon excess in Auger data
- Coherent Cherenkov radio pulses from hadronic showers up to EeV energies
- LHC updated hadronic interaction packages analyzed up to cosmic-ray energies
- Lorentz invariance violation as an explanation of muon excess in Auger data
- A comprehensive study of shower to shower fluctuations
- Investigating the influence of diffractive interactions on ultra - high energy extensive air showers