Inelasticity in p-nucleus collisions and its application to high energy cosmic-ray cascades
arXiv:astro-ph/9704061 · doi:10.1103/PhysRevD.56.3135
Abstract
We employ a simple multiple scattering model to investigate the inclusive reaction p + A --> p + X for projectile momenta in the 100-200 GeV/c range. We find that data are consistent with a class of interaction models in which the stopping power of nuclei is rather low. We discuss extrapolation to ultra-high energy and the application to interpretation of cosmic-ray air showers at energies up to 10^20 eV.
9 pages, RevTeX, revtex.sty, psfig.sty
Cited by in corpus (17)
- Ultra-High-Energy Cosmic Rays
- Cosmic Neutrino Pevatrons: A Brand New Pathway to Astronomy, Astrophysics, and Particle Physics
- Extensive Air Shower Simulations at the Highest Energies
- The AGASA/SUGAR Anisotropies and TeV Gamma Rays from the Galactic Center: A Possible Signature of Extremely High-energy Neutrons
- Pinning down the cosmic ray source mechanism with new IceCube data
- The Composition of Cosmic Rays at the Knee
- Proton-air cross section measurement with the ARGO-YBJ cosmic ray experiment
- On total inelastic cross-sections and the average depth of the maximum of extensive air showers
- Estimating the inelasticity with the information theory approach
- Hadronic interactions models beyond collider energies
- Estimating the contribution of Galactic sources to the diffuse neutrino flux
- Inelaticity in hadron-nucleus collisions from emulsion chamber studies
- Systematics of Leading Particle Production
- Investigating starburst-driven neutrino emission from galaxies in the Great Observatories All-Sky LIRG Survey
- Behavior of the diffractive cross section in hadron-nucleus collisions
- Leading nucleon and inelasticity in hadron-nucleus interactions
- Diffractive dissociation in proton-nucleus collisions at collider energies