Hadronic High Energy Interactions and Atmospheric Cascades

Details Hadronic High Energy Interactions and Atmospheric Cascades Hadronic High Energy Interactions and Atmospheric Cascades

Sep 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011aipc.1367...64p&link_type=abstract

INTERNATIONAL SYMPOSIUM ON THE RECENT PROGRESS OF ULTRA-HIGH ENERGY COSMIC RAY OBSERVATION. AIP Conference Proceedings, Volume

Physics

Cosmic Ray Showers, Energy Loss Of Particles, Acceleration, Perturbation Theory, Cosmic Ray Interactions, Extensive Air Showers, Energy Loss And Stopping Power, Particle Acceleration, Perturbative Calculations, Cosmic-Ray Interactions

Scientific paper

The main observables of high energy air showers depend on the nature and energy of the primary cosmic ray particles. As a result, simulation of showers initiated by hadronic particles will have a strong dependence on the physics of hadronic interactions at energies well above even the LHC. Using a simplified model to describe hadronic and electromagnetic air shower development, the source of uncertainties in air shower observables can be understood. We will consider how a realistic description of hadronic interactions and detailed simulations of air showers can be achieved with our current knowledge of particle physics and show the consequences on the interpretation of charged cosmic ray data.

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