Cosmic ray shower simulations and the primary energy spectrum above 100,000 TeV

Details Cosmic ray shower simulations and the primary energy spectrum above 100,000 TeV Cosmic ray shower simulations and the primary energy spectrum above 100,000 TeV

Jan 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975jphg....1..134t&link_type=abstract

Journal of Physics, Part G - Nuclear Physics, vol. 1, Jan. 10, 1975, p. 134-149. Research supported by the Science Research Cou

Physics

Nuclear Physics

5

Astronomical Models, Computerized Simulation, Cosmic Ray Showers, Energy Spectra, High Energy Interactions, Primary Cosmic Rays, Electron Distribution, Particle Interactions, Particle Size Distribution, Photon Density, Proton-Proton Reactions, Scattering Cross Sections

Scientific paper

The consequences of applying the model for air shower development suggested by Gaisser (1974) to primaries of energy between 100,000 and 1,000,000 TeV are investigated. It is shown that there is as good agreement between the predictions from this model with observations of average shower characteristics as there was between the observations and earlier simulation data based upon simple models for high-energy interactions. The effects of adopting the Gaisser model on the conversion of observational data to the primary particle energy spectrum are considered.

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