Small air showers and collider physics

Details Small air showers and collider physics Small air showers and collider physics

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....7...24c&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 7 p 24-27 (SEE N85-35968 24-93)

Mathematics

Cosmic Ray Showers, Nucleon-Nucleon Interactions, Nucleons, Proton-Proton Reactions, Protons, Simulation, Comparison, Decay, Distribution (Property), Energy Spectra, Mathematical Models, Monte Carlo Method, Particle Collisions

Scientific paper

At energies lower than 2.5 X 10 to the 5 GeV (in Lab. system), more accurate information on nucleon-nucleon collision (p-p collider and on primary composition now exist. The behavior of those both basic elements in cosmic ray phenomenology from ISR energy suggests some tendencies for reasonable extrapolation in the next decade 2.0x10 to the 5 to 2.0x10 to the 6 GeV. Small showers in altitude, recorded in the decade 2 X 10 to the 4 to 2 X 10 to the 5 GeV offers a good tool to testify the validity of all the Monte-Carlo simulation analysis and appreciate how nucleon-air collision are different from nucleon-nucleon collisions.

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