Electrons, muons and hadrons in extensive air showers and how do they depend on nuclear interaction model, part 1

Details Electrons, muons and hadrons in extensive air showers and how do they depend on nuclear interaction model, part 1 Electrons, muons and hadrons in extensive air showers and how do they depend on nuclear interaction model, part 1

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....7...12w&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 7 p 12-15 (SEE N85-35968 24-93)

Mathematics

Cosmic Ray Showers, Electrons, Hadrons, High Energy Interactions, Nuclear Interactions, Photons, Simulation, Distribution (Property), Energy Spectra, Mathematical Models, Monte Carlo Method, Particle Production

Scientific paper

Monte Carlo simulations of extensive air showers were performed using a
couple of different nuclear interaction models and obtaining a variety
of shower characteristics. The discussion of these shows that the
sensitivity of observables to the primary mass spectrum is significantly
stronger than to the interaction model, the latter being quite weak.

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