Electrons, muons and hadrons in extensive air showers and how do they depend on nuclear interaction model, part 2

Details Electrons, muons and hadrons in extensive air showers and how do they depend on nuclear interaction model, part 2 Electrons, muons and hadrons in extensive air showers and how do they depend on nuclear interaction model, part 2

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....7....1w&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 7 p 1-4 (SEE N85-35968 24-93)

Physics

1

Cosmic Ray Showers, Electrons, Models, Muons, Nuclear Interactions, Protons, Distribution (Property), Energy Spectra, Errors, Monte Carlo Method, Particle Production, Simulation

Scientific paper

Some of the results of Monte Carlo simulations of extensive air showers for nuclear interactions models are presented. The most significant part of scaling violation effect is generated by the inclusion of rising cross-section. Among the models considered the lowest value for Eo/N(max) is obtained when rapidly rising cross-section and charge exchange are both included (model R-F01). The value is still 1.38 GeV/electron. Except at the highest energies, the sensitivity to atomic mass of the primary is greater than to specific assumptions about multiple production.

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