Calculation of Secondary Particles in Atmosphere and Hadronic Interactions

Details Calculation of Secondary Particles in Atmosphere and Hadronic Interactions Calculation of Secondary Particles in Atmosphere and Hadronic Interactions

Aug 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002madm.conf..155b&link_type=abstract

MATTER, ANTI-MATTER AND DARK MATTER. Proceedings of the Second International Workshop. Held 29-30 October 2001 in Trento, Italy.

Physics

Cosmic Rays, Monte Carlo, Hadronic Interactions

Scientific paper

Calculation of secondary particles produced by the interaction of cosmic rays with the nuclei of Earth's atmosphere pose important requirements to particle production models. Here we summarize the important features of hadronic simulations, stressing the importance of the so called "microscopic" approach, making explicit reference to the case of the FLUKA code. Benchmarks are also presented.

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