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

2002-02-19

arxiv.org/abs/hep-ph/0202182v1

Int.J.Mod.Phys. A17 (2002) 1743-1754

Physics

High Energy Physics

High Energy Physics - Phenomenology

10 pages, 4 figures. Extended version of report given at the IInd Workshop on Matter and anti-Matter, Trento, Oct. 2001

Scientific paper

10.1142/S0217751X02011242

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. Some benchmarks are also presented.

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