Diffractive Contribution to the Elasticity and the Nucleonic Flux in the Atmosphere

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We calculate the average elasticity considering non-diffractive and single diffractive interactions and perform an analysis of the cosmic-ray flux by means of an analytical solution for the nucleonic diffusion equation. We show that the diffractive contribution is important for the adequate description of the nucleonic and hadronic fluxes in the atmosphere.
10 pages, latex, 2 figures (uuencoded PostScript)

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High Energy Physics - Phenomenology

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http://salesiana.dossiersoluciones.com/handle/123456789/187001

Consulte el texto completo en el siguiente enlace:

https://arxiv.org/abs/hep-ph/9507346
 http://arxiv.org/abs/hep-ph/9507346
 J.Phys.G23:125-134,1997
 doi:10.1088/0954-3899/23/1/010

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arXiv