On the deficit of calculated muon flux at sea level for energies $>100$ GeV

Details On the deficit of calculated muon flux at sea level for energies $>100$ GeV On the deficit of calculated muon flux at sea level for energies $>100$ GeV

2005-03-04

arxiv.org/abs/astro-ph/0503092v1

Int.J.Mod.Phys. A20 (2005) 6959-6961

Astronomy and Astrophysics

Astrophysics

To be published in proceedings of the 19 ECRS (Florence, Italy, 2004)

Scientific paper

10.1142/S0217751X05030594

In this paper we discuss the problem, why the use of the direct data on primary nuclei spectra together with the modern hadronic interaction models leads to significant deficit of computed vertical muon flux at sea level for energies $>100$ GeV. We suggest, that to find out the source of this inconsistency it is necessary to perform an analysis of sensitivity of emulsion chamber data to variations of hadron-nucleus interaction characteristics. Such analysis will give more ground for discussion of adequacy of the up-to-date interaction models and of mutual compatibility of primary nuclei spectra, obtained in direct and EAS experiments.

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