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Percolation and cosmic ray physics above $10^{17}$eV

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arxiv hep-ph/0511279 v1 pith:226M5JJ6 submitted 2005-11-23 hep-ph

P. Brogueira , J. Dias de Deus , M.C. Espirito Santo , M. Pimenta This is my paper · ORCID
classification hep-ph
keywords energyabovedependencepercolationarguearoundaveragechange
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abstract

We argue that the energy dependence of the average position of the shower maximum, $\bar X_{max}$, and of the number of produced muons, $N_{\mu}$, can be explained by a change, around $10^{17}$eV, in the energy dependence of the inelasticity $K$, which decreases with the energy above the string percolation threshold.

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