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

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

2005-11-23

arxiv.org/abs/hep-ph/0511279v1

Physics

High Energy Physics

High Energy Physics - Phenomenology

8 pages, 4 figures (6 eps files), latex

Scientific paper

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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