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

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dc.creatorBrogueira, P.
dc.creatorde Deus, J. Dias
dc.creatorSanto, M. C. Espirito
dc.creatorPimenta, M.
dc.date2005-11-23
dc.date.accessioned2026-07-07T06:50:07Z
dc.date.available2026-07-07T06:50:07Z
dc.descriptionWe argue that the energy dependence of the average position of the shower maximum, $\bar X_{max}$, and of the number of produced muons, $N_μ$, 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.
dc.description8 pages, 4 figures (6 eps files), latex
dc.identifierhttps://arxiv.org/abs/hep-ph/0511279
dc.identifierhttp://arxiv.org/abs/hep-ph/0511279
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/104586
dc.subjectHigh Energy Physics - Phenomenology
dc.titlePercolation and cosmic ray physics above $10^{17}$eV
dc.typetext

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