Roberto Aloisio
Published 2011-04-02Version 1
The status of the observations of Ultra High Energy Cosmic Rays will be reviewed, focusing on the the latest results of HiRes and Auger observatories. A comprehensive analytical computation scheme to compute the expected UHECR spectrum on earth will be presented, applying such scheme to interpret the experimental results. The phenomenological scenarios favored by HiRes and Auger in terms of chemical composition and spectrum will be also presented.
Comments: 6 pages, 5 eps figures, invited review talk at the International Symposium on the Recent Progress of Ultra High Energy Cosmic Ray Observation, Nagoya (Japan) Dec 10-12 2010
Journal: AIP Conf.Proc. 1367 (2011) 114-119
The Production of Ultra High Energy Cosmic Rays during the Early Epochs of Radio-loud AGN
Ultra High Energy Cosmic Rays: Anisotropies and Spectrum
Resolution of (Heavy) Primaries in Ultra High Energy Cosmic Rays
![QR code for arXiv:1104.0329 [astro-ph.HE]](http://oss.arxitics.com/images/favicon.svg)