Roberto Aloisio
Published 2012-07-09Version 1
We discuss the basic features of the propagation of Ultra High Energy Cosmic Rays in astrophysical backgrounds, comparing two alternative computation schemes to compute the expected fluxes. We also discuss the issue of the transition among galactic and extra-galactic cosmic rays using theoretical results on fluxes to compare different models.
Comments: 6 pages, 6 .eps figures, invited talk given at the 'International Symposium on Future Directions in UHECR Physics', 13-16 February 2012, CERN, Geneva (Switzerland)
Journal: EPJ Web of Conferences 53, 06001 (2013)
Diffusive Propagation of High Energy Cosmic Rays in Galaxy: Effect of Hall Drift
Radio emission of extensive air shower at CODALEMA: Polarization of the radio emission along the v*B vector
Experimental/Observational Summary - Very High Energy Cosmic Rays and their Interactions
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