| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 5493699 | Nuclear and Particle Physics Proceedings | 2016 | 5 Pages |
Abstract
Ultra-high energy cosmic ray experimental data are now of very good statistical significance even in the region of the expected GZK feature. The identification of their sources requires sophisticate analysis of their propagation in the extragalactic space. When looking at the details of this propagation some unforeseen features emerge. We will discuss some of these “surprises”.
Related Topics
Physical Sciences and Engineering
Physics and Astronomy
Nuclear and High Energy Physics
Authors
Denise Boncioli, Armando di Matteo, Aurelio Grillo, Pierre Auger Collaboration Pierre Auger Collaboration,