The Pierre Auger Observatory is the largest ultrahigh-energy cosmic ray observatory in the world. The huge amount of high quality data collected since 2004 up to now led to great improvements in our knowledge of the ultra-energetic cosmic rays. The suppression of the cosmic-ray flux at highest energies was clearly established, and the extra-galactic origin of these particles was confirmed. On the other hand, measurements of the depth of shower maximum indicate a puzzling trend in the mass composition of cosmic rays at energy around the ankle up to the highest energy. The just started upgrade of the Observatory, dubbed AugerPrime, will improve the identification of the mass of primaries allowing us to disentangle models of origin and propagation of cosmic rays.

Buscemi M. (2018). The Pierre Auger Observatory: Latest results and future perspectives. EPJ WEB OF CONFERENCES, 182, 02023 [10.1051/epjconf/201818202023].

The Pierre Auger Observatory: Latest results and future perspectives

Buscemi M.
2018-08-03

Abstract

The Pierre Auger Observatory is the largest ultrahigh-energy cosmic ray observatory in the world. The huge amount of high quality data collected since 2004 up to now led to great improvements in our knowledge of the ultra-energetic cosmic rays. The suppression of the cosmic-ray flux at highest energies was clearly established, and the extra-galactic origin of these particles was confirmed. On the other hand, measurements of the depth of shower maximum indicate a puzzling trend in the mass composition of cosmic rays at energy around the ankle up to the highest energy. The just started upgrade of the Observatory, dubbed AugerPrime, will improve the identification of the mass of primaries allowing us to disentangle models of origin and propagation of cosmic rays.
3-ago-2018
Settore FIS/01 - Fisica Sperimentale
6th International Conference on New Frontiers in Physics, ICNFP 2017
OAC, grc
2017
Buscemi M. (2018). The Pierre Auger Observatory: Latest results and future perspectives. EPJ WEB OF CONFERENCES, 182, 02023 [10.1051/epjconf/201818202023].
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/10447/546624
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