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Astroparticle and particle physics at ultra-high energy: results from the Pierre Auger Observatory
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The scientific achievements of the Pierre Auger Collaboration cover diverse and complementary fields of research. The search for the origin of ultra-high energy cosmic rays (UHECRs) is based on the measurement of the energy spectrum and mass composition of the primaries, on studies of multi-messengers, and on extensive anisotropy searches. With the collected data it is also possible to explore the characteristics of hadronic interactions at energies unreachable at human-made accelerators, and to assess the existence of non-standard physics effects. A selection of the latest results is presented and the emerging picture is discussed.
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What do we know about cosmic rays with energies above 5 EeV?
Above 5 EeV, cosmic rays are extragalactic atomic nuclei whose average mass rises with energy, with arrival directions clustering toward nearby galaxies, but their sources are still unknown.
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