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Astroparticle and particle physics at ultra-high energy: results from the Pierre Auger Observatory
by Antonella Castellina
This Submission thread is now published as
Submission summary
| Authors (as registered SciPost users): | Antonella Castellina |
| Submission information | |
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| Preprint Link: | https://arxiv.org/abs/2209.15310v2 (pdf) |
| Date accepted: | 2023-06-22 |
| Date submitted: | 2022-12-02 10:50 |
| Submitted by: | Castellina, Antonella |
| Submitted to: | SciPost Physics Proceedings |
| Proceedings issue: | 21st International Symposium on Very High Energy Cosmic Ray Interactions (ISVHECRI2022) |
| Ontological classification | |
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| Academic field: | Physics |
| Specialties: |
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| Approach: | Experimental |
Abstract
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.
Author comments upon resubmission
The paper has been revised according almost all the comments of the anonymous referee. The limited total length of the proceeding did not allow to include more details about the results, but the provided bibliography can help in this respect.
Published as SciPost Phys. Proc. 13, 034 (2023)
Anonymous on 2022-12-19 [id 3156]
The reviewer thanks the author for the changes and accepts this paper for publication as it is.