SciPost Submission Page
Astroparticle and particle physics at ultra-high energy: results from the Pierre Auger Observatory
by Antonella Castellina, for the Pierre Auger Collaboration
This is not the latest submitted version.
This Submission thread is now published as
Submission summary
| Authors (as registered SciPost users): | Antonella Castellina |
| Submission information | |
|---|---|
| Preprint Link: | scipost_202209_00067v1 (pdf) |
| Date submitted: | 2022-09-30 15:10 |
| Submitted by: | Castellina, Antonella |
| Submitted to: | SciPost Physics Proceedings |
| Proceedings issue: | 21st International Symposium on Very High Energy Cosmic Ray Interactions (ISVHECRI2022) |
| Ontological classification | |
|---|---|
| Academic field: | Physics |
| Specialties: |
|
| 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.
Current status:
Reports on this Submission
Strengths
This is an interesting paper worth publishing after revision
Weaknesses
The author frequently uses jargon formulations, which need to be reformulated.
Also, the author is using long sentences, which are not characteristic for the English language; these need to be split into 2 (or more) separate sentences.
Report
This article meets the journal acceptance criteria, but the text needs language and formulation revision
Requested changes
the suggested changes and requests are inserted directly in the attached PDF file