| Issue |
EPJ Web Conf.
Volume 283, 2023
Ultra High Energy Cosmic Rays (UHECR 2022)
|
|
|---|---|---|
| Article Number | 04004 | |
| Number of page(s) | 7 | |
| Section | UHECR Sources, Acceleration Mechanisms and Multi-Messenger Astrophysics | |
| DOI | https://doi.org/10.1051/epjconf/202328304004 | |
| Published online | 28 April 2023 | |
https://doi.org/10.1051/epjconf/202328304004
Multi-messenger studies with the Pierre Auger Observatory
Universtità del Salento and INFN Lecce (Italy)
* Corresponding author: lorenzo.perrone@le.infn.it
** Corresponding author: spokespersons@auger.org
Published online: 28 April 2023
The combination of data from observatories measuring ultra-high energy cosmic rays, photons, neutrinos and gravitational waves has provided new insights into the most extreme phenomena in the Universe. Sharing information within a broad community is the foundation of the multi-messenger approach. The Pierre Auger Observatory, the world’s largest cosmic ray detector, provides sensitivity to photons and neutrinos above 1017 eV, thus contributing significantly to this joint effort. The latest results from diffuse and targeted searches will be reviewed here, along with results from follow-up analyses and future perspectives. In particular, preliminary limits on photon fluence from a selection of gravitational wave sources detected by LIGO/Virgo and results of the search for ultra-high energy neutrinos from binary black hole mergers will be presented.
Observatorio Pierre Auger, Av. San Martín Norte 304, 5613 Malargüe, Argentina
Full author list: https://www.auger.org/archive/authors_2022_10.html
© The Authors, published by EDP Sciences, 2023
This is an Open Access article distributed under the terms of the Creative Commons Attribution License 4.0, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
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