Issue |
EPJ Web Conf.
Volume 280, 2023
RICAP-22, 8th Roma International Conference on Astroparticle Physics
|
|
---|---|---|
Article Number | 07001 | |
Number of page(s) | 4 | |
Section | Indirect DM Search | |
DOI | https://doi.org/10.1051/epjconf/202328007001 | |
Published online | 20 March 2023 |
https://doi.org/10.1051/epjconf/202328007001
Pierre Auger Observatory and Super Heavy Dark Matter
1
Gran Sasso Science Institute,
viale F. Crispi 7,
67100
L’Aquila,
Italy
2
INFN - Laboratori Nazionali Gran Sasso,
via G. Acitelli 22,
67100
Assergi (AQ), Italy
3
Observatorio Pierre Auger,
Av. San Martín Norte 304,
5613
Malargüe, Argentina
* roberto.aloisio@gssi.it
** spokespersons@auger.org. A complete list of authors can be found at https://www.auger.org/archive/authors_2022_09.html
Published online: 20 March 2023
We briefly discuss the connection of the Pierre Auger Observatory data with a large class of dark matter models based on the early universe generation of super heavy particles, their role in the solution of the dark matter problem, highlighting the remarkable constraining capabilities of the Auger observations.
© 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 (http://creativecommons.org/licenses/by/4.0/).
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.