SciPost Submission Page
Limits to gauge coupling in the dark sector of super-heavy dark matter particles from the Pierre Auger Observatory data
by Olivier Deligny for the Pierre Auger Collaboration
Submission summary
| Authors (as registered SciPost users): | Olivier Deligny |
| Submission information | |
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| Preprint Link: | scipost_202209_00056v1 (pdf) |
| Date accepted: | Aug. 28, 2023 |
| Date submitted: | Sept. 27, 2022, 12:48 p.m. |
| Submitted by: | Olivier Deligny |
| 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
Assuming that the energy density of super-heavy particles matches that of dark matter observed today, tight constraints on the couplings governing the decay process are presented as a function of the particle mass. These constraints are obtained from the lack of signatures that would be suggestive of decaying super-heavy $X$ particles in the data of the Pierre Auger Observatory. In particular, instanton-induced decay processes allow us to derive a bound on the reduced coupling constant of gauge interactions in the dark sector: \boldmath $\alpha_X \lesssim 0.09$,\unboldmath\, for \boldmath $10^{9} \lesssim M_X/\mathrm{GeV} < 10^{19}$\unbolmath . Cosmological aspects for super-heavy dark matter production during the reheating epoch are discussed.
Published as SciPost Phys. Proc. 13, 013 (2023)
Reports on this Submission
Report #1 by Subir Sarkar (Referee 1) on 2022-11-21 (Contributed Report)
- Cite as: Subir Sarkar, Report on arXiv:scipost_202209_00056v1, delivered 2022-11-21, doi: 10.21468/SciPost.Report.7724
