Hunting for super-heavy dark matter with the highest-energy cosmic rays
arXiv:1903.05429 · doi:10.1103/PhysRevD.99.103016
Abstract
In 15 years of data taking the Pierre Auger Observatory has observed no events beyond GeV. This null result translates into an upper bound on the flux of ultrahigh-energy cosmic rays implying GeV) km sr yr, at the 90\%C.L. We interpret this bound as a constraint on extreme-energy photons originating in the decay super-heavy dark matter (SHDM) particles clustered in the Galactic halo. Armed with this constraint we derive the strongest lower limit on the lifetime of hadronically decaying SHDM particles with masses in the range, GeV . We also explore the capability of future NASA's POEMMA mission to search for SHDM signals.
Matching version accepted for publication in PRD
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- GCOS -- The Global Cosmic Ray Observatory
- Limits to gauge coupling in the dark sector set by the non-observation of instanton-induced decay of Super-Heavy Dark Matter in the Pierre Auger Observatory data
- Diffuse flux of ultra-high energy photons from cosmic-ray interactions in the disk of the Galaxy and implications for the search for decaying super-heavy dark matter
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- Gravitational Atoms
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