Do active galactic nuclei convert dark matter into visible particles?
A. A. Grib, Yu. V. Pavlov

TL;DR
This paper explores the hypothesis that dark matter particles, possibly superheavy and metastable, can decay into visible particles in active galactic nuclei, potentially explaining ultra high energy cosmic rays.
Contribution
It investigates a novel mechanism where dark matter decay in active galactic nuclei produces observable high-energy cosmic rays, linking dark matter properties to astrophysical phenomena.
Findings
Dark matter particles can decay into visible particles in AGN environments.
Decay processes may account for ultra high energy cosmic rays observed by Auger.
Numerical estimates support the feasibility of the proposed decay mechanism.
Abstract
The hypothesis that dark matter consists of superheavy particles with the mass close to the Grand Unification scale is investigated. These particles were created from vacuum by the gravitation of the expanding Universe and their decay led to the observable baryon charge. Some part of these particles with the lifetime larger than the time of breaking of the Grand Unification symmetry became metastable and survived up to the modern time as dark matter. However in active galactic nuclei due to large energies of dark matter particles swallowed by the black hole the opposite process can occur. Dark matter particles become interacting. Their decay on visible particles at the Grand Unification energies leads to the flow of ultra high energy cosmic rays observed by the Auger group. Numerical estimates of the effect leading to the observable numbers are given.
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