Abstract
Consider a non-stationary extension of black hole solutions to the quantum-extended (one-loop GR) system of Einstein–Maxwell equations with a complex scalar field. Important representatives of these solutions are non-stationary rotating black holes located inside the active galactic nuclei. Computing the local energy density of a freely falling observer one finds, upon appropriate boundary conditions, the trans-Planckian leap of the local energy density near the event horizons. Thus, one locates a “Firewall”, which, on one hand, serves as a source of fluxes of ultra-high-energy cosmic rays out of the active galactic nuclei, and, on the other hand, is originally designed to resolve the Hawking paradox in black hole physics.
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ACKNOWLEDGMENTS
I wish to thank the Organizers of International Bogolyubov Conference “Problems of Theoretical and Mathematical Physics” 2019. I am grateful to In-Yong Park for stimulating discussions and pleasant collaboration. This work is partially supported by Ministry of Science and Education of Ukraine under the “Science in Universities” program.
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Nurmagambetov, A.J. Quantum Leaps in the Vicinity of One-Loop Gravity Black Holes. Phys. Part. Nuclei 51, 739–743 (2020). https://doi.org/10.1134/S1063779620040553
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DOI: https://doi.org/10.1134/S1063779620040553