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- W4381572783 abstract "The Kazakov-Solodukhin black hole metric represents a spherically symmetric deformation of the Schwarzschild solution due to quantum-gravity corrections. Assuming the absence of nonspherical deformations of the metric, this problem was solved nonperturbatively. In this study, we investigate the intensity of Hawking radiation in the background of such quantum-corrected black holes. Our findings indicate that while the geometry and various classical characteristics, such as the fundamental quasinormal modes or radius of the shadow, are only slightly altered, the Hawking radiation undergoes a much more significant change. Quantum corrections lead to a considerable enhancement of the Hawking radiation of the Standard Model fields. This effect arises due to much larger grey-body factors, while the Hawking temperature remains unaffected by the deformation." @default.
- W4381572783 created "2023-06-22" @default.
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- W4381572783 date "2023-06-19" @default.
- W4381572783 modified "2023-10-18" @default.
- W4381572783 title "Quantum gravity effects may accelerate black hole evaporation" @default.
- W4381572783 doi "https://doi.org/10.48550/arxiv.2306.11083" @default.
- W4381572783 hasPublicationYear "2023" @default.
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