Abstract
The Asymptotic Safety scenario in quantum gravity provides a powerful framework to investigate the properties of black holes and spacetime singularities near the Planck scale. A rather robust prediction of this approach is that the final state of the black hole evaporation process is a Planck size remnant. Moreover, if the black hole is formed during a realistic gravitational collapse, quantum gravitational effects tend to suppress the inflation of the mass function at the Cauchy horizon. The scalar singularity in the future evolution of the spacetime is still present although its strength is much weaker than the classical case.
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Acknowledgments
It is a pleasure to thank Piero Nicolini and all the organizers of the KSM 2013 meeting for the warm hospitality and the exciting scientific environment.
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Bonanno, A. (2016). Black Holes in the Asymptotic Safety Program. In: Nicolini, P., Kaminski, M., Mureika, J., Bleicher, M. (eds) 1st Karl Schwarzschild Meeting on Gravitational Physics. Springer Proceedings in Physics, vol 170. Springer, Cham. https://doi.org/10.1007/978-3-319-20046-0_17
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