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Black Holes in the Asymptotic Safety Program

  • Alfio BonannoEmail author
Chapter
Part of the Springer Proceedings in Physics book series (SPPHY, volume 170)

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.

Keywords

Black Hole Gravitational Wave Outer Horizon Cauchy Horizon Spacetime Singularity 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

Notes

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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Copyright information

© Springer International Publishing Switzerland 2016

Authors and Affiliations

  1. 1.Istituto Nazionale di AstrofisicaOsservatorio Astrofisico di CataniaCataniaItaly
  2. 2.Istituto Nazionale di Fisica NucleareSezione di CataniaCataniaItaly

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