Quantum-corrected geometry of horizon vicinity
arXiv:1704.04685 · doi:10.1002/prop.201700038
Abstract
We study the deformation of the horizon-vicinity geometry caused by quantum gravitational effects. Departure from the semi-classical picture is noted, and the fact that the matter part of the action comes at a higher order in Newton's constant than does the Einstein-Hilbert term is crucial for the departure. The analysis leads to a Firewall-type energy measured by an infalling observer for which quantum generation of the cosmological constant is critical. The analysis seems to suggest that the Firewall should be a part of such deformation and that the information be stored both in the horizon-vicinity and asymptotic boundary region. We also examine the behavior near the cosmological horizon.
31 pages, 1 figure, refs added, version to appear in Fortschritte der Physik
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- Revisit of renormalization of Einstein-Maxwell theory at one-loop
- Quantization of gravity and finite temperature effects
- Quantum-gravitational trans-Planckian energy of a time-dependent black hole
- Scattering on Quasi-Spherical Black-Holes: Features and Beyond
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