On Firewalls in quantum-corrected General Relativity
arXiv:1909.10048 · doi:10.1088/1742-6596/1390/1/012091
Abstract
We consider the information loss paradox at different angles, from the standard semi-classical approximation of General Relativity to the recently proposed scenarios of black holes evolution caused by effects of gravity quantization. Focusing on the Firewall proposal, we study the loop effects on the geometry and boundary conditions in black hole spacetimes and analyze the energy measured by an infalling observer near their horizons. As a result we obtain a trans-Planckian energy transition for the time-dependent black hole solution on the quantum-induced AdS background, the importance of which for the black hole (in)formation is discussed.
8 pp., 2 Figs. Based on the AJN's talk at ICPPA-2018, October 2018, Moscow, Russia. V2: minor changes, Refs updated
References in corpus (22)
- Area laws for the entanglement entropy - a review
- Black Holes: Complementarity or Firewalls?
- Information in Black Hole Radiation
- The Stretched Horizon and Black Hole Complementarity
- The fuzzball proposal for black holes: an elementary review
- Jerusalem Lectures on Black Holes and Quantum Information
- Better Late than Never: Information Retrieval from Black Holes
- The fuzzball proposal for black holes
- Information Loss
- Observation of two resonances in the systems and precise measurement of and properties
- Boundary conditions in the Unruh problem
- Backreaction of Hawking Radiation on a Gravitationally Collapsing Star I: Black Holes?
- Entanglement of the Vacuum between Left, Right, Future, and Past: The Origin of Entanglement-Induced Quantum Radiation
- Pure states and black hole complementarity
- Energy-momentum tensor and metric near the Schwarzschild sphere
- Quantum-induced trans-Planckian energy near horizon
- Quantum-corrected geometry of horizon vicinity
- Thermality from a Rindler quench
- Revisit of renormalization of Einstein-Maxwell theory at one-loop
- Entanglement-induced quantum radiation
- Quest for a 'direct' observation of the Unruh effect with classical electrodynamics: In honor of Atsushi Higuchi 60th anniversary
- Quantum-gravitational trans-Planckian energy of a time-dependent black hole