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Published on: August 12, 2013
Gauge-gravity duality and the black hole interior.
Donald Marolf1, Joseph Polchinski
1Department of Physics, University of California, Santa Barbara, California 93106-9530, USA.
This study presents a new argument for black hole firewalls, independent of external entanglement. It also challenges the idea that highly entangled states can be represented as smooth wormholes in spacetime.
Area of Science:
- Theoretical Physics
- Quantum Gravity
- Black Hole Physics
Background:
- The firewall paradox in black hole physics questions the validity of the equivalence principle at the event horizon.
- Existing arguments often rely on entanglement between the black hole interior and external systems.
- The ER=EPR conjecture proposes a connection between entanglement and wormholes.
Purpose of the Study:
- To present a novel argument for the existence of firewalls at the event horizon of black holes with field theory duals.
- To demonstrate that this argument is independent of entanglement with distant systems.
- To analyze the ER=EPR conjecture, specifically concerning the geometric interpretation of highly entangled states.
Main Methods:
- Development of a new theoretical argument for black hole firewalls.
- Analysis of entanglement properties in quantum field theory and black hole thermodynamics.
- Investigation of the geometric interpretation of quantum correlations in the context of the ER=EPR conjecture.
Main Results:
- A new argument supports the presence of firewalls at black hole horizons, irrespective of external entanglement.
- This firewall argument is not circumvented by identifying internal and external degrees of freedom.
- Correlations in generic highly entangled states cannot be geometrically represented as smooth wormholes.
Conclusions:
- The firewall paradox persists even when considering internal black hole degrees of freedom.
- The ER=EPR conjecture, in its simplest geometric interpretation, may not fully capture the nature of quantum correlations in highly entangled states.
- Further theoretical developments are needed to reconcile quantum mechanics and general relativity in the context of black holes.
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