AbstractPure states in quantum field theory can be represented by many-fingered block-time wave functions, which treat time on an equal footing with space and make the notions of “time evolution” and “state at a given time” fundamentally irrelevant. Instead of information destruction resulting from an attempt to use a “state at a given time” to describe semi-classical black-hole evaporation, the full many-fingered block-time wave function of the universe conserves information by describing the correlations of outgoing Hawking particles in the future with ingoing Hawking particles in the past
We study information retrieval from evaporating black holes, assuming that the internal dynamics of ...
The recent progress in string theory strongly suggests that formation and evaporation of black holes...
The black hole information paradox arises from an apparent conflict between the Hawking black hole r...
AbstractPure states in quantum field theory can be represented by many-fingered block-time wave func...
In a recent article, we have shown how quantum fluctuations of the background geometry modify Hawkin...
A paradigm describing black hole evaporation in non-perturbative quantum gravity is developed by com...
In a recent article, we have shown how quantum fluctuations of the background geometry modify Hawkin...
We propose a resolution to the black-hole information-loss paradox: in one formulation of physical t...
In a recent article, we have shown how quantum fluctuations of the background geometry modify Hawkin...
In a recent article, we have shown how quantum fluctuations of the background geometry modify Hawkin...
In a recent article, we have shown how quantum fluctuations of the background geometry modify Hawkin...
In a recent article, we have shown how quantum fluctuations of the background geometry modify Hawkin...
We show that, in order to preserve the equivalence principle until late times in unitarily evaporati...
We construct and discuss the form of the (effective) spacetime geometry inside a black hole undergoi...
Continuity across the shock wave of two regions in the metric during the formation of a black hole c...
We study information retrieval from evaporating black holes, assuming that the internal dynamics of ...
The recent progress in string theory strongly suggests that formation and evaporation of black holes...
The black hole information paradox arises from an apparent conflict between the Hawking black hole r...
AbstractPure states in quantum field theory can be represented by many-fingered block-time wave func...
In a recent article, we have shown how quantum fluctuations of the background geometry modify Hawkin...
A paradigm describing black hole evaporation in non-perturbative quantum gravity is developed by com...
In a recent article, we have shown how quantum fluctuations of the background geometry modify Hawkin...
We propose a resolution to the black-hole information-loss paradox: in one formulation of physical t...
In a recent article, we have shown how quantum fluctuations of the background geometry modify Hawkin...
In a recent article, we have shown how quantum fluctuations of the background geometry modify Hawkin...
In a recent article, we have shown how quantum fluctuations of the background geometry modify Hawkin...
In a recent article, we have shown how quantum fluctuations of the background geometry modify Hawkin...
We show that, in order to preserve the equivalence principle until late times in unitarily evaporati...
We construct and discuss the form of the (effective) spacetime geometry inside a black hole undergoi...
Continuity across the shock wave of two regions in the metric during the formation of a black hole c...
We study information retrieval from evaporating black holes, assuming that the internal dynamics of ...
The recent progress in string theory strongly suggests that formation and evaporation of black holes...
The black hole information paradox arises from an apparent conflict between the Hawking black hole r...