International audienceAt the end of the Hawking evaporation the horizon of a black hole enters a physical region where quantum gravity cannot be neglected. The physics of this region has not been much explored. We characterize its physics and introduce a technique to study it
This paper argues that the effect of Hawking radiation on an astro-physical black hole situated in a...
We propose that in quantum gravity one needs to impose a final state boundary condition at black hol...
A coherent picture of the quantum mechanics of a collapse-formed, evaporating black hole is presente...
International audienceAt the end of the Hawking evaporation the horizon of a black hole enters a phy...
International audienceWe derive an explicit expression for the transition amplitude from black to wh...
The formation and semiclassical evaporation of two-dimensional black holes is studied in an exactly ...
The impact of the leading quantum gravity effects on the dynamics of the Hawking evaporation process...
We incorporate elements of the recently discovered exact solutions of the quantum constraints of loo...
One of the most intriguing problem of modern physics is the question of the endpoint of black hole e...
International audienceWe construct and discuss the form of the (effective) spacetime geometry inside...
We present a semi-classical model for the formation and evaporation of a four dimensional black hole...
A paradigm describing black hole evaporation in non-perturbative quantum gravity is developed by com...
We investigate a model where the quantum dynamics of black hole evaporation is determined by imposin...
The inclusion of the back-reaction in the Hawking effect leads to the result that, if vector boson f...
In this paper, we argue that once quantum gravitational effects change the classical geometry of a b...
This paper argues that the effect of Hawking radiation on an astro-physical black hole situated in a...
We propose that in quantum gravity one needs to impose a final state boundary condition at black hol...
A coherent picture of the quantum mechanics of a collapse-formed, evaporating black hole is presente...
International audienceAt the end of the Hawking evaporation the horizon of a black hole enters a phy...
International audienceWe derive an explicit expression for the transition amplitude from black to wh...
The formation and semiclassical evaporation of two-dimensional black holes is studied in an exactly ...
The impact of the leading quantum gravity effects on the dynamics of the Hawking evaporation process...
We incorporate elements of the recently discovered exact solutions of the quantum constraints of loo...
One of the most intriguing problem of modern physics is the question of the endpoint of black hole e...
International audienceWe construct and discuss the form of the (effective) spacetime geometry inside...
We present a semi-classical model for the formation and evaporation of a four dimensional black hole...
A paradigm describing black hole evaporation in non-perturbative quantum gravity is developed by com...
We investigate a model where the quantum dynamics of black hole evaporation is determined by imposin...
The inclusion of the back-reaction in the Hawking effect leads to the result that, if vector boson f...
In this paper, we argue that once quantum gravitational effects change the classical geometry of a b...
This paper argues that the effect of Hawking radiation on an astro-physical black hole situated in a...
We propose that in quantum gravity one needs to impose a final state boundary condition at black hol...
A coherent picture of the quantum mechanics of a collapse-formed, evaporating black hole is presente...
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