It has recently been proposed that the Hawking picture of black hole evaporation breaks down when the back reaction of the emitted radiation is included. Our reanalysis shows that the equation for the evolution of the horizon has well-behaved solutions which closely follow the Hawking picture
The formation and semiclassical evaporation of two-dimensional black holes is studied in an exactly ...
We investigate a model where the quantum dynamics of black hole evaporation is determined by imposin...
We propose a modified version of the Horowitz-Maldacena final-state boundary condition based upon a ...
Restricted Access.It has recently been proposed that the Hawking picture of previous termblack hole ...
The scope of this book is two-fold: the first part gives a fully detailed and pedagogical presentati...
An approach toward a self-consistent treatment, at a semiclassical level, of black hole evaporation ...
The inclusion of the back-reaction in the Hawking effect leads to the result that, if vector boson f...
Usually, Hawking radiation is derived assuming (i) that a future eternal event horizon forms, and (i...
We propose a simple quantum field theoretical toy model for black-hole evaporation and study the bac...
It is argued that primordial black holes with initial masses satisfying M<1015 g, instead of having ...
Empirical justification of the Hawking effect is carried out by adaptation of quantum field flat-spa...
This paper considers the effect of Hawking radiation on an eternal black hole- that is. a maximally ...
Abstract The near-horizon geometry of evaporation black holes is determined according to the semi-cl...
none2siWe study the evaporation of black holes in space-times with extra dimensions of size L by emp...
This paper argues that the effect of Hawking radiation on an astro-physical black hole situated in a...
The formation and semiclassical evaporation of two-dimensional black holes is studied in an exactly ...
We investigate a model where the quantum dynamics of black hole evaporation is determined by imposin...
We propose a modified version of the Horowitz-Maldacena final-state boundary condition based upon a ...
Restricted Access.It has recently been proposed that the Hawking picture of previous termblack hole ...
The scope of this book is two-fold: the first part gives a fully detailed and pedagogical presentati...
An approach toward a self-consistent treatment, at a semiclassical level, of black hole evaporation ...
The inclusion of the back-reaction in the Hawking effect leads to the result that, if vector boson f...
Usually, Hawking radiation is derived assuming (i) that a future eternal event horizon forms, and (i...
We propose a simple quantum field theoretical toy model for black-hole evaporation and study the bac...
It is argued that primordial black holes with initial masses satisfying M<1015 g, instead of having ...
Empirical justification of the Hawking effect is carried out by adaptation of quantum field flat-spa...
This paper considers the effect of Hawking radiation on an eternal black hole- that is. a maximally ...
Abstract The near-horizon geometry of evaporation black holes is determined according to the semi-cl...
none2siWe study the evaporation of black holes in space-times with extra dimensions of size L by emp...
This paper argues that the effect of Hawking radiation on an astro-physical black hole situated in a...
The formation and semiclassical evaporation of two-dimensional black holes is studied in an exactly ...
We investigate a model where the quantum dynamics of black hole evaporation is determined by imposin...
We propose a modified version of the Horowitz-Maldacena final-state boundary condition based upon a ...
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