AbstractWe investigate a universal behavior of thermodynamics and evaporation process for the regular black holes. We observe an important point where the temperature is maximum, the heat capacity is changed from negative infinity to positive infinity, and the free energy is minimum. Furthermore, this point separates the evaporation process into the early stage with negative heat capacity and the late stage with positive heat capacity. The latter represents the quantum cooling evaporation process. As a result, the whole evaporation process could be regarded as the inverse Hawking–Page phase transition
In this paper we obtain the black hole metric from a semiclassical analysis of loop quantum black ho...
We review (anti)evaporation phenomena within the context of quantum gravity and extended theories of...
An approach toward a self-consistent treatment, at a semiclassical level, of black hole evaporation ...
We investigate a universal behavior of thermodynamics and evaporation process for the regular black ...
AbstractWe consider Hawking radiation as due to a tunneling process in a black hole were quantum cor...
In the model of Expansive Nondecelerative Universe, black hole cannot totally evaporate via quantum ...
We describe the black hole evaporation process driven by the dynamical evolution of the quantum grav...
The impact of the leading quantum gravity effects on the dynamics of the Hawking evaporation process...
We present a semi-classical model for the formation and evaporation of a four dimensional black hole...
A model based on the topology change of a quantum manifold is used to explain the origin of the blac...
In 1974 Steven Hawking showed that black holes emit thermal radiation, which eventually causes them ...
In the present paper we consider, using our earlier results, the process of quantum gravitational co...
Abstract The semi-classical Hawking evaporation process of Reissner–Nordström black holes is analyze...
We propose a modified version of the Horowitz-Maldacena final-state boundary condition based upon a ...
We propose a modified version of the Horowitz-Maldacena final-state boundary condition based upon a ...
In this paper we obtain the black hole metric from a semiclassical analysis of loop quantum black ho...
We review (anti)evaporation phenomena within the context of quantum gravity and extended theories of...
An approach toward a self-consistent treatment, at a semiclassical level, of black hole evaporation ...
We investigate a universal behavior of thermodynamics and evaporation process for the regular black ...
AbstractWe consider Hawking radiation as due to a tunneling process in a black hole were quantum cor...
In the model of Expansive Nondecelerative Universe, black hole cannot totally evaporate via quantum ...
We describe the black hole evaporation process driven by the dynamical evolution of the quantum grav...
The impact of the leading quantum gravity effects on the dynamics of the Hawking evaporation process...
We present a semi-classical model for the formation and evaporation of a four dimensional black hole...
A model based on the topology change of a quantum manifold is used to explain the origin of the blac...
In 1974 Steven Hawking showed that black holes emit thermal radiation, which eventually causes them ...
In the present paper we consider, using our earlier results, the process of quantum gravitational co...
Abstract The semi-classical Hawking evaporation process of Reissner–Nordström black holes is analyze...
We propose a modified version of the Horowitz-Maldacena final-state boundary condition based upon a ...
We propose a modified version of the Horowitz-Maldacena final-state boundary condition based upon a ...
In this paper we obtain the black hole metric from a semiclassical analysis of loop quantum black ho...
We review (anti)evaporation phenomena within the context of quantum gravity and extended theories of...
An approach toward a self-consistent treatment, at a semiclassical level, of black hole evaporation ...