We describe the ground state for a gravitationally collapsed ball of dust as the direct product of wavefunctions for dust particles distributed over an arbitrary number of nested layers. This allows us to estimate the expectation value of the global radius as well as the effective energy density and pressures for the dust core of quantum black holes. In particular, the size of the quantum core does not depend on the number of layers and the mass function is shown to grow linearly with the areal radius up to the outermost layer.Comment: 9 pages, 2 figures. Version to appear in PL
We study the quantum dynamics of the Lema\^itre-Tolman-Bondi space-times using a polymer quantizatio...
International audienceThe fate of matter forming a black hole is still an open problem, although mod...
Quantum gravity suggests that the paradox recently put forward by Almheiri et al. (AMPS) can be reso...
We describe the ground state for a gravitationally collapsed ball of dust as the direct product of w...
Gravitational collapses are natural laboratories where observable signatures of a quantum theory of...
We present a simple quantum description of the gravitational collapse of a ball of dust which exclud...
We present a new quantum description for the Oppenheimer-Snyder model of gravitational collapse of a...
We study the effect of rotation on the spectrum of bound states for dust cores that source (quantum)...
If we consider the gravitational collapse of a material object to a black hole, we would expect, for...
The gravitational collapse plays an important role in the formation of black holes as well as for ou...
This paper considers the quantum collapse of infinitesimally thin dust shells in 2+1 gravity. In 2+1...
Astrophysical objects and the surrounding geometry must be described by suitable states in the compl...
The relative flow of the Schwarzschild vs. the proper time during the classical evolution of a colla...
The Schwarzschild black hole can be viewed as the special case of the marginally bound Lema\^\i tre-...
We solve the Klein-Gordon equation for a scalar field, in the background geometry of a dust cloud co...
We study the quantum dynamics of the Lema\^itre-Tolman-Bondi space-times using a polymer quantizatio...
International audienceThe fate of matter forming a black hole is still an open problem, although mod...
Quantum gravity suggests that the paradox recently put forward by Almheiri et al. (AMPS) can be reso...
We describe the ground state for a gravitationally collapsed ball of dust as the direct product of w...
Gravitational collapses are natural laboratories where observable signatures of a quantum theory of...
We present a simple quantum description of the gravitational collapse of a ball of dust which exclud...
We present a new quantum description for the Oppenheimer-Snyder model of gravitational collapse of a...
We study the effect of rotation on the spectrum of bound states for dust cores that source (quantum)...
If we consider the gravitational collapse of a material object to a black hole, we would expect, for...
The gravitational collapse plays an important role in the formation of black holes as well as for ou...
This paper considers the quantum collapse of infinitesimally thin dust shells in 2+1 gravity. In 2+1...
Astrophysical objects and the surrounding geometry must be described by suitable states in the compl...
The relative flow of the Schwarzschild vs. the proper time during the classical evolution of a colla...
The Schwarzschild black hole can be viewed as the special case of the marginally bound Lema\^\i tre-...
We solve the Klein-Gordon equation for a scalar field, in the background geometry of a dust cloud co...
We study the quantum dynamics of the Lema\^itre-Tolman-Bondi space-times using a polymer quantizatio...
International audienceThe fate of matter forming a black hole is still an open problem, although mod...
Quantum gravity suggests that the paradox recently put forward by Almheiri et al. (AMPS) can be reso...