期刊
PHYSICS LETTERS B
卷 747, 期 -, 页码 245-250出版社
ELSEVIER SCIENCE BV
DOI: 10.1016/j.physletb.2015.05.078
关键词
Gravitational collapse; Black holes; Singularities; Quantum gravity; Information paradox
资金
- Ministerio de Economia y Competitividad (Spain) [MTM2014-54855-P]
Based on a previously found general class of quantum improved exact solutions composed of non-interacting (dust) particles, we model the gravitational collapse of stars. As the modeled star collapses a closed apparent 3-horizon is generated due to the consideration of quantum effects. The effect of the subsequent emission of Hawking radiation related to this horizon is taken into consideration. Our computations lead us to argue that a total evaporation could be reached. The inferred global picture of the spacetime corresponding to gravitational collapse is devoid of both event horizons and shell-focusing singularities. As a consequence, there is no information paradox and no need of firewalls. (C) 2015 The Authors. Published by Elsevier B.V.
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