On the quantum corrected gravitational collapse
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10.1016/j.physletb.2015.05.078
Inclou dades d'ús des de 2022
Cita com:
hdl:2117/78988
Tipus de documentArticle
Data publicació2015-06-09
EditorElsevier
Condicions d'accésAccés obert
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continguts d'aquesta obra estan subjectes a la llicència de Creative Commons
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Reconeixement 3.0 Espanya
ProjecteASPECTOS GEOMETRICOS EN MECANICA, CONTROL, TEORIA DE CAMPOS Y GRAVITACION (MINECO-MTM2014-54855-P)
Abstract
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.
CitacióTorres, R., Fayos, F. On the quantum corrected gravitational collapse. "Physics letters B", 09 Juny 2015, vol. 747, p. 245-250.
ISSN0370-2693
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Fitxers | Descripció | Mida | Format | Visualitza |
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DustEvaporante_PdfLaTeX_arXiv_v2.pdf | Article principal | 908,4Kb | Visualitza/Obre |