Singularity-free gravitational collapse and asymptotic safety
A general class of quantum improved stellar models with interiors composed of non-interacting (dust) particles is obtained and analyzed in a framework compatible with asymptotic safety. First, the effective exterior, based on the Quantum Einstein Gravity approach to asymptotic safety is presented an...
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| Tipo de recurso: | artículo |
| Fecha de publicación: | 2014 |
| País: | España |
| Institución: | Universitat Politècnica de Catalunya (UPC) |
| Repositorio: | UPCommons. Portal del coneixement obert de la UPC |
| Idioma: | inglés |
| OAI Identifier: | oai:upcommons.upc.edu:2117/25170 |
| Acceso en línea: | https://hdl.handle.net/2117/25170 https://dx.doi.org/10.1016/j.physletb.2014.04.010 |
| Access Level: | acceso abierto |
| Palabra clave: | Black holes (Astronomy) Gravitational collapse Black holes Singularities Quantum gravity Asymptotic safety Naked singularities General relativity Black-holes Spacetimes Time Gravitació Forats negres (Astronomia) Àrees temàtiques de la UPC::Física::Relativitat |
| Sumario: | A general class of quantum improved stellar models with interiors composed of non-interacting (dust) particles is obtained and analyzed in a framework compatible with asymptotic safety. First, the effective exterior, based on the Quantum Einstein Gravity approach to asymptotic safety is presented and, second, its effective compatible dust interiors are deduced. The resulting stellar models appear to be devoid of shell-focusing singularities. (C) 2014 The Author. Published by Elsevier B.V. |
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