Black hole in asymmetric cosmological bounce
We determine the causal structure of the McVittie spacetime for a cosmological model with an asymmetric bounce. The analysis includes the computation of trapping horizons, regular, trapped, and anti-trapped regions, and the integration of the trajectories of radial null geodesics before, during, and...
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2021
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Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/124532 |
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I19-R120-10915-1245322023-06-07T14:18:03Z http://sedici.unlp.edu.ar/handle/10915/124532 issn:0004-6337 issn:1521-3994 Black hole in asymmetric cosmological bounce Pérez, Daniela Pérez Bergliaffa, Santiago Esteban Romero, Gustavo Esteban 2021 2021-09-09T16:29:15Z en Astronomía Black holes General Relativity Cosmology We determine the causal structure of the McVittie spacetime for a cosmological model with an asymmetric bounce. The analysis includes the computation of trapping horizons, regular, trapped, and anti-trapped regions, and the integration of the trajectories of radial null geodesics before, during, and after the bounce. We find a trapped region since the beginning of the contracting phase up to shortly before the bounce, thus showing the existence of a black hole. When the universe reaches a certain minimum scale in the contracting phase, the trapping horizons disappear and the central singularity becomes naked. These results suggest that neither a contracting nor an expanding universe can accommodate a black hole at all times. Facultad de Ciencias Astronómicas y Geofísicas Instituto Argentino de Radioastronomía Articulo Preprint http://creativecommons.org/licenses/by-nc-sa/4.0/ Creative Commons Attribution-NonCommercial-ShareAlike 4.0 International (CC BY-NC-SA 4.0) application/pdf 69-74 |
institution |
Universidad Nacional de La Plata |
institution_str |
I-19 |
repository_str |
R-120 |
collection |
SEDICI (UNLP) |
language |
Inglés |
topic |
Astronomía Black holes General Relativity Cosmology |
spellingShingle |
Astronomía Black holes General Relativity Cosmology Pérez, Daniela Pérez Bergliaffa, Santiago Esteban Romero, Gustavo Esteban Black hole in asymmetric cosmological bounce |
topic_facet |
Astronomía Black holes General Relativity Cosmology |
description |
We determine the causal structure of the McVittie spacetime for a cosmological model with an asymmetric bounce. The analysis includes the computation of trapping horizons, regular, trapped, and anti-trapped regions, and the integration of the trajectories of radial null geodesics before, during, and after the bounce. We find a trapped region since the beginning of the contracting phase up to shortly before the bounce, thus showing the existence of a black hole. When the universe reaches a certain minimum scale in the contracting phase, the trapping horizons disappear and the central singularity becomes naked. These results suggest that neither a contracting nor an expanding universe can accommodate a black hole at all times. |
format |
Articulo Preprint |
author |
Pérez, Daniela Pérez Bergliaffa, Santiago Esteban Romero, Gustavo Esteban |
author_facet |
Pérez, Daniela Pérez Bergliaffa, Santiago Esteban Romero, Gustavo Esteban |
author_sort |
Pérez, Daniela |
title |
Black hole in asymmetric cosmological bounce |
title_short |
Black hole in asymmetric cosmological bounce |
title_full |
Black hole in asymmetric cosmological bounce |
title_fullStr |
Black hole in asymmetric cosmological bounce |
title_full_unstemmed |
Black hole in asymmetric cosmological bounce |
title_sort |
black hole in asymmetric cosmological bounce |
publishDate |
2021 |
url |
http://sedici.unlp.edu.ar/handle/10915/124532 |
work_keys_str_mv |
AT perezdaniela blackholeinasymmetriccosmologicalbounce AT perezbergliaffasantiagoesteban blackholeinasymmetriccosmologicalbounce AT romerogustavoesteban blackholeinasymmetriccosmologicalbounce |
_version_ |
1768268489550725120 |