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245 10 $a Black hole in asymmetric cosmological bounce / $c Daniela Pérez, Santiago E. Perez Bergliaffa, Gustavo E. Romero.
490 0# $a Trabajos publicados del IAR ; $v no. 1593
520 ## $a 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 antitrapped 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.
773 0# $7 ||as $t Astronomische Nachrichten $d Wiley $x 1521-3994 $g Vol. (2021), p.
100 1# $a Pérez, D. $q (Daniela)
700 1# $a Pérez-Bergliaffa, S. E. $q (Santiago Esteban)
700 1# $a Romero, G. E. $q (Gustavo Esteban)
653 ## $a Black holes.
653 ## $a Cosmology.
653 ## $a General Relativity.
040 ## $a AR-BaBIR
856 ## $u https://doi.org/10.1002/asna.202113883 $y DOI
856 ## $u https://www.iar.unlp.edu.ar/biblio/htdocs/artic/contri/1593.pdf $y PDF
856 ## $u https://www.iar.unlp.edu.ar/biblio/htdocs/artic/contri/1594.pdf $y PDF

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