The C-metric black hole near the IR-brane in the AdS_4 space
| dc.creator | Zakout, I. | |
| dc.date | 2002-10-07 | |
| dc.date.accessioned | 2026-07-07T04:14:15Z | |
| dc.date.available | 2026-07-07T04:14:15Z | |
| dc.description | We study the black hole shape using the C-metric solution for a matter trapped near the IR-brane in the ${AdS}_4$ space. In the AdS/CFT duality, the IR-brane is introduced by embedding a 2-brane at the ${AdS}_4$ radius $z=l$, while the UV-brane is defined by the ${AdS}_4$ boundary. We find the C-metric solution generates a negative tension IR-brane and a negative thermal energy gas of colliding particles. We analyze the momentum energy tensor at the ${AdS}_4$ boundary. We find that the negative energy black hole solution is entirely unstable even for a small perturbation in the Poincare coordinate space. However, such a black hole decays very rapidly due to the imaginary part emerges in the ADM mass. This imaginary part appears because of the orbifold constraints of the C-metric solution in the unusual coordinates. Moreover, this decay rate diverges at the UV-brane. This implies that the black hole evaporates instantaneously otherwise the boundary itself will collapse. | |
| dc.description | 12 pages+ 2 figs | |
| dc.identifier | https://arxiv.org/abs/hep-th/0210063 | |
| dc.identifier | http://arxiv.org/abs/hep-th/0210063 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/51554 | |
| dc.subject | High Energy Physics - Theory | |
| dc.title | The C-metric black hole near the IR-brane in the AdS_4 space | |
| dc.type | text |