Radiation from accelerated black holes in an anti-de Sitter universe

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dc.creatorPodolsky, Jiri
dc.creatorOrtaggio, Marcello
dc.creatorKrtous, Pavel
dc.date2003-07-25
dc.date2003-12-02
dc.date.accessioned2026-07-07T03:28:01Z
dc.date.available2026-07-07T03:28:01Z
dc.descriptionWe study gravitational and electromagnetic radiation generated by uniformly accelerated charged black holes in anti-de Sitter spacetime. This is described by the C-metric exact solution of the Einstein-Maxwell equations with a negative cosmological constant Lambda. We explicitly find and interpret the pattern of radiation that characterizes the dependence of the fields on a null direction from which the (timelike) conformal infinity is approached. This directional pattern exhibits specific properties which are more complicated if compared with recent analogous results obtained for asymptotic behavior of fields near a de Sitter-like infinity. In particular, for large acceleration the anti-de Sitter-like infinity is divided by Killing horizons into several distinct domains with a different structure of principal null directions, in which the patterns of radiation differ.
dc.description19 pages, 11 colour figures, submitted to Phys. Rev. D [Low quality figures are included in this version because of arXive size restrictions. The version with the standard quality figures is available at http://utf.mff.cuni.cz/~podolsky/jppubl.htm.]
dc.identifierhttps://arxiv.org/abs/gr-qc/0307108
dc.identifierhttp://arxiv.org/abs/gr-qc/0307108
dc.identifierPhys.Rev. D68 (2003) 124004
dc.identifierdoi:10.1103/PhysRevD.68.124004
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/34661
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectHigh Energy Physics - Theory
dc.titleRadiation from accelerated black holes in an anti-de Sitter universe
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