Quantum Effects in Black Holes from the Schwarzschild Black String?

Simple item page
dc.creatorFabbri, Alessandro
dc.creatorProcopio, Giovanni Paolo
dc.date2007-04-27
dc.date2007-09-05
dc.date.accessioned2026-07-07T11:56:44Z
dc.date.available2026-07-07T11:56:44Z
dc.descriptionThe holographic conjecture for black holes localized on a 3-brane in Randall-Sundrum braneworld models RS2 predicts the existence of a classical 5D time dependent solution dual to a 4D evaporating black hole. After briefly reviewing recent criticism and presenting some difficulties in the holographic interpretation of the Gregory-Laflamme instability, we simulate some basic features of such a solution by studying null geodesics of the Schwarzschild black string, in particular those propagating nontrivially in the bulk, and using holographic arguments.
dc.description15 pages, 2 figures, expanded version, including a discussion on the GL instability; to appear in Class. Quant. Grav
dc.identifierhttps://arxiv.org/abs/0704.3728
dc.identifierhttp://arxiv.org/abs/0704.3728
dc.identifierClass.Quant.Grav.24:5371-5382,2007
dc.identifierdoi:10.1088/0264-9381/24/22/003
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/205639
dc.subjectHigh Energy Physics - Theory
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleQuantum Effects in Black Holes from the Schwarzschild Black String?
dc.typetext

Files

Collections

arXiv