Quantum Effects in Black Holes from the Schwarzschild Black String?
arXiv:0704.3728 · doi:10.1088/0264-9381/24/22/003
Abstract
The 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.
15 pages, 2 figures, expanded version, including a discussion on the GL instability; to appear in Class. Quant. Grav
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