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.
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