Holography beyond the horizon and cosmic censorship

Details Holography beyond the horizon and cosmic censorship Holography beyond the horizon and cosmic censorship

2003-04-17

arxiv.org/abs/hep-th/0304150v2

Phys.Rev. D68 (2003) 044005

Physics

High Energy Physics

High Energy Physics - Theory

21 pages, 3 figures, v2: minor changes

Scientific paper

10.1103/PhysRevD.68.044005

We investigate the description of the region behind the event horizon in rotating black holes in the AdS/CFT correspondence, using the rotating BTZ black hole as a concrete example. We extend a technique introduced by Kraus, Ooguri and Shenker [hep-th/0212277], based on analytically continuing amplitudes defined in a Euclidean space, to include rotation. In the rotating case, boundary amplitudes again have two different bulk descriptions, involving either integration only over the regions outside the black holes' event horizon, or integration over this region and the region between the event horizon and the Cauchy horizon (inner horizon). We argue that generally, the holographic map will relate the field theory to the region bounded by the Cauchy horizons in spacetime. We also argue that these results suggest that the holographic description of black holes will satisfy strong cosmic censorship.

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