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On Charged Black Holes in Anti-de Sitter Space
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On Charged Black Holes in Anti-de Sitter Space
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We study the region inside the event horizon of charged black holes in five dimensional asymptotically anti-de Sitter space, using as a probe two-sided correlators which are dominated by spacelike geodesics penetrating the horizon. The spacetimes we investigate include the Reissner-Nordstrom black hole and perturbations thereof. The perturbed spacetimes can be found exactly, enabling us to perform a local scan of the region between the inner and outer horizons. Surprisingly, the two-sided correlators we calculate seem to be geometrically protected from the instability of the inner horizon.
Forward citations
Cited by 2 Pith papers
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Complex Geodesics in the Nariai Geometry
Two-point functions in Nariai geometry are sums over complex geodesics whose phases must be retained to eliminate artificial singularities.
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Complex Geodesics in the Nariai Geometry
Obtains the two-point correlator in Nariai geometry as a sum over complex geodesics via heat kernel approximation on sphere products followed by analytic continuation, extending de Sitter results.
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