On Charged Black Holes in Anti-de Sitter Space

Abstract

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.

arXiv comment1+37 pages, 20 ps and eps figures, LaTeX. References added and changes made to section 5

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Cited by in corpus (23)

• Excursions beyond the horizon: Black hole singularities in Yang-Mills theories (I)
• Charged spherically symmetric black holes in $f(R)$ gravity and their stability analysis
• States and Boundary Terms: Subtleties of Lorentzian AdS/CFT
• Rotating AdS black holes in Maxwell-$f(T)$ gravity
• Gravitational duals to the grand canonical ensemble abhor Cauchy horizons
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• Butterflies with rotation and charge
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• Holographic Probes of Inner Horizons
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• Tomograms of Spinning Black Holes
• Quantum Field Theory, Black Holes and Holography
• Maxwell-$f(Q)$ theory
• Holographic flows with scalar self-interaction toward the Kasner universe
• Geodesic motion in the five-dimensional Myers-Perry-AdS spacetime
• On the gauge invariance and coordinate transformations of non-Abelian D-brane actions
• A Note on Particles and Scalar Fields in Higher Dimensional Nutty Spacetimes
• Quasinormal Modes and the Switchback Effect in Schwarzschild-de Sitter
• Bulk Cluster Decomposition in AdS/CFT and A No-Go Theorem for Correlators in Microstates of Extremal Black Holes
• Thermal radiation in curved spacetime using influence functional formalism