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Accelerated black holes in an anti-de Sitter universe
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The C-metric is one of few known exact solutions of Einstein's field equations which describes the gravitational field of moving sources. For a vanishing or positive cosmological constant, the C-metric represents two accelerated black holes in asymptotically flat or de Sitter spacetime. For a negative cosmological constant the structure of the spacetime is more complicated. Depending on the value of the acceleration, it can represent one black hole or a sequence of pairs of accelerated black holes in the spacetime with an anti-de Sitter-like infinity. The global structure of this spacetime is analyzed and compared with an empty anti-de Sitter universe. It is illustrated by 3D conformal-like diagrams.
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Holographic correlation functions from wedge
Correlation functions of heavy operators can be computed from the on-shell action of a wedge excised from AdS3, verified in Poincaré, global, and BTZ backgrounds.
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