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Accelerating black hole in 2+1 dimensions and 3+1 black (st)ring

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arxiv 1101.2616 v2 pith:2AZH2WGZ submitted 2011-01-13 gr-qc astro-ph.COhep-th

classification gr-qcastro-ph.COhep-th
keywords blackacceleratingconstantcosmologicaldimensionsholeringaccelerated
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A C-metric type solution for general relativity with cosmological constant is presented in 2+1 dimensions. It is interpreted as a three-dimensional black hole accelerated by a strut. Positive values of the cosmological constant are admissible too. Some embeddings of this metric in the 3+1 space-time are considered: accelerating BTZ black string and a black ring where the gravitational force is sustained by the acceleration.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Generalized Fefferman-Graham gauge and boundary Weyl structures

    hep-th 2024-11 conditional novelty 6.0 of 10

    In the generalized Fefferman-Graham gauge, three-dimensional AdS gravity produces a boundary Weyl connection, a Weyl-covariant stress tensor and trace anomaly, and requires a new corner counterterm that fixes the Eucl...

  2. Holographic correlation functions from wedge

    hep-th 2024-11 conditional novelty 6.0 of 10

    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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