Accelerating black holes in anti-de Sitter universe

Abstract

A physical interpretation of the C-metric with a negative cosmological constant $\Lambda$ is suggested. Using a convenient coordinate system it is demonstrated that this class of exact solutions of Einstein's equations describes uniformly accelerating (possibly charged) black holes in anti-de Sitter universe. Main differences from the analogous de Sitter case are emphasised.

8 pages, 2 figures

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• Accelerated sources in de Sitter spacetime and the insufficiency of retarded fields
• Null limits of the C-metric
• The collision and snapping of cosmic strings generating spherical impulsive gravitational waves
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Cited by in corpus (64)

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• Charged accelerating black hole in $f(R)$ gravity
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• Finely Split Phase Transitions of Rotating and Accelerating Black Holes
• Thermodynamics of accelerating AdS${}_4$ black holes from the covariant phase space
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• The bizarre anti-de Sitter spacetime
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• New family of C-metrics in $\mathcal{N}=2$ gauged supergravity
• A new form of the C-metric with cosmological constant
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• A closer glance at black hole pair creation
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• Pair creation of anti-de Sitter black holes on a cosmic string background
• Wormhole $C$ metric
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• Thermodynamic relation of accelerating black holes in anti-de Sitter spacetime
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• Photon rockets in (anti-)de Sitter universe
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• On the gravitational entropy of accelerating black holes
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• Black Hole Solutions and Pair Creation of Black Holes in Three, Four and Higher Dimensional Spacetimes
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• Effects of the acceleration on holographic complexity
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• C-metric in a (nut)shell
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