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• W2076357046 abstract "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." @default.
• W2076357046 created "2016-06-24" @default.
• W2076357046 creator A5065031432 @default.
• W2076357046 date "2005-12-19" @default.
• W2076357046 modified "2023-10-14" @default.
• W2076357046 title "Accelerated black holes in an anti-de Sitter universe" @default.
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• W2076357046 doi "https://doi.org/10.1103/physrevd.72.124019" @default.
• W2076357046 hasPublicationYear "2005" @default.
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