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On the spinning C-metric

V. Pravda·A. Pravdova
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Abstract

Physical interpretation of some stationary and non-stationary regions of the spinning C-metric is presented. They represent different spacetime regions of a uniformly accelerated Kerr black hole. Stability of geodesics corresponding to equilibrium points in a general stationary spacetime with an additional symmetry is also studied and results are then applied to the spinning C-metric.

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V. Pravda, A. Pravdova. 2002-01-08. On the spinning C-metric. https://doi.org/10.1142/9789812776938_0008

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