Global aspects of accelerating and rotating black hole space-times

Details Global aspects of accelerating and rotating black hole space-times Global aspects of accelerating and rotating black hole space-times

2005-11-22

arxiv.org/abs/gr-qc/0511122v1

Class.Quant.Grav. 23 (2006) 555-568

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

15 pages, 1 figure. To appear in Class. Quantum Grav

Scientific paper

10.1088/0264-9381/23/2/019

The complete family of exact solutions representing accelerating and rotating black holes with possible electromagnetic charges and a NUT parameter is known in terms of a modified Plebanski-Demianski metric. This demonstrates the singularity and horizon structure of the sources but not that the complete space-time describes two causally separated black holes. To demonstrate this property, the metric is first cast in the Weyl-Lewis-Papapetrou form. After extending this up to the acceleration horizon, it is then transformed to the boost-rotation-symmetric form in which the global properties of the solution are manifest. The physical interpretation of these solutions is thus clarified.

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