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Rotating charged black holes accelerated by an electric field

MPG-Autoren

Bicak,  Jiri
Geometric Analysis and Gravitation, AEI-Golm, MPI for Gravitational Physics, Max Planck Society;

Kofron,  David
Geometric Analysis and Gravitation, AEI-Golm, MPI for Gravitational Physics, Max Planck Society;

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Volltexte (frei zugänglich)

PRD_82_2_024006.pdf
(beliebiger Volltext), 233KB

1006.4072v1.pdf
(Preprint), 156KB

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Zitation

Bicak, J., & Kofron, D. (2010). Rotating charged black holes accelerated by an electric field. Physical Review D., 82(2): 024006. doi:10.1103/PhysRevD.82.024006.


Zitierlink: http://hdl.handle.net/11858/00-001M-0000-0012-CBDD-E
Zusammenfassung
The Ernst method of removing nodal singularities from the charged C-metric representing a uniformly accelerated black hole with mass m, charge q and acceleration A by “adding” an electric field E is generalized. Utilizing the new form of the C-metric found recently, Ernst’s simple “equilibrium condition” mA=qE valid for small accelerations is generalized for arbitrary A. The nodal singularity is removed also in the case of accelerating and rotating charged black holes, and the corresponding equilibrium condition is determined.