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Charged Rotating Black Holes in Equilibrium

G. G. Varzugin·A. S. Chistyakov
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Abstract

Axially symmetric, stationary solutions of the Einstein-Maxwell equations with disconnected event horizon are studied by developing a method of explicit integration of the corresponding boundary-value problem. This problem is reduced to non-leaner system of algebraic equations which gives relations between the masses, the angular momenta, the angular velocities, the charges, the distance parameters, the values of the electromagnetic field potential at the horizon and at the symmetry axis. A found solution of this system for the case of two charged non-rotating black holes shows that in general the total mass depends on the distance between black holes. Two-Killing reduction procedure of the Einstein-Maxwell equations is also discussed.

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G. G. Varzugin, A. S. Chistyakov. 2002-01-11. Charged Rotating Black Holes in Equilibrium. https://doi.org/10.1088/0264-9381%2F19%2F17%2F307

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