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Stationary black diholes

In this paper we present and analyze the simplest physically meaningful model for stationary black diholes - a binary configuration of counter-rotating Kerr-Newman black holes endowed with opposite electric charges - elaborated in a physical parametrization on the basis of one of the Ernst-Manko-Ruiz equatorially antisymmetric solutions of the Einstein-Maxwell equations. The model saturates the Gabach-Clement inequality for interacting black holes with struts, and in the absence of rotation it reduces to the Emparan-Teo electric dihole solution. The physical characteristics of each dihole constituent satisfy identically the well-known Smarr's mass formula.

preprint2015arXivOpen access
V. S. MankoR. I. RabadánJ. D. Sanabria-Gómez
gr-qc
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Open access3 authors1 topic
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V. S. MankoR. I. RabadánJ. D. Sanabria-Gómez

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