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paper

Rotating normal and phantom Einstein--Maxwell--dilaton black holes: Geodesic analysis

arXiv:1807.01600 · doi:10.1142/S0218271819500639

Abstract

Depending on five parameters, rotating counterparts of Einstein--Maxwell--dilaton black holes are derived. We discuss their physical and geometric properties and investigate their null and time-like geodesics including circular orbits. The Lense--Thirring effect is considered.

29 pages, 13 figures