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