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
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- Thin accretion disks and charged rotating dilaton black holes
- Spinning black holes with a separable Hamilton-Jacobi equation from a modified Newman-Janis algorithm
- Shadows of rotating Einstein-Maxwell-dilaton black holes surrounded by a plasma
- Thermodynamic topology of topological charged dilatonic black holes
- Equivalence between two charged black holes in dynamics of orbits outside the event horizons
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