Rotating normal and phantom Einstein-Maxwell-dilaton black holes: Geodesic analysis
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 timelike geodesics including circular orbits. The Lense-Thirring effect is considered.
- Publication:
-
International Journal of Modern Physics D
- Pub Date:
- 2019
- DOI:
- 10.1142/S0218271819500639
- arXiv:
- arXiv:1807.01600
- Bibcode:
- 2019IJMPD..2850063A
- Keywords:
-
- Einstein–Maxwell–dilaton theory;
- rotating solutions;
- geodesic motion;
- Lense–Thirring effect;
- 04.20.‑q;
- 04.20.Jb;
- 04.70.Bw;
- 04.25.‑g;
- Exact solutions;
- Classical black holes;
- General Relativity and Quantum Cosmology;
- High Energy Physics - Theory
- E-Print:
- 29 pages, 13 figures