Rotating normal and phantom Einstein--Maxwell--dilaton black holes: Geodesic analysis
General Relativity and Quantum Cosmology
2018-12-21 v2 High Energy Physics - Theory
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.
Cite
@article{arxiv.1807.01600,
title = {Rotating normal and phantom Einstein--Maxwell--dilaton black holes: Geodesic analysis},
author = {Mustapha Azreg-Aïnou and Sumarna Haroon and Mubasher Jamil and Muhammad Rizwan},
journal= {arXiv preprint arXiv:1807.01600},
year = {2018}
}
Comments
29 pages, 13 figures