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arXiv · 1807.01600

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

Mustapha Azreg-Aïnou·Sumarna Haroon·Mubasher Jamil·Muhammad Rizwan
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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.

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Mustapha Azreg-Aïnou, Sumarna Haroon, Mubasher Jamil, Muhammad Rizwan. 2018-07-03. Rotating normal and phantom Einstein--Maxwell--dilaton black holes: Geodesic analysis. https://doi.org/10.1142/s0218271819500639

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