Rotating normal and phantom Einstein--Maxwell--dilaton black holes: Geodesic analysis
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🌀 gr-qc
hep-th
keywords
blackeinstein--maxwell--dilatonholesrotatinganalysiscircularconsideredcounterparts
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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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