Rotating normal and phantom Einstein-Maxwell-dilaton black holes: Geodesic analysis
Tarih
2019Yazar
Azreg-Ninou, Mustapha
Haroon, Sumarna
Jamil, Mubasher
Rizwan, Muhammed
Üst veri
Tüm öğe kaydını gösterÖzet
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.