Geodesics and Geodesic Deviation in static Charged Black Holes

Abstract

The radial motion along null geodesics in static charged black hole space-times, in particular, the Reissner-Nordström and stringy charged black holes are studied. We analyzed the properties of the effective potential. The circular photon orbits in these space-times are investigated. We found that the radius of circular photon orbits in both charged black holes are different and differ from that given in Schwarzschild space-time. We studied the physical effects of the gravitational field between two test particles in stringy charged black hole and compared the results with that given in Schwarzschild and Reissner-Nordström black holes.

12 pages, 5 figures, small changes, figures and references added, conclusions changed. A improved, version accepted in Astrophysics and Space Science

References in corpus (3)

• Energy Distribution of a Stringy Charged Black Hole
• Geodesics and geodesic deviation in a two-dimensional black hole
• On the Singularities of Reissner-Nordström Space-Time

Cited by in corpus (10)

• Motion of charged test particles in Reissner--Nordström spacetime
• Geodesic Motion in Schwarzschild Spacetime Surrounded by Quintessence
• Tidal effects in Schwarzschild black hole in holographic massive gravity
• Some Astrophysical Aspects of a Schwarzschild Geometry Equipped with a Minimal Measurable Length
• Geodesic Motion in a Charged 2D Stringy Blackhole Spacetime
• Motion of charged particles around a magnetic black hole/topological star with a compact extra dimension
• Geodesic motion in R- charged black hole space-times
• The warped product approach to magnetically charged GMGHS spacetime
• The geodesic motion near hypersurfaces in the warped products spacetime
• Different Regular Black Holes: Geodesic Structures of Test Particles