Geodesic Motion in a Charged 2D Stringy Blackhole Spacetime
arXiv:1406.3918 · doi:10.1142/S0217732314501570
Abstract
We study the timelike geodesics and geodesic deviation for a two-dimensional stringy blackhole spacetime in Schwarzschild gauge. We have analyzed the properties of effective potential along with the structure of the possible orbits for test particles with different settings of blackhole parameters. The exactly solvable geodesic deviation equation is used to obtain corresponding deviation vector. The nature of deviation and tidal force is also examined in view of the behavior of corresponding deviation vector.The results are also compared with an another two-dimensional stringy blackhole spacetime.
17 pages, 6 figures
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- Stability Analysis of Geodesics and Quasinormal Modes of a Dual Stringy Black Hole Via Lyapunov Exponents
- Geodesic motion in R- charged black hole space-times
- Geodesic flows around charged black holes in two dimensions
- Causal structure and the geodesics in the hairy extension of the Bertotti-Robinson spacetime
- Born-Infeld AdS Black Holes Surrounded by Perfect Fluid Dark Matter