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
References in corpus (4)
- Circular motion of neutral test particles in Reissner-Nordström spacetime
- Geodesics of electrically and magnetically charged test particles in the Reissner-Nordström space-time: analytical solutions
- Analytic solutions of the geodesic equation in higher dimensional static spherically symmetric space-times
- Kinematics of geodesic flows in stringy black hole backgrounds