Geodesic Motion in a Charged 2D Stringy Blackhole Spacetime
Rashmi Uniyal, Hemwati Nandan, K.D. Purohit

TL;DR
This paper investigates the motion of particles and tidal effects in a two-dimensional stringy blackhole spacetime, providing exact solutions and analyzing orbit structures and deviations.
Contribution
It offers a detailed analysis of geodesic motion and deviation in a specific 2D stringy blackhole, including exact solutions and comparison with another spacetime.
Findings
Characterization of effective potential and possible orbits.
Exact solutions for geodesic deviation equations.
Insights into tidal forces and deviations in the spacetime.
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.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
