Geodesic stability for KS Black hole in Horava-Lifshitz gravity via Lyapunov exponents
M. R. Setare, D. Momeni
TL;DR
This paper investigates the stability of equatorial timelike geodesics around KS black holes in Horava-Lifshitz gravity by calculating Lyapunov exponents, revealing two stable regions in space.
Contribution
It introduces a stability analysis of geodesics in KS black holes using Lyapunov exponents, highlighting regions of stability not previously characterized.
Findings
Two regions of stable geodesics identified
Lyapunov exponents used to measure geodesic stability
Stability regions depend on black hole parameters
Abstract
By computing the Lyapunov exponent, which is the inverse of the instability time scale associated with this geodesic motion we show that there is two region of space which in both of them the equatorial timelike geodesics are stable via Lyapunov measure of stability.
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.