Geometric Approach to Light Rings in Axially Symmetric Spacetimes
Chenkai Qiao, Ming Li, Donghui Xie, Minyong Guo

TL;DR
This paper extends a geometric method for analyzing light rings from spherically symmetric to axially symmetric spacetimes, providing a universal, metric-independent way to determine and classify photon orbits using optical geometry and Finsler geometry.
Contribution
It introduces a geometric approach based on intrinsic curvatures in optical geometry to identify and analyze light rings in axially symmetric spacetimes, generalizing previous spherically symmetric results.
Findings
Light rings are determined by vanishing geodesic curvature.
Stability of light rings is classified via flag curvature.
The geometric approach is equivalent to the conventional effective potential method.
Abstract
Circular photon orbits have become an attractive topic in recent years. They play extremely important roles in black hole shadows, gravitational lensings, quasi-normal modes, and spacetime topological properties. In our recent work, \href{https://doi.org/10.1103/PhysRevD.106.L021501}{Phys. Rev. D \textbf{106}, L021501 (2022)}, a geometric approach to circular photon orbits was proposed for spherically symmetric spacetimes. In the present study, we extend this geometric approach from spherically symmetric spacetimes to axially symmetric spacetimes. In this geometric approach, light rings in the equatorial plane are determined by the intrinsic curvatures in the optical geometry of Lorentz spacetime, which gives rise to a Randers-Finsler geometry in axially symmetric cases. Specifically, light rings can be precisely determined by the vanishing of geodesic curvature, and the stability of…
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Taxonomy
TopicsAdvanced Differential Geometry Research · Cosmology and Gravitation Theories · Geometric Analysis and Curvature Flows
