Applies KCC theory for Jacobi stability analysis of geodesics in dynamical Chern-Simons rotating black holes and compares advantages versus Lyapunov stability.
https://arxiv.org/abs/2403.13062
2 Pith papers cite this work. Polarity classification is still indexing.
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UNVERDICTED 2representative citing papers
Shadows of superspinars in rKdS spacetimes differ from standard KdSNS only for large cosmological constants and remain unobservable for real values.
citing papers explorer
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Stability analysis of geodesics in dynamical Chern-Simons black holes: a geometrical perspective
Applies KCC theory for Jacobi stability analysis of geodesics in dynamical Chern-Simons rotating black holes and compares advantages versus Lyapunov stability.
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Shadows of naked singularities and superspinars related to the revisited Kerr-de Sitter spacetimes
Shadows of superspinars in rKdS spacetimes differ from standard KdSNS only for large cosmological constants and remain unobservable for real values.