Analysis reveals chaos in geodesics of black holes in astrophysical environments, indicating significant effects on gravitational waves.
Key Points
The study identifies chaos in geodesics around rotating black holes, leading to altered orbital dynamics and gravitational wave signals.
Environmental factors modify orbital paths, as shown by resonant island formations that emerge in non-integrable geodesics.
The loss of a Carter-like constant in rotating black holes contributes to non-integrability, affecting the lifespan of orbital resonances.
Findings imply a need for revised gravitational wave modeling to account for new effects from astrophysical environments on extreme-mass-ratio binaries.