Research Paper#Black Hole Physics, Chaos Theory, General Relativity🔬 ResearchAnalyzed: Jan 3, 2026 19:32
Physical Constraints on Black Hole Chaos
Published:Dec 28, 2025 08:27
•1 min read
•ArXiv
Analysis
This paper addresses inconsistencies in the study of chaotic motion near black holes, specifically concerning violations of the Maldacena-Shenker-Stanford (MSS) chaos-bound. It highlights the importance of correctly accounting for the angular momentum of test particles, which is often treated incorrectly. The authors develop a constrained framework to address this, finding that previously reported violations disappear under a consistent treatment. They then identify genuine violations in geometries with higher-order curvature terms, providing a method to distinguish between apparent and physical chaos-bound violations.
Key Takeaways
- •Correctly accounting for angular momentum is crucial for accurately assessing chaos near black holes.
- •Apparent violations of the MSS chaos-bound can arise from incorrect treatment of orbital parameters.
- •Genuine violations can occur in geometries with higher-order curvature terms.
- •The paper provides a framework for distinguishing between apparent and physical chaos-bound violations.
Reference
“The paper finds that previously reported chaos-bound violations disappear under a consistent treatment of angular momentum.”