Precise Gravitational Wave Scattering by Black Holes
Analysis
Key Takeaways
- •Develops a rigorous, divergence-free method for calculating GW scattering by black holes.
- •Provides a more accurate framework for modeling GW lensing, especially near the optical axis.
- •Highlights discrepancies between the new method and conventional asymptotic approaches.
- •Offers a foundation for improved GW observation accuracy and understanding of black hole environments.
“The paper reveals the formation of the Poisson spot and pronounced wavefront distortions, and finds significant discrepancies with conventional methods at high frequencies.”