From the Gravitational Compton Amplitude to Black Hole Perturbation Theory
Abstract
We employ a single worldline effective field theory in a Schwarzschild-Tangherlini background to compute the gravitational Compton amplitude up to third post-Minkowskian order. After excising the infrared divergences associated with the Weinberg phase, we establish a direct and exact map to results in black hole perturbation theory with a natural resummation and regularization of the forward divergences of the Compton amplitude. We also outline possible applications of this useful computational bridge for Compton amplitudes that include spin and tidal effects.
Fields of Study & Subjects
Black Holes and Theoretical Physics
Pulsars and Gravitational Waves Research
Relativity and Gravitational Theory
Publication details
- Journal / source
- Physical Review Letters
- Volume
- 137
- Issue
- 13
- Pages
- 131601–131601
- Publication date
- 31 August 2026
- Language
- EN