Snowmass White Paper: Gravitational Waves and Scattering Amplitudes
Alessandra Buonanno, Mohammed Khalil, Donal O'Connell, Radu Roiban, Mikhail P. Solon, Mao Zeng
TL;DR
The Snowmass white paper proposes leveraging scattering amplitudes, the double copy, and EFT to build a precision, systematically improvable framework for gravitational-wave predictions in binary black hole and neutron star systems. It surveys the classical-limit foundations (KMOC, eikonal, amplitude-action relations) and reports progress toward state-of-the-art conservative and radiative dynamics, including spins and tides, with integration into EFT-based and NR benchmarks. It also outlines a rich toolkit—EFT matching, advanced loop integration, and generating-function formalisms—that connects quantum amplitudes to classical observables and waveforms, while highlighting theoretical structures that could sharpen predictions and reveal new insights. Looking ahead, the paper identifies major challenges and directions, such as higher-order calculations, nonlocal radiation effects, multi-body dynamics, and tests of GR or new physics, aiming to transform GW modeling and deepen our understanding of gravity through quantum-field-theoretic methods.
Abstract
We review recent progress and future prospects for harnessing powerful tools from theoretical high-energy physics, such as scattering amplitudes and effective field theory, to develop a precise and systematically improvable framework for calculating gravitational-wave signals from binary systems composed of black holes and/or neutron stars. This effort aims to provide state-of-the-art predictions that will enable high-precision measurements at future gravitational-wave detectors. In turn, applying the tools of quantum field theory in this new arena will uncover theoretical structures that can transform our understanding of basic phenomena and lead to new tools that will further the cycle of innovation. While still in a nascent stage, this research direction has already derived new analytic results in general relativity, and promises to advance the development of highly accurate waveform models for ever more sensitive detectors.
