Les Houches Lectures on Effective Field Theories and Gravitational Radiation
Walter D. Goldberger
TL;DR
The paper presents Les Houches lectures on applying effective field theory to gravitational radiation from compact binaries, framing the problem with multiple separated scales and introducing a tower of EFTs to organize the post-Newtonian expansion. It develops a two-stage NRGR approach, first integrating out the internal structure to a point-particle EFT and then integrating out orbital-scale potential modes to obtain a radiation EFT with multipole degrees of freedom, enabling a controlled calculation of observables such as gravitational-wave power. Key results include explicit matching procedures, velocity-counting rules, and the emergence of the leading quadrupole radiation formula, along with an assessment of finite-size effects and their suppression. The framework provides a scalable and extensible toolkit for LIGO/LISA science and for future connections to numerical relativity and other astrophysical GW sources.
Abstract
These lectures give an overview of the uses of effective field theories in describing gravitational radiation sources for LIGO or LISA. The first lecture reviews some of the standard ideas of effective field theory (decoupling, matching, power counting) mostly in the context of a simple toy model. The second lecture sets up the problem of calculating gravitational wave emission from non-relativistic binary stars by constructing a tower of effective theories that separately describe each scale in the problem: the internal size of each binary constituent, the orbital separation, and the wavelength of radiated gravitons.
