Much of the success of gravitational-wave astronomy rests on perturbation theory.
Historically, perturbative analysis of gravitational-wave sources has largely focused on post …

We report the observation of gravitational waves from a binary-black-hole coalescence
during the first two weeks of LIGO's and Virgo's third observing run. The signal was recorded …

Spin precession is one of the key physical effects that coul unveil the origin of the compact
binaries detected by ground-and space-based gravitational-wave (GW) detectors, and shed …

We produce gravitational waveforms for nonspinning compact binaries undergoing a
quasicircular inspiral. Our approach is based on a two-timescale expansion of the Einstein …

We present SEOBNRv5HM, a more accurate and faster inspiral-merger-ringdown
gravitational waveform model for quasicircular, spinning, nonprecessing binary black holes …

We present the fastemriwaveforms (FEW) package, a collection of tools to build and analyze
extreme mass ratio inspiral (EMRI) waveforms. Here, we expand on [AJK Chua, Phys. Rev …

Within the framework of self-force theory, we compute the gravitational-wave energy flux
through second order in the mass ratio for compact binaries in quasicircular orbits. Our …

The future space mission LISA will observe a wealth of gravitational-wave sources at
millihertz frequencies. Of these, the extreme-mass-ratio inspirals of compact objects into …

To fully exploit the capabilities of next-generation gravitational wave detectors, we need to
significantly improve the accuracy of our models of gravitational-wave-emitting systems. This …

To enable detection and maximize the physics output of gravitational wave observations
from compact binary systems, the availability of accurate waveform models is crucial. The …