As gravitational-wave detectors become more sensitive and broaden their frequency
bandwidth, we will access a greater variety of signals emitted by compact binary systems …

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 improve the accuracy of the effective-one-body (EOB) waveforms that were employed
during the first observing run of Advanced LIGO for binaries of spinning, nonprecessing …

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

For the first time, we construct an inspiral-merger-ringdown waveform model within the
effective-one-body formalism for spinning, nonprecessing binary black holes that includes …

In Abbott et al.[Phys. Rev. X 6, 041014 (2016) PRXHAE 2160-3308 10.1103/PhysRevX.
6.041014], the properties of the first gravitational wave detected by LIGO, GW150914, were …

We leverage recent breakthrough calculations using second-order gravitational self-force
(2GSF) theory to improve both the gravitational-mode amplitudes and radiation-reaction …

Scientific analysis for the gravitational wave detector LISA will require theoretical waveforms
from extreme-mass-ratio inspirals (EMRIs) that extensively cover all possible orbital and spin …

Orbital eccentricity is a crucial physical effect to unveil the origin of compact-object binaries
detected by ground-and spaced-based gravitational-wave (GW) observatories. Here, we …

We present a frequency-domain reduced-order model (ROM) for the aligned-spin effective-
one-body model for binary black holes (BBHs) seobnrv4hm that includes the spherical …