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 …

We construct an inspiral-merger-ringdown eccentric gravitational-wave (GW) model for
binary black holes with non-precessing spins within the effective-one-body formalism. This …

Highly accurate models of the gravitational wave signal from coalescing compact binaries
are built by completing analytical computations of the binary dynamics with nonperturbative …

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 new effective-one-body (EOB) model for eccentric binary coalescences. The
model stems from the state-of-the-art model TEOBiResumS_SM for circularized coalescing …

Only a few years after the first detection of gravitational waves from coalescing stellar-mass
black holes, the field of gravitational-wave astronomy is now firmly established after the …

Eccentric compact binary mergers are significant scientific targets for current and future
gravitational wave observatories. To detect and analyze eccentric signals, there is an …

While most binary inspirals are expected to have circularized before they enter the
LIGO/Virgo frequency band, a small fraction of those binaries could have non-negligible …

Black hole (BH) binary mergers formed through dynamical interactions in dense star clusters
are believed to be one of the main sources of gravitational waves (GWs) for Advanced LIGO …

The modeling of unequal mass binary black hole systems is of high importance to detect and
estimate parameters from these systems. Numerical relativity (NR) is well suited to study …