The Laser Interferometer Space Antenna (LISA) has the potential to reveal wonders about the
fundamental theory of nature at play in the extreme gravity regime, where the gravitational …

Accurate models of gravitational waves from merging black holes are necessary for detectors
to observe as many events as possible while extracting the maximum science. Near the …

Testing general relativity in the nonlinear, dynamical, strong-field regime of gravity is one of
the major goals of gravitational wave astrophysics. Performing precision tests of general …

We produce the first numerical relativity binary black hole gravitational waveforms in a
higher-curvature theory beyond general relativity. In particular, we study head-on collisions of …

A present challenge in testing general relativity (GR) with binary black hole gravitational
wave detections is the inability to perform model-dependent tests due to the lack of merger …

We produce the first astrophysically relevant numerical binary black hole gravitational waveform
in a higher-curvature theory of gravity beyond general relativity. We simulate a system …

The final stage of a binary black hole merger is ringdown, in which the system is described
by a Kerr black hole with quasinormal mode perturbations. It is far from straightforward to …

We apply common gravitational wave inference procedures on binary black hole merger
waveforms beyond general relativity. We consider dynamical Chern-Simons gravity, a modified …

We perform a new test of general relativity (GR) with signals from GWTC-2, the LIGO and
Virgo catalog of gravitational wave detections. We search for the presence of amplitude …

We study $$ \mathcal{N} = 2 $$ supersymmetric four-dimensional gauge theories, in a certain
525-02 = 2 supergravity background, called theΩ-background. The partition function of the …