collaborators

6 papers

gr-qc2026

A comprehensive look into the accuracy of SpEC binary black hole waveforms

Taylor Knapp, Katerina Chatziioannou, Keefe Mitman +4

Numerical relativity simulations provide a full description of the dynamics of binary systems, including gravitational radiation. The waveforms produced by these simulations have a…

gr-qc2026

Revisiting the Coprecessing Frame in the Presence of Orbital Eccentricity

Lucy M. Thomas, Katerina Chatziioannou, Sam Johar +2

Accurate inclusion of both spin precession and orbital eccentricity effects in gravitational waveform models represents a key hurdle in our ability to fully characterize the proper…

gr-qc2026

No hair but plenty of feathers: are birds black holes?

Andrew Laeuger, Taylor Knapp

The imitative verb "chirp" is thought to originate from 16th-century Middle English. Meanwhile, this same word has been used to describe the gravitational waves (GWs) emitted from…

gr-qc2025

Model-agnostic gravitational-wave background characterization algorithm

Taylor Knapp, Patrick M. Meyers, Arianna I. Renzini

As ground-based gravitational-wave (GW) detectors improve in sensitivity, gravitational-wave background (GWB) signals will progressively become detectable. Currently, searches for…

gr-qc2025

The SXS Collaboration's third catalog of binary black hole simulations

Mark A. Scheel, Michael Boyle, Keefe Mitman +56

We present a major update to the Simulating eXtreme Spacetimes (SXS) Collaboration's catalog of binary black hole simulations. Using highly efficient spectral methods implemented i…

gr-qc2025

Parameter control for eccentric, precessing binary black hole simulations with SpEC

Taylor Knapp, Katerina Chatziioannou, Harald Pfeiffer +2

Numerical relativity simulations of merging black holes provide the most accurate description of the binary dynamics and the emitted gravitational wave signal. However, practical c…