783 citations · 9.6k across the 95 of their papers we have counts for
98 papers
Fast and Fourier: Extreme Mass Ratio Inspiral Waveforms in the Frequency Domain
Lorenzo Speri, Michael L. Katz, Alvin J. K. Chua +5
Extreme Mass Ratio Inspirals (EMRIs) are one of the key sources for future space-based gravitational wave interferometers. Measurements of EMRI gravitational waves are expected to…
Extreme mass-ratio inspiral of a spinning body into a Kerr black hole I: Evolution along generic trajectories
Lisa V. Drummond, Alexandra G. Hanselman, Devin R. Becker +1
The study of spinning bodies moving in curved spacetime has relevance to binary black hole systems with large mass ratios, as well as being of formal interest. At zeroth order in a…
Asymptotic gravitational-wave fluxes from a spinning test body on generic orbits around a Kerr black hole
Viktor Skoupý, Georgios Lukes-Gerakopoulos, Lisa V. Drummond +1
This work provides gravitational wave energy and angular momentum asymptotic fluxes from a spinning body moving on generic orbits in a Kerr spacetime up to linear in spin approxima…
Bi-orthogonal harmonics for the decomposition of gravitational radiation II: applications for extreme and comparable mass-ratio black hole binaries
L. London, S. A. Hughes
The estimation of a physical system's normal modes is a fundamental problem in physics. The quasi-normal modes of perturbed Kerr black holes, with their related spheroidal harmonic…
Measuring quasi-normal mode amplitudes with misaligned binary black hole ringdowns
Halston Lim, Gaurav Khanna, Scott A. Hughes
In recent work, we examined how different modes in the ringdown phase of a binary coalescence are excited as a function of the final plunge geometry. At least in the large mass rat…
Surrogate model for gravitational wave signals from non-spinning, comparable- to large-mass-ratio black hole binaries built on black hole perturbation theory waveforms calibrated to numerical relativity
Tousif Islam, Scott E. Field, Scott A. Hughes +6
We present a reduced-order surrogate model of gravitational waveforms from non-spinning binary black hole systems with comparable to large mass-ratio configurations. This surrogate…