468 citations · 7k across the 69 of their papers we have counts for
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Complete waveform model for compact binaries on eccentric orbits
E. A. Huerta, Prayush Kumar, Bhanu Agarwal +11
We present a time domain waveform model that describes the inspiral-merger-ringdown (IMR) of compact binary systems whose components are non-spinning, and which evolve on orbits wi…
Initial data for black hole-neutron star binaries, with rotating stars
Nick Tacik, Francois Foucart, Harald P. Pfeiffer +4
The coalescence of a neutron star with a black hole is a primary science target of ground-based gravitational wave detectors. Constraining or measuring the neutron star spin direct…
Modeling the source of GW150914 with targeted numerical-relativity simulations
Geoffrey Lovelace, Carlos O. Lousto, James Healy +11
In fall of 2015, the two LIGO detectors measured the gravitational wave signal GW150914, which originated from a pair of merging black holes. In the final 0.2 seconds (about 8 grav…
Simulations of inspiraling and merging double neutron stars using the Spectral Einstein Code
Roland Haas, Christian D. Ott, Bela Szilagyi +11
We present results on the inspiral, merger, and post-merger evolution of a neutron star - neutron star (NSNS) system. Our results are obtained using the hybrid pseudospectral-finit…
Effects of neutron-star dynamic tides on gravitational waveforms within the effective-one-body approach
Tanja Hinderer, Andrea Taracchini, Francois Foucart +11
Extracting the unique information on ultradense nuclear matter from the gravitational waves emitted by merging, neutron-star binaries requires robust theoretical models of the sign…
Accuracy of binary black hole waveform models for aligned-spin binaries
Prayush Kumar, Tony Chu, Heather Fong +6
Coalescing binary black holes are among the primary science targets for second generation ground-based gravitational wave (GW) detectors. Reliable GW models are central to detectio…