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20142026
most citedComplete waveform model for compact binaries on eccentric orbits

133 citations · 525 across the 38 of their papers we have counts for

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Showing 2024Show all

8 papers · 1 filter

gr-qc2024★ 14 cited

Late-time tails in nonlinear evolutions of merging black holes

Marina De Amicis, Hannes Rüter, Gregorio Carullo +17

We uncover late-time gravitational-wave tails in fully nonlinear 3+1 dimensional numerical relativity simulations of merging black holes, using the highly accurate SpEC code. We ac…

gr-qc2024★ 57 cited

Accurate waveforms for eccentric, aligned-spin binary black holes: The multipolar effective-one-body model SEOBNRv5EHM

Aldo Gamboa, Alessandra Buonanno, Raffi Enficiaud +9

The measurement of orbital eccentricity in gravitational-wave (GW) signals will provide unique insights into the astrophysical origin of binary systems, while ignoring eccentricity…

gr-qc2024★ 34 cited

Overtones and Nonlinearities in Binary Black Hole Ringdowns

Matthew Giesler, Sizheng Ma, Keefe Mitman +11

Using high-accuracy numerical relativity waveforms, we confirm the presence of numerous overtones of the , quasinormal mode early in the ringdown of binary black hole…

gr-qc2024★ 3 cited

Relieving scale disparity in binary black hole simulations

Nikolas A. Wittek, Leor Barack, Harald P. Pfeiffer +7

Worldtube excision is a method of reducing computational burden in Numerical Relativity simulations of binary black holes in situations where there is a good analytical model of th…

gr-qc2024★ 12 cited

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…

gr-qc2024★ 10 cited

Simulating binary black hole mergers using discontinuous Galerkin methods

Geoffrey Lovelace, Kyle C. Nelli, Nils Deppe +28

Binary black holes are the most abundant source of gravitational-wave observations. Gravitational-wave observatories in the next decade will require tremendous increases in the acc…

gr-qc2024★ 6 cited

Quasistationary hair for binary black hole initial data in scalar Gauss-Bonnet gravity

Peter James Nee, Guillermo Lara, Harald P. Pfeiffer +1

Recent efforts to numerically simulate compact objects in alternative theories of gravity have largely focused on the time-evolution equations. Another critical aspect is the const…

gr-qc2024★ 7 cited

Worldtube excision method for intermediate-mass-ratio inspirals: self-consistent evolution in a scalar-charge model

Nikolas A. Wittek, Adam Pound, Harald P. Pfeiffer +1

This is a third installment in a program to develop a method for alleviating the scale disparity in binary black hole simulations with mass ratios in the intermediate astrophysical…