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20142022
most citedThe SXS Collaboration catalog of binary black hole simulations

451 citations · 1.1k across the 13 of their papers we have counts for

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9 papers · 1 filter

gr-qc2022★ 172 cited

Nonlinearities in Black Hole Ringdowns

Keefe Mitman, Macarena Lagos, Leo C. Stein +11

The gravitational wave strain emitted by a perturbed black hole (BH) ringing down is typically modeled analytically using first-order BH perturbation theory. In this Letter we show…

gr-qc2022★ 11 cited

Late-time post-merger modeling of a compact binary: effects of relativity, r-process heating, and treatment of transport effects

Milad Haddadi, Matthew D. Duez, Francois Foucart +8

Detectable electromagnetic counterparts to gravitational waves from compact binary mergers can be produced by outflows from the black hole-accretion disk remnant during the first t…

gr-qc2021★ 12 cited

A high-order shock capturing discontinuous Galerkin-finite-difference hybrid method for GRMHD

Nils Deppe, François Hébert, Lawrence E. Kidder +1

We present a discontinuous Galerkin-finite-difference hybrid scheme that allows high-order shock capturing with the discontinuous Galerkin method for general relativistic magnetohy…

gr-qc2021★ 30 cited

Comparing Remnant Properties from Horizon Data and Asymptotic Data in Numerical Relativity

Dante A. B. Iozzo, Neev Khera, Leo C. Stein +10

We present a new study of remnant black hole properties from 13 binary black hole systems, numerically evolved using the Spectral Einstein Code. The mass, spin, and recoil velocity…

gr-qc2020★ 21 cited

High-accuracy waveforms for black hole-neutron star systems with spinning black holes

Francois Foucart, Alexander Chernoglazov, Michael Boyle +10

The availability of accurate numerical waveforms is an important requirement for the creation and calibration of reliable waveform models for gravitational wave astrophysics. For b…

gr-qc2020★ 20 cited

A comparison of momentum transport models for numerical relativity

Matthew D. Duez, Alexander Knight, Francois Foucart +6

The main problems of nonvacuum numerical relativity, compact binary mergers and stellar collapse, involve hydromagnetic instabilities and turbulent flows, so that kinetic energy at…

gr-qc2019★ 20 cited

Smooth equations of state for high-accuracy simulations of neutron star binaries

Francois Foucart, Matthew D. Duez, Alana Gudinas +4

High-accuracy numerical simulations of merging neutron stars play an important role in testing and calibrating the waveform models used by gravitational wave observatories. Obtaini…

gr-qc2019★ 451 cited

The SXS Collaboration catalog of binary black hole simulations

Michael Boyle, Daniel Hemberger, Dante A. B. Iozzo +37

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 tim…

gr-qc2014★ 108 cited

What does a binary black hole merger look like?

Andy Bohn, William Throwe, François Hébert +4

We present a method of calculating the strong-field gravitational lensing caused by many analytic and numerical spacetimes. We use this procedure to calculate the distortion caused…