activity
20132025
most citedThe SXS Collaboration catalog of binary black hole simulations

451 citations · 3.2k across the 29 of their papers we have counts for

collaborators

29 papers

gr-qc2025★ 53 cited

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-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★ 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

Binary neutron star mergers using a discontinuous Galerkin-finite difference hybrid method

Nils Deppe, Francois Foucart, Marceline S. Bonilla +18

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-qc2023★ 15 cited

Extending black-hole remnant surrogate models to extreme mass ratios

Matteo Boschini, Davide Gerosa, Vijay Varma +19

Numerical-relativity surrogate models for both black-hole merger waveforms and remnants have emerged as important tools in gravitational-wave astronomy. While producing very accura…

gr-qc2022★ 15 cited

Multipole moments on the common horizon in a binary-black-hole simulation

Yitian Chen, Prayush Kumar, Neev Khera +8

We construct the covariantly defined multipole moments on the common horizon of an equal-mass, non-spinning, quasicircular binary-black-hole system. We see a strong correlation bet…

gr-qc2022★ 5 cited

Success of the small mass ratio approximation during the final orbits of binary black hole simulations

Sergi Navarro Albalat, Aaron Zimmerman, Matthew Giesler +1

Recent studies have shown the surprising effectiveness of the small mass-ratio approximation (SMR) in modeling the relativistic two-body problem even at comparable masses. Up to no…

gr-qc2022

Redshift factor and the small mass-ratio limit in binary black hole simulations

Sergi Navarro Albalat, Aaron Zimmerman, Matthew Giesler +1

We present a calculation of the Detweiler redshift factor in binary black hole simulations based on its relation to the surface gravity. The redshift factor has far-reaching applic…

gr-qc2022★ 52 cited

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…

gr-qc2022★ 54 cited

Targeted large mass ratio numerical relativity surrogate waveform model for GW190814

Jooheon Yoo, Vijay Varma, Matthew Giesler +5

Gravitational wave observations of large mass ratio compact binary mergers like GW190814 highlight the need for reliable, high-accuracy waveform templates for such systems. We pres…

gr-qc2021★ 40 cited

Search of the Early O3 LIGO Data for Continuous Gravitational Waves from the Cassiopeia A and Vela Jr. Supernova Remnants

The LIGO Scientific Collaboration, the Virgo Collaboration, R. Abbott +1411

We present directed searches for continuous gravitational waves from the neutron stars in the Cassiopeia A (Cas A) and Vela Jr. supernova remnants. We carry out the searches in the…

gr-qc2021★ 16 cited

Simulating magnetized neutron stars with discontinuous Galerkin methods

Nils Deppe, François Hébert, Lawrence E. Kidder +33

Discontinuous Galerkin methods are popular because they can achieve high order where the solution is smooth, because they can capture shocks while needing only nearest-neighbor com…

gr-qc2021★ 196 cited

GWTC-2.1: Deep Extended Catalog of Compact Binary Coalescences Observed by LIGO and Virgo During the First Half of the Third Observing Run

The LIGO Scientific Collaboration, the Virgo Collaboration, R. Abbott +1429

The second Gravitational-Wave Transient Catalog reported on 39 compact binary coalescences observed by the Advanced LIGO and Advanced Virgo detectors between 1 April 2019 15:00 UTC…

gr-qc2021★ 26 cited

Universal features of gravitational waves emitted by superkick binary black hole systems

Sizheng Ma, Matthew Giesler, Vijay Varma +2

We use numerical relativity to study the merger and ringdown stages of "superkick" binary black hole systems (those with equal mass and anti-parallel spins). We find a universal wa…

gr-qc2021★ 115 cited

Search for anisotropic gravitational-wave backgrounds using data from Advanced LIGO and Advanced Virgo's first three observing runs

The LIGO Scientific Collaboration, the Virgo Collaboration, the KAGRA Collaboration +1589

We report results from searches for anisotropic stochastic gravitational-wave backgrounds using data from the first three observing runs of the Advanced LIGO and Advanced Virgo det…

gr-qc2021★ 8 cited

Extending superposed harmonic initial data to higher spin

Sizheng Ma, Matthew Giesler, Mark Scheel +1

Numerical simulations of binary black holes are accompanied by an initial spurious burst of gravitational radiation (called `junk radiation') caused by a failure of the initial dat…

gr-qc2021★ 445 cited

Upper Limits on the Isotropic Gravitational-Wave Background from Advanced LIGO's and Advanced Virgo's Third Observing Run

The LIGO Scientific Collaboration, the Virgo Collaboration, the KAGRA Collaboration +1587

We report results of a search for an isotropic gravitational-wave background (GWB) using data from Advanced LIGO's and Advanced Virgo's third observing run (O3) combined with upper…

gr-qc2020★ 135 cited

Testing the black-hole area law with GW150914

Maximiliano Isi, Will M. Farr, Matthew Giesler +2

We present observational confirmation of Hawking's black-hole area theorem based on data from GW150914, finding agreement with the prediction with 97% (95%) probability when we mod…

gr-qc2020★ 38 cited

Spin and Eccentricity Evolution in Triple Systems: from the Lidov-Kozai Interaction to the Final Merger of the Inner Binary

Hang Yu, Sizheng Ma, Matthew Giesler +1

We study the spin and eccentricity evolution of black-hole (BH) binaries that are perturbed by tertiary masses and experience the Lidov-Kozai (LK) excitation. We focus on three asp…

gr-qc2019★ 407 cited

Testing the no-hair theorem with GW150914

Maximiliano Isi, Matthew Giesler, Will M. Farr +2

We analyze gravitational-wave data from the first LIGO detection of a binary black-hole merger (GW150914) in search of the ringdown of the remnant black hole. Using observations be…

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-qc2019★ 270 cited

Black hole ringdown: the importance of overtones

Matthew Giesler, Maximiliano Isi, Mark Scheel +1

It is possible to infer the mass and spin of the remnant black hole from binary black hole mergers by comparing the ringdown gravitational wave signal to results from studies of pe…

gr-qc2019★ 105 cited

On the properties of the massive binary black hole merger GW170729

Katerina Chatziioannou, Roberto Cotesta, Sudarshan Ghonge +53

We present a detailed investigation into the properties of GW170729, the gravitational wave with the most massive and distant source confirmed to date. We employ an extensive set o…

gr-qc2018★ 24 cited

Measuring the properties of nearly extremal black holes with gravitational waves

Katerina Chatziioannou, Geoffrey Lovelace, Michael Boyle +7

Characterizing the properties of black holes is one of the most important science objectives for gravitational-wave observations. Astrophysical evidence suggests that black holes t…