activity
20232026
most citedLaying the foundation of the effective-one-body waveform models SEOBNRv5: improved accuracy and efficiency for spinning non-precessing binary black holes

159 citations · 477 across the 33 of their papers we have counts for

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Showing 2025Show all

11 papers · 1 filter

gr-qc2025

Eccentric binary black holes: A new framework for numerical relativity waveform surrogates

Peter James Nee, Adhrit Ravichandran, Scott E. Field +17

Mounting evidence indicates that some of the gravitational wave signals observed by the LIGO/Virgo/KAGRA observatories might arise from eccentric compact object binaries, increasin…

gr-qc2025★ 1 cited

A comprehensive look into the accuracy of SpEC binary black hole waveforms

Taylor Knapp, Katerina Chatziioannou, Keefe Mitman +4

Numerical relativity simulations provide a full description of the dynamics of binary systems, including gravitational radiation. The waveforms produced by these simulations have a…

gr-qc2025★ 6 cited

Biased parameter inference of eccentric, spin-precessing binary black holes

Divyajyoti, Isobel M. Romero-Shaw, Vaishak Prasad +8

While the majority of gravitational wave (GW) events observed by the LIGO and Virgo detectors are consistent with mergers of binary black holes (BBHs) on quasi-circular orbits, som…

gr-qc2025

Error quantification and comparison of binary neutron star gravitational waveforms from numerical relativity codes

Sarah Habib, Elias R. Most, Nils Deppe +11

Future gravitational wave detections of merging binary neutron star systems have the possibility to tightly constrain the equation of state of dense nuclear matter. In order to ext…

gr-qc2025★ 15 cited

Defining eccentricity for spin-precessing binaries

Md Arif Shaikh, Vijay Varma, Antoni Ramos-Buades +4

Standardizing the definition of eccentricity is necessary for unambiguous inference of the orbital eccentricity of compact binaries from gravitational wave observations. In previou…

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-qc2025★ 1 cited

Modeling the BMS transformation induced by a binary black hole merger

Guido Da Re, Keefe Mitman, Leo C. Stein +12

Understanding the characteristics of the remnant black hole formed in a binary black hole merger is crucial for conducting gravitational wave astronomy. Typically, models of remnan…

gr-qc2025

Probing the ringdown perturbation in binary black hole coalescences with an improved quasi-normal mode extraction algorithm

Keefe Mitman, Isabella Pretto, Harrison Siegel +9

Using gravitational waves to probe the geometry of the ringing remnant black hole formed in a binary black hole coalescence is a well-established way to test Einstein's theory of g…

gr-qc2025★ 18 cited

Impact of eccentricity and mean anomaly in numerical relativity mergers

Peter James Nee, Aldo Gamboa, Harald P. Pfeiffer +8

Accurate modelling of black hole binaries is critical to achieve the science goals of gravitational-wave detectors. Modelling such configurations relies strongly on calibration to…

gr-qc2025★ 8 cited

Robustness of extracting quasinormal mode information from black hole merger simulations

Leda Gao, Gregory B. Cook, Lawrence E. Kidder +8

In linear perturbation theory, the ringdown of a gravitational wave (GW) signal is described by a linear combination of quasinormal modes (QNMs). Detecting QNMs from GW signals is…

gr-qc2025★ 6 cited

Length dependence of waveform mismatch: a caveat on waveform accuracy

Keefe Mitman, Leo C. Stein, Michael Boyle +4

The Simulating eXtreme Spacetimes Collaboration's code SpEC can now routinely simulate binary black hole mergers undergoing orbits, with the longest simulations undergoing…