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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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35 papers · 1 filter

gr-qc2026

How accurate is Spectral Einstein Code (SpEC)? And what limits its accuracy?

Himanshu Chaudhary, Mark A. Scheel, Robert Owen +4

The improved sensitivity of upcoming gravitational-wave detectors will require correspondingly more accurate binary black hole (BBH) simulations. Given the high cost of such simula…

gr-qc2026

A catalog of long, eccentric and precessing binary black hole simulations from ICTS-TIFR

Vaishak Prasad, Prayush Kumar, Michael Boyle +3

We present a catalogue of 31 binary black hole simulations performed with the Spectral Einstein Code (SpEC) on the Sonic cluster at ICTS-TIFR, Bengaluru between August 2023 and Dec…

gr-qc2026

Quadratic Gravitational-Wave Scattering by Kerr Black Holes

Lennox S. Keeble, Hengrui Zhu, Lawrence E. Kidder +2

Second-order black-hole perturbation theory will be an important component of precision gravitational-wave modeling and tests of strong-field gravity with next-generation detectors…

gr-qc2026

Enabling gravitational-wave astronomy with spin-precessing black holes on generic orbits

Aldo Gamboa, Lorenzo Pompili, Alessandra Buonanno +7

Binary black holes (BBHs) formed in dense stellar environments or in hierarchical triples can coalesce on eccentric orbits and carry spins of arbitrary orientation, leaving distinc…

gr-qc2026

High-accuracy drivers to simulate black hole binaries beyond general relativity with the fixing-the-equations approach

Guillermo Lara, Harald P. Pfeiffer, Nils Deppe +9

We implement the "fixing-the-equations" approach [Phys.Rev.D 96 (2017) 8, 084043] in spectre, an NR code using a pseudo-spectral discontinuous Galerkin scheme, to produce long and…

gr-qc2026

Towards long and accurate numerical relativity waveforms of binary black holes beyond general relativity

Guillermo Lara, Harald P. Pfeiffer, Nils Deppe +9

Numerical relativity (NR) simulations of compact binaries in theories beyond general relativity (GR) will be pivotal for the continued development of future tests of gravity with g…

gr-qc2026

Accurate waveforms for generic planar-orbit binary black holes: The multipolar effective-one-body model SEOBNRv6EHM

Aldo Gamboa, Alessandra Buonanno, Lorenzo Pompili +8

Accurate and computationally efficient waveform models are required to infer the parameters of compact binaries from their gravitational wave (GW) emission. Among these parameters,…

gr-qc2026

Merger remnant and eccentricity dynamics surrogates for eccentric nonspinning black hole binaries

Adhrit Ravichandran, Peter James Nee, Keefe Mitman +22

Accurate models of merger remnants are increasingly important for gravitational-wave science, including precision tests of gravity with ringdown, inference of black-hole population…

gr-qc2026

Including higher-order modes in a quadrupolar eccentric numerical relativity surrogate using universal eccentric modulation functions

Tousif Islam, Adhrit Ravichandran, Peter James Nee +15

\texttt{gwNRHME} is a framework that converts multi-modal (i.e., containing several spherical harmonic modes) quasi-circular waveforms into their eccentric counterparts, provided t…

gr-qc2025★ 3 cited

Black-hole scattering with numerical relativity: Self-force extraction and post-Minkowskian validation

Oliver Long, Harald P. Pfeiffer, Lawrence E. Kidder +1

The asymptotic nature of unbound binary-black-hole encounters provides a clean method for comparing different approaches for modeling the two-body problem in general relativity. In…

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★ 1 cited

Chase Orbits, not Time: A Scalable Paradigm for Long-Duration Eccentric Gravitational-Wave Surrogates

Akash Maurya, Prayush Kumar, Scott E. Field +6

Orbital eccentricity is a key tracer of the astrophysical origins of compact binaries. Yet it remains absent from routine LIGO-Virgo-KAGRA analyses, in part because of the prohibit…

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★ 1 cited

Parameter control for binary black hole initial data

Iago B. Mendes, Nils L. Vu, Oliver Long +2

When numerically solving Einstein's equations for binary black holes (BBH), we must find initial data on a three-dimensional spatial slice by solving constraint equations. The cons…

gr-qc2025★ 5 cited

Emergent Turbulence in Nonlinear Gravity

Sizheng Ma, Luis Lehner, Huan Yang +3

Gravity in nonlinear and dynamical regimes underpins spectacular astrophysical phenomena and observable consequences, from the early universe to black hole collisions. In these 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★ 8 cited

Highly accurate simulations of asymmetric black-hole scattering and cross validation of effective-one-body models

Oliver Long, Harald P. Pfeiffer, Alessandra Buonanno +6

The study of unbound binary-black-hole encounters provides a gauge-invariant approach to exploring strong-field gravitational interactions in two-body systems, which can subsequent…

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

Signatures from metastable oppositely-charged black hole binaries in scalar Gauss-Bonnet gravity

Guillermo Lara, Maxence Corman, Peter James Nee +14

We conduct numerical simulations of inspiraling, oppositely-charged black holes in the class of scalar-Gauss-Bonnet theories that exhibit spontaneous black hole scalarization. For…

gr-qc2025★ 8 cited

Ringdown spectroscopy of phenomenologically modified black holes

Spyros Thomopoulos, Sebastian H. Völkel, Harald P. Pfeiffer

The characteristic oscillations of black holes, as described by their quasinormal mode (QNM) spectrum, play a fundamental role in testing general relativity with gravitational wave…

gr-qc2025★ 97 cited

The Science of the Einstein Telescope

Adrian Abac, Raul Abramo, Simone Albanesi +485

Einstein Telescope (ET) is the European project for a gravitational-wave (GW) observatory of third-generation. In this paper we present a comprehensive discussion of its science ob…

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…