activity
20102023
most citedThe SXS Collaboration catalog of binary black hole simulations

451 citations · 3.1k across the 46 of their papers we have counts for

collaborators

47 papers

gr-qc2023★ 2 cited

Rapid localization and inference on compact binary coalescences with the Advanced LIGO-Virgo-KAGRA gravitational-wave detector network

Soichiro Morisaki, Rory Smith, Leo Tsukada +4

We present a rapid parameter estimation framework for compact binary coalescence (CBC) signals observed by the LIGO-Virgo-KAGRA (LVK) detector network. The goal of our framework is…

astro-ph.HE2023

The LIGO HET Response (LIGHETR) Project to Discover and Spectroscopically Follow Optical Transients Associated with Neutron Star Mergers

M. J. Bustamante-Rosell, Greg Zeimann, J. Craig Wheeler +20

The LIGO HET Response (LIGHETR) project is an enterprise to follow up optical transients (OT) discovered as gravitational wave merger sources by the LIGO/Virgo collaboration (LVC).…

gr-qc2023★ 2 cited

Rogue echoes from exotic compact objects

Aaron Zimmerman, Richard N. George, Yanbei Chen

Binary systems containing exotic compact objects may emit repeated bursts of gravitational waves (GWs) following coalescence. Such GW echoes would provide a clear signature of new…

gr-qc2023★ 2 cited

In Pursuit of Love: First Templated Search for Compact Objects with Large Tidal Deformabilities in the LIGO-Virgo Data

Horng Sheng Chia, Thomas D. P. Edwards, Digvijay Wadekar +6

We report results on the first matched-filtering search for binaries with compact objects having large tidal deformabilities in the LIGO-Virgo gravitational wave (GW) data. The tid…

astro-ph.GA2023★ 1 cited

Constraining intermediate-mass black holes from the stellar disc of SgrA*

Jean-Baptiste Fouvry, María José Bustamante-Rosell, Aaron Zimmerman

Stars evolving around a supermassive black hole see their orbital orientations diffuse efficiently, a process called "vector resonant relaxation". In particular, stars within the s…

astro-ph.IM2023★ 53 cited

Improved ranking statistics of the GstLAL inspiral search for compact binary coalescences

Leo Tsukada, Prathamesh Joshi, Shomik Adhicary +37

Starting from May 2023, the LIGO Scientific, Virgo and KAGRA Collaboration is planning to conduct the fourth observing run with improved detector sensitivities and an expanded dete…

astro-ph.IM2023★ 1 cited

ripple: Differentiable and Hardware-Accelerated Waveforms for Gravitational Wave Data Analysis

Thomas D. P. Edwards, Kaze W. K. Wong, Kelvin K. H. Lam +4

We propose the use of automatic differentiation through the programming framework jax for accelerating a variety of analysis tasks throughout gravitational wave (GW) science. First…

gr-qc2022★ 1 cited

Dimensionally Reduced Waveforms for Spin-Induced Quadrupole Searches

Horng Sheng Chia, Thomas D. P. Edwards, Richard N. George +5

We present highly accurate, dimensionally-reduced gravitational waveforms for binary inspirals whose components have large spin-induced quadrupole moments. The spin-induced quadrup…

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★ 68 cited

An approach to computing spectral shifts for black holes beyond Kerr

Asad Hussain, Aaron Zimmerman

Recent measurements of gravitational-wave ringdown following the merger of binary black holes raise the prospect of precision black hole spectroscopy in the near future. To perform…

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…

stat.ML2022★ 7 cited

A stochastic Stein Variational Newton method

Alex Leviyev, Joshua Chen, Yifei Wang +2

Stein variational gradient descent (SVGD) is a general-purpose optimization-based sampling algorithm that has recently exploded in popularity, but is limited by two issues: it is k…

gr-qc2022

Matters of Gravity: The Newsletter of the Division of Gravitational Physics of the American Physical Society. Number 55. April 2022

Aaron Zimmerman

Contents: APS April Meeting, by Aaron Zimmerman; Cosmic Explorer, the Next Exploration Step, by Varun Srivastava, Kathryne J. Daniel, and Stefan Ballmer

astro-ph.IM2022★ 19 cited

Efficient Gravitational Wave Template Bank Generation with Differentiable Waveforms

Adam Coogan, Thomas D. P. Edwards, Horng Sheng Chia +6

The most sensitive search pipelines for gravitational waves from compact binary mergers use matched filters to extract signals from the noisy data stream coming from gravitational…

gr-qc2021★ 116 cited

General-relativistic precession in a black-hole binary

Mark Hannam, Charlie Hoy, Jonathan E. Thompson +24

The general-relativistic phenomenon of spin-induced orbital precession has not yet been observed in strong-field gravity. Gravitational-wave observations of binary black holes (BBH…

astro-ph.IM2021

Multi-messenger parameter inference of gravitational-wave and electromagnetic observations of white dwarf binaries

Peyton T. Johnson, Michael W. Coughlin, Ashlie Hamilton +7

The upcoming Laser Interferometer Space Antenna (LISA) will detect a large gravitational-wave foreground of Galactic white dwarf binaries. These sources are exceptional for their p…

gr-qc2021★ 19 cited

Gravitational Wave Timing Array

María José Bustamante-Rosell, Joel Meyers, Noah Pearson +2

We describe the design of a gravitational wave timing array, a novel scheme that can be used to search for low-frequency gravitational waves by monitoring continuous gravitational…

astro-ph.IM2020

Automating the Inclusion of Subthreshold Signal-to-Noise Ratios for Rapid Gravitational-Wave Localization

Cody Messick, Surabhi Sachdev, Kipp Cannon +29

The accurate localization of gravitational-wave (GW) events in low-latency is a crucial element in the search for further multimessenger signals from these cataclysmic events. The…

gr-qc2020★ 30 cited

Source properties of the lowest signal-to-noise-ratio binary black hole detections

Yiwen Huang, Carl-Johan Haster, Salvatore Vitale +6

We perform a detailed parameter estimation study of binary black hole merger events reported in Zackay et al. and Venumadhav et al.. These are some of the faintest signals reported…

gr-qc2020★ 401 cited

Prospects for Fundamental Physics with LISA

Enrico Barausse, Emanuele Berti, Thomas Hertog +318

In this paper, which is of programmatic rather than quantitative nature, we aim to further delineate and sharpen the future potential of the LISA mission in the area of fundamental…

astro-ph.HE2019★ 53 cited

Probing the Nature of Black Holes: Deep in the mHz Gravitational-Wave Sky

Vishal Baibhav, Leor Barack, Emanuele Berti +26

Black holes are unique among astrophysical sources: they are the simplest macroscopic objects in the Universe, and they are extraordinary in terms of their ability to convert energ…

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…

astro-ph.IM2019★ 52 cited

On combining information from multiple gravitational wave sources

Aaron Zimmerman, Carl-Johan Haster, Katerina Chatziioannou

In the coming years, advanced gravitational wave detectors will observe signals from a large number of compact binary coalescences. The majority of these signals will be relatively…

gr-qc2018★ 115 cited

Mitigation of the instrumental noise transient in gravitational-wave data surrounding GW170817

Chris Pankow, Katerina Chatziioannou, Eve A. Chase +9

In the coming years gravitational-wave detectors will undergo a series of improvements, with an increase in their detection rate by about an order of magnitude. Routine detections…