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20182021
most citedEccentric binary black hole surrogate models for the gravitational waveform and remnant properties: comparable mass, nonspinning case

129 citations · 129 across the 1 of their papers we have counts for

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gr-qc2021

High-precision source characterization of intermediate mass-ratio black hole coalescences with gravitational waves: The importance of higher-order multipoles

Tousif Islam, Scott E. Field, Carl-Johan Haster +1

Intermediate mass ratio inspiral (IMRI) binaries -- containing stellar-mass black holes coalescing into intermediate-mass black holes () -- are a highly anticipated…

gr-qc2021

Bayesian inference for gravitational waves from binary neutron star mergers in third-generation observatories

Rory Smith, Ssohrab Borhanian, Bangalore Sathyaprakash +10

Third-generation (3G) gravitational-wave detectors will observe thousands of coalescing neutron star binaries with unprecedented fidelity. Extracting the highest precision science…

gr-qc2021

Learning orbital dynamics of binary black hole systems from gravitational wave measurements

Brendan Keith, Akshay Khadse, Scott E. Field

We introduce a gravitational waveform inversion strategy that discovers mechanical models of binary black hole (BBH) systems. We show that only a single time series of (possibly no…

gr-qc2021129 cited

Eccentric binary black hole surrogate models for the gravitational waveform and remnant properties: comparable mass, nonspinning case

Tousif Islam, Vijay Varma, Jackie Lodman +6

We develop new strategies to build numerical relativity surrogate models for eccentric binary black hole systems, which are expected to play an increasingly important role in curre…

gr-qc2019

Impact of subdominant modes on the interpretation of gravitational-wave signals from heavy binary black hole systems

Feroz H. Shaik, Jacob Lange, Scott E. Field +5

Over the past year, a handful of new gravitational wave models have been developed to include multiple harmonic modes thereby enabling for the first time fully Bayesian inference s…

gr-qc2019

A Surrogate Model for Gravitational Wave Signals from Comparable- to Large- Mass-Ratio Black Hole Binaries

Nur E. M. Rifat, Scott E. Field, Gaurav Khanna +1

Gravitational wave signals from compact astrophysical sources such as those observed by LIGO and Virgo require a high-accuracy, theory-based waveform model for the analysis of the…