collaborators

5 papers

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…

gr-qc2019

Surrogate models for precessing binary black hole simulations with unequal masses

Vijay Varma, Scott E. Field, Mark A. Scheel +5

Only numerical relativity simulations can capture the full complexities of binary black hole mergers. These simulations, however, are prohibitively expensive for direct data analys…

gr-qc2019

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-qc2018

Surrogate model of hybridized numerical relativity binary black hole waveforms

Vijay Varma, Scott E. Field, Mark A. Scheel +3

Numerical relativity (NR) simulations provide the most accurate binary black hole gravitational waveforms, but are prohibitively expensive for applications such as parameter estima…