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Accounting for numerical-relativity calibration uncertainty in gravitational-wave modeling and inference

Lorenzo Pompili ^1,*, Alessandra Buonanno ^1,2, and Michael Pürrer ^3,4,1

¹Max Planck Institute for Gravitational Physics (Albert Einstein Institute), Am Mühlenberg 1, Potsdam 14476, Germany
²Department of Physics, University of Maryland, College Park, Maryland 20742, USA
³Department of Physics, East Hall, University of Rhode Island, Kingston, Rhode Island 02881, USA
⁴Center for Computational Research, Tyler Hall, University of Rhode Island, Kingston, Rhode Island 02881, USA

^*Contact author: lorenzo.pompili@aei.mpg.de

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Articles Citing

Accounting for numerical-relativity calibration uncertainty in gravitational-wave modeling and inference

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

When Vacuum Breaks: A Self-Consistency Test for Astrophysical Environments in Extreme Mass Ratio Inspirals

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

Adding equatorial-asymmetric effects for spin-precessing binaries into the seobnrv5phm waveform model

Impact of numerical-relativity waveform calibration on parametrized post-Einsteinian tests

End-to-end autonomous collision avoidance control for unmanned surface vessels based on Transformer-TD3 and DWA

The Science of the Einstein Telescope

Accounting for the known unknowns: A parametric framework to incorporate systematic waveform errors in gravitational-wave parameter estimation

Systematic biases in parameter estimation on LISA binaries: The effect of excluding higher harmonics for non-spinning binaries

Novel stacked hybrid autoencoder for imputing LISA data gaps

GW231123: A Binary Black Hole Merger with Total Mass 190–265 M ⊙

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