BOB the (Waveform) Builder: Optimizing Analytical Black-Hole Binary Merger Waveforms
Anuj Kankani, Sean T. McWilliams

TL;DR
The paper introduces BOB, an analytical model for black-hole binary merger waveforms, validated against numerical relativity, offering high accuracy with minimal tuning and broad applicability for gravitational wave analysis.
Contribution
It presents a fully analytical, physically motivated waveform model (BOB) that matches the accuracy of calibrated models and works well across sparse parameter regions.
Findings
BOB accurately models the dominant gravitational wave mode.
BOB's amplitude link to quasinormal modes is verified.
A minimal-parameter BOB matches overtone-fitting models.
Abstract
The Backwards-One-Body (BOB) model provides a fully analytical and physically motivated description of the merger-ringdown gravitational radiation emanating from a black hole binary merger. We perform a comprehensive validation of BOB for the dominant mode of quasi-circular and non-precessing systems, assessing its accuracy against numerical relativity (NR) simulations, state-of-the-art waveform models, and a sum of quasinormal modes. We demonstrate that BOB most accurately describes the gravitational wave news, achieving accuracy comparable to highly-calibrated Effective-One-Body and NR surrogate models. Because BOB is minimally tuned to NR catalogs, it retains a high level of accuracy in regions of the parameter space sparsely covered by current NR catalogs. BOB yields an analytic link between the amplitude of the fundamental quasinormal mode and the peak amplitude of the…
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