Flexible mapping of ringdown amplitudes for nonprecessing binary black holes
Costantino Pacilio, Swetha Bhagwat, Francesco Nobili, Davide Gerosa

TL;DR
This paper introduces a highly accurate, flexible surrogate model for ringdown amplitudes and phases of nonprecessing binary black holes, improving gravitational wave analysis and enabling future extensions to more complex systems.
Contribution
A novel data-driven surrogate model for ringdown amplitudes and phases that includes multiple modes and overtones, with significantly reduced errors and adaptable to future complexities.
Findings
Achieves reconstruction errors ~100 times smaller than measurement errors
Includes 16 emission modes with overtones and quadratic contributions
Flexible framework allows future extensions to eccentricity and precession
Abstract
The remnant black hole from a binary coalescence emits ringdown gravitational waves characterized by quasinormal modes, which depend solely on the remnant's mass and spin. In contrast, the ringdown amplitudes and phases are determined by the properties of the merging progenitors. Accurately modeling these amplitudes and phases reduces systematic biases in parameter estimation and enables the development and performance of rigorous tests of general relativity. We present a state-of-the-art, data-driven surrogate model for ringdown amplitudes and phases, leveraging Gaussian process regression trained against SXS numerical-relativity simulations. Focusing on nonprecessing, quasicircular binary black holes, our model offers the most comprehensive fit that includes 16 emission modes, incorporating overtones and quadratic contributions. Our surrogate model achieves reconstruction errors that…
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Taxonomy
TopicsGeophysics and Sensor Technology · Pulsars and Gravitational Waves Research · Astrophysical Phenomena and Observations
