Using machine learning to parametrize postmerger signals from binary neutron stars
Tim Whittaker, William E. East, Stephen R. Green, Luis Lehner, Huan, Yang

TL;DR
This paper introduces a machine learning approach using a conditional variational autoencoder to model postmerger gravitational wave signals from binary neutron stars, addressing uncertainties and limited data in waveform construction.
Contribution
It demonstrates that a CVAE can accurately generate postmerger waveforms and encode physical parameters like the equation of state within its latent space.
Findings
CVAE accurately reproduces synthetic postmerger waveforms
The model encodes the neutron star equation of state in latent variables
Proof-of-principle shows potential for future waveform modeling
Abstract
There is growing interest in the detection and characterization of gravitational waves from postmerger oscillations of binary neutron stars. These signals contain information about the nature of the remnant and the high-density and out-of-equilibrium physics of the postmerger processes, which would complement any electromagnetic signal. However, the construction of binary neutron star postmerger waveforms is much more complicated than for binary black holes: (i) there are theoretical uncertainties in the neutron-star equation of state and other aspects of the high-density physics, (ii) numerical simulations are expensive and available ones only cover a small fraction of the parameter space with limited numerical accuracy, and (iii) it is unclear how to parametrize the theoretical uncertainties and interpolate across parameter space. In this work, we describe the use of a…
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