Fast and Accurate Inference on Gravitational Waves from Precessing Compact Binaries
Rory Smith, Scott E. Field, Kent Blackburn, Carl-Johan Haster, Michael, P\"urrer, Vivien Raymond, Patricia Schmidt

TL;DR
This paper introduces the first reduced order models for gravitational-wave signals from precessing compact binaries, significantly speeding up Bayesian inference without bias, thus enhancing gravitational-wave data analysis.
Contribution
The authors develop the first ROMs for precessing binary signals including inspiral, merger, and ringdown, enabling faster Bayesian inference with minimal bias.
Findings
Inference speed increased by up to 300 times.
Computational time reduced from half a year to half a day.
ROM and ROQ are integrated into LALInference for practical use.
Abstract
Inferring astrophysical information from gravitational waves emitted by compact binaries is one of the key science goals of gravitational-wave astronomy. In order to reach the full scientific potential of gravitational-wave experiments we require techniques to mitigate the cost of Bayesian inference, especially as gravitational-wave signal models and analyses become increasingly sophisticated and detailed. Reduced order models (ROMs) of gravitational waveforms can significantly reduce the computational cost of inference by removing redundant computations. In this paper we construct the first reduced order models of gravitational-wave signals that include the effects of spin-precession, inspiral, merger, and ringdown in compact object binaries, and which are valid for component masses describing binary neutron star, binary black hole and mixed binary systems. This work utilizes the…
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