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Real-time gravitational-wave science with neural posterior estimation

MPS-Authors
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Green,  Stephen
Astrophysical and Cosmological Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society;

/persons/resource/persons238174

Gair,  Jonathan
Astrophysical and Cosmological Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society;

/persons/resource/persons127862

Buonanno,  Alessandra
Astrophysical and Cosmological Relativity, AEI-Golm, MPI for Gravitational Physics, Max Planck Society;

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2106.12594.pdf
(Preprint), 5MB

PhysRevLett.127.241103.pdf
(Publisher version), 709KB

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Citation

Dax, M., Green, S., Gair, J., Macke, J. H., Buonanno, A., & Schölkopf, B. (2021). Real-time gravitational-wave science with neural posterior estimation. Physical Review Letters, 127(24): 241103. doi:10.1103/PhysRevLett.127.241103.


Cite as: https://hdl.handle.net/21.11116/0000-0008-C84A-4
Abstract
We demonstrate unprecedented accuracy for rapid gravitational-wave parameter
estimation with deep learning. Using neural networks as surrogates for Bayesian
posterior distributions, we analyze eight gravitational-wave events from the
first LIGO-Virgo Gravitational-Wave Transient Catalog and find very close
quantitative agreement with standard inference codes, but with inference times
reduced from O(day) to a minute per event. Our networks are trained using
simulated data, including an estimate of the detector-noise characteristics
near the event. This encodes the signal and noise models within millions of
neural-network parameters, and enables inference for any observed data
consistent with the training distribution, accounting for noise nonstationarity
from event to event. Our algorithm -- called "DINGO" -- sets a new standard in
fast-and-accurate inference of physical parameters of detected
gravitational-wave events, which should enable real-time data analysis without
sacrificing accuracy.