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This research applies a hybrid CNN-Transformer architecture to estimate parameters for binary black hole systems using gravitational wave data. By shifting from traditional template matching to deep learning point estimation, the study demonstrates robust performance on both simulated signals and real astrophysical events without generating full posterior distributions. The work highlights how advanced neural network architectures are being integrated into high-energy physics instrumentation to accelerate fundamental cosmological analysis.
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Binary Black Hole Parameter Estimation with Hybrid CNN-Transformer Neural Networks

arXiv2 min read

arXiv:2606.13941v1 Announce Type: cross Abstract: The detection of gravitational waves has revolutionized our ability to explore fundamental aspects of the Universe. Traditionally, modeled gravitational-wave signals have been identified using template-based matched filtering, followed by coincidence analysis across multiple detectors in the signal-to-noise ratio time series. Recent advances in Machine Learning and Deep Learning have sparked growing interest in their application to both signal detection and parameter estimation. In this study, a hybrid Deep Learning strategy is proposed that leverages the effectiveness of Transformer encoders alongside well-established Convolutional Neural Network architectures in an attempt to estimate the intrinsic and extrinsic parameters of non-precessing binary black hole systems. The primary focus of this work is point estimation, producing single best-fit values for each parameter rather than full posterior distributions. This method is evaluated on both simulated signals embedded in Gaussian noise and real gravitational-wave events, and it demonstrates strong predictive performance and robustness across key astrophysical parameters.

Abstract:The detection of gravitational waves has revolutionized our ability to explore fundamental aspects of the Universe. Traditionally, modeled gravitational-wave signals have been identified using template-based matched filtering, followed by coincidence analysis across multiple detectors in the signal-to-noise ratio time series. Recent advances in Machine Learning and Deep Learning have sparked growing interest in their application to both signal detection and parameter estimation. In this study, a hybrid Deep Learning strategy is proposed that leverages the effectiveness of Transformer encoders alongside well-established Convolutional Neural Network architectures in an attempt to estimate the intrinsic and extrinsic parameters of non-precessing binary black hole systems. The primary focus of this work is point estimation, producing single best-fit values for each parameter rather than full posterior distributions. This method is evaluated on both simulated signals embedded in Gaussian noise and real gravitational-wave events, and it demonstrates strong predictive performance and robustness across key astrophysical parameters.

Accepted manuscript. 12 pages, 10 figures

General Relativity and Quantum Cosmology (gr-qc); Instrumentation and Methods for Astrophysics (astro-ph.IM); Machine Learning (cs.LG)

arXiv:2606.13941 [gr-qc]

(or arXiv:2606.13941v1 [gr-qc] for this version)

https://doi.org/10.48550/arXiv.2606.13941 Focus to learn more arXiv-issued DOI via DataCite (pending registration)

Astronomy and Computing, vol. 54, 101027 (2026)

https://doi.org/10.1016/j.ascom.2025.101027 Focus to learn more DOI(s) linking to related resources

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Full text under the publisher's open licence · 279 words

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