Entropy-based classification of core-collapse supernova gravitational waves for nuclear equation-of-state inference

Abstract Gravitational waves from core-collapse supernovae provide a unique probe of the physical processes occurring during stellar collapse and of the properties of dense nuclear matter. In this work we investigate the classification of supernova gravitational-wave signals associated with different nuclear equations of state using an entropy-based machine learning framework. The analysis combines signal decomposition, feature extraction, and feature selection techniques to identify informative characteristics of the waveforms and distinguish between different equation of state models. We evaluate the performance of several machine learning classifiers using a compact set of selected features and assess their robustness in the presence of detector noise. We find that entropy-based representations capture the underlying differences between waveform classes and enable accurate classification while maintaining better performance compared to raw data under noisy conditions. These results demonstrate the potential of complexity-based feature extraction as an efficient and interpretable approach for gravitational wave studies of core-collapse supernovae.

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Publication Details

Journal
Classical and Quantum Gravity
Published
2026-10-30
DOI
https://doi.org/10.1088/1361-6382/aebc03
Primary Topic
Pulsars and Gravitational Waves Research
Type
article
Field-Weighted Citation Impact
0.00

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article

Entropy-based classification of core-collapse supernova gravitational waves for nuclear equation-of-state inference

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Classical and Quantum Gravity
Pulsars and Gravitational Waves Research
article

Entropy-based classification of core-collapse supernova gravitational waves for nuclear equation-of-state inference

Y. Sultan Abylkairov, M. C. Edwards, Ernazar B. Abdikamalov, Almat Akhmetali, Marat Zaidyn, Alisher Zhunuskanov, A. Sakan, José Antonio Font, Nurzhan Ussipov
article en

Abstract

Abstract Gravitational waves from core-collapse supernovae provide a unique probe of the physical processes occurring during stellar collapse and of the properties of dense nuclear matter. In this work we investigate the classification of supernova gravitational-wave signals associated with different nuclear equations of state using an entropy-based machine learning framework. The analysis combines signal decomposition, feature extraction, and feature selection techniques to identify informative characteristics of the waveforms and distinguish between different equation of state models. We evaluate the performance of several machine learning classifiers using a compact set of selected features and assess their robustness in the presence of detector noise. We find that entropy-based representations capture the underlying differences between waveform classes and enable accurate classification while maintaining better performance compared to raw data under noisy conditions. These results demonstrate the potential of complexity-based feature extraction as an efficient and interpretable approach for gravitational wave studies of core-collapse supernovae.

Classical and Quantum Gravity
University of Auckland (NZ), Universitat de València (ES), Al-Farabi Kazakh National University (KZ), Astana IT University (KZ), Nazarbayev University (KZ)
Generalitat Valenciana, Nazarbayev University, Agencia Estatal de Investigación
Openalex Percentile: Top 14%
Pulsars and Gravitational Waves Research
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