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The study demonstrates a graph neural network's capabilities in classifying plasma crystal symmetries, suggesting new insights into noise-resilient methods.
The formation and classification of crystalline structures in complex plasmas is a interesting topic in plasma physics, particularly under dynamic conditions such as microgravity. While previous work has largely focused on well-ordered cubic structures, the identification of more complex symmetries remains challenging, especially in noisy experimental data. In this study, we present an SE(3)-equivariant graph neural network capable of classifying a broad range of plasma crystal symmetries, including face-centered cubic (fcc), hexagonal close-packed (hcp), body-centered cubic (bcc),face-centered orthorhombic (fco), body-centered orthorhombic (bco), and face-centered tetragonal (fct). Our model combines equivariant message passing with Voronoi-based shape descriptors to capture both local geometric features and global symmetries. It is trained on synthetic datasets and validated against experimental data from PK-4 under laboratory and microgravity conditions. The network significantly outperforms conventional approaches such as WignerNet, particularly on non-cubic structures. Time-resolved analysis reveals how crystal formation depends sensitively on external parameters such as gas pressure and excitation frequency. Under microgravity, crystalline phases appear less frequently, which we attribute to reduced particle compression and altered spatial confinement. Overall, the results highlight the effectiveness of symmetry-aware machine learning models in capturing structural complexity in physical systems. The method enables accurate classification of ordered structures and provides a powerful tool for investigating phase behavior in complex plasmas.
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Dormagen et al. (2025) studied this question.
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