Abstract:
As statistical systems, galaxies exhibit a rich interplay between organized structure and stochastic fluctuations
across a broad range of spatial scales. This duality motivates the need for quantitative frameworks capable of
capturing their morphological complexity. The ordinal patterns framework, along with its associated statistical
measures: permutation entropy (H), disequilibrium (DE), statistical complexity (C), and ordinal network node
entropy, has recently emerged as a powerful tool for analyzing such complexity in physical systems. We apply
this framework in a multiwavelength, multiscale analysis of the galaxy NGC 628, utilizing observations in the
near-ultraviolet, near-infrared, mid-infrared, and millimeter bands. Our results reveal a characteristic spatial scale of approximately 200 pc, marking the transition from small-scale structures influenced by star formation and stellar feedback to larger-scale morphology governed by the galaxy’s dynamics. Furthermore, we find that the C versus H trajectories for all wavelengths converge toward a common attractor curve, consistent with the behavior of isotropic Gaussian random fields. This convergence suggests a universal statistical behavior in galactic structure at large scales, despite the differing physical processes traced by each wavelength.
