A Dynamical-Photometric Phase Space for Spiral Galaxies: Probing the Local Coupling Between Light and Gravity
arXiv:2608.11264 · doi:10.1093/mnras/stag1270
Abstract
The interplay between luminous matter distribution and the local gravitational field within disc galaxies encodes physical information beyond that captured by global scaling relations. We introduce a \emph{dynamical--photometric phase space} defined by the kinematic variable and the photometric variable , placing the local gravitational scale and the logarithmic surface brightness gradient into direct pointwise correspondence at each galactocentric radius . The quantity represents the angular frequency of circular motion and acts as a probe of the local mean mass density, while measures the radial steepness of the stellar light distribution. The baryon-dominated inner disc is characterized by large negative , whereas the dark-matter-dominated outer region approaches . This two-regime behaviour is described by the smooth sigmoid relation , which reduces to the logarithmic coupling in the baryonic zone. We apply this framework to 136 late-type galaxies from the SPARC database, spanning inclinations --, distances --\,Mpc, and five decades in stellar mass. The median coefficient of determination is . Statistical validation includes eight independent tests together with 5-fold cross-validation. The transition parameter identifies the onset of dark-matter dominance, corresponding to a median transition radius \,kpc across the sample.
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