We apply the Chaining Force framework — a speculative theory of complexity-driven organization in which matter is driven toward higher complexity over time via the stochastic wave equation □ϕ + (2GM/r)ϕ = τ·ξ(x,t) — to the problem of stellar dynamics and migration in the universe. We argue that stars are not passively distributed in space but follow trajectories shaped by the competition between gravity and the Chaining Force. Three distinct dynamical regimes emerge naturally from the equation of motion: a gravity-dominated regime for young structures, a balanced regime for intermediate ages, and a complexity-driven regime for old structures. We show that this framework provides a natural interpretation of stellar accumulation in galaxies, the formation of galactic structure, and the role of supermassive black holes as attractors. Galaxy mergers are interpreted as complexity amplification events. The paper is explicitly speculative and all results are presented as open conjectures.
Judicael Brindel (Fri,) studied this question.