Paper 66: Boundary-Seeded Strain-Coherence Vortices, Inward Drift, and Delayed Galaxy Assembly in Holosphere Theory

This paper studies a new idea for how galaxies might begin in Holosphere Theory. Instead of starting with a large clump of matter that collapses, the model tests whether a rotating strain–coherence vortex can form first, remain stable, move inward through a vacancy-gradient environment, and reorganize nearby matter into a later visible structure. The goal is not to present a complete cosmology, but to test whether this transport mechanism is dynamically possible. To do this, the paper uses a reduced physics-based solver with four main ingredients: a prescribed inward-increasing vacancy background, a seeded strain–coherence vortex, explicit transport laws for coherence amplitude and phase structure, and a responding matter field. The solver was developed in stages, beginning with planar prototypes and ending with a three-dimensional FCC/cuboctahedral implementation that is closer to Holosphere packing geometry. The final FCC runs include explicit mass conservation so that any shell formation must come from matter redistribution rather than numerical mass growth. The results show that the seeded vortex can remain identifiable, drift inward, and reorganize matter into a bulge-plus-shell pattern. These results do not yet establish a full theory of galaxy formation, and the model still omits gravity, radiative cooling, and other astrophysical processes. However, they do show that a boundary-launched or migration-onset strain–coherence vortex can act as a plausible pre-galactic organizing scaffold in a reduced real-physics setting.