This project archives the finalized empirical validation of a unified cosmological framework that models the universe as a continuous viscous thermodynamic fluid. By synthesizing rotation curve telemetry from both massive spiral galaxies and dwarf galaxy populations, the study identifies a fundamental density-dependent transition in the vacuum medium. The findings demonstrate that emergent gravity coupling remains an invariant constant above a critical density threshold while transitioning to an active kinematic driver in low-density regimes. This research provides a parameter-free resolution to the structural dynamics of the cosmos and defines the physical boundary conditions for the fluid dynamics of spacetime.
Lee Holmes (Thu,) studied this question.