A Unified Dissipative Framework: Linking Cosmological Viscosity to Nuclear Binding Energy via Three-Dimensional Geometric Normalization

We present a universal dissipative framework establishing a quantitative connection between cosmological-scale observations and nuclear binding energies through a single dimensionless viscosity parameter eta. Calibrating the optico-hydrodynamic vacuum (OHV) distance metric on the Pantheon+ Type Ia supernova dataset (N = 1590, z > 0.01) yields a reduced chi-square of 0.901, statistically comparable to the flat Lambda-CDM model (0.884). The optimized parameters imply a characteristic vacuum viscosity coefficient eta = 0.4182 percent.