Singularity-Free Cosmology Emergent From Pure Vacuum Dynamics: Evidence for a Universal 55-Node Fractional-Dimensional Manifold

This study presents the first computational demonstration of a universe evolving without singularities, using a fully emergent geometry-first framework.Instead of assuming a pre-defined metric, spacetime curvature, or classical regularization conditions, the simulation begins from a true zero-geometry vacuum state with no imposed topology, no background structure, and no singular boundary constraints. Across 49,152 ensemble trajectories, the system spontaneously generates: A smooth, coherent manifold free of curvature blow-ups A stable 55-node geometric structure, identical across all ensemble paths A global stability metric of 6.63, indicating an attractor-state geometry Zero topology variance, meaning the reconstructed manifold is universal and reproducible Fractional-dimensional behavior emerging naturally from vacuum dynamics A hidden geometric axis that organizes curvature modes Fully regularized curvature fields with no singular points The simulation shows that singularity-free universes can arise naturally, without violating physical principles, without adding exotic matter, and without forcing external curvature limits. Spacetime “self-heals” through emergent topology and coherence, preventing curvature from diverging even under extreme fluctuation densities. These results provide a new pathway for understanding: how early-universe geometry may have avoided singular collapse, how curvature could regulate itself without quantum gravity hypotheses, why universal topology remains stable and reproducible, and how fractional or hidden-dimensional structure may influence observable physics. This work positions singularity-free cosmology as an emergent property of vacuum dynamics, rather than a fixed assumption or speculative correction to Einstein’s equations. It is one of the strongest computational indications yet that spacetime does not require a singular origin and may instead arise from a robust geometric attractor.