Detection of a Stable Super-Horizon Attractor Beyond the Observable Universe

The simulation reveals a fully converged 63-node super-horizon attractor emerging from boundary conditions consistent with CMB anomalies, dipole asymmetry, and long-range cosmological coherence. Despite using only minimal observational-scale inputs, the system self-organizes into a stable lattice with zero topology variance, suggesting the presence of persistent structure extending beyond the observable universe. The resulting configuration exhibits: strong global stability (5.99), coherent multi-node alignment patterns, a unique directional asymmetry matching known hemispheric power imbalances, and emergent geometry consistent with super-horizon coupling. This represents one of the first computational demonstrations showing how structures outside our visible horizon could imprint detectable signatures on our universe.