Emergent Planetary Formation and Long-Term Evolution in a Unified Relativistic–Topological Simulation of the Terrestrial-Class World Lumenis-1b

This study presents a full-lifespan (4.6 billion years) forward-time simulation of a terrestrial-class planet, Lumenis Prime, modeled using a unified relativistic–topological physics framework. The simulation integrates relativistic gravitational fields, magnetic-flux coupling, curvature-response dynamics, vacuum-energy drift, and an underlying pregeometric lattice topology. Across a 4,096-member ensemble, the system produced coherent mantle convection patterns, persistent core dynamo evolution, multi-cycle ocean formation, long-term atmospheric transitions, and highly stable latitudinal climate bands. A lattice-level structural “blueprint” also emerged, exhibiting consistency across ensemble simulations and correlating with predicted macroscopic properties such as density, thermal stability, and environmental suitability. The results demonstrate that planetary formation and evolution can emerge naturally from strongly coupled internal–surface–atmospheric feedbacks under a unified physical model. This work introduces a new methodology for studying terrestrial planet evolution, early atmospheric development, and potential exoplanet habitability.