Book

Boundary-Driven Cosmogenesis presents a computational approach to one of the oldest questions in science: how an organized universe can emerge from a prior, non-geometric source. Instead of beginning with a fully formed spacetime, the book develops a staged framework in which a boundary driver activates a phase, passes through closure conditions, and only then yields an effective geometric sector in which distances, curvature, and large-scale structure become meaningful. The central aim is not to claim a finished cosmology, but to define a falsifiable pipeline. Each stage is treated as a bounded transformation that can be examined through mechanism tests, robustness checks, recovery behavior, geometry-separation criteria, and exploratory prime-structured advantage tests. In this way, the book turns broad metaphysical intuition into a disciplined research program. A major theme of the work is the distinction between pre-geometry and effective geometry. The book argues that geometric language should not be used too early: before a geometry sector is established, one should speak in terms of source conditions, activation, closure, and transition maps rather than curvature, metric, or spacetime flow. This separation is essential for conceptual clarity and for avoiding category errors in early-universe modeling. Written in a structured and accessible style, the book is intended for curious readers, independent researchers, and scholars interested in cosmology, complex systems, and theoretical modeling. It offers both a conceptual roadmap and a benchmark-oriented framework for asking when a universe-like system genuinely passes from latent structure to effective organization.