The Information-Capacity Framework for Cosmogenesis

This work presents a cosmological framework in which a new universe nucleates as a finite bubble inside a parent black hole and inherits a fixed information budget from a patch of the parent horizon. The inherited information forms a dark‑matter lattice whose excitation energy generates the visible sector, while the geometric mismatch between the excited lattice and the initial bubble volume produces a constant outward pressure identified as dark energy. In this model, dark energy is interpreted not as an energy density but as a geometric expansion requirement: the irreversible growth of the bubble needed to accommodate its inherited information when excited.The inherited information seed contains approximately bits, corresponding to the minimum horizon area of a parent black hole of mass . As the bubble expands, its horizon area grows holographically from the inherited bits to the present bits. This area growth naturally locks the mass–radius relation of the universe to a Schwarzschild‑like form throughout cosmic history, explaining why the observable universe maintains a near black‑hole mass–radius proportion despite cosmic expansion.By comparing the inherited entropy at nucleation with the present cosmological horizon entropy, the model predicts that the total bubble radius today is only a factor of larger than the visible radius, implying that the actual universe is times larger in volume than the observable region. Dark energy, horizon growth, and entropy increase emerge as a single geometric process, providing a unified explanation for cosmic acceleration, holography, and the dark‑to‑visible matter ratio.This dataset includes the full manuscript, derivations, and supporting calculations for the inheritance‑based cosmological model.