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Rupture Cosmology

Year: 2026
Type: preprint
Abstract: Rupture Cosmology — Summary Rupture Cosmology proposes that our universe began not from a singular explosion, but from a controlled release of energy through a microscopic rupture in a high‑pressure pre‑universe state. Before our universe existed, all energy was confined within a dense, chaotic “bubble” of raw potential. This bubble was stable but not perfectly uniform. A tiny instability formed — a microscopic weakness in its boundary. Through this weakness, the first small squirts of energy escaped, producing the earliest fluctuations that would later seed cosmic structure. As the instability grew, the rupture widened and a massive outflow of energy burst through. This was the universe’s true beginning: a directional release that expanded into a new region, forming space and time as it spread. When enough energy escaped, the pressure difference dropped, the rupture sealed, and the pre‑universe bubble stabilized again. The newly released energy expanded and cooled, but not uniformly. Because the rupture was localized, the universe inherited gradients — variations in density, temperature, and entropy. These uneven cooling conditions became the engine of complexity, shaping the cosmic web, galaxies, stars, planets, chemistry, and eventually life. In Rupture Cosmology, structure exists because cooling was uneven, and cooling was uneven because the universe began through a rupture, not a uniform event. The universe is the aftermath of a pressure release, and complexity is the signature of its directional birth.
DOI: 10.5281/zenodo.22077490
Language: English
Open Access status: green
OpenAlex ID: W7204126123
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