A geometric investigation of cosmic collapse, compression, and the origins of expansion
Using the same methodological discipline that underlies TBA, OCT, and MPDEC, MORK addresses the question MPDEC deliberately left open: if cosmic expansion is driven by black holes — and OCT shows that black holes can become dormant — what happens when the universe contains too few active black holes to sustain expansion?
It collapses.
Not catastrophically, but naturally, as spacetime relaxes toward its neutral state.
MORK then asks the next logical question: What would the early universe look like if OCT and MPDEC are true? The calculations reveal a surprising result — the universe would not simply relax. It would compress, entering a high‑curvature regime that reshapes how we interpret the Big Bang and the cosmic microwave background.
This compression insight opens new avenues for understanding the origin of expansion, the structure of the CMB, and the geometric conditions that precede a reset. MORK explores these questions mathematically, providing a coherent picture of how a contracting universe transitions into rapid expansion without invoking singularities, inflation, or exotic physics.
A full manuscript detailing the geometry, validation, and observational implications is forthcoming.
Status: Research complete, full manuscript and mathematical reproduction pipeline in development.