Randomized trial explores topology transitions in quantum gravity, indicating implications for dark matter detection.
Quantum Geometro-Topodynamics provides a self-consistent, unitary framework for spatial topology transitions in non-perturbative quantum gravity. By formulating Wheeler–DeWitt evolution in a stratified Hilbert space equipped with an Ashtekar–Lewandowski-derived topological measure, the framework eliminates black hole singularities via Loop Quantum Gravity cutoff boundaries and restores exact unitarity through child universe creation. Dynamizing the vacuum topological angle into an axionic condensate naturally resolves the gravitational CP problem, while its relic abundance matches observed cold dark matter density (Omega_a h^2 approx 0.12). Crucially, the model yields a definitive observational signature: a cosmic microwave background birefringence angle beta_CMB ~ 0.1°–0.5° testable by upcoming LiteBIRD and CMB-S4 missions, elevating topology-changing quantum gravity from theoretical formalisms to an empirically falsifiable science.
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Maksym Koresh (2026) studied this question.
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