This release presents the MEON R192 Integrated Release, a speculative effective-field-theory framework combining an analytical spin-torsion field-theory core with a reproducible numerical cosmology and perturbation pipeline. The analytical part formulates MEON as a topologically selected effective spin-torsion theory in four-dimensional spacetime. It includes the effective action, the massive axial-torsion/Proca sector, the topological vacuum-selection term Gammaₜop, the Fibonacci-Lucas and spin-Casimir resonance structure, and the proposed interpretation of the dark sector as a combination of a topological vacuum component and local torsion-lensing proxy effects. The computational part contains the R189-R192 numerical pipeline. R189 performs a Mukhanov-Sasaki perturbation test on the MEON attractor-plateau background. R190 extends this to a robustness and normalization audit. R191 adds a proxy-likelihood comparison against observationally motivated nₛ and r target ranges. R192 provides bridge and normalization outputs for future CLASS/CAMB/Cobaya-based analysis. Within the stated toy-model and effective-field-theory assumptions, the preferred R192 parameter point yields approximately nₛ = 0. 9639 and r = 0. 00156, with a phenomenological normalization to Aₛ = 2. 1 × 10^-9 and an inflationary energy-scale proxy V^ (1/4) ≈ 6. 47 × 10¹5 GeV. This release should be understood as an integrated EFT and computational audit package. It is not an official Planck/BICEP likelihood analysis, not a UV-complete quantum-gravity derivation, and not a final proof of the model. The absolute Aₛ normalization, the UV origin of Gammaₜop, the canonical MEON perturbation normalization, and the microscopic reheating mechanism remain open theoretical tasks.
Asil Karahan (Sun,) studied this question.