MEON R192 Integrated Release: Effective Spin-Torsion Field Theory, Resonance Structure, and Cosmological Perturbation Pipeline

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 Gamma_top, 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 n_s 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 n_s = 0.9639 and r = 0.00156, with a phenomenological normalization to A_s = 2.1 × 10^-9 and an inflationary energy-scale proxy V^(1/4) ≈ 6.47 × 10^15 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 A_s normalization, the UV origin of Gamma_top, the canonical MEON perturbation normalization, and the microscopic reheating mechanism remain open theoretical tasks.