This release presents the MEON v1. 1 / MEON-R2 framework as a phenomenological modified-gravity and field-theory candidate for galaxy-scale dynamics and early-universe effective clustering. The MEON v1. 1 weak-field sector is tested against 165 usable SPARC galaxy rotation curves using bounded per-galaxy stellar mass-to-light nuisance fits. In the reported bounded-disk run, the fixed MEON v1. 1 candidate with q = 1. 25 and eₑxt = 0. 01 achieves a global reduced chi-square of approximately 9. 178, compared with approximately 10. 098 for the Standard MOND reference and approximately 161. 531 for Newtonian baryons alone. The accompanying MEON-R2 sector is introduced as an induction-driven membrane-tension prototype. In this model, cosmological flux evolution induces a tension current, which generates a redshift-dependent membrane tension. This tension activates an effective cold clustering sector near recombination, with Omegaₑff h² close to 0. 12, near-zero effective equation of state, and negligible effective sound speed, while dynamically decoupling at late times to preserve the validated MEON v1. 1 galaxy-scale limit. This archive contains the final polished manuscript material, candidate field-equation formulation, SPARC validation outputs, R2 induction-tension calculator outputs, diagnostic plots, code, and release notes. The results should be interpreted conservatively: MEON v1. 1 is presented as a galaxy-scale phenomenological modified-gravity candidate, while MEON-R2 is a quantitative early-clustering prototype rather than a final covariant CMB proof. A complete cosmological validation requires a fully covariant action, linear perturbation equations, implementation in a Boltzmann solver, and comparison against full CMB TT/TE/EE plus lensing likelihoods.
Asil Karahan (Thu,) studied this question.