MEON v1. 1/R2 is presented as a staged framework for testing a modified weak-field gravitational response at galaxy scales and a possible effective extension toward early-universe clustering. The late-time MEON v1. 1 sector is tested on the SPARC rotation-curve sample using a bounded 165-galaxy comparison with fixed field parameters q = 1. 25 and eₑxt = 0. 01. In this bounded per-galaxy nuisance-fit setting, MEON v1. 1 achieves a global reduced chi-square of approximately 9. 18, compared with approximately 10. 10 for the Standard MOND reference and approximately 161. 53 for the Newtonian baryons-only limit. The archive also includes diagnostic material for weak-lensing and CMB compatibility. The MEON-R2 Bubble-Tension sector is not claimed as a final CMB proof. It is presented as an effective mathematical prototype showing that a redshift-dependent bubble/membrane tension can generate a cold early clustering sector with Omegaₑff h² ≈ 0. 12 near recombination, wₑff ≈ 0, cₛ² << 1, and negligible late-time interference with the validated galaxy-scale MEON v1. 1 regime. In a CAMB effective-cold-clustering proxy test, the R2 sector reproduces the Planck-like acoustic TT structure at the same level as the corresponding Lambda-CDM-like proxy, while a naive baryon-only/no-CDM case fails strongly. The scientific claim is deliberately conservative: MEON v1. 1 is a tested late-universe galaxy-scale model candidate, while MEON-R2 is a calculated effective route toward CMB compatibility. A final cosmological claim requires a covariant action, background equations, linear perturbation equations, and implementation in a full Boltzmann solver.
Asil Karahan (Wed,) studied this question.
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