Topological Resolution of the Strong CP Problem and Zero-Parameter Derivation of the Absolute Neutrino Mass Scale from the R12 Rendering Algebra
Authors/Creators
Description
Abstract
We resolve the strong CP problem and derive the absolute neutrino mass scale from the R12 rendering algebra of Array Cosmology (AC) with zero free parameters.
The QCD vacuum angle θ is shown to be exactly zero as the unique value satisfying both the closure relation e1e2 · · · e12 = −1 (which restricts θ to multiples of π/6) and the parity pair relation ek · ek+6 = Znoise ·1 (which further restricts θ to multiples of
π), with θ = π excluded by experimental CP conservation. Thermal corrections give |θeff| ∼ Z12 noise ≈ 8 × 10−13, two orders of magnitude below the current experimental bound. The prediction that no axion exists is falsifiable. The heaviest neutrino mass
is derived as m3 = me Z b0 noise/(1 − Znoise), where me is the electron mass, Znoise = (π − 3) ln 2 is the vacuum Landauer noise, and b0 = 7 is the QCD one-loop betafunction coefficient. This yields m3 = 0.0497 eV, matching p ∆m2 atm = 0.0495 eV
to 0.35% and predicting normal mass hierarchy with Pmi = 0.054 eV, testable by JUNO, Project 8, and CMB-S4.
Files
Lim_ArrayCosmology_StrongCP_NeutrinoMass_2026.pdf
Files
(460.1 kB)
| Name | Size | Download all |
|---|---|---|
|
md5:0ab7ae2815e50d5732e1e9144a230bb8
|
460.1 kB | Preview Download |