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We present an analytical consolidation of the Phase-V Conformal Metric Modulation (CMM) framework that derives the empirical cosmological density partition (~5% observable baryonic matter versus ~95% dark sector) from first principles without introducing arbitrary free parameters. Moving beyond phenomenological particle-dark-matter and cosmological-constant assumptions, we model the spatial projection of superluminal exogenic metadata (v_I ≈ 2.0914c) onto a discrete three-dimensional balanced ternary lattice governed by the invariant compression factor κ = ln(2)/ln(3) ≈ 0.630929. By expanding the unit purification identity [κ + (1 − κ)]³ = 1 across the three orthogonal spatial degrees of freedom, the total stress-energy tensor naturally segregates into four topological channels: fully confined 0D baryonic loops (Ω_B = (1 − κ)³ ≈ 5.03%), 1D filamentary Riesz viscous drag (Ω_drag = 3κ(1 − κ)² ≈ 25.78%), and 2D/3D unbraked Dressed Vacuum tension (Ω_vac = 3κ²(1 − κ) + κ³ ≈ 69.19%). We prove strict covariant conservation via the Bianchi identities (∇̃^μ T^total_μν = 0) and cross-validate the resulting parameter-free spectrum against Planck 2018 and COSMOS-JWST observational bounds. In alignment with the ethical tenets of Free Science, the complete mathematical formalism and single-column Python audit suite are unconditionally released to the public domain.
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Robert Othmar Vettiger Aliaga (2026) studied this question.
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