Theoretical exploration of dark matter and dark energy as a unified substrate, indicating new cosmic phenomena.
ZEN28 This dossier develops the cosmological articulation of the Theory of Quantum Oceans (TOQ) for the current relaxation phase of the Plenum, designated as the T⁻ phase. It proposes the structural identification T⁻ = DM + DE, interpreting dark matter and dark energy not as independent exotic components, but as two complementary regimes of a single dynamic substrate. Dark matter is described as the gravitational signature of local hyper-relaxation clouds induced around baryonic structures, producing optically neutral but gravitationally active halo-like distributions. Dark energy is interpreted as the effective expression of the structural angular advancement of the T⁻ half-cycle, leading to a non-constant effective component Ω_Λ_eff. The dossier introduces a Friedmann-TOQ equation: H²(a, θ) = H₀² × [Ω_m · a⁻³ + Ω_Λ · sin²(θ/2)/sin²(50°)] Under explicit observational parameters and a calibrated phenomenological θ(t), the framework conditionally retrieves the observed transition between decelerated and accelerated expansion, with z_trans ≈ 0.66, and provides a present-day deceleration parameter q₀ ≈ −0.60. The note also records three observational alignments: the intrinsic value ε = π⁴/T₁₁³ ≈ 339,000 years compared with recombination-scale estimates, its positioning within the opacity transition zone of the cosmic microwave background, and the qualitative convergence between a non-constant effective dark energy component and recent DESI indications of possible dark energy evolution. A final section introduces the hypothesis of a global cosmological asymmetry of the Plenum beyond the observable horizon, backed by recent discussions of cosmic dipole anomalies and large-scale bulk flows. The dossier concludes by identifying open programmes, including the derivation of Ω_m and Ω_Λ from TOQ axiomatic invariants, the structural derivation of θ(t), and future confrontations with CMB, supernova, weak-lensing, S₈, Euclid and SKA datasets.
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Régis GUERRERO (2026) studied this question.
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