Randomized trial predicts dark energy state in Cosmology, indicating consistency with upcoming data.
Within the framework of the Dynamic Abstract Sphere (DAS) theory, dark energy arises as the potential energy of a covariant scalar field δ(xᵘ) — the 'thickness of the present moment' — near its equilibrium value δ̄₀. We derive the dark energy equation of state w(z) = −1 + 2εδ/(1+z)^α, where εδ is the slow-roll parameter at z = 0. For natural DAS parameter values (c₄ = π²/8, c₂ = 3π/128G, c₀ ~ O(100)), we obtain εδ ≈ 0.085, predicting w₀ = −0.83. The DESI collaboration (BAO Year 1 2024, combined with CMB and PantheonPlus supernovae) measures w₀ = −0.827 ± 0.061, consistent with the DAS prediction at the 0.05σ level. The prediction was derived independently of DESI data. Additional consequences are discussed: the same field δ predicts ultralight dark matter with mass mδ ~ 10⁻²² eV, and DESI Year 5 data will test the prediction wₐ = −0.34.
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Yuri P.; Claude (Anthropic) Gorenstein (2026) studied this question.
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