The MOND acceleration scale as a de Sitter curvature scale
One claim: the acceleration scale of the mass-discrepancy–acceleration relation is set by the dark-energy density.
Realised as modified gravity — the modified-inertia arm was closed by lensing in August 2026 — with the Milgrom–Sanders (2008) kernel ν(y) = 1/(1 − e^(−√y)) as the operative interpolation. κ = ½ is fitted, not derived: measured 0.551 ± 0.043 (distance-free) and 0.465 ± 0.076 (Tully–Fisher). Because a₀ tracks the dark-energy density it cannot track the expansion rate: a₀(z)/a₀(0) = √(ρ_DE(z)/ρ_DE(0)) exactly, which is flat if Λ is constant, 13% lower by z = 2 on DESI’s w₀wₐ fit, and within ±20% of today’s value out to z = 3 for any dark energy the data allow — against ×3 for a₀ ∝ H(z) and ×1.8 for ΛCDM’s emergent scale. That is the one statement here that ΛCDM does not make.
Attribution — what is and is not original here
This law is not new, and neither is its derivation. Milgrom (1999, Phys. Lett. A 253, 273, Eqs. 6–9) derives this exact law from the de Sitter–Unruh balance and fixes its coefficient at a₀ = 2 c H_Λ. His Eq. (9) is identically the relation above — verified symbolically, difference exactly zero. The same law was independently re-derived entropically by Pikhitsa (2010) and Klinkhamer & Kopp (2011), both also landing on 2 c H_Λ.
So the de Sitter–Unruh argument does not leave the coefficient free — it predicts one, and that prediction is 11.58× the value used here. What this programme actually contributes is therefore narrow and should be stated as such: a re-normalisation of the coefficient to fit data (κ = ½ in place of Milgrom’s 2), plus the relativistic completion — the scale embedded in Aether–Scalar–Tensor theory — and its derived a₀(z). It is not a derivation of the law, and not a derivation of its scale.