David Rømer Voigt

Does the Galactic Acceleration Scale Track H(z)? A direct comparison of the a₀–H coincidence with the first measurements of RAR evolution

The galactic acceleration scale a₀ ≈ 1.2 × 10⁻¹⁰ m s⁻² numerically satisfies a₀ ≈ cH₀/2π to within ~10%, a coincidence noted since Milgrom (1983) and still unexplained. Milgrom has long drawn the consequence: if the link is to the expansion rate rather than to Λ alone, a₀ is not...

Does the Galactic Acceleration Scale Track H(z)? A direct comparison of the a₀–H coincidence with the first measurements of RAR evolution

The galactic acceleration scale a₀ ≈ 1.2 × 10⁻¹⁰ m s⁻² numerically satisfies a₀ ≈ cH₀/2π to within ~10%, a coincidence noted since Milgrom (1983) and still unexplained. Milgrom has long drawn the consequence: if the link is to the expansion rate rather than to Λ alone, a₀ is not...