a_0 from H_0 Tension
a_0 = c*H_0*iota_tau/2 evaluated at low-redshift (local) H_0=73.0 gives 0.9% from MOND; at CMB H_0=67.4 gives -6.9%. Galaxy rotation curves probe local H_0. The H_0 tension structurally manifests as uncertainty in the galactic acceleration scale. Falsifiable: BTFR normalization A
What this page is
This is a public Results-lane surface for a noteworthy Physics Registry item. It is generated from the Corpus Registry triage catalogue and keeps the generic Result catalogue unchanged.
Registry evidence
- Registry item: V.P122
- Type: proposition
- Scope: tau-effective
- Lean status: formalized
- Book / part / chapter: Book V · Part 5 · Chapter 37
Result summary
a_0 = cH_0iota_tau/2 evaluated at low-redshift (local) H_0=73.0 gives 0.9% from MOND; at CMB H_0=67.4 gives -6.9%. Galaxy rotation curves probe local H_0. The H_0 tension structurally manifests as uncertainty in the galactic acceleration scale. Falsifiable: BTFR normalization A should shift as H_0 tension resolves.
Related Results surfaces
- Galaxy rotation problem
- Flat Galaxy Rotation Curves from Capacity Gradient
- Galaxy Rotation Curves without Dark Matter
- Not MOND
- Galaxy Rotation Curve (NGC 3198)
- galaxy-rotation-problem
- Flat Galaxy Rotation Curves from Capacity Gradient
Reading role
Use as Registry evidence for an existing Results surface.
Claim boundary
This page reports a Registry-backed internal result surface. It is not an external validation claim, a scientific consensus claim, or independent acceptance.
Curation rationale
- physics-facing terms: cmb, galaxy, rotation
- candidate is better handled as evidence for an inferred existing public surface
Review notes
- No additional review notes recorded.