Baryonic Tully-Fisher
Mbar = V4/(G·a0) predicts slope exactly 4.0
Observed: 3.68±0.12 (M/L uncertainty shifts toward 4)
RAR Universality
One relation for all galaxy types with scatter at measurement limit
Scatter: 0.144 dex (limit: 0.119)
Deep MOND Regime
gobs → √(gbar·a0) continues to hold at very low accelerations
Scatter only 15% higher than transition region
Weak Gravitational Lensing
Fagin 2024 SLACS power-law index
Khronon β=6.2 (2.4σ) vs CDM β=8.0 (6.8σ)
Tidal Dwarf Galaxies
TDGs follow the same RAR without pre-existing dark matter halos
Predicted V=35 km/s, observed: 30–40 km/s
MW Escape Velocity
Predicted from baryonic mass alone
558 km/s (observed: 550±30)
Fast Bar Pattern Speeds
No dynamical friction from dark matter halo
R = 1.0–1.3 (fast), CDM predicts 1.7 (slow)
LSB Disk Stability
Toomre Q crosses 1 naturally without overstabilization
CDM: Q=2.8 (overstabilized), Khronon: Q crosses 1
External Field Effect
Satellite galaxies affected by host potential
Σ-hierarchy: uses potential, not acceleration gradient
Globular Clusters
Σ-hierarchy predicts GCs stay Newtonian in MW potential
RMS: 186% → 33% after Σ-hierarchy correction
Dwarf Irregulars
Non-circular motions and M/L floor limit accuracy
Residual: −15.7% → −6.7% with quality cuts
Wide Binaries
8–13% velocity boost predicted at large separations
Awaiting Gaia DR4 confirmation