Detection of Gravitational Anomaly at Low Acceleration from a Highest-quality Sample of 36 Wide Binaries with Accurate 3D Velocities
This study analyzes a high-quality sample of 36 wide binary stars with accurate 3D velocities to detect a significant gravitational anomaly at low accelerations, revealing a gravity boost factor of approximately 1.6 that rules out standard Newtonian dynamics and exceeds MOND predictions, a result primarily driven by two specific binary systems exhibiting unbound relative velocities.