Galactic flat rotation curves and the acceleration scale a0 are attributed to slow time-dependent growth of galaxy mass and radius, rather than dark matter or modified gravity.
The Bullet cluster at its best: Weighing stars, gas, and dark matter
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The Galactic Pizza: Flat Rotation Curves in the Context of Cosmological Time-Energy Coupling
Galactic flat rotation curves and the acceleration scale a0 are attributed to slow time-dependent growth of galaxy mass and radius, rather than dark matter or modified gravity.