Galaxy rotations from quantised inertia and visible matter only
@article{Mcculloch2017GalaxyRF, title={Galaxy rotations from quantised inertia and visible matter only}, author={M. E. Mcculloch}, journal={Astrophysics and Space Science}, year={2017}, volume={362}, pages={1-5} }
It is shown here that a model for inertial mass, called quantised inertia, or MiHsC (Modified inertia by a Hubble-scale Casimir effect) predicts the rotational acceleration of the 153 good quality galaxies in the SPARC dataset (2016 AJ 152 157), with a large range of scales and mass, from just their visible baryonic matter, the speed of light and the co-moving diameter of the observable universe. No dark matter is needed. The performance of quantised inertia is comparable to that of MoND, yet…
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