First 3D N-body simulations of a rotating, shear-free Newtonian universe show more than 1% anisotropy between polar and equatorial expansion rates at maximal allowed rotation.
Monthly Notices of the Royal Astronomical Society 162:307
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Simulating Rotating Newtonian Universes
First 3D N-body simulations of a rotating, shear-free Newtonian universe show more than 1% anisotropy between polar and equatorial expansion rates at maximal allowed rotation.