It was shown here that the faraway matter can exert a force of such a magnitude
as to account for the observed rotation velocity curves in spiral galaxies,
if the force is assumed to be decorrelated beyond a sufficiently large distance,
of the order of 1 kpc. In particular we fit the rotation curves of the galaxies
NGC 3198, NGC 2403, UGC 2885 and NGC 4725 without any need to
introduce dark matter at all.
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