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Dark matter density and current for equatorial plane accretion onto moving Kerr black hole

Grid of 20x20=400 models for velocities between 0 and 0.95c and dimensionless Kerr parameter alpha=a/M. Gas is boosted to the left, i.e., black hole moves to the right. Rotation is counterclockwise. Traveling salesman path (left side) has been used to scan entire plane continuously. Movie created for public lecture, soon available on Bliżej Nauki channel.