Timelike geodesics in the rotating Hayward regular black hole admit a Carter-like fourth constant of motion, and out-of-plane orbits differ from Kerr mainly at low spin and large length parameter g.
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Geodesic structure of a rotating regular black hole
Timelike geodesics in the rotating Hayward regular black hole admit a Carter-like fourth constant of motion, and out-of-plane orbits differ from Kerr mainly at low spin and large length parameter g.