  In this article, we explore the geodesics motion of neutral test particles
and the process of energy extraction from a regular rotating Hayward black
hole. We analyse the effect of spin, as well as deviation parameter $g$, on
ergoregion, event horizon and static limit of the said black hole. By making
use of geodesic equations on the equatorial plane, we determine the innermost
stable circular and photon orbits. Moreover, we investigate the effective
potentials and effective force to have information on motion and the stability
of circular orbits. On studying the negative energy states, we figure out the
energy limits of Penrose mechanism. Using Penrose mechanism, we found
expression for the efficiency of energy extraction and observed that both spin
and deviation parameters, contribute to the efficiency of energy extraction.
Finally, the obtained results are compared with that acquired from Kerr and
braneworld Kerr black holes.
