Spinning test particle motion around a rotating wormhole

In this work, we investigated the motion of spinning test particles around a rotating wormhole, extending, in way, previous work Benavides-Gallego et al. [Phys. Rev. D 101, 124024 (2020)] to general case. Using Mathisson-Papapetrou-Dixon equations, study effective potential, circular orbits, and innermost stable orbit (ISCO) particles. We found that both particle wormhole spins affect location ISCO significantly. On other hand, similar nonrotating case, also two possible configurations potential: plus minus. Furthermore, minimum value potential is not at throat due its spin $a$, contrast nonspinning where symmetric, wormhole. case ISCO, it increases as $a$ increases, black holes presence decreases ISCO. Finally, since dynamical four-momentum kinematical four-velocity are always parallel, consider superluminal bound, finding allowed values dimensionless particle's $s$ change wormhole's increases.