  The trajectories of test particles with spin orbiting a black hole depend on
the geometry of space-time and the intrinsic physical characteristics of the
test particles. In this work the motion of test particles with spin on the
innermost stable circular orbit of a quantum improved rotating black hole is
studied. A computational implementation is presented through the Mathematica
program, which can calculate and graph the radius, angular momentum and energy
as a function of the spin of the test particles and for various geometric
parameters of the rotating black hole, as they are the spin $a$ and the mass
$M$ of the rotating black hole and the quantum parameters $\gamma$ and
$\omega$. Additionally, the program calculates the maximum spin physically
possible for the test particles. At the end, some results given by the program
are discussed and it is shown that these are consistent with those previously
reported, both for the classical black holes of Schwarzschild and Kerr and for
the quantum improved ones.
