Geodesic motions near an improved Schwarzschild black hole

In this paper, we studied the geodesics of timelike and null like particles near an improved Schwarzschild black hole. The lapse function has been plotted was found that only one horizon is possible. equation motion effective potential test particle have calculated. This importance in studying radial free fall stability orbits (trajectories). energy angular momentum also calculated to analysis cicrular circular orbits. Moreover, Innermost stable orbit radius determined. To get a deeper insight nature these trajectories, with help dynamical systems approach. us determine as well fixed point phase space trajectories.