  In this paper, we introduce a metric ansatz for describing spherically
symmetric quantum corrected black hole (BH) space-time within an AdS
background, incorporating both ordinary and phantom global monopoles.
Afterwards, we focus into the thermodynamic properties of this BH, calculating
essential parameters such as the Hawking temperature and the specific heat
capacity. Moving forward, we analyze the effective potential of the system for
both null and time-like geodesics, as well as the shadow radius of the BH.
Additionally, we compute the emission rate of particles from this BH. Finally,
we explore the geodesic equations of motion and visualize the trajectories of
massive particles within the BH. Throughout our investigation, we examine how
the presence of ordinary and phantom global monopoles, alongside the quantum
corrected parameter, influences various thermal properties, the effective
potential of the system, the BH shadow radius, energy emission rate, and the
trajectories of massive particles. Importantly, through the generation of
figures depicting these phenomena, we highlight the distinctions between
results obtained with ordinary global monopoles and phantom ones, across a
range of quantum corrected parameter values considering small values of the
energy scale parameter.
