This research aims to investigate the dynamics and properties of accretion disks around black holes using Computational Fluid Dynamics (CFD) simulations. Accretion disks play a crucial role in astrophysics, and understanding their behavior is essential for studying the physics of black holes and their associated phenomena. The proposed research will employ CFD techniques to model the complex fluid flow within the accretion disk, considering factors such as viscosity, magnetic fields, and relativistic effects near the event horizon. The simulation results will be analyzed to gain insights into the disk's structure, energy transport mechanisms, and radiation emissions. The research findings will contribute to advancing our understanding of black hole accretion processes and their impact on astrophysical phenomena.