Hydrodynamic radioactive transfer process around Active galactic nuclei

Abstract

This thesis investigates the physical processes governingActiveGalacticNuclei(AGNs) andtheir interaction with surrounding environments, focusing on the interplay of hy drodynamics and radiative transfer. The model equations used were that of the stan dard AGNmodelsrooted in Einstein General Relativity. The study aims to understand radiation emission and absorption around AGNs, quantify radiation near the central black hole, model radiation transfer to the host galaxy, and simulate the effects of hydrodynamics and radiative transfer on the host galaxy’s energy output. Analytical methods and computational simulations were used to explore AGN behavior and its impact on the cosmic environment where the latest Python3 has used in computa tions and simulations. The results are well pleased with the previous theoretical works of the others and with observation under the minimal boundary conditions set.