Processos de geração de gama em núcleos ativos de galáxias

Abstract

The first part of this study analyzes the generation processes of gamma radiation in active galactic nuclei, exploring physical mechanisms, observation methodologies, and computational modeling. With a detailed bibliographical survey, the research investigates types of observatories, emission sources and simulation programs. The second part, in turn, presents the modeling and data fitting for three radio galaxies using the AGNpy software. The critical analysis of the data aims to contribute to the advancement of high-energy astrophysics, providing an understanding of extreme phenomena such as particle acceleration and emission around black holes. These studies are fundamental for cosmology, helping to map the distribution of matter and the evolution of cosmic structures, and for particle astrophysics by identifying cosmic-ray sources. Investigations in this field promise to broaden our understanding of high-energy physics and cosmic dynamics.