ELEMENTARY STUDY OF STABILITY AND STRUCTURE OF ACCRETION DISKS AROUND COMPACT OBJECTS

• Main Author: Gautama Saputta, Rivaldo
• Format: Final Project
• Language: Indonesia
• Online Access: https://digilib.itb.ac.id/gdl/view/85682
• Institution: Institut Teknologi Bandung

An accretion disk is an important structure that forms around compact objects such as black holes, neutron stars, or white dwarfs, where material from the surrounding environment flows and forms a rotating disk. This research focuses on the elementary study of the stability and structure of accretion disks around compact objects. The primary goals of this study are to identify and analyze the factors influencing the stability of accretion disks and to examine the variations in disk structure around various types of compact objects, such as neutron stars and black holes. By analyzing the dynamics and structure of accretion disks, this research aims to provide a better understanding of how changes in the stability and structure of these disks affect astronomical observations, including radiation emissions and other astrophysical phenomena. The results of this study are expected to significantly contribute to the understanding of matter interactions around compact objects and their implications for theories on the formation and evolution of astrophysical systems.