| Name: | Navneet Mishra |
| Affiliation: | Student |
| Conference ID : | ASI2024_333 |
| Title : | Quasinormal modes of Schwarzschild black hole. |
| Authors : | Navneet Mishra1, Dr. Tejinder P Singh2. |
| Authors Affiliation: | 1 Student, St. Xavier's College (Autonomous), Mumbai-400001, India.
2 Professor, Tata Institute of Fundamental Research, Mumbai-400005, India. |
| Mode of Presentation: | Poster |
| Abstract Category : | High Energy Phenomena, Fundamental Physics and Astronomy |
| Abstract : | Black holes, enigmatic cosmic phenomena concealed by singularities beneath event horizons, offer exact solutions within the realm of general relativity. Within this intricate framework, the theory of black hole perturbations plays a pivotal role in the interpretation and analysis of data from gravitational wave observatories.
This master's thesis embarks on a comprehensive exploration of the classical theory of linear perturbations in Schwarzschild black holes, with a specific focus on quasinormal modes.
The presentation begins with a rigorous explanation of the foundational principles underpinning linear perturbations in the context of Schwarzschild black holes. Subsequently, our examination delves into the intricate study of quasinormal modes, shedding light on their profound significance within the broader tapestry of black hole physics. A central aspect of our inquiry is the Regge-Wheeler equation, a crucial element in understanding the intricate vibrational dynamics of black holes.
This literature survey stands as a valuable resource for physicists and researchers immersed in the realm of black hole physics and the exploration of gravitational wave phenomena. By integrating the existing body of knowledge in these areas, this work aims to deepen our understanding of the fundamental principles and intricacies of perturbations and quasinormal modes inherent to the Schwarzschild black hole paradigm. In doing so, it significantly contributes to the ongoing advancement of this vital field of astrophysical inquiry. |
