A Study of Quasi-Normal Modes of Different Kinds of Black Holes
Department of Physics, Indian Institute of Technology Indore
Calculated Quasi-Normal Modes (QNMs) for Kerr Black Holes using a novel technique, comparing results with Leaver's method. Investigated Kerr-Sen Black Holes to establish a relationship between shadow radius and quasi-normal frequencies. Extended the analysis to Kerr-Newman Black Holes with implications for gravitational wave astronomy.