Studies on Quasinormal Modes and Late-time Tails in Black Hole Spacetimes
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30/10/2013
30/10/2013
01/10/2012
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Resumo |
This thesis Entitled Studies on Quasinormal modes and Late-time tails black hole spacetimes. In this thesis, the signature of these new theories are probed on the evolution of field perturbations on the black hole spacetimes in the theory. Chapter 1 gives a general introduction to black holes and its perturbation formalism. Various concepts in the area covered by the thesis are also elucidated in this chapter. Chapter 2 describes the evolution of massive, charged scalar field perturbations around a Reissner-Nordstrom black hole surrounded by a static and spherically symmetric quintessence. Chapter 3 comprises the evolution of massless scalar, electromagnetic and gravitational fields around spherically symmetric black hole whose asymptotes are defined by the quintessence, with special interest on the late-time behavior. Chapter 4 examines the evolution of Dirac field around a Schwarzschild black hole surrounded by quintessence. Detailed numerical simulations are done to analyze the nature of field on different surfaces of constant radius . Chapter 5is dedicated to the study of the evolution of massless fields around the black hole geometry in the HL gravity. Department of Physics, Cochin University of Scienceand Technology Cochin University of Science and Technology |
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Cochin University of Science and Technology |
Palavras-Chave | #From "Dark Stars" to "Black Holes #QNMs of black holes #Scalar perturbations #Gravity and Quantization #Black holes in HL gravity |
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Thesis |