Abstract
Using the WKB approximation, we evaluate both the massless and massive scalar and Dirac fields quasinormal modes (QNMs) of a Schwarzschild-de Sitter black hole. The result shows that the field with higher masses and larger cosmological constant λ will decay more slowly. We also found that the global monopole is similar to a factor to modify the κ of Dirac field or l of scalar field, where κ is the angular momentum number of Dirac field, and l is the angular momentum number of scalar field.
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Chang, JF., Shen, YG. Massive Quasinormal Modes of a Schwarzschild-de Sitter Black Hole with a Global Monopole. Int J Theor Phys 45, 2319–2338 (2006). https://doi.org/10.1007/s10773-006-9200-6
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DOI: https://doi.org/10.1007/s10773-006-9200-6