Quasinormal modes for massless topological black holes
classification
✦ hep-th
gr-qc
keywords
blackcurvaturemasslessmodesquasinormalscalartopologicalassumed
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An exact expression for the quasinormal modes of scalar perturbations on a massless topological black hole in four and higher dimensions is presented. The massive scalar field is nonminimally coupled to the curvature, and the horizon geometry is assumed to have a negative constant curvature.
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Cited by 1 Pith paper
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Quasinormal modes of black holes: from astrophysics to string theory
This review surveys calculations and interpretations of quasinormal modes for black holes in astrophysics, higher dimensions, and holographic duals without presenting new results.
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