arXiv · 0806.1788
Quasi-Normal Modes in Topologically Massive Gravity
Abstract
We determine the black hole quasi-normal mode spectrum for tensor perturbations in topologically massive AdS-gravity. In the special case of chiral gravity quasi-normal modes are absent despite of the presence of a horizon. In the process we uncover a simple algebraic structure in the quasi normal modes spectrum: the tower of QNM's consists of descendents of a "chiral highest weight'' QNM which in turn satisfies a first order equation.
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Ivo Sachs, Sergey N. Solodukhin. 2008-09-15. Quasi-Normal Modes in Topologically Massive Gravity. https://doi.org/10.1088/1126-6708%2F2008%2F08%2F003
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