Quasi-Normal Modes in Topologically Massive Gravity

Details Quasi-Normal Modes in Topologically Massive Gravity Quasi-Normal Modes in Topologically Massive Gravity

2008-06-11

arxiv.org/abs/0806.1788v3

JHEP 0808:003,2008

Physics

High Energy Physics

High Energy Physics - Theory

13 pages, typos corrected

Scientific paper

10.1088/1126-6708/2008/08/003

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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