Abstract
We obtain the quasi-normal mode (QNM) frequencies of scalar perturbation on new type black holes in three-dimensional new massive gravity. In some special cases, the exact QNM frequencies are obtained by solving scalar field equations exactly. On some parameter regions, the highly damped QNM frequencies are obtained in an analytic form by the so-called Stokes line method. This study on QNMs sheds some light on the mysterious nature of these black holes. We also comment about the AdS/CFT correspondence and the entropy/area spectrum for new type black holes.
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