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arxiv: 1003.1381 · v3 · pith:MPRJQQ7Dnew · submitted 2010-03-06 · ✦ hep-th · gr-qc

Chern-Simons black holes: scalar perturbations, mass and area spectrum and greybody factors

classification ✦ hep-th gr-qc
keywords blackchern-simonsholestheyabsorptionanalyticallyareacalculate
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We study the Chern-Simons black holes in d-dimensions and we calculate analytically the quasi-normal modes of the scalar perturbations and we show that they depend on the highest power of curvature present in the Chern-Simons theory. We obtain the mass and area spectrum of these black holes and we show that they have a strong dependence on the topology of the transverse space and they are not evenly spaced. We also calculate analytically the reflection and transmission coefficients and the absorption cross section and we show that at low frequency limit there is a range of modes which contributes to the absorption cross section.

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Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Quasinormal modes of black holes: from astrophysics to string theory

    gr-qc 2011-02 accept novelty 1.0

    This review surveys calculations and interpretations of quasinormal modes for black holes in astrophysics, higher dimensions, and holographic duals without presenting new results.