Dirac Quasinormal Modes of New Type Black Holes in New Massive Gravity

Abstract

We study new type black holes in three-dimensional New Massive Gravity and we calculate analytically the quasinormal modes for fermionic perturbations for some special cases. Then, we show that for these cases the new type black holes are stable under fermionic field perturbations.

improved version. arXiv admin note: text overlap with arXiv:1306.5974, arXiv:1404.3172

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Cited by in corpus (8)

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• Scalar field instabilities in charged BTZ black holes
• Quasinormal modes of charged BTZ black holes
• Scalar field quasinormal modes on asymptotically locally flat rotating black holes in three dimensions
• Aspects of regular and singular electromagnetic-generalized-quasitopological-gravities black holes in (2+1) dimensions
• Spectral Bifurcations in Quasinormal Modes of Regular BTZ Black Holes
• Exact scalar (quasi-)normal modes of black holes and solitons in gauged SUGRA