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

2014/04/28 by P. A. Gonzalez, Yerko Vasquez · 1 citation
Physics and Astronomy · #gr-qc

paper · pdf · doi:10.1140/epjc/s10052-014-2969-1

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

arxiv created 2014/04/28 · arxiv updated 2015/06/19

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.

Citations

• Dirac quasinormal modes of Chern-Simons and BTZ black holes with torsion
• Quasinormal modes and greybody factors of a four-dimensional Lifshitz black hole with z=0

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