Dirac Quasinormal Modes of New Type Black Holes in New Massive Gravity
P. A. Gonzalez, Yerko Vasquez
TL;DR
This paper analytically calculates fermionic quasinormal modes of new type black holes in three-dimensional New Massive Gravity, demonstrating their stability under such perturbations and contributing to understanding their dynamical properties.
Contribution
It provides the first analytical computation of fermionic quasinormal modes for these black holes, establishing their stability in specific cases.
Findings
Black holes are stable under fermionic perturbations.
Analytical expressions for quasinormal modes are derived.
Stability is confirmed for certain special cases.
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.
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