Dirac Quasinormal modes of MSW black holes

Abstract

In this paper we study the Dirac quasinormal modes of an uncharged 2 + 1 black hole proposed by Mandal et. al and referred to as MSW black hole in this work. The quasi- normal mode is studied using WKB approximation method. The study shows that the imaginary part of quasinormal frequencies increases indicating that the oscillations are damping and hence the black hole is stable against Dirac perturbations.

8 page, 3 figure, Appear in MPLA

References in corpus (1)

• Spectroscopy and Thermodynamics of MSW Black Hole

Cited by in corpus (4)

• Perturbations and Quasinormal Modes of the Dirac Field in Effective Quantum Gravity
• Long-lived Quasinormal modes around regular black holes and wormholes in Covariant Effective Quantum Gravity
• Collision of particles near charged MSW black hole in 2 + 1 dimensions
• Scalar and Spinor Quasi Normal Modes of a 2D Dilatonic Blackhole