Scalar field quasinormal frequencies of Reissner-Nordström black hole surrounded by quintessence by using he continued fraction method

Abstract

We evaluate the quasinormal modes of massless scalar field around Reissner-Nordstr$\ddot{\text{o}}$m black hole surrounded by a static and spherically symmetric quintessence by using the continued fraction method. The appropriate Frobenius series for three special cases of the quintessence parameter $\epsilon =-1/3,-2/3$ and $-1$ are derived successfully. We show that the variation of quasinormal frequencies with charge of the black hole and the quintessential parameters. The numerical results show that quintessence field decreases oscillation frequencies of all angular momentum $l$ modes and increases the damping time of $l>0$ modes.

17 pages, 2 figures

References in corpus (2)

• Viscosity, Black Holes, and Quantum Field Theory
• Decay of a charged scalar and Dirac fields in the Kerr-Newman-de Sitter background

Cited by in corpus (1)

• Quasibound states of the Dirac field in Schwarzschild and Reissner-Nordström black hole backgrounds