Modos cuasi--normales de un agujero negro de Einstein--Gauss--Bonnet rodeado de quintaesencia: perturbaciones escalares y electromagnéticas
DOI:
https://doi.org/10.31349/RevMexFis.68.050704Keywords:
Quasi--normal modes, Quintessence, WKB approximation, Lyapunov exponentAbstract
In this work, we study the quasi-normal modes for scalar and electromagnetic perturbations for an Einstein–Gauss–Bonnet black hole surrounded by quintessence using the third-order WKB method and the Eikonal limit. First, the critical values of the Gauss–Bonnet coupling constant and the normalization factor related to the quintessence are established, to describe the event horizons of the solution. We have studied the condition of extreme horizons and the quasi–normal modes are performed by setting the quintessence state parameter in the particular case of ωq = −2/3
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