Modos cuasi--normales de un agujero negro de Einstein--Gauss--Bonnet rodeado de quintaesencia: perturbaciones escalares y electromagnéticas


  • G. Barrientos Universidad Autónoma del Estado de Hidalgo
  • Omar Pedraza Universidad Autónoma del Estado de Hidalgo
  • L. A. López Universidad Autónoma del Estado de Hidalgo
  • R. Arceo Universidad Autónoma de Chiapas



Quasi--normal modes, Quintessence, WKB approximation, Lyapunov exponent


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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How to Cite

G. Barrientos, O. Pedraza, L. A. López, and R. Arceo, “Modos cuasi--normales de un agujero negro de Einstein--Gauss--Bonnet rodeado de quintaesencia: perturbaciones escalares y electromagnéticas”, Rev. Mex. Fís., vol. 68, no. 5 Sep-Oct, pp. 050704 1–, Aug. 2022.



07 Gravitation, Mathematical Physics and Field Theory