Electromagnetic quasinormal modes of dyonic AdS black holes with quasitopological electromagnetism in a Horndeski gravity theory mimicking EGB gravity at D? 4

We investigate some properties of a black hole in a Horndeski gravity theory mimicking EGB gravity at D ? 4. Borrowing ideas from quasitopological gravities provide a matter source of dyonic fields, in which the black hole solution carries two charges, electric and magnetic, in the context of the Einstein-Gauss-Bonnet (EGB) gravity. However, due to several limitations of the EGB gravity in D ? 4, we consider a Horndeski gravity theory which can mimic EGB gravity in D ? 4. The essential practice used in this paper is the electromagnetic quasinormal modes process, with the goal of discovering the spectrum of such an electromagnetic perturbation over the black hole spacetime. The Wentzel-Kramer-Brillouin (WKB) approximation is used to achieve the desired results. The study shows that both the charges have similar impacts on the quasinormal modes.

Automated summary

This paper investigates properties of a black hole in a Horndeski gravity theory that mimics EGB gravity in D ≤ 4, using quasitopological gravities to provide a matter source of dyonic fields. By studying the electromagnetic quasinormal modes process, the authors aim to understand the spectrum of such perturbations over the black hole spacetime. The study reveals that both electric and magnetic charges have similar impacts on the quasinormal modes.