Double shadow of a 4D Einstein-Gauss-Bonnet black hole and their connection between with quasinormal modes

Abstract

In this paper, we study the shadow of a 4D Einstein-Gauss-Bonnet black hole as photons couple to the Weyl tensor and find that the propagation of light depends on its polarization which leads to the existence of a double shadow. Then, we discuss the effect of the coupling parameter $\lambda$, the polarization of light and the Gauss-Bonnet coupling constant $\alpha$ on shadow. Further we explore the influence of the Gauss-Bonnet coupling constant $\alpha$ on the quasinormal modes (QNMs) of massless scalar field and investigate the connection between the real part of QNMs in the eikonal limit and the shadow radius of black holes. We find that in the eikonal limit the real part of QNMs is inversely proportional to the shadow radius under the case of the photons uncoupled to the Weyl tensor.

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Cited by in corpus (5)

• Quasinormal modes-shadow correspondence for rotating regular black holes
• Eikonal quasinormal modes, photon sphere and shadow of a charged black hole in the 4D Einstein-Gauss-Bonnet gravity
• Massive scalar field perturbations of 4D de Sitter Einstein-Gauss-Bonnet black holes
• Quasinormal modes and greybody factor of charged black hole in non-commutative geometry
• Cosmological Constraints on 4D Einstein-Gauss-Bonnet Gravity and Kaniadakis Holographic Dark Energy: Implications for Black Hole Shadows