arXiv · 2112.11869
Bardeen black hole in magnetically charged four-dimensional Einstein-Gauss-Bonnet gravity
Abstract
In this paper, we investigate the shadow radius and quasinormal modes of a four-dimensional magnetically charged Einstein-Gauss-Bonnet Bardeen black hole and point out a simple connection between them in the eikonal limit. By studying a massless scalar field perturbation in this spacetime background and using the sixth-order Wentzel-Kramers-Brillouin(WKB) approximation, we get the quasinormal modes(QNMs) and perform a detailed analysis. It shows that the quasinormal modes are depend on the Gauss-Bonnet coupling constant and the magnetic charge. We also give a formula of the QNMs and shadow radius in the eikonal limit and check it numerically for the real and imaginary part of it, respectively.
Explore related subjects
Keep this discovery
Shu-Jun Zhang, He-Xu Zhang, Lei Shao, Jian-Bo Deng, Xian-Ru Hu. 2021-12-22. Bardeen black hole in magnetically charged four-dimensional Einstein-Gauss-Bonnet gravity. https://arxiv.org/abs/2112.11869
Cite the original work for its findings. Save a collection to share your selection of sources.