Slowly Rotating Charged Gauss-Bonnet Black holes in AdS Spaces
Hyeong-Chan Kim, Rong-Gen Cai
TL;DR
This paper derives slowly rotating charged Gauss-Bonnet black hole solutions in higher-dimensional AdS spaces, analyzing their physical properties and showing the Gauss-Bonnet term does not influence the gyromagnetic ratio.
Contribution
It provides new solutions for rotating charged Gauss-Bonnet black holes in higher dimensions and examines their electromagnetic properties.
Findings
Gauss-Bonnet term does not affect the gyromagnetic ratio.
Solutions are valid in the small angular momentum limit.
Calculated angular momentum, magnetic dipole moment, and gyromagnetic ratio.
Abstract
Rotating charged Gauss-Bonnet black hole solutions in higher dimensional (), asymptotically anti-de Sitter spacetime are obtained in the small angular momentum limit. The angular momentum, magnetic dipole moment, and the gyromagnetic ratio of the black holes are calculated and it turns out that the Gauss-Bonnet term does not affect to the gyromagnetic ratio.
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