Rotating charged Gauss-Bonnet black hole solutions in higher dimensional ($d>4$), 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 the gyromagnetic ratio.
No takes yet. Share an insight, caveat, or question.
Kim et al. (2008) studied this question.
Synapse has enriched 5 closely related papers on similar clinical questions. Consider them for comparative context: