Abstract
In this paper, we study slowly rotating black hole solutions in Lovelock gravity (n = 3). These solutions are obtained in uncharged and charged cases, respectively. Up to the linear order of the rotating parameter a, the entropy and gyromagnetic ratio of black holes keep invariant after introducing the Gauss-Bonnet and third order Lovelock interactions.
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Yue, R., Zou, D., Yu, T. et al. Slowly rotating charged black holes in anti-de Sitter third order Lovelock gravity. Gen Relativ Gravit 43, 2103–2114 (2011). https://doi.org/10.1007/s10714-011-1164-z
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DOI: https://doi.org/10.1007/s10714-011-1164-z