Thermodynamics of Slowly Rotating Charged Black Holes in Anti-de Sitter Einstein–Gauss–Bonnet Gravity

By using a new approach, we demonstrate the analytic expressions for slowly rotating Gauss–Bonnet charged black hole solutions with one non-vanishing angular momentum in higher-dimensional anti-de Sitter spaces. Up to linear order of the rotating parameter a, the mass, Hawking temperature and entropy of the charged black holes get no corrections from rotation.