Rotating black holes at large $D$ in Einstein-Gauss-Bonnet theory

Applying the large $D$ approach to the Einstein-Gauss-Bonnet theory, we construct equally rotating black hole solutions in odd dimensions. This provides the first example of the analytic solutions which describes not-slowly rotating black holes. For the next-leading order solutions in the $1\mathrm{/}D$ expansion, we discuss the physical aspects such as thermodynamics and the phase diagram.