Holography for rotating black holes in f(T) gravity

We extend the black hole holography to the case of an asymptotically anti-de Sitter (AdS) rotating charged black holes in f(T) = T + alpha T-2 gravity, where a is a constant. We find that the scalar wave radial equation at the near-horizon region implies the existence of the 2D conformal symmetries. We show that choosing proper central charges for the dual CFT, we produce exactly the macroscopic Bekenstein-Hawking entropy from the microscopic Cardy entropy for the dual CFT. These observations suggest that the rotating charged AdS black hole in f(T) gravity is dual to a 2D CFT at finite temperatures.