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 [Formula: see text] gravity, where [Formula: see text] 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 by 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 [Formula: see text] gravity is dual to a 2D CFT at finite temperatures.