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The nonextremal Kerr black holes have been considered to be holographicallydual to two-dimensional (2D) conformal field theories (CFTs). In this paper, weextend the holography to the case of an asymptotically anti--de Sitter (AdS)rotating charged black holes in $f$($T$) gravity, where $f(T) = T + \alphaT^2$, where $\alpha$ is a constant. We find that the scalar wave radialequation at the near-horizon region implies the existence of the 2D conformalsymmetries. We note that the $2\pi$ identification of the azimuthal angle$\phi$ in the black hole line element, corresponds to a spontaneous breaking ofthe conformal symmetry by left and right temperatures $T_{L}$ and $T_{R}$,respectively. We show that choosing proper central charges for the dual CFT, weproduce exactly the macroscopic Bekenstein-Hawking entropy from the microscopicCardy entropy for the dual CFT. These observations suggest that the rotatingcharged AdS black hole in $f$($T$) gravity is dual to a 2D CFT at finitetemperatures $T_{L}$ and $T_{R}$ for a specific value of mass $M$, rotational,charge, and $f$($T$) parameters, $\Omega$, $Q$, and $|\alpha|$, respectively.

Hidden conformal symmetry of the rotating charged AdS black holes in quadratic $f$($T$) gravity