  The nonextremal Kerr black holes have been considered to be holographically
dual to two-dimensional (2D) conformal field theories (CFTs). In this paper, we
extend the holography to the case of an asymptotically anti--de Sitter (AdS)
rotating charged black holes in $f$($T$) gravity, where $f(T) = T + \alpha
T^2$, where $\alpha$ 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 note that the $2\pi$ identification of the azimuthal angle
$\phi$ in the black hole line element, corresponds to a spontaneous breaking of
the conformal symmetry by left and right temperatures $T_{L}$ and $T_{R}$,
respectively. 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 $T_{L}$ and $T_{R}$ for a specific value of mass $M$, rotational,
charge, and $f$($T$) parameters, $\Omega$, $Q$, and $|\alpha|$, respectively.
