Locally Rotationally Symmetric Bianchi Type-I cosmological model in
  $f(T)$ gravity: from early to Dark Energy dominated universe
  We study the locally rotational symmetry Bianchi type-I dark energy model in
the framework of $f(T)$ theory of gravity, where $T$ denotes the torsion
scalar. A viable cosmological model is undertaken and the isotropization of
this latter is checked, yielding a result that reflects the real evolution of
our universe. Moreover, still in the anisotropic optic, a more complicated
$f(T)$ model is obtained from the cosmological reconstruction scheme and the
analysis shows that the universe is more anisotropic at the beginning if the
terms of higher order in $T$ are not considered. This means that the non-linear
model should be favoured by observational data.
