Parametrized Post-Newtonian Limit of Teleparallel Dark Energy Model
  We study the post-Newtonian limit in the teleparallel equivalent of General
Relativity with a scalar field which non-minimally couples to gravity. The
metric perturbation is obtained from the vierbein field expansion with respect
to the Minkowski background. Due to the structure of the teleparallel gravity
Lagrangian, the potential of the scalar field shows no effect to the
parametrized post-Newtonian parameters, and compatible results with Solar
System observations are found.
