Phase Plane Analysis of Metric-Scalar Torsion Model for Interacting Dark
  Energy
  We study the phase space dynamics of the non-minimally coupled
Metric-Scalar-Torsion model in both Jordan and Einstein frames. We specifically
check for the existence of critical points which yield stable solutions
representing the current state of accelerated expansion of the universe fuelled
by the Dark Energy. It is found that such solutions do indeed exist, subject to
constraints on the free model parameter. In fact the evolution of the universe
at these stable critical points exactly matches the evolution given by the
cosmological solutions we found analytically in our previous work on the
subject.
