  The present work deals with an interacting dark energy model in the framework
of f(T) cosmology. A cosmologically viable form of f(T) is chosen (T is the
torsion scalar in teleparallelism) in the background of flat homogeneous and
isotropic Friedmann-Robertson-Walker (FRW) space-time model of the universe.
The matter content of the universe is chosen as dust interacting with minimally
coupled scalar field. The evolution equations are reduced to an autonomous
system of ordinary differential equations by suitable transformation of
variables. The nature of critical points are analyzed by evaluating the
eigenvalues of the linearized Jacobi matrix and stable attractors are examined
from the point of view of cosmology. Finally, both classical and quantum
stability of the model have been discussed.
