  In the present paper, we study the thermodynamics behavior of the field
equations for the generalized f(T) gravity with an arbitrary coupling between
matter and the torsion scalar. In this regard, we explore the verification of
the first law of thermodynamics at the ap- parent horizon of the
Friedmann-Robertson-Walker universe in two different perspectives namely the
non-equilibrium and equilibrium de- scriptions of thermodynamics. Furthermore,
we investigate the valid- ity of the second law of thermodynamics for both
descriptions of this scenario with assumption that the temperature of matter
inside the horizon is similar to that of horizon.
