  The present paper examines the validity of energy bounds in a modified theory
of gravity involving non-minimal coupling of torsion scalar and perfect fluid
matter. In this respect, we formulate the general inequalities of energy
conditions by assuming the flat FRW universe. For the application of these
bounds, we particularly focus on two specific models that are recently proposed
in literature and also choose the power law cosmology. We find the feasible
constraints on the involved free parameters and evaluate their possible ranges
graphically for the consistency of these energy bounds.
