  This paper is devoted to study the energy conditions in F(R,T) gravity for
FRW universe with perfect fluid, where $R$ is the Ricci scalar and $T$ is the
torsion scalar. We construct the general energy conditions in this theory and
reduce them in F(R) as well as F(T) theory of gravity. Further, we assume some
viable models and investigate bounds on their constant parameters to satisfy
the energy condition inequalities. We also plot some of the cases using
present-day values of the cosmological parameters. It is interesting to mention
here that the model F(R,T)=\mu R+ \nu T satisfies the energy conditions for
different ranges of the parameters.
