  In this work, the study of traversable wormholes in $f(R)$-massive gravity
with the function $f(R)=R+\alpha_{1} R^{n}$, where $\alpha_{1}$ and $n$ are
arbitrary constants, is considered. We choose the modified shape function
$b(r)$. We consider a spherically symmetric and static wormhole metric and
derive field equations. Moreover, we visualize the wormhole geometry using
embedding diagrams. Furthermore, we check the null, weak, dominant and strong
energy conditions at the wormhole throat with a radius $r_{0}$ invoking three
types of redshift functions, $\Phi={\rm
constant},\gamma_{1}/r,\,\log(1+\gamma_{2}/r)$ with $\gamma_{1}$ and
$\gamma_{2}$ are arbitrary real constants. We also compute the volume integral
quantifier to calculate the amount of the exotic matter near the constructed
wormhole throat.
