  In this study we present evolving wormhole configurations in third-order
{Lovelock} gravity and investigate the possibility that these solutions satisfy
the energy conditions. Using a generalized Friedmann-Robertson-Walker
spacetime, we derive evolving wormhole geometries by considering a constraint
on the Ricci scalar. In standard cosmological models, the Ricci scalar is
independent of the radial coordinate $r$ and is only a function of time. We use
this property to introduce dynamic wormhole solutions expanding in an
inflationary cosmological background and explore the effects of higher-order
{Lovelock} terms on the dynamics of such wormholes. Our analysis shows that for
suitable third-order {Lovelock} coefficients, there are wormhole solutions that
respect the weak energy condition {(WEC)}. In addition to this, we also present
other wormhole solutions that satisfy the WEC throughout their respective
evolution.
