  Morris and Thorne developed wormhole solutions in the late 1980s when they
discovered a recipe that wormholes must follow for travelers to cross them
safely. They describe exotic matter as satisfying $-p_{r} > \rho$, where
$p_{r}$ is the radial pressure and $\rho$ is the energy density of the
wormhole. This is a notable characteristic of the General Relativity Theory.
The current article discusses traversable wormhole solutions in $f(R, L,
T)=R+\alpha L+\beta T$, with $\alpha$ and $\beta$ are model parameters. The
wormhole solutions presented here satisfy the metric constraints of
traversability while remarkably avoiding the exotic matter condition,
indicating that $f(R, L, T)$ gravity wormholes can be filled with ordinary
matter. The derived solutions for the shape function of the wormhole meet the
required metric conditions. They exhibit behavior that is comparable to that of
wormholes reported in earlier references, which is also the case for our
solutions for the energy density of such objects.
