  In the present manuscript, we study traversable wormhole solutions in the
background of extended symmetric teleparallel gravity with matter coupling.
With the anisotropic matter distribution we probe the wormhole geometry for two
different gravity models. Primarily, we consider the linear model $ f(Q,T) =Q +
2 \, \xi \,T$. Firstly, we presume a logarithmic form of shape function and
analyze the scenario for different redshift functions. Secondly, for a specific
form of energy density, we derive a shape function and note its satisfying
behavior. Next, for the non-linear model $f(Q,T) = Q + \alpha ,Q^2 + \beta ,T$
and a specific shape function we examine the wormhole solution. Further, with
the aid of embedding diagrams, we interpreted the geometry of wormhole models.
Finally, we conclude results.
