  The presence of exotic matter for the existence of the wormhole geometry has
been an unavoidable problem in GR. In recent studies researchers have tried to
deal with this issue using modified gravity theories where the WH geometry is
explained by the extra curvature terms and NEC's are not violated signifying
the standard matter in the WH geometry. In the present article we are trying to
find the solutions of traversable wormholes with normal matter in the throat
within the framework of symmetric teleparallel gravity $f(Q)$ where $Q$ is the
non metricity scalar which defines the gravitational interaction. We will
examine the wormhole geometries for three forms of function $f(Q)$. First is
the linear form $f(Q)=\alpha Q$, second a non -linear form $f(Q)=\alpha Q^2 +
\beta$ and third one a more general quadratic form $f(Q)=\alpha Q^2 + \beta Q +
\gamma$ with $\alpha$, $\beta$ and $\gamma$ being the constants. For all the
three cases the shape function is taken as $b(r) =
{\frac{r_{0}\ln(r+1)}{\ln({r_0}+1)}}$ where $r_0$ is the throat radius. A
special variable redshift function is considered for the discussion. All the
energy conditions are then examined for the existence and the stability of the
wormhole geometry.
