we can obtain the wormhole space–time configuration through the function $f(r)$, which characterizes the embedded surface of the wormhole. This function is defined as $$\frac{df}{dr}=\pm\frac{1}{\sqrt{\frac{r}{b(r)}-1}}. \label{12}$$ Then, we can construct the profile curve and the concrete embedded diagram by solving this equation numerically. It is noteworthy that we assumed a throat radius of the wormhole of $r_0=10$ m and an EoS parameter of $\omega_{eff}=-1.074$ (see Figs. \[f4\] and \[f5\]). Following our previous studies [@39; @40; @41; @42], here we conduct a wormhole traversability analysis, which may be the most interesting and attractive consideration in wormhole physics. In general, three necessary ingredients are required for a human being in a spaceship who tries to successfully traverse a wormhole:

$\star$ The acceleration felt by the travelers should not exceed Earth’s gravitational acceleration $g_\oplus$.

$\star$ The tidal acceleration should not exceed Earth’s gravitational acceleration.

$\star$ The traversal time measured by the travelers and the observers who stay at rest at a space station should satisfy several quantitative relationships.

For the conveniences of calculations, we just derive the key formula obtained by some straightforward calculations in the following manner: $$v\leqslant r_0\sqrt{\frac{\omega_{eff}(z) g_\oplus}{\omega_{eff}(z)+1}}, \label{13}$$ where $v$ is the traversal velocity, $r_0$ is the throat radius 