  In this work, we calculate the quasi-normal frequencies from a bumblebee
traversable wormhole. The bumblebee wormhole model is based on the bumblebee
gravity, which exhibits a spontaneous Lorentz symmetry breaking. Supporting by
the Lorentz violation parameter $\lambda$, this model allows the fulfillment of
the flare-out and energy conditions, granted non-exotic matter to the wormhole.
We analyze the parameters of bumblebee wormhole in order to obtain a
Reege-Wheeler's equation with a bell-shaped potential. We obtain the
quasi-normal modes (QNMs) via the WKB approximation method for both scalar and
gravitational perturbations. All frequencies obtained are stable and the time
domain profiles have decreasing oscillation (damping) profiles for the
bumblebee wormhole.
