  This work presents new three-dimensional traversable wormhole solutions
sourced by the Casimir density and pressures related to the quantum vacuum
fluctuations in Yang-Mills (Y-M) theory. We begin by analyzing the
noninteracting Y-M Casimir wormholes, initially considering an arbitrary state
parameter $\omega$ and determine a simple constant wormhole shape function.
Next, we introduce a new methodology for deforming the state parameter to find
well-behaved redshift functions. The wormhole can be interpreted as a
legitimate Casimir wormhole with an expected average state parameter of
$\omega=2$. Then, we investigate the wormhole curvature properties, energy
conditions, and stability. Furthermore, we discover a novel family of
traversable wormhole solutions sourced by the quantum vacuum fluctuations of
interacting Yang-Mills fields with a more complex shape function. Deforming the
effective state parameter similarly, we obtain well-behaved redshift functions
and traversable wormhole solutions. Finally, we examine the energy conditions
and stability of solutions in the interacting scenario and compare to the
noninteracting case.
