  In this paper, we obtain novel traversable, static, and spherically symmetric
wormhole solutions, derived from the effective energy density and isotropic
pressure resulting from the Casimir effect, corrected by the Generalized
Uncertainty Principle (GUP) within the framework of Loop Quantum Cosmology
(LQC). The goal is to explore the interplay between competing quantum gravity
effects and quantum vacuum phenomena in the emergence of non-trivial spacetime
structures. We examine features such as traversability, embedding diagrams,
energy conditions, curvature, and stability of the obtained solutions.
Additionally, we analyze the junction conditions required to integrate the
wormhole spacetime with an external Schwarzschild spacetime and calculate the
amount of exotic matter needed to maintain the wormhole. Finally, we evaluate
the conditions under which this latter remains visible or is hidden by the
event horizon associated with the Schwarzschild spacetime.
