  In this paper, we investigate new exact and analytic solutions of the
Einstein Maxwell field equations describing Casimir wormholes with and without
the effect of the Generalized Uncertainty Principle (GUP). We consider a
specific type of the GUP relations and study three specific models of the
redshift function along with two different EoS of state. Here we obtain a class
of asymptotically flat Casimir wormhole solutions with and without GUP
corrections under the effect of electric charge. Furthermore we check the null,
weak, strong and dominant energy conditions at the wormhole throat of radius,
and show at the wormhole throat that the classical energy conditions are
violated by some arbitrary small quantity. We also examine the wormhole
geometry with semiclassical corrections by using embedding diagrams. We use the
volume integral quantifier to quantify the amount of the exotic matter near the
wormhole throat. Additionally, we investigate exotic fluid near WH throat using
the so called exoticity parameter and discuss the speed of sound.
