  In this work, we consider a Yukawa modification of the Casimir wormhole. With
the help of an Equation of State, we impose Zero Tidal Forces. We will examine
two different approaches: in a first approach, we will fix the form of the
shape function of the Casimir wormholes modified by a Yukawa term in three
different ways and finally a superposition of different profiles. In the second
approach, we will consider the original Casimir source modified by a Yukawa
term in three different ways and we will deduce the form of the shape function
In both the approaches the reference energy density will be that of the Casimir
source. Connection with the Absurdly Benign Traversable Wormhole are also
discussed.
