Gravitational bending angle with finite distances by Casimir wormholes

In this paper, we investigate the gravitational bending angle due to Casimir wormholes, which consider energy as source. Furthermore, some of these wormholes regard Generalized Uncertainty Principle (GUP) corrections energy. We use Ishihara method for Jacobi metric, allows us study light and massive test particles finite distances. Beyond uncorrected source, many GUP corrections, namely, Kempf, Mangano Mann (KMM) model, Detournay, Gabriel Spindel (DGS) so-called type II model principle. also find deflection in case receiver source are far away from lens. case, compute optical scalars: convergence shear a weak Our self-consistent iterative calculations indicate by previous paper.