  In this article, we look into geodesics in the Schwarzschild-Anti-de Sitter
metric in (3+1) spacetime dimensions. We investigate the class of marginally
bound geodesics (timelike and null), while comparing their behavior with the
normal Schwarzschild metric. Using $\textit{Mathematica}$, we calculate the
shear and rotation tensors, along with other components of the Raychaudhuri
equation in this metric and we argue that marginally bound timelike geodesics,
in the equatorial plane, always have a turning point, while their null
analogues have at least one family of geodesics that are unbound. We also
present associated plots for the geodesics and geodesic congruences, in the
equatorial plane.
