  In this article, we present a stationary metric ansatz to describe a rotating
traversable wormhole in the presence of the topological defect produced by a
global monopole charge. This particular rotating space-time is referred to as
the topologically charged rotating Schwarzschild-Klinkahmer wormhole. Our study
involves the analysis of geodesic motion for test particles and photon rays in
the context of this topologically charged rotating traversable wormhole. We aim
to analyze the effects of global monopole charge and other parameters on the
outcomes of this investigation. Additionally, we explore the matter-energy
distribution within this rotating wormhole, considering it as a non-vacuum
solution of Einstein's field equation. Notably, we demonstrate that the energy
density of the matter content satisfies the criteria of the weak energy
condition.
