  In the present work we investigate evolving wormhole configurations described
by a constant redshift function in Einstein-Cartan theory ({{\sf ECT}}). The
matter content consists of a Weyssenhoff fluid along with an anisotropic matter
which together generalize the anisotropic energy momentum tensor in general
relativity ({{\sf GR}}) in order to include the effects of intrinsic angular
momentum (spin) of particles. Using a generalized Friedmann-Robertson-Walker
({\sf FRW}) spacetime, we derive analytical evolving wormhole geometries by
assuming a particular equation of state ({{\sf EoS}}) for energy density and
pressure profiles. We introduce exact asymptotically flat and anti-de Sitter
spacetimes that admit traversable wormholes and respect energy conditions
throughout the spacetime. The rate of expansion of these evolving wormholes is
determined only by the Friedmann equation in the presence of spin effects.
