  In the present work we investigate wormhole structures and the energy
conditions supporting them, 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}) to include spin effects. Assuming that the radial
pressure and energy density obey a linear equation of state, we introduce exact
asymptotically flat and anti-de-Sitter spacetimes that admit traversable
wormholes and respect energy conditions. Such wormhole solutions are studied in
detail for two specific forms for the redshift function, namely a constant
redshift function and the one with power law dependency.
