Published reconstructions of radiocarbon in the Atlantic sector of the Southern Ocean indicate that there is amid-depth maximum in radiocarbon age during the Last Glacial Maximum (LGM). This is in contrast to the modern ocean where intense mixing between water masses results in a relatively homogenous radiocarbon profile. Ferrari et al. (2014) suggested that the extended Antarctic sea ice cover during the LGM necessitated a shallower boundary between the upper and lower branches of the meridional overturning circulation. This shoaled boundary lay above major topographic features associated with strong diapycnal mixing, isolating dense southern sourced water in the lower branch of the overturning circulation. This isolation would have allowed radiocarbon to decay and thus provides a possible explanation for the mid-depth radiocarbon age bulge. We test this hypothesis using an idealized, 2-D, residual-mean dynamicalmodel of the global overturning circulation. Concentration distributions of a decaying tracer that is advected by the simulated overturning are compared to published radiocarbon data. We find that a 600 km (similar to 5 degrees of latitude) increase in sea ice extent shoals the boundary between the upper and lower branches of the overturning circulation at 45 degrees S by 600 m and shoals the depth of North Atlantic Deep Water convection at 50 degrees N by 2500m. This change in circulation configuration alone decreases the radiocarbon content in the mid-depth South Atlantic at 45 degrees S by 40%, even without an increase in surface radiocarbon age in the source region of deep waters during the LGM.