  In this work we investigate the renormalization group flow of the
cosmological constant $\Lambda$ induced by the change in space-time curvature
in the electroweak vacuum. We calculate the generic magnitude resulting from
running in the standard model in a subtraction scheme that respects the
Appelquist-Carazzone decoupling theorem. Interestingly, we find in this
prescription that for a non-minimal coupling $\xi\lesssim 10^4$ the magnitude
of the generated contribution remains below the value consistent with
observations.
