  The condensation of scalar bilinear in a classically scale invariant strongly
interacting hidden sector is used to generate the electroweak scale, where the
excitation of the condensate is identified as dark matter. We formulate an
effective theory for the condensation of the scalar bilinear and find in the
self-consistent mean field approximation that the dark matter mass is of $O(1)$
TeV with the spin-independent elastic cross section off the nucleon slightly
below the LUX upper bound.
