  Prepared for Snowmass 2013 e-Proceedings. We review a testable dark matter
model outside of the standard WIMP paradigm in which the observed ratio
Omega_{dark} ~ 5 Omega_{visible} for visible and dark matter densities finds
its natural explanation as a result of their common QCD origin. Special
emphasis is placed on the observational consequences of this model and on the
detection prospects for present or planned experiments. In particular, we argue
that the relative intensities for a number of observed excesses of emission
(covering more than 11 orders of magnitude) can be explained by this model
without any new fundamental parameters as all relative intensities for these
emissions are determined by standard and well established physics.
