  We study the possibility that dark matter is a baryon of a new strongly
interacting gauge theory, which was introduced in the low energy theory of
Cosmological SUSY Breaking (CSB). This particle can fit the observed dark
matter density if an appropriate cosmological asymmetry is generated. The same
mechanism can also explain the dark/baryonic matter ratio in the universe. The
mass of the dark matter particle is in the multiple TeV range, and could be as
high as 20 TeV.
