  The problems of simple elementary weakly interacting massive particles
(WIMPs) appeal to extend the physical basis for nonbaryonic dark matter. Such
extension involves more sophisticated dark matter candidates from physics
beyond the Standard Model (BSM) of elementary particles. We discuss several
models of dark matter, predicting new colored, hyper-colored or techni-colored
particles and their accelerator and non-accelerator probes. The nontrivial
properties of the proposed dark matter candidates can shed new light on the
dark matter physics. They provide interesting solutions for the puzzles of
direct and indirect dark matter search.
