  For the last few years the Cold Dark Matter model (ticker: CDM), has been the
dominant theory of structure formation. We briefly review the recent
advancements and predictions of the model in the field of galaxy clusters. A
new set of very high resolution simulations of galaxy clusters show that they
have (1) density profiles with central slopes very close to -1.6 and (2)
abundance of subhalos similar to the ones observed in real clusters. These
results show a remarkably small cluster to cluster variation and a weak
dependence from the particular CDM cosmology chosen (LCDM having ~40% less
substructure than SCDM). While still a speculative theory with a high
prediction/evidence ratio, subject to strong challenges from observational data
and competition from other hierarchical theories, we give CDM a rating of
``market outperform'' and of ``long term BUY''.
