We analyse a high resolution simulation of the formation of a cluster's
dark-matter halo in a ΛCDM cosmology (Springel et al. 2001). The
resolution achieved allows us to map the phase-space structure in detail, and
characterize its evolution and degree of lumpiness. Scaling down the cluster
halo to a Milky-Way size halo, we probe the substructure expected in the solar
neighbourhood. Here we specifically address the relevance of such substructure
for direct detection experiments aimed at determining the nature of
dark-matter.Comment: 4 pages, 5 figures, uses dunk2001_asp.sty, to appear in "The
Dynamics, Structure and History of Galaxies: A Workshop in Honour of Prof.
Ken Freeman", (eds) G. S. Da Costa & E. M. Sadler, ASP Conf Serie