In this brief review of recent theoretical developments associated with the
search for dark matter I describe the following: why baryons are now ruled out
as dark matter candidates; SUSY WIMPS and signatures in the MSSM and NMSSM why
claimed indirect signatures are probably not WIMP related, why axions may be of
new interest, how WIMP detection might tell us about the galactic halo, and how
theorists are preparing to avoid the next generation of experimental
constraints.Comment: 6 pages, Invited Review talk, Neutrino 2006. To appear in Proceeding