This write-up gives a rather elementary introduction into particle phy
sics aspects of the cosmological dark matter puzzle. A fairly comprehe
nsive list of possible candidates is given; in each case the productio
n mechanism and possible ways to detect them (if any) are described. I
then describe detection of the, in my view, most promising candidates
, weakly interacting massive particles or WIMPs, in slightly more deta
il. The main emphasis will be on recent developments.