  These lectures on non-baryonic dark matter matter are divided into two parts.
In the first part, I discuss the need for non-baryonic dark matter in light of
recent results in cosmology, and I present some of the most popular candidates
for non-baryonic dark matter. These include neutrinos, axions, neutralinos,
WIMPZILLAs, etc. In the second part, I overview several observational
techniques that can be employed to search for WIMPs (weakly interacting massive
particles) as non-baryonic dark matter. Among these techniques, I discuss the
direct detection of WIMP dark matter, and its indirect detection through
high-energy neutrinos, gamma-rays, positrons, etc.
