Collider, direct and indirect detection of susy dark matter

The minimal supergravity model (mSUGRA) was established by Pran Nath and others over 20 years ago, and serves as the paradigm model for supersymmetry phenomenology. A standard prediction is that the lightest neutralino comprises the bulk of dark matter in the universe. I outline expectations for indirect detection of neutralino dark matter via neutralino annihilation in the solar core, and in the galactic halo. These rates are compared to direct detection rates and also to prospects for supersymmetry detection at the Fermilab Tevatron, CERN LHC and a 0.5-1 TeV linear e(+)e(-) collider.