  A new set of supersymmetric benchmark scenarios has recently been proposed in
the context of the constrained MSSM (CMSSM) with universal soft
supersymmetry-breaking masses, taking into account the constraints from LEP, $b
\to s \gamma$ and $g_\mu - 2$. These points have previously been used to
discuss the physics reaches of different accelerators. In this paper, we
discuss the prospects for discovering supersymmetric dark matter in these
scenarios. We consider direct detection through spin-independent and
spin-dependent nuclear scattering, as well as indirect detection through relic
annihilations to neutrinos, photons, and positrons. We find that several of the
benchmark scenarios offer good prospects for direct detection via
spin-independent nuclear scattering and indirect detection via muons produced
by neutrinos from relic annihilations inside the Sun, and some models offer
good prospects for detecting photons from relic annihilations in the galactic
centre.
