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SUSY Dark Matter and Colliders - whepp-9

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Summary<br />

• Markov chains bring out the multi-dimensionality<br />

of the space: is a lot less constrained than in 2d<br />

• Still, current data is constraining<br />

• LHC could produce copious amounts of <strong>SUSY</strong><br />

dark matter<br />

• Want to measure σ in order to predict Ωh 2 <strong>and</strong><br />

test cosmological assumptions<br />

• 10% accuracy will require ILC+LHC data<br />

• Can control many uncertainties by measuring<br />

additional quantities: Γ A , m˜τ − M χ<br />

0<br />

1<br />

, . . .<br />

• Non mSUGRA case could well be easier.<br />

• Have not discussed direct detection yet<br />

<strong>SUSY</strong> <strong>Dark</strong> <strong>Matter</strong> <strong>and</strong> <strong>Colliders</strong><br />

B.C. Allanach – p.32/53

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