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SUSY Dark Matter and Colliders - whepp-9

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Focus mSUGRA Accuracies<br />

a<br />

0.0003<br />

0.05<br />

45<br />

α s (M Z )<br />

∆A 0<br />

m t 0.045<br />

a(m 0 )<br />

a(M<br />

0.00025<br />

0.04<br />

1/2 )<br />

40<br />

a(tanβ)<br />

0.035<br />

35<br />

0.0002<br />

0.03<br />

0.06<br />

0.06<br />

0.05<br />

0.05 0.025<br />

30<br />

0.00015<br />

0.04<br />

0.04<br />

0.02<br />

0.03<br />

0.03<br />

25<br />

0.02<br />

0.02<br />

0.015<br />

0.0001<br />

0.01<br />

0.01 0.01<br />

m 20<br />

0<br />

b<br />

200 300 400 0 0.005<br />

5e-05<br />

0<br />

150 200 250 300 350 400 450 100 200 300 400 500 15<br />

M 0 χ1<br />

(GeV)<br />

M 0 χ1<br />

(GeV)<br />

a<br />

∆A 0 (GeV)<br />

∆A 0 (GeV)<br />

δm t = 30 MeV might be possible at future ILC but<br />

a(m 0 ) < 0.5% looks completely unfeasible.<br />

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

B.C. Allanach – p.40/53

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