SUSY Dark Matter and Colliders - whepp-9
SUSY Dark Matter and Colliders - whepp-9
SUSY Dark Matter and Colliders - whepp-9
You also want an ePaper? Increase the reach of your titles
YUMPU automatically turns print PDFs into web optimized ePapers that Google loves.
mSUGRA Coannihilation<br />
Uncertainties<br />
a<br />
0.16<br />
0.14<br />
0.12<br />
0.1<br />
0.08<br />
0.06<br />
0.04<br />
0.02<br />
a(M 1/2 )<br />
a(m 0 )<br />
∆A 0<br />
-<br />
a(tanβ)<br />
180<br />
160<br />
140<br />
120<br />
100<br />
80<br />
0<br />
60<br />
100 150 200 250 300 350 400 450<br />
m~ (GeV)<br />
τ<br />
∆A 0<br />
- (GeV)<br />
a(m 0 ) ≈ a(M 1/2 ) comes from the sensitivity to<br />
exp[−(m˜τ − M χ<br />
0<br />
1<br />
)]<br />
<strong>SUSY</strong> <strong>Dark</strong> <strong>Matter</strong> <strong>and</strong> <strong>Colliders</strong><br />
B.C. Allanach – p.28/53