SUSY Dark Matter and Colliders - whepp-9
SUSY Dark Matter and Colliders - whepp-9
SUSY Dark Matter and Colliders - whepp-9
Create successful ePaper yourself
Turn your PDF publications into a flip-book with our unique Google optimized e-Paper software.
PmSUGRA Dependencies<br />
∆M (GeV)<br />
10<br />
1<br />
0.4<br />
∆M<br />
9<br />
cos2θ τ 0.99 0.35<br />
8<br />
0.98<br />
7<br />
0.3<br />
6<br />
0.97<br />
0.25<br />
5<br />
0.96<br />
4<br />
0.2<br />
0.95<br />
3<br />
0.15<br />
0.94<br />
2<br />
1<br />
0.93<br />
0.1<br />
0<br />
0.92 0.05<br />
100 150 200 250 300 350 400 450<br />
m~ (GeV) τ<br />
cos2θ τ<br />
-<br />
∆cos2θ τ required, a(M)<br />
∆cos2θ τ<br />
- required<br />
δM required<br />
a(M χ )<br />
1.3<br />
1.2<br />
1.1<br />
0.9<br />
0.8<br />
0.7<br />
0.6<br />
100 150 200 250 300 350 400 450<br />
m~<br />
τ (GeV)<br />
1<br />
δM required (GeV)<br />
LHS: plots of quantities along mSUGRA slope. Below<br />
∆M = 1.78 GeV, no two-body stau decay. LC studies<br />
indicate ∆M > 5 GeV is OK.<br />
<strong>SUSY</strong> <strong>Dark</strong> <strong>Matter</strong> <strong>and</strong> <strong>Colliders</strong><br />
B.C. Allanach – p.30/53