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SUSY Dark Matter and Colliders - whepp-9

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Fitting to <strong>SUSY</strong> Breaking<br />

Model<br />

m 1/2 [GeV]<br />

480<br />

460<br />

440<br />

420<br />

400<br />

380<br />

Softsusy<br />

Spheno<br />

Suspect<br />

Isajet<br />

360<br />

200 300 400 500 600<br />

m 0 [GeV]<br />

tan β<br />

2.4<br />

2.2<br />

2.<br />

1.8<br />

1.6<br />

Spheno<br />

Softsusy<br />

Suspect<br />

Isajet<br />

200 300 400 500 600<br />

m 0 [GeV]<br />

• Experimenters pick a <strong>SUSY</strong> breaking point<br />

• They derive observables <strong>and</strong> errors after detector<br />

simulation<br />

• We fit<br />

this “data” with our codes<br />

BCA, S Kraml, W Porod, JHEP 0303 (2003) 016<br />

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

B.C. Allanach – p.46/53

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