SUSY Dark Matter and Colliders - whepp-9

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High tan β BCA, Belanger, Boudjema, Pukhov, Porod, hep-ph/0402161. Baer et al Figure 0: High tan β region. Full: SoftSusy, dotted: SPheno, dashed: SuSpect. Get annihilation into A. SUSY Dark Matter and Colliders B.C. Allanach – p.53/53
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SUSY Dark Matter and Colliders by B
Page 3 and 4:
The Supersymmetric Standard Model S
Page 5 and 6:
Broken Symmetry 3 components of the
Page 7 and 8:
WMAP Results SUSY Dark Matter and C
Page 9 and 10:
SUSY Prediction of Ωh 2 • Assume
Page 11 and 12:
Universality Reduces number of SUSY
Page 13 and 14:
Constraints on SUSY Models mSUGRA w
Page 15 and 16: Markov-Chain Monte Carlo Markov cha
Page 17 and 18: Convergence We run 9×1 000 000 poi
Page 19 and 20: Annihilation Mechanism Define stau
Page 21 and 22: 0.0015 0.03 0.08 L/GeV 0.001 0.0005
Page 23 and 24: LHC (ATLAS) SUSY Dark Matter and Co
Page 25 and 26: Collider SUSY Dark Matter Productio
Page 27 and 28: Coannihilation Slope annihilation (
Page 29 and 30: Coannihilation Theory Uncertainties
Page 31 and 32: Iterative Procedure What change in
Page 33 and 34: mSUGRA Coannihilation Uncertainties
Page 35 and 36: PmSUGRA Coannihilation a(tanβ, µ)
Page 37 and 38: PmSUGRA Dependencies ∆M (GeV) 10
Page 39 and 40: PmSUGRA Dependencies ∆M (GeV) 10
Page 41 and 42: Summary • Markov chains bring out
Page 43 and 44: Likelihood L ≡ p(d|m) is pdf of r
Page 45 and 46: Funnel Slope GeV 1400 1200 1000 800
Page 47 and 48: Funnel Theory Uncertainties Ωh 2 0
Page 49 and 50: Funnel Accuracies SM inputs and tan
Page 51 and 52: Focus Point Slope mass (GeV) 1000 9
Page 53 and 54: Focus mSUGRA Accuracies a 0.0003 0.
Page 55 and 56: LHC SUSY Measurements q l + l −
Page 57 and 58: Edge Positions endpoint S5 fit O1 f
Page 59 and 60: Fitting to SUSY Breaking Model m 1/
Page 61 and 62: Other Observables Often more compli
Page 63 and 64: Cuts Example We use ATLFAST2.16, HE
Page 65: Focus Point Figure 0: Focus point r
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SUSY Dark Matter and Colliders - whepp-9

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