杨 金 民 理论物理研究所 arXiv: , in PRD(R) arXiv: , in JHEP

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1 SUSY Dark Matter Detection at CDMS/XENON & Correlation for LHC Higgs Search
杨 金 民 理论物理研究所 arXiv: , in PRD(R) arXiv: , in JHEP With Cao, Hikasa, Wang, Yu 北京

2 Outline 1 Introduction: SUSY—Dark Matter—Higgs
2 Experimental Constraints 2.1 Collider Constraints 2.2 Dark Matter Constraints 3 Direct Detection of SUSY Dark Matter 4 LHC Higgs Search 5 Conclusion

3 1. Introduction 超对称--黑格斯--暗物质 超 对 称 暗物质 黑格斯

4 黑格斯 LHC 超对称 暗物质

5 1.1 超对称 Edward Witten --standard non-standard theory – David Gross
1.1 超对称 --standard non-standard theory – David Gross Edward Witten International Conference on String Theory, Beijing, (Aug 17, 2002)

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10 SUSY Models: · · · · MSSM nMSSM Split-SUSY mSUGRA
So we see exploring SUSY is very important ! Different models give different phenomenology MSSM NMSSM nMSSM Split-SUSY mSUGRA · · · · SUSY Models: MSSM SUSY nMSSM NMSSM

11 1.2 暗物质: ---超对称的副产品 暗物质的自然、 完美的候选者 ! ~ 0 1

12 1.3 黑格斯（上帝粒子） h, H, A, H ---超对称是黑格斯的天堂 SM SUSY Will be found at LHC !
(more than 5 Higgs) (only one Higgs boson) Will be found at LHC ! h, H, A, H

13 2 Experimental Constraints on SUSY
direct bounds (LEPI, LEPII, Tevatron) EW (S,T,U) Rb B-decays muon anomalous a dark matter DM meet all constraints at 2- level

14 2.1 Collider Constraints (1) Direct Bounds: LEP I LEP II Tevatron

15 (2) Precision EW Data S, T, U Rb (3) a (4) B-decays and mixings