SUSY Dark Matter Detection at CDMS/XENON & Correlation for LHC Higgs Search 杨 金 民 理论物理研究所 arXiv: 1006.4811, in PRD(R) arXiv: 1005.0761, in JHEP With Cao, Hikasa, Wang, Yu 2010.12.14 北京
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
1. Introduction 超对称--黑格斯--暗物质 超 对 称 暗物质 黑格斯
黑格斯 LHC 超对称 暗物质
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)
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
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
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
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
2.1 Collider Constraints (1) Direct Bounds: LEP I LEP II Tevatron
(2) Precision EW Data S, T, U Rb (3) a (4) B-decays and mixings