朱守华(Shou-huaZhu)PekingUniversity-NAOCCosmologyGroup.ppt

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1、朱守华, 北京大学物理学院,1,朱守华, 北京大学物理学院,2,Dark matter and normal matter have been wrenched apart by the tremendous collision of two large clusters of galaxies. The discovery, using NASAs Chandra X-ray Observatory and other telescopes, gives direct evidence for the existence of dark matter.,朱守华, 北京大学物理学院,3,Q:

2、Is dark matter relevant to weak scale physics? A: Likely.Q: If yes, where to insert dark matter sector? A: Most likely in Higgs sector because success of standard model of particle physics permits naturally the additional sector in Higgs sector.,朱守华, 北京大学物理学院,4,Scalar Cold Dark Matter (CDM) and Higg

3、s BosonHep-ph/0601224Hep-ph/0512055 (EPJC2006),朱守华(Shou-hua Zhu)Peking University,朱守华, 北京大学物理学院,5,I: Light (mw) new freedom could exist in Higgs sector,朱守华, 北京大学物理学院,6,Existence of CDM is well-established(?) and we know:,朱守华, 北京大学物理学院,7,Which particle is CDM?,But we dont know:,Neutralino in SUSY mod

4、els?,(SM gauge group) singlet scalar?,朱守华, 北京大学物理学院,8,Scalar cold dark matter model:,Assume:,(simplest model),朱守华, 北京大学物理学院,9,In simplest cold dark matter model:,朱守华, 北京大学物理学院,10,Relic density of CDM (standard procedure):,SM particles: ff-barWW(*)ZZ(*),朱守华, 北京大学物理学院,11,Calculation of CDM relic densi

5、ty: C. Burgess etal, NPB619(2001)709,朱守华, 北京大学物理学院,12,Allowed region,朱守华, 北京大学物理学院,13,Relic density of DM + Higgs mass lower and upper bounds =,So what?,朱守华, 北京大学物理学院,14,Background + signal describe EGRET data! by W. de Boer etal.,朱守华, 北京大学物理学院,15,Summary from W. De Boer,10 EGRET excess shows all ke

6、y features from DM annihilation:,Excess has same shape in all sky directions: everywhere it is perfectly (only?) explainable with superposition of background AND mono-energetic quarks of 50-100 GeV Results consistent with minimal SUPERSYMMETRY,Excess is TRACER OF DM, since it can explain peculiar sh

7、ape of rotation curve,Excess follows expectations from galaxy formation: cored 1/r2 profile with substructure, visible matter/DM0.02,Conventional models CANNOT explain above points SIMULTANEOUSLY,especially spectrum of gamma rays in all directions, shape of rotation curve, stability of ring of stars

8、 at 14 kpc and ring of H2 at 4 kpc.,.,Results model independent, since only KNOWN spectral shapes of signal and background used, NO model dependent calculations of absolute fluxes.,Significance 10 with 1400 indep. data points,朱守华, 北京大学物理学院,16,In other words:,Mono-energetic quarks (50-100 GeV),朱守华, 北

9、京大学物理学院,17,Invisible Higgs decay: H-SS,朱守华, 北京大学物理学院,18,Invisible Higgs decay: H-SS,朱守华, 北京大学物理学院,19,II: Detecting light invisible Higgs Boson via pp-ZH mode,朱守华, 北京大学物理学院,20,Why ZH channel?,ZH is similar to Zhu (thank you, F. Lu!)ZH tends to have SM-like couplingZ can be excellently reconstructed v

10、ia charged lepton pair,朱守华, 北京大学物理学院,21,朱守华, 北京大学物理学院,22,朱守华, 北京大学物理学院,23,朱守华, 北京大学物理学院,24,My contributions,朱守华, 北京大学物理学院,25,朱守华, 北京大学物理学院,26,朱守华, 北京大学物理学院,27,朱守华, 北京大学物理学院,28,朱守华, 北京大学物理学院,29,朱守华, 北京大学物理学院,30,朱守华, 北京大学物理学院,31,Summary,Seems everything is perfect: Higgs mass bounds can predict scalar CDM value and EGRET prefers the same mass region. The Higgs boson is light and may decay dominantly into DM.,We are listening what LHC/ILC will tell us!,朱守华, 北京大学物理学院,32,Thanks for your attention!,

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