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首页> 外文期刊>International journal of modern physics, D. Gravitation, astrophysics, cosmology >Scalar dark matter and standard model with four generations
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Scalar dark matter and standard model with four generations

机译:标量暗物质和四代标准模型

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This talk is based on the previous paper [X. G. He et al., Phys. Rev. D 82 (2010) 035016]. We consider a scalar dark-matter model, the SM4+D, consisting of the standard model with four generations (SM4) and a real gauge-singlet scalar called darkon, D, as the weakly interacting massive particle (WIMP) dark-matter (DM) candidate. We explore constraints on the darkon sector of the SM4+D from WIMP DM direct-search experiments, and from the decay of a B meson into a kaon plus missing energy. Since the darkon-Higgs interaction may give rise to considerable enhancement of the Higgs invisible decay mode, the existence of the darkon could lead to the weakening or evasion of some of the restrictions on the Higgs mass in the presence of fourth-generation quarks. In addition, it can affect the flavor-changing decays of these new heavy quarks into a lighter quark and the Higgs boson, as the Higgs may subsequently decay invisibly. Therefore, we also study these flavor-changing neutral transitions involving the darkon, as well as the corresponding top-quark decay t → cDD, some of which may be observable at the Tevatron or LHC and thus provide additional tests for the SM4+D.
机译:本演讲基于先前的论文[X. G.He等,《物理学报》。 Rev.D 82(2010)035016]。我们将标量暗物质模型SM4 + D视为具有弱相互作用的大质量粒子(WIMP)暗物质,该模型由具有四代(SM4)的标准模型和称为暗子D的实数标量单标量组成。 DM)候选人。我们从WIMP DM直接搜索实验以及从B介子衰变为kaon以及缺少能量的过程中探索了SM4 + D暗区的约束。由于达克顿与希格斯的相互作用可能会大大提高希格斯的无形衰变模式,因此在存在第四代夸克的情况下,达克顿的存在可能导致对希格斯质量的某些限制的减弱或逃逸。此外,它还会影响这些新的重夸克变成淡的夸克和希格斯玻色子的变味腐烂,因为希格斯随后可能会无形地腐烂。因此,我们还研究了涉及Darkon的这些改变风味的中性过渡以及相应的顶夸克衰变t→cDD,其中一些在Tevatron或LHC上可以观察到,因此为SM4 + D提供了额外的测试。

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