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首页> 外文期刊>The journal of high energy physics >Phenomenology in supersymmetric neutrinophilic Higgs model with sneutrino dark matter
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Phenomenology in supersymmetric neutrinophilic Higgs model with sneutrino dark matter

机译:Sneutrino暗物质的超对称中性粒细胞HIGGS模型的现象学

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摘要

A bstract We study a supersymmetric neutrinophilic Higgs model with large neutrino Yukawa couplings where neutrinos are Dirac particles and the lightest right-handed (RH) sneutrino is the lightest supersymmetric particle (LSP) as a dark matter candidate. Neutrinophilic Higgs bosons need to be rather heavy by the precise determination of the muon decay width and dark radiation constraints for large Yukawa couplings. From the Large Hadron Collider constraints, neutrinophilic Higgsino mass need to be heavier than several hundred GeV or close to the RH sneutrino LSP mass. The latter case is interesting because the muon anomalous magnetic dipole moment can be explained with a relatively large lightest neutrino mass, if RH sneutrino mixings are appropriately fine tuned in order to avoid stringent lepton flavor violation constraints. Dark matter is explained by asymmetric RH sneutrino dark matter in the favoured region by the muon anomalous magnetic dipole moment. In other regions, RH sneutrino could be an usual WIMP dark matter.
机译:Bstract我们研究了具有大中微核育川联轴器的超对称中嗜型HIGGS模型,其中Nultinos是Dirac颗粒,最轻的右手(RH)Sneutrino是作为暗物质候选的最轻的超对称颗粒(LSP)。中源性HIGGS玻色子需要通过精确测定大型Yukawa联轴器的μ子衰减宽度和暗辐射约束的精确测定。从大型强子撞机约束中,中性嗜中性嗜睡素物质需要比数百GEV或靠近Rh Sneutin LSP质量。后一种情况是有趣的,因为如果rh Sneutin混合被适当微调,可以用相对较大的浅中子核来解释μ子异常磁性偶极偶像,以避免严格的Lepton风味违规约束。通过μ子异常磁性偶极矩在有利区域中的不对称Rh sneutrino暗物质解释了暗物质。在其他地区,Rh Sneutrino可能是一个通常的黑猩猩暗物质。

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