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Probing Non-holomorphic MSSM via Precision Constraints, Dark Matter and LHC Data

机译:通过精确约束,暗物质和LHC数据探测非全统称MSSM

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93.1 Non-holomorphic MSSM The Higgs Boson @ 125 GeV requires large radiative corrections demanding heavier stops, or effectively a large trilinear stop mixing soft parameter. A large region of pMSSM parameter space associated with large tan β is ruled out via Br(B→X_s + Y). On the other hand, in a single component dark matter (DM) setup, a well motivated higgsino DM of the right relic density leads to enhanced Electro-Weak Fine Tuning (EWFT). Moreover, (g - 2)_μ limits require either a light lighter chargino or light smuons, hardly allowed by LHC data in generic scenarios. With identical particle content as that of MSSM Non-holomorphic MSSM (NHSSM) can successfully cover these issues by including NH soft terms.
机译:93.1非全统称MSSM HIGGS BOSON @ 125 GEV需要大的辐射校正要求较重的停止,或有效地是大型三线性停止混合软参数。通过BR(B→X_S + Y)排除了与大TANβ相关联的PMSSM参数空间的大区域。另一方面,在单个组件的暗物质(DM)设置中,右依赖密度的良好动机的Higgsino DM导致增强的电弱微调(EWFT)。此外,(G-2)_μ极限需要轻较轻的Chargino或灯泡,几乎不能通过通用场景中的LHC数据允许。具有相同的颗粒含量,因为MSSM非全象MSSM(NHSSM)可以通过包括NH软术语成功覆盖这些问题。

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