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arXiv 2201.02531hep-phhep-exhep-th
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根据最新LHC数据与暗物质约束重新审视pMSSM中的胶微子质量极限

Revisiting the gluino mass limits in the pMSSM in the light of the latest LHC data and Dark Matter constraints

Abhi Mukherjee, Saurabh Niyogi, Sujoy Poddar

AI总结:

本文在pMSSM框架下重新分析LHC第二轮运行数据对胶微子质量的限制,发现其高度依赖标量夸克质量层级和较轻电弱微子组成,并进一步结合暗物质遗迹密度与直接探测约束,指出少量道联合分析可给出更可靠的质量极限。

摘要:

本文的目的是通过分析大型强子对撞机(LHC)实验的第二轮运行数据,检验对胶微子质量所施加的严格约束的模型依赖性。这些数据使用了基于若干特设的超粒子谱的特定简化模型,而这些谱即使在相当通用的唯象最小超对称标准模型(pMSSM)中也无法实现。我们首先重新审视了ATLAS合作组利用$1l + jets + \met$数据对胶微子质量施加的限制。我们表明,在pMSSM情景下,$M_{\widetilde{g}}-M_{\widetildeχ^0_1}$平面中的排除区域敏感地依赖于左右标量夸克之间的质量层级以及较轻电弱微子的组成,并在较小程度上依赖于其他参数。最重要的是,对于希格斯微子型较轻电弱微子(最轻超对称粒子LSP除外),来自该道对胶微子质量的限制实际上消失了。然而,如果此类模型面对ATLAS的$jets + \met$数据,则会重新获得相当强的限制。因此,在pMSSM中,涉及少量道的分析可能提供更可靠的质量极限。我们还对我们所研究的模型中的中性微子暗物质(DM)约束进行了详细分析,并发现在相当大的LSP质量范围内,来自WMAP/PLANCK数据的遗迹密度约束得到满足,并且LSP-胶微子共湮灭在遗迹密度产生中起着重要作用。我们还检验了本文所研究模型与直接暗物质探测以及LHC约束的同时兼容性。

英文摘要:

The purpose of this paper is to examine the model dependence of the stringent constraints on the gluino mass obtained from the Large Hadron Collider (LHC) experiments by analyzing the Run II data using specific simplified models based on several ad hoc sparticle spectra which cannot be realized even in the fairly generic pMSSM models. We first revisit the bounds on the gluino mass placed by the ATLAS collaboration using the $1l + jets + \met$ data. We show that the exclusion region in the $M_{\widetilde{g}}-M_{\widetildeχ^0_1}$ plane in the pMSSM scenario sensitively depends on the mass hierarchy between the left and right squarks and composition of the lighter electroweakinos and, to a lesser extent, other parameters. Most importantly, for higgsino type lighter electroweakinos (except for the LSP), the bound on the gluino mass from this channel practically disappears. However, if such models are confronted by the ATLAS $jets + \met$ data, fairly strong limits are regained. Thus in the pMSSM an analysis involving a small number of channels may provide more reliable mass limits. We have also performed detailed analyses on neutralino dark matter (DM) constraints in the models we have studied and have found that for a significant range of LSP masses, the relic density constraints from the WMAP/PLANCK data are satisfied and LSP-gluino coannihilation plays an important role in relic density production. We have also checked the simultaneous compatibility of the models studied here with the direct DM detection, and the LHC constraints.

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