论文标题

自然超对称:状态和前景

Natural Supersymmetry: Status and Prospects

论文作者

Tata, Xerxes

论文摘要

如果超对称性(SUSY)在弱尺度上轻轻折断,则可以稳定Higgs扇区,这使许多作者探索了它在粒子物理学中的作用。人们普遍认为,一旦在高能量碰撞中探测了TEV量表后,超级零件人会揭示自己。 LHC的实验尚未显示出直接生产超级零部队的任何迹象,也没有针对标准模型以外的任何其他物理学的迹象。这使一些作者质疑弱小的苏西是否在稳定希格斯行业中起着作用。我们表明,只有最小粒子含量的SUSY模型很可能与数据一致,并且同时可以稳定HIGGS扇区,如果通常认为模型参数是独立的,则可以适当地关联。我们认为,鉴于我们不了解Susy Breaking的潜在机制,忽略这种可能性将为时过早。我们提倡使用Electroweak量表$ \ dewew $来确定是否可能是由低调的理论引起的,即使存在上述参数相关性,也可能引起。我们发现所有此类模型都包含Light Higgsinos,这导致了寻找Susy的新策略的可能性。我们讨论了这些模型对LHC搜索的现象学意义及其发光度和能量升级以及将来的电子峰壳相结合者。我们得出的结论是,自然苏西(Natural Susy)定义为30微调的零件,不会在27〜TEV运行的$ pp $对撞机和15〜AB $^{ - 1} $的集成光度或以电子峰值碰撞器与600 gev的中心能量的电子碰撞器相撞。

The realization that supersymmetry (SUSY), if softly broken at the weak scale, can stabilize the Higgs sector led many authors to explore the role it may play in particle physics. It was widely anticipated that superpartners would reveal themselves once the TeV scale was probed in high energy collisions. Experiments at the LHC have not yet revealed any sign for direct production of superpartners, or for any other physics beyond the Standard Model. This has led to some authors to question whether weak scale SUSY has a role to play in stabilizing the Higgs sector. We show that SUSY models with just the minimal particle content may well be consistent with data and simultaneously serve to stabilize the Higgs sector, if model parameters generally regarded as independent turn out to be appropriately correlated. In our view, it would be premature to ignore this possibility, given that we do not understand the underlying mechanism of SUSY breaking. We advocate using the electroweak scale quantity, $\delew$, to determine whether a given SUSY spectrum might arise from a theory with low fine-tuning, even when the parameters correlations mentioned above are present. We find that all such models contain light higgsinos and that this leads to the possibility of new strategies for searching for SUSY. We discuss phenomenological implications of these models for SUSY searches at the LHC and its luminosity and energy upgrades, as well as at future electron-positron colliders. We conclude that natural SUSY, defined as no worse than a part in 30 fine-tuning, will not escape detection at a $pp$ collider operating at 27~TeV and an integrated luminosity of 15~ab$^{-1}$, or at an electron-positron collider with a centre-of-mass energy of 600~GeV.

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