论文标题
部分可观测时空混沌系统的无模型预测
Standard model anomalies: Lepton flavour non-universality, g-2 and W-mass
论文作者
论文摘要
我们批判性地分析了结果的体系,这些结果暗示了LHCB实验可能违反Lepton普遍性的新物理学的存在,以$μ/e $ $ r_ $ r_ {k {k} $和$ r_ {k^*} $对$ g-2 $ g-2 $ lepton anomalies。分析从理论上深入研究$μ/e $ $比率$ r_ {k} $和$ r_ {k^*} $以及该过程$ b_s \rightarrowμ^+μ^ - $。在这里,我们考虑了复杂的威尔逊系数的影响,并对它们的虚构和真实部分产生了限制。然后,我们与实验结果进行了全面的比较。我们表明,通过安装一个威尔逊系数,当仅包括HADRONES不敏感可观察值时,与标准模型的偏差为$4.7σ$级别,而当包括Hadronic敏感的情况下,它将增加到$6.1σ$。当打开所有相关的Wilson系数并将HADRONIC敏感和不敏感的数据结合到拟合度中时,与标准模型的偏差为$7.2σ$,如果我们假设$ r_k $和$ r_k $和$ r_ {k^{\ ast}}的中心值为$4.9σ$级别。我们进一步估算了其他未指责的其他因素,并表明它们的包容性仍然需要新的物理学来适合数据。然后,我们介绍了$ G-2 $ Lepton异常以及最近的$ W $质量结果。考虑了可以解释与标准模型的差异的不同理论模型。在我们工作的最后部分,我们估计了LHCB(来自LHC Run3)和Belle II的即将到来的数据的影响,何时将累积$ 5〜AB^{ - 1} $。
We critically analyze the body of results that hints to the existence of New Physics from possible violations of lepton universality observed by the LHCb experiment in the $μ/e$ ratios $R_{K}$ and $R_{K^*}$ to the $g-2$ lepton anomalies. The analysis begins with a theoretical, in depth, study of the $μ/e$ ratios $R_{K}$ and $R_{K^*}$ as well as the process $B_s \rightarrow μ^+ μ^-$. Here we consider the impact of complex Wilson coefficients and derive constraints on their imaginary and real parts. We then move to a comprehensive comparison with experimental results. We show that, by fitting a single Wilson coefficient, the deviations from the Standard Model are at the $4.7σ$ level when including only the hadronic insensitive observables while it increases to $6.1σ$ when including also the hadronic sensitive ones. When switching on all relevant Wilson coefficients and combining both hadronic sensitive and insensitive data into the fit, the deviation from the Standard Model peaks at $7.2σ$ and decreases at the $4.9σ$ level if we assume that the central values of $R_K$ and $R_{K^{\ast}}$ are taken to be unity. We further estimate other unaccounted for SM contributions and show that their inclusion still requires New Physics to fit the data. We then introduce the $g-2$ lepton anomalies as well as the most recent $W$-mass results. Different theoretical models are considered that can explain the discrepancies from the Standard Model. In the final part of our work we estimate the impact of the forthcoming data from LHCb (coming from LHC Run3) and Belle II, when it will have accumulated about $5~ab^{-1}$.