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arXiv 1609.04026hep-phhep-ex
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用$L_μ- L_τ$模型解释暗物质和$B$衰变异常

Explaining Dark Matter and $B$ Decay Anomalies with an $L_μ- L_τ$ Model

Wolfgang Altmannshofer, Stefania Gori, Stefano Profumo, Farinaldo S. Queiroz

摘要:

我们提出了一个黑暗的部门模型的基础上测量的$L_μ- L_τ$对称性,解决异常$b \rightarrow s μ^+ μ^-$衰变,并具有粒子暗物质候选人。候选的暗物质粒子是一个矢量状的狄拉克费米子,耦合到$L_μ-L_τ$对称的$Z^\prime$规范玻色子。我们计算了暗物质的热残余密度,它的对湮灭截面,以及环抑制的暗物质-核子散射截面,并将我们的预测与当前和未来的实验结果进行了比较。我们表明,考虑到从$B_s$介子振荡,暗物质直接检测,和CMB的界限后,该模型是高度预测:$B$物理异常和可行的粒子暗物质候选人,质量为$\sim (5-23)$ ~GeV,可以容纳只有在一个严格约束的参数空间区域,与未来的实验测试尖锐的预测。如果允许暗物质具有比SM轻子小的$L_μ-L_τ$电荷,则参数空间的可行区域扩大。

英文摘要:

We present a dark sector model based on gauging the $L_μ- L_τ$ symmetry that addresses anomalies in $b \rightarrow s μ^+ μ^-$ decays and that features a particle dark matter candidate. The dark matter particle candidate is a vector-like Dirac fermion coupled to the $Z^\prime$ gauge boson of the $L_μ-L_τ$ symmetry. We compute the dark matter thermal relic density, its pair-annihilation cross section, and the loop-suppressed dark matter-nucleon scattering cross section, and compare our predictions with current and future experimental results. We demonstrate that after taking into account bounds from $B_s$ meson oscillations, dark matter direct detection, and the CMB, the model is highly predictive: $B$ physics anomalies and a viable particle dark matter candidate, with a mass of $\sim (5-23)$~GeV, can be accommodated only in a tightly-constrained region of parameter space, with sharp predictions for future experimental tests. The viable region of parameter space expands if the dark matter is allowed to have $L_μ-L_τ$ charges that are smaller than those of the SM leptons.

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