论文标题
辐射校正以停止灭绝灭绝glu和轻夸克
Radiative corrections to stop-antistop annihilation into gluons and light quarks
论文作者
论文摘要
我们提出了完整的单环SUSY-QCD校正,以在最小的超对称标准模型中停止抗抗晶状和光夸克,包括sommerfeld增强效应,从传入的颗粒之间的多个振奋物进行交换。这些校正很重要,因为停止(CO)an灭成为对场景的遗物密度的主要贡献,而中性诺和停止之间的质量差异很小,而停止的质量差异很小,而这受到当前LHC搜索的限制,并且与观察到125 GEV Smlike smlike smlike smlike higgs boson的约束。我们讨论了我们的一环,实际排放和重新召集计算的重要技术细节,我们特别关注红外差异的取消以及偶极形式的相关应用在大量的初始标量中。校正已在暗物质精密工具DM@nlo中实现,该工具使我们能够以数字研究这些校正对歼灭横截面的影响。我们发现,对于所选的参考方案,主要校正来自Sommerfeld效应,并且纯NLO校正低于3%。这些辐射校正的包含仍然足够大,可以将遗物密度降低10%以上,并将宇宙学首选的参数区域移动几个GEV,相对于标准的Micromegas结果。因此,如果将实验误差视为理论值的上限和下限,则必须包含这些校正。
We present the full one-loop SUSY-QCD corrections to stop-antistop annihilation into gluons and light quarks within the Minimal Supersymmetric Standard Model including Sommerfeld enhancement effects from the exchange of multiple gluons between the incoming particles. These corrections are important as stop (co)annihilation becomes the dominant contribution to the relic density for scenarios with a small mass difference between the neutralino and the stop which are less constrained by current LHC searches and consistent with the observation of a 125 GeV SM-like Higgs boson. We discuss important technical details of our one-loop, real emission, and resummation calculations where we pay particular attention to the cancellation of infrared divergences and the associated application of the dipole formalism for massive initial scalars. The corrections have been implemented in the dark matter precision tool DM@NLO which allows us to study numerically the impact of these corrections on the annihilation cross section. We find that for the chosen reference scenario the dominant correction comes from the Sommerfeld effect and that the pure NLO correction is below 3%. The inclusion of these radiative corrections is still large enough to decrease the relic density by more than 10% and shift the cosmologically preferred parameter region by a few GeV relative to the standard MicrOMEGAs result. Therefore, the inclusion of these corrections is mandatory if the experimental errors are taken as upper and lower bounds of the theory value.