We present an implementation of the CMS-EXO-17-015 analysis in the MadAnalysis 5 framework. The analysis targets a search for dark matter in a channel in which it originates from the production and decay of a pair of scalar leptoquarks. This search considers a luminosity [Formula: see text] of CMS data collected in 2016 and 2017, in proton-proton collisions at a center-of-mass energy of 13 TeV. The final state signature is comprised of one isolated highly-energetic muon, one jet with a large transverse momentum and a significant amount of missing transverse energy. We validate our implementation in MadAnalysis 5 for a specific leptoquark/dark matter benchmark scenario. In particular, we compare predictions obtained with MadAnalysis 5 with the official CMS results for various kinematical distributions relevant for the CMS-EXO-17-015 analysis, as well as detailed cut-flow tables. We have found an excellent agreement.

中文翻译：

---

在 MadAnalysis 5 框架中实施 CMS-EXO-17-015 分析（轻夸克和暗物质，带有一个 μ 子、一个射流和缺少横向能量；77.4 fb-1）

我们在 MadAnalysis 5 框架中展示了 CMS-EXO-17-015 分析的实现。该分析的目标是在一个通道中寻找暗物质，该通道源于一对标量轻夸克的产生和衰变。该搜索考虑了 2016 年和 2017 年收集的 CMS 数据的光度 [公式：见正文]，质子 - 质子碰撞的质心能量为 13 TeV。最终状态特征包括一个孤立的高能 μ 子、一个具有大横向动量的喷流和大量缺失的横向能量。我们针对特定的轻夸克/暗物质基准场景验证了我们在 MadAnalysis 5 中的实现。特别是，我们将使用 MadAnalysis 5 获得的预测与 CMS-EXO-17-015 分析相关的各种运动分布的官方 CMS 结果进行比较，以及详细的切割流表。我们找到了一个很好的协议。