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Improvement in fast particle track reconstruction with robust statistics

机译:强大的统计功能可改善快速粒子轨道重建

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摘要

The IceCube project has transformed 1 km~3 of deep natural Antarctic ice into a Cherenkov detector. Muon neutrinos are detected and their direction is inferred by mapping the light produced by the secondary muon track inside the volume instrumented with photomultipliers. Reconstructing the muon track from the observed light is challenging due to noise, light scattering in the ice medium, and the possibility of simultaneously having multiple muons inside the detector, resulting from the large flux of cosmic ray muons. This paper describes work on two problems: (1) the track reconstruction problem, in which, given a set of observations, the goal is to recover the track of a muon; and (2) the coincident event problem, which is to determine how many muons are active in the detector during a time window. Rather than solving these problems by developing more complex physical models that are applied at later stages of the analysis, our approach is to augment the detector's early reconstruction with data filters and robust statistical techniques. These can be implemented at the level of on-line reconstruction and, therefore, improve all subsequent reconstructions. Using the metric of median angular resolution, a standard metric for track reconstruction, we improve the accuracy in the initial reconstruction direction by 13%. We also present improvements in measuring the number of muons in coincident events: we can accurately determine the number of muons 98% of the time.
机译:IceCube项目已将1 km〜3的深层自然南极冰转变为Cherenkov探测器。检测μ子中微子,并通过映射由装有光电倍增管的体积内的次级μ子轨道产生的光来推断其中微子的方向。由于噪声,冰介质中的光散射以及由于宇宙射线μ子的大通量而在检测器内部同时具有多个μ子的可能性,因此从观察到的光中重建μ子轨道非常具有挑战性。本文描述了两个问题的工作:(1)轨道重建问题,其中给出一组观察结果,目标是恢复μ子的轨道; (2)同步事件问题,即确定在一个时间窗口内检测器中有多少个μ子处于活动状态。我们的方法不是通过开发在分析的后续阶段应用的更复杂的物理模型来解决这些问题,而是采用数据过滤器和强大的统计技术来增强探测器的早期重建。这些可以在在线重建的级别上实现,因此可以改善所有后续重建。使用中位角分辨率的度量(轨道重建的标准度量),我们将初始重建方向的精度提高了13%。我们还提出了在同时发生的事件中测量μ子数的改进:我们可以在98%的时间内准确确定μ子数。

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