KM3NeT/ARCA探测器包含顶点的高能中微子事件分析。

K. Pikounis, E. Tzamariudaki, F. C. Collaboration
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引用次数: 0

摘要

KM3NeT是位于地中海深处的下一代中微子探测器的研究基础设施。ARCA探测器目前正在建设中,它被优化用于搜索来自天体物理源的中微子,以及测量漫射天体物理通量。冰立方对地外中微子的明确探测导致了对高能天体物理中微子通量的首次测量。海水的特性使我们能够以极好的角度分辨率测量中微子的方向,无论是轨迹还是级联事件。本文将一种区分轨道和阵雨事件的方法和一种从开始的轨道类事件中拒绝大气介子背景的方法结合在一起进行分析。分析了KM3NeT/ARCA利用探测器体积内重构顶点的事件发现弥漫性天体物理中微子通量的潜力。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Analysis of vertex-contained high energy neutrino events for the KM3NeT/ARCA detector.
KM3NeT is a research infrastructure housing the next generation neutrino detectors in the depths of the Mediterranean Sea. The ARCA detector, which is currently under construction, is optimized for searches for neutrinos from astrophysical sources as well as measurements of the diffuse astrophysical flux. The unambiguous detection of neutrinos of extraterrestrial origin by IceCube has led to the first measurement of a high energy astrophysical neutrino flux. The properties of sea water allow for a measurement of the neutrino direction with an excellent angular resolution for both track and cascade events. Here a method to differentiate track and shower events and a method to reject the atmospheric muon background from starting track-like events are combined in one analysis. The analysis on the discovery potential of KM3NeT/ARCA for a diffuse astrophysical neutrino flux using events with the reconstructed vertex inside the detector volume will be presented.
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