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Improving Composition of Ultrahigh Energy Cosmic Rays with Ground Detector Data

PHYSICAL REVIEW D(2024)

Jozef Stefan Inst

Cited 0|Views10
Abstract
We show that the maximum shower depth distributions of Ultra-High Energy Cosmic Rays (UHECRs), as measured by fluorescence telescopes, can be augmented by building a mapping to observables collected by surface detectors. The resulting statistical improvement of such augmented dataset depends in a universal way on the strength of the correlation exhibited by the mapping. Building upon the publicly available data on "golden hybrid" events from the Pierre Auger Observatory we project possible improvements in the inferred composition of UHECRs for a range of possible mappings with varying correlation strengths.
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要点】:本文提出利用地面探测器数据改进超高能宇宙射线组成分析,通过建立与荧光望远镜测量的最大簇射深度分布之间的映射关系,实现了统计上的优化。

方法】:研究基于将地面探测器收集的可观测量与荧光望远镜测量的最大簇射深度分布相结合,构建映射关系以增强数据集的统计性能。

实验】:使用皮埃尔·奥格观测站公开的“黄金混合”事件数据,预测了不同相关性强度的映射关系对推断超高能宇宙射线组成的可能改进效果。