超出10^{20} eV的宇宙射线的同变性有利于它们的重质量组成
R U Abbasi1, Y Abe2, T Abu-Zayyad1,3
1Department of Physics, Loyola University Chicago, Chicago, Illinois 60660, USA.
Physical review letters
|August 9, 2024
概括
我们使用天空分布数据估计了超高能宇宙射线 (UHECR) 的组成. 结果表明,在非常高的能量下重的组成,在较低的能量下可能更轻,这取决于银河系外磁场.
科学领域:
- 天体物理学 天体物理学
- 粒子物理学 粒子物理学
背景情况:
- 超高能宇宙射线 (UHECR) 是能量超过1018 eV的粒子.
- 了解UHECR的组成对于识别它们的来源和传播机制至关重要.
研究的目的:
- 估计10eEV以上的能量时注入的UHECR的质量组成.
- 研究银河系外磁场 (EGMF) 对UHECR组成估计的影响.
主要方法:
- 分析了望远镜阵列表面探测器观察到的UHECR事件的能源依赖的天空分布.
- 将UHECR事件分布与局部宇宙的大规模结构进行比较.
- 模拟不同强度的银河系外和银河系磁场的场景.
主要成果:
- 一个相对较重的注射组合被推断为大约10 EeV,变得更轻到100 EeV.
- 在能量超过100 EeV的UHECR组合被发现是非常重的,即使有强大的EGMF.
- 如果存在强大的EGMF,则在较低的能量下可能会产生更轻的组成;银河系磁场的不确定性具有主导作用.
结论:
- 注射的UHECR成分显示出显著的能源依赖.
- 银河系外磁场在解释UHECR组成方面起着至关重要的作用,特别是在较低的能量下.
- 观察到的UHECR很可能源自不同元素组成的混合来源.
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