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通过表面探测器阵列观测到的极其高能量的宇宙射线
, R U Abbasi1, M G Allen2
1Physics Department, Loyola University Chicago, Chicago, IL, USA.
科学家使用望远镜阵列实验检测到一个极其有活力的宇宙射线粒子. 它的起源指向宇宙空白, 暗示未知的天体物理源或超越标准模型的物理.
科学领域:
- 天体物理学
- 粒子物理学
- 宇宙射线物理
背景情况:
- 太空射线是来自外太空的高能量带电粒子.
- 据信最有能量的宇宙射线来自银河系外的来源.
- 检测这些罕见的高能事件需要具有大量收集面积的仪器.
研究的目的:
- 通过望远镜阵列实验检测到一个极其高能粒子.
- 分析这个检测到的粒子的能量和到达方向.
- 探索这种高能宇宙射线事件的潜在起源和影响.
主要方法:
- 使用望远镜阵列实验的表面探测器阵列进行粒子探测.
- 计算了检测到的粒子的能量.
- 确定粒子的到达方向以追踪其宇宙起源.
主要成果:
- 一个能量大约为40朱尔的极高能量的粒子被成功检测出来.
- 粒子到达的方向可以追溯到宇宙大规模结构中的空隙.
- 这些数据表明与当前天体物理模型存在潜在的差异.
结论:
- 探测到的粒子起源于一个宇宙空虚,
- 可能的解释包括星系间磁场的大量偏移.
- 其他假设涉及到一个未知的局部外星系来源或当前粒子物理学理解的差距.
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