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从无线电观测中发现的10~17~17.5电子伏特的宇宙射线的大光质量组成部分
S Buitink1,2, A Corstanje2, H Falcke2,3,4,5
1Astrophysical Institute, Vrije Universiteit Brussel, Pleinlaan 2, 1050 Brussels, Belgium.
Nature
|March 4, 2016
概括
使用无线电探测研究了高能宇宙射线, 这一发现表明这些能量粒子的另一个银河系来源.
科学领域:
- 宇宙射线物理
- 天体粒子物理学
背景情况:
- 太空射线是自然界中能量最高的粒子.
- 了解它们的来源 (银河系与外银河系) 对于天体粒子物理学至关重要.
- 目前测量宇宙射线质量组成的方法有局限性.
研究的目的:
- 测量能量为1017-1018 eV的宇宙射线的质量组成.
- 研究宇宙射线的起源及其与天体物理中微子信号的关系.
- 通过无线电探测精确测量空气淋浴特性.
主要方法:
- 使用无线电探测由宇宙射线发起的空气淋浴.
- 用高精度测量了淋浴的最大大气深度 (Xmax) (16 g/cm^2的平均不确定性).
- 聚焦在能量在10^17和10^17.5 eV之间的宇宙射线.
主要成果:
- 在研究的能量范围内确定宇宙射线的混合质量组成.
- 发现光质量分数 (质子和核) 约为80%.
- 在Xmax测量中实现了高分辨率,使详细的成分分析成为可能.
结论:
- 观测到的光组成表明宇宙射线的额外的星系成分.
- 这挑战了当前对10^17.5 eV以下银河系外贡献的预期.
- 无线电探测为未来的宇宙射线组成研究提供了一个有前途的技术.
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