太阳周期中的反质子和基本粒子:阿尔法磁谱仪的结果
M Aguilar1, G Ambrosi2, H Anderson3
1Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas (CIEMAT), 28040 Madrid, Spain.
Physical review letters
|February 21, 2025
概括
在11年的太阳周期中,宇宙反质子 (p[over ̄]) 流量变化比其他宇宙射线要小. 对于所有带电粒子,刚性光谱形状和流量变量大小之间存在一个普遍的关系.
科学领域:
- 宇宙射线物理学 宇宙射线物理学
- 太空物理学 太空物理学
- 天体物理学 天体物理学
背景情况:
- 宇宙射线,包括质子 (p),电子 (e^{-}) 和正电子 (e^{+}),在11年的太阳周期中表现出显著的时间变化.
- 反质子 (p[over ̄]) 是二次宇宙射线粒子,其流量变化为太阳调制过程提供了洞察力.
研究的目的:
- 为了分析宇宙反质子流在11年的太阳周期中的行为.
- 将反质子的时间变化与质子,电子和正子的时间变化进行比较.
- 为了研究不同带电粒子的光谱形状和流量变化大小之间的关系.
主要方法:
- 对1.1×10^{6}宇宙反质子事件的分析.
- 研究涵盖11年太阳周期的数据.
- 对刚性光谱和流量时间变化的模型独立分析.
主要成果:
- 反质子流的时间变化大小明显小于质子,电子和正电子的变化大小.
- 在反质子和质子流之间观察到歇斯底里.
- 在反质子和电子流之间发现了线性相关性.
- 在正负电荷粒子的刚性光谱形状和流量时间变化大小之间确定了通用关系.
结论:
- 与其他宇宙射线相比,反质子表现出明显的调制特性.
- 观察到的关系为了解日球中的粒子运输提供了关键数据.
- 同时测量各种带电粒子,为太阳能调制机制提供了独特的见解.
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