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幻影和大TeV环球脉冲星因宇宙射线传播而抵消
Yiwei Bao1,2,3,4, Gwenael Giacinti1,2,5, Ruo-Yu Liu3,4
1Shanghai Jiao Tong University, Tsung-Dao Lee Institute, Shanghai 201210, China.
Physical review letters
|November 21, 2025
概括
脉冲星附近的不对称宇宙射线扩散可以解释多个马射线源和大偏移,挑战天体物理学中对称传播的假设.
科学领域:
- 天体物理学 天体物理学
- 高能天体物理学 高能天体物理学
- 宇宙射线物理学 宇宙射线物理学
背景情况:
- 扩展的马射线源通常以对称的宇宙射线扩散为模型.
- 最近的观测显示了脉冲星附近的多个来源,以及TeV光环中心体和它们的母脉冲星之间的显著偏移.
- 对称扩散的假设可能是一种过度简单化.
研究的目的:
- 研究不对称的宇宙射线传播对扩展马射线源的形态的影响.
- 为了解释观测到的多个来源和脉冲星附近的大偏移.
- 为了提供一种替代的解释,使检测到的来源感到困惑,而无需援引新的物理.
主要方法:
- 宇宙射线传播的理论建模.
- 来自脉冲星加速器的不对称扩散模拟.
- 模型预测与TeV光环观测数据的比较.
主要成果:
- 不对称的宇宙射线传播自然会产生多个TeV源,而不是单个对称的.
- 这种机制解释了TeV光环中心体和它们的母脉冲星之间观察到的显著偏移.
- 在不需要额外的隐形加速器的情况下,解释了几个以前令人困惑的来源.
结论:
- 宇宙射线扩散并不总是对称的,特别是在像脉冲星这样的加速器附近.
- 非对称传播是一种可行的机制,可以解释复杂的马射线源分布.
- 这一发现简化了观察到的TeV光环及其母脉冲星的解释.
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