概括
在皮埃尔·奥格尔天文台检测到的高能宇宙射线与附近的活跃星系核 (AGN) 相对应. 这表明这些能量粒子起源于75兆帕塞克内的银河系外来源.
科学领域:
- 天体物理学 天体物理学
- 粒子物理学 粒子物理学
- 宇宙射线物理学 宇宙射线物理学
背景情况:
- 超高能宇宙射线 (UHECR) 的起源在天体物理学中仍然是一个重大的团.
- 了解UHECR源对于理解宇宙中的粒子加速机制至关重要.
研究的目的:
- 调查UHECR和已知天体的到达方向之间的潜在相关性.
- 测试一个同otropic分布的假设与一个异otropic,源驱动分布的UHECRs.
主要方法:
- 在Pierre Auger天文台收集了超过3.7年的宇宙射线数据的分析.
- 统计比较UHECR到达方向与特定距离内的活跃星系核 (AGN) 的位置.
主要成果:
- 在UHECRs (能量> 6 x 10 ^ 19 eV) 和附近AGN的位置 (在75Mpc以内) 之间发现了统计学上显著的相关性.
- 同位态宇宙射线分布的假设被拒绝了>99%的信心.
- 观察到的相关性支持了这些高能粒子起源于附近的银河系外来源的理论.
结论:
- 活跃的银河系核 (AGN) 或类似的空间分布的物体可能是最高能量的宇宙射线的来源.
- 这些发现表明,来自宇宙背景辐射相互作用的流量减少最小,这意味着源的接近.
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