作为超高能宇宙射线源的二进制共振
Jonas P Pereira1,2, Carlos H Coimbra-Araújo3,4, Rita C Dos Anjos3,4,5,6
1Núcleo de Astrofísica e Cosmologia (Cosmo-Ufes) & Departamento de Física, Universidade Federal do Espírito Santo, Vitória, 29075-910, ES, Brazil.
Physical review letters
|March 15, 2024
概括
强磁场中涉及黑洞 (BHs) 的二进制凝聚能可以产生超高能宇宙射线 (UHECRs). 在引力波旁检测UHECR可以限制中子星 (NS) 和BH参数.
科学领域:
- 天体物理学 天体物理学
- 引力波天文学 引力波天文学
- 粒子物理学 粒子物理学
背景情况:
- 黑洞 (BHs) 和中子星 (NSs) 的二元凝聚是引力波 (GWs) 的主要来源.
- 理论上,强磁场存在于像BHs和NSs这样的紧物体周围.
研究的目的:
- 研究二进制凝聚的潜力,以产生超高能宇宙射线 (UHECRs).
- 探索BH事件视界附近的带电粒子可以达到超高能量的条件.
主要方法:
- 在聚合BHs周围强磁场中的粒子碰撞的理论建模.
- 在BH-NS和BH-BH二进制系统中分析粒子质量中心能量.
主要成果:
- 嵌入磁场 (B 10^10 G) 的BH可以将带电粒子加速到超高能量 (10^18 eV).
- 这种现象在BH-NS二进制文件中很可能很常见,并且可能在带电的BH-BH二进制文件中具有积累盘.
- 在系统合并之前,这种高能碰撞的数量可以从几到数百万不等.
结论:
- 二进制凝聚,特别是BH-NS系统,可能是UHECR的重要来源.
- 同时检测UHECR和GW可以为NS和BH参数提供新的约束.
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