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微夸星V4641 Sgr及其与LACT作为宇宙射线超级PeVatron的深度调查
Zhen Cao1,2,3, Dmitriy Khangulyan1,2, Jiali Liu1,2
1State Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China.
LHAASO仪器检测到微准星V4641 Sgr的超高能马射线辐射,这表明它是.
科学领域:
- 高能天体物理学 高能天体物理学
- 粒子加速机制 粒子加速机制
- 宇宙射线物理学 宇宙射线物理学
背景情况:
- 微类星 V4641 Sgr 是已知的马射线发射源.
- 之前由LHAASO进行的测量表明,功率规律光谱延伸到0.8 PeV.
研究的目的:
- 调查V4641 Sgr作为一个潜在的超级PeVatron,加速超过10 PeV的粒子.
- 展示大阵列对大气切伦科夫望远镜 (LACT) 的成像能力,进行详细的源研究.
主要方法:
- 来自V4641 Sgr. 的玛射线辐射数据的分析.
- 使用计划中的LACT阵列进行模拟和可行性研究.
- 观测策略在大的顶峰角度.
主要成果:
- V4641 Sgr的辐射高达0.8 PeV,没有光谱切断,与超级PeVatron候选人一致.
- 在LACT的前四台望远镜可以限制形态特征和光谱变化.
- LACT的观测将为了解宇宙射线加速提供关键数据.
结论:
- V4641 Sgr 是一个超级PeVatron的主要候选人.
- 在研究V4641 Sgr.中的高能过程中,LACT将发挥重要作用.
- 这项研究促进了对宇宙射线起源的理解.
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