GRB 221009A来自重中微子辐射衰变的马射线?
Alexei Y Smirnov1, Andreas Trautner1
1Max-Planck-Institut für Kernphysik, Saupfercheckweg 1, 69117 Heidelberg, Germany.
Physical review letters
|July 28, 2023
概括
涉及重无菌中微子 (N) 的新奇机制解释了GRB 221009A.高能马射线的减弱. 这种无菌中微子衰变 (N→νγ) 为标准马射线衰减模型提供了替代方案.
科学领域:
- 天体物理学 天体物理学
- 粒子物理学 粒子物理学
背景情况:
- 来自马射线爆发 (GRB) 221009A的高能马射线流显示出意想不到的低衰减.
- 玛射线传播的标准模型并不能完全解释这一观测.
研究的目的:
- 提出和研究一种涉及无菌中微子的机制,以减少玛射线衰减.
- 为了解释从GRB 221009A.观察到的高能马射线事件.
主要方法:
- 考虑一个重的,大部分是无菌的中微子 (N),其质量约为0.1-1 MeV.
- 模拟GRB中无菌中微子的产生,通过在pion和kaon衰变过程中与子中微子 (νμ) 混合.
- 对无菌中微子 (N→νγ) 在它们向地球传播期间的辐射衰变进行分析.
主要成果:
- 拟议的机制将指数衰减替换为光学深度的逆衰减.
- 在特定条件下可以解释18 TeV的高能马射线事件.
- 条件包括GRB在观察到的极限附近的活性中微子流动,以及N→νγ的分支比至少为10%.
结论:
- 沉重无菌中微子的存在和辐射衰变为GRB 221009A观察到的高能玛射线的低衰减提供了可行的解释.
- 这种场景为马射线爆发物理和中微子特性提供了新的视角.
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