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原始黑洞爆炸可以解释极高能量的KM3NeT中微子事件吗?
Lua F T Airoldi1, Gustavo F S Alves1, Yuber F Perez-Gonzalez2
1Universidade de São Paulo, Instituto de Física, C.P. 66.318, 05315-970 São Paulo, Brazil.
Physical review letters
|February 16, 2026
概括
原始黑洞 (PBH) 的蒸发可以解释最近的一次高能中微子事件. 然而,由于没有预期的马射线和宇宙射线信号,这种解释被强烈否决.
科学领域:
- 天体物理学 天体物理学
- 粒子物理学 粒子物理学
- 宇宙学的宇宙学是什么?
背景情况:
- 原始黑洞 (PBHs) 是在早期宇宙中形成的假设黑洞.
- 霍金辐射预测黑洞会蒸发,发出粒子.
- 最近的一次PeV中微子事件 (KM3NeT) 可能与PBH爆炸有关.
研究的目的:
- 调查附近的PBH蒸发是否可以解释观察到的PeV中微子事件.
- 搜索与此类事件相关的多传媒信号 (马射线,宇宙射线).
- 根据观测数据来限制PBH蒸发假设.
主要方法:
- 模拟了来自附近PBH的预期马射线和宇宙射线流.
- 集成的时间依赖的观测台视野 (LHAASO,IceCube,KM3NeT).
- 将模拟信号与中微子事件前几个小时的现有观测数据进行了比较.
主要成果:
- 太阳系内的PBH源将产生可检测的马射线和宇宙射线流.
- 在KM3NeT检测之前,LHAASO应该在大约10^8小时内检测到事件.
- 冰立方体和KM3NeT应该在前24小时内检测到数百个中微子事件.
结论:
- 由于没有显著的多传递器信号,特别是来自马射线观测站的信号,这严重不利于对KM3NeT事件的PBH蒸发解释.
- 对于PBH蒸发的最小四维施瓦茨柴尔德场景与当前的观测不一致.
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