银河系中没有大质量黑洞
Przemek Mróz1, Andrzej Udalski2, Michał K Szymański2
1Astronomical Observatory, University of Warsaw, Warsaw, Poland. pmroz@astrouw.edu.pl.
Nature
|June 24, 2024
概括
原始黑洞是一个潜在的暗物质候选者. 一个20年的微镜调查没有发现这些物体的证据, 排除它们作为主要的暗物质组成部分.
科学领域:
- 天体物理学
- 宇宙学
- 引力波天文学
背景情况:
- 引力波探测器显示大质量黑洞与银河系观测不一致.
- 这些黑洞的起源是有争议的,原始黑洞 (PBH) 被提出为一种可能性.
- 如果PBH存在于星系光环中, 它们可能构成了暗物质的重要组成部分, 并解释了合并速度.
研究的目的:
- 寻找长时间的引力微透镜事件表明PBHs.
- 在特定的质量范围内限制PBH的丰度.
主要方法:
- 分析了大麦哲伦星云中近8000万颗恒星的20年光曲线数据.
- 搜索持续时间超过一年的微镜头事件.
主要成果:
- 没有发现超过一年的微透镜事件.
- 较短的探测事件可以归因于已知的恒星群.
- 紧的物体在1.8×10-4M和6.3M之间不能构成超过1%的暗物质.
- 紧的物体在1.3×10-5M和860M之间不能构成超过10%的暗物质.
结论:
- 这项研究排除了PBH在研究的质量范围内作为暗物质的重要组成部分.
- PBHs不能同时解释观测到的重力波事件和显著的暗物质部分.
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