相关实验视频
Updated: Jul 11, 2026

10:42
Preparing an Isotopically Pure 229Th Ion Beam for Studies of 229mTh
Published on: May 3, 2019
概括
天文学家发现了框架拖动的潜在证据,这是一个相对论效应,旋转物质扭曲时空. 使用X射线数据观察中子星的这一发现,为极端物理学提供了新的见解.
科学领域:
- 天体物理学 天体物理学
- 一般相对论一般相对论.
背景情况:
- 中子星是大质量恒星的残余,表现出极端的物理性质.
- 框架拖动 (或Lense-Thirring效应) 是爱因斯坦广义相对论的一个预测.
研究的目的:
- 为了寻找框架拖动的观测证据.
- 为了研究快速旋转的中子星周围的时空环境.
主要方法:
- 来自NASA的罗西X射线计时探测器的X射线数据的分析.
- 研究二进制星系中三颗中子星的闪模式.
主要成果:
- 间接证据表明被检测到的框架拖动.
- 观测到的闪模式与旋转中子星扭曲时空是一致的.
结论:
- 这一发现可能是框架拖动效应的第一个明确证据.
- 需要进一步的观测来确认框架在中子星周围拖动的存在.
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