用微分引力闪测量纳米赫兹引力波的宇宙膨胀
1University of Toronto, University of Toronto, University of Toronto, Canadian Institute for Theoretical Astrophysics, 60 St. George Street, Toronto, ON M5S 3H8, Canada; Department of Physics, 60 St. George Street, Toronto, ON M5S 1A7, Canada; and Dunlap Institute for Astronomy & Astrophysics, AB 120-50 St. George Street, Toronto, ON M5S 3H4, Canada.
Physical review letters
|April 18, 2025
概括
脉冲计时阵列 (PTA) 可以检测超长波长的引力波. 银河系盘引力透镜导致波干扰,使得精确的宇宙膨胀测量和红移距离对推断成为可能.
科学领域:
- 天文学和天体物理学
- 宇宙学的宇宙学是什么?
- 引力波物理 引力波物理
背景情况:
- 脉冲星计时阵列 (PTA) 最近使得超长波长引力波的检测成为可能.
- 引力波为基础科学研究提供了新的机会.
研究的目的:
- 研究引力透镜对PTA检测到的超长波长引力波的影响.
- 探索使用这些透镜效应用于宇宙学测量的潜力.
主要方法:
- 分析银河系盘对PTA源的波透镜效应.
- 建模由此产生的干扰或闪模式.
- 与前景红移信息相关联的镜头图案.
主要成果:
- 预计每个PTA源都会被众多银河系盘的衍射透镜所覆盖.
- 这种透镜诱导引力波应变中的适度调制 (Δh/h∼10^{-3}λ_{1 pc}^{-1}).
- 由此产生的闪模式可以通过连贯的PTA来解决.
结论:
- 对PTA源的衍射透镜提供了一种用于精确测量宇宙膨胀的新方法.
- 未来的PTA实验具有足够的信号对噪声,可以从单个来源推断出数百个红移距离对.
- 这种技术为了解宇宙膨胀历史开辟了新的途径.
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