具有阿尔科克-帕奇尼斯基效应的宇宙空间曲率
Luca Amendola1, Marco Marinucci2,3, Miguel Quartin4,5,6
1Institute of Theoretical Physics, Philosophenweg 16, Heidelberg University, 69120, Heidelberg, Germany.
Physical review letters
|March 28, 2025
概括
我们提出了一种新的方法来测量宇宙的空间曲率,使用星系聚类和Alcock-Paczyński效应. 这种独立于模型的方法提供了强大的宇宙学见解.
科学领域:
- 宇宙学的宇宙学是什么?
- 天体物理学 天体物理学
- 银河系的进化 银河系的进化
背景情况:
- 了解宇宙的几何是限制宇宙学模型的关键.
- 以前的方法通常依赖于关于宇宙学参数或星系属性的特定假设.
研究的目的:
- 提出一种新的,与模型无关的方法来测量宇宙空间曲率.
- 为了利用Alcock-Paczyński效应在大规模星系聚类中进行这一测量.
主要方法:
- 利用由阿尔科克-帕奇辛斯基效应引起的统计同otropy 的偏差.
- 分析大规模星系聚类数据,特别是结合功率光谱和双光谱测量.
- 使用来自暗能量光谱仪器 (DESI) 和欧几里得星系调查的数据.
主要成果:
- 拟议的方法独立于标准的,统治者,时钟,功率谱形状,星系偏差,引力理论,暗能量模型和背景宇宙学.
- 联合DESI-欧几里得星系调查可以在1σ C.L.时达到ΔΩk0=0.057的精度. 如果红移z<2.2,则为红移z<2.
结论:
- 这种基于Alcock-Paczyński的方法为宇宙曲率测量提供了一个强大且高度独立于模型的工具.
- 未来的星系调查可以通过这种技术显著限制宇宙的空间曲率.
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