哈勃恒定的最大值估计来自普朗克测量的哈勃恒定
David P Knobles1, Mark F Westling2
1The Platt Institute for Cosmology and Nuclear Physics, Austin, TX 78731, USA.
Entropy (Basel, Switzerland)
|July 29, 2025
概括
一种新的最大的方法从宇宙微波背景数据中推断出哈勃常数. 这一分析表明一个值与早期和晚期宇宙测量一致,可能解决哈勃张力.
科学领域:
- 宇宙学的宇宙学是什么?
- 天体物理学 天体物理学
- 统计力学 统计力学
背景情况:
- 哈勃常数 (H0) 测量了宇宙的膨胀速度.
- 早期和后期宇宙测量H0之间的差异,称为哈勃张力,挑战了标准宇宙学模型.
- 宇宙微波背景 (CMB) 测量提供了重要的早期宇宙数据.
研究的目的:
- 应用最大 (ME) 方法来从普朗克CMB数据推断哈勃常数.
- 评估这种ME方法是否可以协调H0.0的早期和晚期宇宙测量.
- 为 H0.0 提供一个不太依赖假设的不确定性.
主要方法:
- 使用最大 (ME) 方法来推断哈勃常数.
- 采用简单的宇宙学模型进行物理洞察和统计抽样.
- 通过等分定理估计了统计温度,以定义后面的概率分布.
主要成果:
- 推断出哈勃恒定的平均值大约为67公里/秒/Mpc.
- 确定了哈勃常数的约4.4公里/秒/Mpc的保守标准偏差.
- ME推断的值符合早期宇宙 (普朗克,DESI) 和后期宇宙 (CCHP,JWST) 估计的1σ.
结论:
- 最大分析似乎不支持哈勃张力的存在.
- 通过对模型错误进行通用处理,ME方法提供了更广泛的,不太依赖假设的不确定性边界.
- 这一发现表明,可以通过一种新的统计方法来解决哈勃张力问题.
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