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Testing anisotropic Hubble expansion

delete2025-03-26
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OA
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M
Matthew Colless
K
Khaled Said
L
L. Staveley‐Smith
DOI:10.1088/1475-7516/2025/03/066delete
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摘要

摘要

En 中文
宇宙学原理断言宇宙在大尺度上的均匀性,是标准宇宙学模型的一个可检验的假设。我们通过测量来自Tully-Fisher距离估计器微分零点测量的Hubble常数H0的方向变化,来探索对各向异性膨胀的限制。我们使用全天空Cosmicflows-4目录中的Tully-Fisher数据集,拟合了H0方向变化的多种模型。最佳拟合的偶极变化在方向(& ell;, b) = (142 +/- 30 degrees,52 +/- 10 degrees)上的振幅为0.063 +/- 0.016 mag。如果这是由于各向异性膨胀引起的,那么它意味着H0有3%的变化(即ΔH0 = 2.10 +/- 0.53 km s-1 Mpc-1,若H0 = 70 km s-1 Mpc-1),显著性为3.9σ。一个包含H0偶极的模型相对于一个具有恒定H0和与标准Lambda CDM宇宙学一致的Cosmicflows-4采样体积的整体运动的模型,仅表现出微弱的偏好。然而,我们通过模拟表明,来自WALLABY和DESI调查的预期Tully-Fisher数据应该能够在5.8σ置信度下检测到1%的H0偶极各向异性,并区分它与Lambda CDM预测的这些调查体积内的典型整体流动。
Keyword:
cosmic flows
galaxy surveys

期刊

Journal of Cosmology and Astroparticle Physics 封面图
Journal of Cosmology and Astroparticle Physics
IF:
5.9
论文数:
1.3W
被引数:
4.7W

机构

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ozgrav arc ctr excellence gravitat wave discovery
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21
论文数: 10
被引数: 7
A
Australian Natl Univ
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865
论文数: 494
被引数: 212
U
Univ Western Australia
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1.0K
论文数: 720
被引数: 232
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