Hubble Tension: The Evidence of New Physics

被引：106
作者：
Hu, Jian-Ping [1 ]
Wang, Fa-Yin [1 ,2 ]
机构：
[1] Nanjing Univ, Sch Astron & Space Sci, Nanjing 210093, Peoples R China
[2] Nanjing Univ, Key Lab Modern Astron & Astrophys, Minist Educ, Nanjing 210093, Peoples R China
来源：
UNIVERSE | 2023年 / 9卷 / 02期
基金：
中国博士后科学基金; 中国国家自然科学基金;
关键词：
cosmological parameters; cosmology; Hubble constant; GAMMA-RAY BURSTS; INTERACTING DARK ENERGY; PROBE WMAP OBSERVATIONS; MG II QUASARS; X-RAY; MASER EMISSION; LAMBDA-CDM; OBSERVATIONAL CONSTRAINTS; COSMOLOGICAL CONSTRAINTS; LUMINOSITY RELATION;
D O I：
10.3390/universe9020094
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The lambda CDM model provides a good fit to most astronomical observations but harbors large areas of phenomenology and ignorance. With the improvements in the precision and number of observations, discrepancies between key cosmological parameters of this model have emerged. Among them, the most notable tension is the 4 sigma to 6 sigma deviation between the Hubble constant (H0) estimations measured by the local distance ladder and the cosmic microwave background (CMB) measurement. In this review, we revisit the H0 tension based on the latest research and sort out evidence from solutions to this tension that might imply new physics beyond the lambda CDM model. The evidence leans more towards modifying the late-time universe.
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页数：35
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