Using lower redshift, non-CMB, data to constrain the Hubble constant and other cosmological parameters

被引：71

作者：

Cao, Shulei ^{[1
]}

Ratra, Bharat ^{[1
]}

机构：

[1] Kansas State Univ, Dept Phys, 116 Cardwell Hall, Manhattan, KS 66506 USA

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 2022年 / 513卷 / 04期

关键词：

cosmological parameters; dark energy; cosmology: observations; BARYON ACOUSTIC-OSCILLATION; QUASAR X-RAY; DARK ENERGY DYNAMICS; UV FLUX MEASUREMENTS; SPECTROSCOPIC SURVEY MEASUREMENT; RADIUS-LUMINOSITY RELATION; PLANCK; 2015; CONSTRAINTS; II STARBURST GALAXY; E-ISO CORRELATION; SPATIAL CURVATURE;

D O I：

10.1093/mnras/stac1184

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We use updated Hubble parameter and baryon acoustic oscillation data, as well as other lower redshift Type Ia supernova, Mg II reverberation-measured quasar, quasar angular size, H II starburst galaxy, and Amati-correlated gamma-ray burst data, to jointly constrain cosmological parameters in six cosmological models. The joint analysis provides model-independent determinations of the Hubble constant, H-0 = 69.7 +/- 1.2 km s(-1) Mpc(-1) and the current non-relativistic matter density parameter, Omega(m0) = 0.295 +/- 0.017. These error bars are factors of 2.2 and 2.3 larger than the corresponding error bars in the flat Lambda CDM model from Planck TT,TE,EE+lowE + lensing cosmic microwave background anisotropy data. Based on the deviance information criterion (DIC), the flat Lambda CDM model is most favoured but mild dark energy dynamics and a little spatial curvature are not ruled out.

引用

页码：5686 / 5700

页数：15

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