Using Pantheon and DES supernova, baryon acoustic oscillation, and Hubble parameter data to constrain the Hubble constant, dark energy dynamics, and spatial curvature

被引:85
作者
Cao, Shulei [1 ]
Ryan, Joseph [1 ]
Ratra, Bharat [1 ]
机构
[1] Kansas State Univ, Dept Phys, 116 Cardwell Hall, Manhattan, KS 66502 USA
关键词
cosmological parameters; cosmology: observations; dark energy; PLANCK; 2015; CONSTRAINTS; DECELERATION-ACCELERATION TRANSITION; OBSERVATIONAL CONSTRAINTS; INDEPENDENT DETERMINATION; REDSHIFT; MODELS; FLAT;
D O I
10.1093/mnras/stab942
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We use Pantheon Type Ia supernova (SN Ia) apparent magnitude, DES-3 yr binned SN Ia apparent magnitude, Hubble parameter, and baryon acoustic oscillation measurements to constrain six spatially flat and non-flat cosmological models. These sets of data provide mutually consistent cosmological constraints in the six cosmological models we study. A joint analysis of these data sets provides model-independent estimates of the Hubble constant, H-0 = 68.8 +/- 1.8 kms(-1) Mpc(-1), and the non-relativistic matter density parameter, Omega(m0) = 0.294 +/- 0.020. Although the joint constraints prefer mild dark energy dynamics and a little spatial curvature, they do not rule out dark energy being a cosmological constant and flat spatial hypersurfaces. We also add quasar angular size and H II starburst galaxy measurements to the combined data set and find more restrictive constraints.
引用
收藏
页码:300 / 310
页数:11
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