Cosmological mplications of different baryon acoustic oscillation data

doi:http://dx.doi.org/10.1007/s11433-016-0486-6

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	Cosmological mplications of different baryon acoustic oscillation data
	Wang, S; Hu, YZ; Li, M; Wang, S (reprint author), Sun Yat Sen Univ, Sch Phys & Astron, Zhuhai 519082, Peoples R China.
刊名	SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY
	2017
卷号	60 期号:4 页码:40411
关键词	Cosmology Dark Energy Observations Cosmological Parameters
DOI	http://dx.doi.org/10.1007/s11433-016-0486-6
英文摘要	In this work, we explore the cosmological implications of different baryon acoustic oscillation (BAO) data, including the BAO data extracted by using the spherically averaged one-dimensional galaxy clustering (GC) statistics (hereafter BAO1) and the BAO data obtained by using the anisotropic two-dimensional GC statistics (hereafter BAO2). To make a comparison, we also take into account the case without BAO data (hereafter NO BAO). Firstly, making use of these BAO data, as well as the SNLS3 type Ia supernovae sample and the Planck distance priors data, we give the cosmological constraints of the ?CDM, the wCDM, and the Chevallier-Polarski-Linder (CPL) model. Then, we discuss the impacts of different BAO data on cosmological consquences, including its effects on parameter space, equation of state (EoS), figure of merit (FoM), deceleration-acceleration transition redshift, Hubble parameter H(z), deceleration parameter q(z), statefinder hierarchy S(1)3(z), S(1)4(z) and cosmic age t(z). We find that: (1) NO BAO data always give a smallest fractional matter density ?m0, a largest fractional curvature density ?k0 and a largest Hubble constant h; in contrast, BAO1 data always give a largest ?m0, a smallest ?k0 and a smallest h. (2) For the wCDM and the CPL model, NO BAO data always give a largest EoS w; in contrast, BAO2 data always give a smallest w. (3) Compared with the case of BAO1, BAO2 data always give a slightly larger FoM, and thus can give a cosmological constraint with a slightly better accuracy. (4) The impacts of different BAO data on the cosmic evolution and the comic age are very small, and can not be distinguished by using various dark energy diagnosis and the cosmic age data.
学科主题	Physics
语种	英语
内容类型	期刊论文
源URL	[http://ir.itp.ac.cn/handle/311006/22096]
专题	理论物理研究所_理论物理所1978-2010年知识产出
通讯作者	Wang, S (reprint author), Sun Yat Sen Univ, Sch Phys & Astron, Zhuhai 519082, Peoples R China.
推荐引用方式 GB/T 7714	Wang, S,Hu, YZ,Li, M,et al. Cosmological mplications of different baryon acoustic oscillation data[J]. SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY,2017,60(4):40411.
APA	Wang, S,Hu, YZ,Li, M,&Wang, S .(2017).Cosmological mplications of different baryon acoustic oscillation data.SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY,60(4),40411.
MLA	Wang, S,et al."Cosmological mplications of different baryon acoustic oscillation data".SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY 60.4(2017):40411.