Impacts of different SNLS3 light-curve fitters on cosmological consequences of interacting dark energy models

doi:http://dx.doi.org/10.1051/0004-6361/201526946

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	Impacts of different SNLS3 light-curve fitters on cosmological consequences of interacting dark energy models
	Wang, S (reprint author), Sun Yat Sen Univ, Sch Astron & Space Sci, Guangzhou 510275, Guangdong, Peoples R China.; Li, M; Hu, YZ; Li, N; Wang, S
刊名	ASTRONOMY & ASTROPHYSICS
	2016
卷号	592 页码:A101
关键词	Dark Energy Cosmology:Observations Cosmological Parameters
DOI	http://dx.doi.org/10.1051/0004-6361/201526946
英文摘要	We explore the cosmological consequences of interacting dark energy (IDE) models using the SNLS3 supernova samples. In particular, we focus on the impacts of different SNLS3 light-curve fitters (LCF; referred to in this paper as SALT2, SiFTO and combined sample). Firstly, making use of the three SNLS3 data sets, as well as the Planck distance priors data and the galaxy clustering data, we constrain the parameter spaces of three IDE models. Then, we study the cosmic evolutions of Hubble parameter H(z), deceleration diagram q(z), statefinder hierarchy S-3((1))(z) and S-4((1))(z), and check whether or not these dark energy diagnosis can distinguish the differences among the results of different SNLS3 LCF. Finally, we perform a high redshift cosmic age test using three old high redshift objects (OHRO), and explore the fate of the Universe. We find that the impacts of different SNLS3 LCF are rather small, and can not be distinguished using H(z), q(z), S-3((1))(z),S-4((1))(z)and the age data of OHRO. In addition, we infer, from the current observations, how far we are from a cosmic doomsday in the worst case, and find that the combined sample always gives the largest 2 sigma lower limit of the time interval between "big rip" and today, while the results given by the SALT2 and the SiFTO sample are similar. These conclusions are insensitive to a specific form of dark sector interaction. Our method can be used to distinguish the differences among various cosmological observations.
学科主题	Astronomy & Astrophysics
语种	英语
内容类型	期刊论文
源URL	[http://ir.itp.ac.cn/handle/311006/21571]
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 Astron & Space Sci, Guangzhou 510275, Guangdong, Peoples R China.
推荐引用方式 GB/T 7714	Wang, S ,Li, M,Hu, YZ,et al. Impacts of different SNLS3 light-curve fitters on cosmological consequences of interacting dark energy models[J]. ASTRONOMY & ASTROPHYSICS,2016,592:A101.
APA	Wang, S ,Li, M,Hu, YZ,Li, N,&Wang, S.(2016).Impacts of different SNLS3 light-curve fitters on cosmological consequences of interacting dark energy models.ASTRONOMY & ASTROPHYSICS,592,A101.
MLA	Wang, S ,et al."Impacts of different SNLS3 light-curve fitters on cosmological consequences of interacting dark energy models".ASTRONOMY & ASTROPHYSICS 592(2016):A101.