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OBSERVATIONAL H(z) DATA AS A COMPLEMENTARITY TO OTHER COSMOLOGICAL PROBES
Lin, Hui; Hao, Cheng; Wang, Xiao; Yuan, Qiang; Yi, Ze-Long; Zhang, Tong-Jie; Wang, Bao-Quan; Lin, H , Peking Univ, Ctr High Energy Phys, Beijing 100871, Peoples R China
2009
发表期刊MODERN PHYSICS LETTERS A
ISSN0217-7323
卷号24期号:21页码:1699-1709
摘要In this paper, we use a set of observational H(z) data (OHD) to constrain the Lambda CDM cosmology. This dataset can be derived from the differential ages of the passively evolving galaxies. Meanwhile, the A-parameter, which describes the Baryonic Acoustic Oscillation (BAO) peak, and the newly measured value of the Cosmic Microwave Background (CMB) shift parameter Rare used to present combinational constraints on the same cosmology. The combinational constraints favor an accelerating flat universe while the flat Lambda CDM cosmology is also analyzed in the same way. We obtain result compatible with that by many other independent cosmological observations. We find that the observational H(z) data set is a complementarity to other cosmological probes.
部门归属[Lin, H; Zhang, TJ] Peking Univ, Ctr High Energy Phys, Beijing 100871, Peoples R China; [Lin, H; Wang, X] Beijing Normal Univ, Sch Math Sci, Dept Stat, Beijing 100875, Peoples R China; [Hao, C] Beijing Normal Univ, Sch Math Sci, Dept Appl Math, Beijing 100875, Peoples R China; [Yuan, Q] Chinese Acad Sci, Inst High Energy Phys, Key Lab Particle Astrophys, Beijing 100049, Peoples R China; [Yi, ZL; Zhang, TJ] Beijing Normal Univ, Dept Astron, Beijing 100875, Peoples R China; [Zhang, TJ] Chinese Acad Sci, Inst Theoret Phys, Kavli Inst Theoret Phys China, KITPC ITP CAS, Beijing 100875, Peoples R China; [Wang, BQ] Dezhou Univ, Dept Phys, Dezhou 253023, Peoples R China
关键词Holographic Dark Energy Equation-of-state Gas Mass Fraction Hubble Parameter Galaxy Clusters Redshift Data Red Galaxies Constraints Ages Supernovae
学科领域Physics
资助者National Science Foundation of China[10473002, 10533010]; Scientific Research Foundation for the Returned Overseas Chinese Scholars, State Education Ministry; [2009CB24901] ; National Science Foundation of China[10473002, 10533010]; Scientific Research Foundation for the Returned Overseas Chinese Scholars, State Education Ministry; [2009CB24901] ; National Science Foundation of China[10473002, 10533010]; Scientific Research Foundation for the Returned Overseas Chinese Scholars, State Education Ministry; [2009CB24901] ; National Science Foundation of China[10473002, 10533010]; Scientific Research Foundation for the Returned Overseas Chinese Scholars, State Education Ministry; [2009CB24901]
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收录类别SCI
资助者National Science Foundation of China[10473002, 10533010]; Scientific Research Foundation for the Returned Overseas Chinese Scholars, State Education Ministry; [2009CB24901] ; National Science Foundation of China[10473002, 10533010]; Scientific Research Foundation for the Returned Overseas Chinese Scholars, State Education Ministry; [2009CB24901] ; National Science Foundation of China[10473002, 10533010]; Scientific Research Foundation for the Returned Overseas Chinese Scholars, State Education Ministry; [2009CB24901] ; National Science Foundation of China[10473002, 10533010]; Scientific Research Foundation for the Returned Overseas Chinese Scholars, State Education Ministry; [2009CB24901]
WOS记录号WOS:000268447400007
引用统计
被引频次:21[WOS]   [WOS记录]     [WOS相关记录]
文献类型期刊论文
条目标识符http://ir.itp.ac.cn/handle/311006/5279
专题理论物理所1978-2010年知识产出
通讯作者Lin, H , Peking Univ, Ctr High Energy Phys, Beijing 100871, Peoples R China
推荐引用方式
GB/T 7714
Lin, Hui,Hao, Cheng,Wang, Xiao,et al. OBSERVATIONAL H(z) DATA AS A COMPLEMENTARITY TO OTHER COSMOLOGICAL PROBES[J]. MODERN PHYSICS LETTERS A,2009,24(21):1699-1709.
APA Lin, Hui.,Hao, Cheng.,Wang, Xiao.,Yuan, Qiang.,Yi, Ze-Long.,...&Lin, H , Peking Univ, Ctr High Energy Phys, Beijing 100871, Peoples R China.(2009).OBSERVATIONAL H(z) DATA AS A COMPLEMENTARITY TO OTHER COSMOLOGICAL PROBES.MODERN PHYSICS LETTERS A,24(21),1699-1709.
MLA Lin, Hui,et al."OBSERVATIONAL H(z) DATA AS A COMPLEMENTARITY TO OTHER COSMOLOGICAL PROBES".MODERN PHYSICS LETTERS A 24.21(2009):1699-1709.
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