IHEP OpenIR  > 粒子天体物理中心
OBSERVATIONAL H(z) DATA AS A COMPLEMENTARITY TO OTHER COSMOLOGICAL PROBES
Lin, H; Hao, C; Wang, X; Yuan, Q; Yi, ZL; Zhang, TJ; Wang, BQ; Yuan Q(袁强)
2009
发表期刊MODERN PHYSICS LETTERS A
卷号24期号:21页码:1699-1709
通讯作者[Lin, Hui ; Zhang, Tong-Jie] Peking Univ, Ctr High Energy Phys, Beijing 100871, Peoples R China ; [Lin, Hui ; Wang, Xiao] Beijing Normal Univ, Sch Math Sci, Dept Stat, Beijing 100875, Peoples R China ; [Hao, Cheng] Beijing Normal Univ, Sch Math Sci, Dept Appl Math, Beijing 100875, Peoples R China ; [Yuan, Qiang] Chinese Acad Sci, Inst High Energy Phys, Key Lab Particle Astrophys, Beijing 100049, Peoples R China ; [Yi, Ze-Long ; Zhang, Tong-Jie] Beijing Normal Univ, Dept Astron, Beijing 100875, Peoples R China ; [Zhang, Tong-Jie] Chinese Acad Sci, Inst Theoret Phys, Kavli Inst Theoret Phys China, KITPC ITP CAS, Beijing 100875, Peoples R China ; [Wang, Bao-Quan] Dezhou Univ, Dept Phys, Dezhou 253023, Peoples R China
文章类型Article
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.
关键词Cosmological parameters distance scale Hubble parameter
学科领域Physics
DOI10.1142/S0217732309030217
URL查看原文
语种英语
WOS研究方向Physics
WOS类目Physics, Nuclear ; Physics, Particles & Fields ; Physics, Mathematical
WOS记录号WOS:000268447400007
引用统计
文献类型期刊论文
条目标识符http://ir.ihep.ac.cn/handle/311005/239487
专题粒子天体物理中心
实验物理中心
中国科学院高能物理研究所_中国散裂中子源
作者单位中国科学院高能物理研究所
推荐引用方式
GB/T 7714
Lin, H,Hao, C,Wang, X,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, H.,Hao, C.,Wang, X.,Yuan, Q.,Yi, ZL.,...&袁强.(2009).OBSERVATIONAL H(z) DATA AS A COMPLEMENTARITY TO OTHER COSMOLOGICAL PROBES.MODERN PHYSICS LETTERS A,24(21),1699-1709.
MLA Lin, H,et al."OBSERVATIONAL H(z) DATA AS A COMPLEMENTARITY TO OTHER COSMOLOGICAL PROBES".MODERN PHYSICS LETTERS A 24.21(2009):1699-1709.
条目包含的文件
文件名称/大小 文献类型 版本类型 开放类型 使用许可
6732.pdf(239KB)期刊论文作者接受稿限制开放CC BY-NC-SA请求全文
个性服务
推荐该条目
保存到收藏夹
查看访问统计
导出为Endnote文件
谷歌学术
谷歌学术中相似的文章
[Lin, H]的文章
[Hao, C]的文章
[Wang, X]的文章
百度学术
百度学术中相似的文章
[Lin, H]的文章
[Hao, C]的文章
[Wang, X]的文章
必应学术
必应学术中相似的文章
[Lin, H]的文章
[Hao, C]的文章
[Wang, X]的文章
相关权益政策
暂无数据
收藏/分享
所有评论 (0)
暂无评论
 

除非特别说明,本系统中所有内容都受版权保护,并保留所有权利。