中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
More on QCD ghost dark energy

文献类型:期刊论文

作者Cai, RG
刊名PHYSICAL REVIEW D
出版日期2012
卷号86期号:2页码:23511
关键词GALAXY REDSHIFT SURVEY DIGITAL SKY SURVEY LARGE-N-LIMIT COSMOLOGICAL CONSTANT CURRENT-ALGEBRA 2DF-SDSS LRG QSO SURVEY UNIVERSE VACUUM MODEL
ISSN号1550-7998
通讯作者Cai, RG (reprint author), Chinese Acad Sci, Inst Theoret Phys, State Key Lab Theoret Phys, POB 2735, Beijing 100190, Peoples R China.
英文摘要The difference between the vacuum energy of quantum fields in Minkowski space and in a Friedmann-Robertson-Walker universe might be related to the observed dark energy. The vacuum energy of the Veneziano ghost field introduced to solve the U(1)(A) problem in QCD is of the form H + O(H-2). Based on this, we study the dynamical evolution of a phenomenological dark energy model whose energy density is of the form alpha H + beta H-2. In this model, the universe approaches a de Sitter phase at late times. We fit the model with current observational data, including SnIa, BAO, CMB, BBN, the Hubble parameter, and the growth rate of matter perturbation. It shows that the universe begins to accelerate at redshift z similar to 0.75, and this model is consistent with current data. In particular, this model fits the data of the growth factor well as the Lambda CDM model.
学科主题Physics
收录类别SCI
资助信息NSFC [10821504, 10975168, 11035008, 11175077]; Ministry of Science and Technology of China [2010CB833004]; Chinese Academy of Sciences [KJCX2-EW-W01]; Natural Science Foundation of Liaoning province [20102124]
原文出处http://dx.doi.org/10.1103/PhysRevD.86.023511
语种英语
WOS记录号WOS:000306193200001
公开日期2014-04-25
源URL[http://ir.itp.ac.cn/handle/311006/15059]  
专题理论物理研究所_理论物理所1978-2010年知识产出
推荐引用方式
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Cai, RG. More on QCD ghost dark energy[J]. PHYSICAL REVIEW D,2012,86(2):23511.
APA Cai, RG.(2012).More on QCD ghost dark energy.PHYSICAL REVIEW D,86(2),23511.
MLA Cai, RG."More on QCD ghost dark energy".PHYSICAL REVIEW D 86.2(2012):23511.

入库方式: OAI收割

来源:理论物理研究所

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