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Growth index of DGP model and current growth rate data
Wei, Hao
2010-05-06 ; 2010-05-06
关键词HUBBLE-SPACE-TELESCOPE DIGITAL SKY SURVEY COSMOLOGICAL CONSTANT PROBLEM HIGH-REDSHIFT SUPERNOVAE PROBE WMAP OBSERVATIONS DARK ENERGY COSMIC ACCELERATION POWER SPECTRUM LEGACY SURVEY CONSTRAINTS Physics, Multidisciplinary
中文摘要Recently, some efforts focus on differentiating dark energy and modified gravity with the growth function delta(z). In the literature, it is useful to parameterize the growth rate f d ln delta/d ln a = Omega(gamma)(m) with the growth index gamma. In this Letter, we consider the general DGP model with any Omega(k). We confront the growth index of DGP model with currently available growth rate data and find that the DGP model is still consistent with it. This implies that more and better growth rate data are required to distinguish between dark energy and modified gravity. (C) 2008 Elsevier B.V. All rights reserved.
语种英语 ; 英语
出版者ELSEVIER SCIENCE BV ; AMSTERDAM ; PO BOX 211, 1000 AE AMSTERDAM, NETHERLANDS
内容类型期刊论文
源URL[http://hdl.handle.net/123456789/15431]  
专题清华大学
推荐引用方式
GB/T 7714
Wei, Hao. Growth index of DGP model and current growth rate data[J],2010, 2010.
APA Wei, Hao.(2010).Growth index of DGP model and current growth rate data..
MLA Wei, Hao."Growth index of DGP model and current growth rate data".(2010).
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