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Wei, Hao; Cai, Rong-Gen; Wei, H , Tsinghua Univ, Dept Phys, Beijing 100084, Peoples R China
A new model of agegraphic dark energy
发表期刊PHYSICS LETTERS B
关键词Karolyhazy Uncertainty Relation Space-time
摘要In this note, we propose a new model of agegraphic dark energy based on the Karolyhazy relation, where the time scale is chosen to be the conformal time eta of the Friedmann-Robertson-Walker (FRW) universe. We find that in the radiation-dominated epoch, the equation-of-state parameter of the new agegraphic dark energy omega(q) = - 1/3 whereas Omega(q) = n(2)a(2); in the matter-dominated epoch, omega(q) = -2/3 whereas Omega(q) = n(2)a(2)/4; eventually, the new agegraphic dark energy dominates; in the late time omega(q) --> -1 when a --> infinity, and the new agegraphic dark energy mimics a cosmological constant. In every stage, all things are consistent. The confusion in the original agegraphic dark energy model proposed in [R.G. Cai, Phys. Lett. B 657 (2007) 228, arXiv: 0707.4049 [hep-th]] disappears in this new model. Furthermore, Omega(q) << 1 is naturally satisfied in both radiation-dominated and matter-dominated epochs where a << 1. In addition, we further extend the new agegraphic dark energy model by including the interaction between the new agegraphic dark energy and background matter. In this case, we find that Wq can cross the phantom divide. (C) 2008 Elsevier B.V. All rights reserved.
2008
ISSN0370-2693
卷号660期号:3页码:113-117
学科领域Physics
收录类别SCI
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被引频次:319[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/311006/5577
专题理论物理所科研产出_SCI论文
通讯作者Wei, H , Tsinghua Univ, Dept Phys, Beijing 100084, Peoples R China
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Wei, Hao,Cai, Rong-Gen,Wei, H , Tsinghua Univ, Dept Phys, Beijing 100084, Peoples R China. A new model of agegraphic dark energy[J]. PHYSICS LETTERS B,2008,660(3):113-117.
APA Wei, Hao,Cai, Rong-Gen,&Wei, H , Tsinghua Univ, Dept Phys, Beijing 100084, Peoples R China.(2008).A new model of agegraphic dark energy.PHYSICS LETTERS B,660(3),113-117.
MLA Wei, Hao,et al."A new model of agegraphic dark energy".PHYSICS LETTERS B 660.3(2008):113-117.
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