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(m, n)-TYPE HOLOGRAPHIC DARK ENERGY MODELS
凌意;Ling, Y; Pan, WJ
2013
发表期刊MODERN PHYSICS LETTERS A
卷号28期号:31页码:1350128
摘要We construct (m,n)-type holographic dark energy models at a phenomenological level, which can be viewed as a generalization of agegraphic model swith the conformal-like age as the holographic characteristic size For some values of (m,n) the holographic dark energy can automatically evolve across omega = -1 into a phantom phase even with-out introducing an interaction between the dark energy and background matter.Our construction is also applicable to the holographic dark energy with generalized future event horizon as the characteristic size.Finally,we address the issue on the stability of our model and show that they are generally stable under the scalar perturbation.
关键词Dark energy theory holographic principle the stability of dark energy model
学科领域Physics
DOI10.1142/S0217732313501289
收录类别SCI
WOS记录号WOS:000324989800003
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被引频次:5[WOS]   [WOS记录]     [WOS相关记录]
文献类型期刊论文
条目标识符http://ir.ihep.ac.cn/handle/311005/224706
专题理论物理室
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凌意;Ling, Y,Pan, WJ. (m, n)-TYPE HOLOGRAPHIC DARK ENERGY MODELS[J]. MODERN PHYSICS LETTERS A,2013,28(31):1350128.
APA 凌意;Ling, Y,&Pan, WJ.(2013).(m, n)-TYPE HOLOGRAPHIC DARK ENERGY MODELS.MODERN PHYSICS LETTERS A,28(31),1350128.
MLA 凌意;Ling, Y,et al."(m, n)-TYPE HOLOGRAPHIC DARK ENERGY MODELS".MODERN PHYSICS LETTERS A 28.31(2013):1350128.
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