Primordial perturbation in Horava-Lifshitz cosmology
Piao, Yun-Song; Piao, YS , Chinese Acad Sci, Coll Phys Sci, Grad Sch, Beijing 100049, Peoples R China
刊名PHYSICS LETTERS B
2009
卷号681期号:1页码:1-4
ISSN号0370-2693
英文摘要Recently, Horava has proposed a renormalizable theory of gravity with critical exponent z = 3 in the UV. This proposal might imply that the scale invariant primordial perturbation can be generated in any expansion of early universe with a similar to t(n) and n > 1/3, which, in this Letter, will be confirmed by solving the motion equation of perturbation mode on super sound horizon scale for any background evolution of early universe. It is found that if enough efolding number of primordial perturbation suitable for observable universe is required, then n I needs to be satisfied, unless the scale of UV regime is quite low. However, the possible UV completeness of HL gravity helps to relax this bound. (C) 2009 Elsevier ON. All rights reserved.
学科主题Physics
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WOS记录号WOS:000271411000001
公开日期2012-08-02
内容类型期刊论文
源URL[http://ir.itp.ac.cn/handle/311006/5224]  
专题理论物理研究所_理论物理所1978-2010年知识产出
通讯作者Piao, YS , Chinese Acad Sci, Coll Phys Sci, Grad Sch, Beijing 100049, Peoples R China
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Piao, Yun-Song,Piao, YS , Chinese Acad Sci, Coll Phys Sci, Grad Sch, Beijing 100049, Peoples R China. Primordial perturbation in Horava-Lifshitz cosmology[J]. PHYSICS LETTERS B,2009,681(1):1-4.
APA Piao, Yun-Song,&Piao, YS , Chinese Acad Sci, Coll Phys Sci, Grad Sch, Beijing 100049, Peoples R China.(2009).Primordial perturbation in Horava-Lifshitz cosmology.PHYSICS LETTERS B,681(1),1-4.
MLA Piao, Yun-Song,et al."Primordial perturbation in Horava-Lifshitz cosmology".PHYSICS LETTERS B 681.1(2009):1-4.
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