Non-Gaussian features from the inverse volume corrections in loop quantum cosmology
Cai, RG; Guo, ZK
刊名PHYSICAL REVIEW D
2012
卷号86期号:4页码:44020
关键词BLACK-HOLE ENTROPY INFLATION GRAVITY GEOMETRY AREA CMB
ISSN号1550-7998
通讯作者Li, LF (reprint author), Chinese Acad Sci, Inst Theoret Phys, State Key Lab Theoret Phys, POB 2735, Beijing 100190, Peoples R China.
英文摘要In this paper we study the non-Gaussian features of the primordial fluctuations in loop quantum cosmology with the inverse volume corrections. The detailed analysis is performed in the single field slow-roll inflationary models. However, our results reflect the universal characteristics of bispectrum in loop quantum cosmology. The main corrections to the scalar bispectrum come from two aspects: one is the modifications to the standard Bunch-Davies vacuum, and the other is the corrections to the background dependent variables, such as slow-roll parameters. Our calculations show that the loop quantum corrections make f(NL) of the inflationary models increase 0.1%. Moreover, we find that two new shapes of non-Gaussian signal arise, which we name F-1 and F-2. The former gives a unique loop quantum feature, which is less correlated with the local, equilateral, and single types, while the latter is highly correlated with the local one.
学科主题Physics
收录类别SCI
资助信息Chinese Academy of Science [2010CB832805, 2010CB833004]; National Natural Science Foundation of China [10821504, 10975168, 11175225, 11035008]
原文出处http://dx.doi.org/10.1103/PhysRevD.86.044020
语种英语
WOS记录号WOS:000307503200006
公开日期2014-04-25
内容类型期刊论文
源URL[http://ir.itp.ac.cn/handle/311006/15050]  
专题理论物理研究所_理论物理所1978-2010年知识产出
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GB/T 7714
Cai, RG,Guo, ZK. Non-Gaussian features from the inverse volume corrections in loop quantum cosmology[J]. PHYSICAL REVIEW D,2012,86(4):44020.
APA Cai, RG,&Guo, ZK.(2012).Non-Gaussian features from the inverse volume corrections in loop quantum cosmology.PHYSICAL REVIEW D,86(4),44020.
MLA Cai, RG,et al."Non-Gaussian features from the inverse volume corrections in loop quantum cosmology".PHYSICAL REVIEW D 86.4(2012):44020.
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