中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Finsler space-time can explain both parity asymmetry and power deficit seen in CMB temperature anisotropies

文献类型:期刊论文

作者Zhao D(赵东); Rath,PK; Chang Z(常哲); Chang, Z; Rath, PK; Sang, Y; Zhao, D; Zhou, Y; Zhou Y(周勇); Sang Y(桑语)
刊名MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
出版日期2018
卷号479期号:1页码:1327-1331
ISSN号0035-8711
关键词cosmic background radiation cosmological parameters
DOI10.1093/mnras/sty1689
文献子类Article
英文摘要We propose a framework of Finsler space-time to explain the observed parity asymmetry and the power deficit in the low-l (2 <= l <= 29) multipole range of cosmic microwave background (CMB) temperature anisotropies. In the 3 + 1 dimensional space-time, the three-dimensional space is described by a Randers-Finsler space, which is spatially irreversible, inducing the parity asymmetry in the CMB angular power spectrum. We estimate the constraints on the two parameters introduced by Finsler space-time via analysing the low-l angular power spectrum in PLANCK 2015 CMB temperature data. We see that the low-l. power suppression in the CMB temperature anisotropies can also be resolved in this scenario. Our study shows that the two low-l. anomalies, i.e. parity asymmetry and power deficit, may have a common origin.
电子版国际标准刊号1365-2966
WOS关键词SPECTRA ; PLANCK ; WMAP ; RELATIVITY ; CURVATURE ; CONSTANT ; SYMMETRY ; MAPS ; SKY
WOS研究方向Astronomy & Astrophysics
语种英语
WOS记录号WOS:000441295800098
源URL[http://ir.ihep.ac.cn/handle/311005/286212]  
专题高能物理研究所_理论物理室
通讯作者Zhao D(赵东)
作者单位中国科学院高能物理研究所
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Zhao D,Rath,PK,Chang Z,et al. Finsler space-time can explain both parity asymmetry and power deficit seen in CMB temperature anisotropies[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2018,479(1):1327-1331.
APA 赵东.,Rath,PK.,常哲.,Chang, Z.,Rath, PK.,...&桑语.(2018).Finsler space-time can explain both parity asymmetry and power deficit seen in CMB temperature anisotropies.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,479(1),1327-1331.
MLA 赵东,et al."Finsler space-time can explain both parity asymmetry and power deficit seen in CMB temperature anisotropies".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 479.1(2018):1327-1331.

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来源:高能物理研究所

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