Finslerian dipolar modulation of the CMB power spectra at scales 2 < l < 600 | |
Li, X (reprint author), Chongqing Univ, Dept Phys, Chongqing 401331, Peoples R China.; Li, X; Lin, HN; Li, X (reprint author), Chinese Acad Sci, Inst Theoret Phys, CAS Key Lab Theoret Phys, Beijing 100190, Peoples R China. | |
刊名 | EUROPEAN PHYSICAL JOURNAL C |
2017 | |
卷号 | 77期号:5页码:316 |
DOI | http://dx.doi.org/10.1140/epjc/s10052-017-4897-3 |
英文摘要 | A common explanation for the CMB power asymmetry is to introduce a dipolar modulation at the stage of inflation, where the primordial power spectrum is spatially varying. If the universe in the stage of inflation is Finslerian, and if the Finsler spacetime is non-reversible under parity flip, x -> -x, then a three dimensional spectrum which is a function of wave vector and direction is valid. In this paper, a three dimensional primordial power spectrum with preferred direction is derived in the framework of Finsler spacetime. It is found that the amplitude of dipolar modulation is related to the Finslerian parameter, which in turn is a function of wave vector. The angular correlation coefficients are presented, and the numerical results for the anisotropic correlation coefficients over the multipole range 2 < l < 600 are given. |
学科主题 | Physics |
语种 | 英语 |
内容类型 | 期刊论文 |
源URL | [http://ir.itp.ac.cn/handle/311006/22054] |
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 | Li, X (reprint author), Chongqing Univ, Dept Phys, Chongqing 401331, Peoples R China.; Li, X (reprint author), Chinese Acad Sci, Inst Theoret Phys, CAS Key Lab Theoret Phys, Beijing 100190, Peoples R China. |
推荐引用方式 GB/T 7714 | Li, X ,Li, X,Lin, HN,et al. Finslerian dipolar modulation of the CMB power spectra at scales 2 < l < 600[J]. EUROPEAN PHYSICAL JOURNAL C,2017,77(5):316. |
APA | Li, X ,Li, X,Lin, HN,&Li, X .(2017).Finslerian dipolar modulation of the CMB power spectra at scales 2 < l < 600.EUROPEAN PHYSICAL JOURNAL C,77(5),316. |
MLA | Li, X ,et al."Finslerian dipolar modulation of the CMB power spectra at scales 2 < l < 600".EUROPEAN PHYSICAL JOURNAL C 77.5(2017):316. |
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