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modelingthewmaplargeangleanomaliesasaneffectofalocaldensityinhomogeneity
He Liping; Guo Quan
2010
Source Publicationresearchinastronomyandastrophysics
ISSN1674-4527
Volume000Issue:002Pages:116
AbstractWe investigate large-angle scale temperature anisotropy in the Cosmic Microwave Background (CMB) with the Wilkinson Microwave Anisotropy Probe (WMAP) data and model the large-angle anomalies as the effect of the CMB quadrupole anisotropies caused by the local density inhomogeneities. The quadrupole caused by the local density inhomogeneities is different from the special relativity kinematic quadrupole. If the observer inhabits a strong inhomogeneous region, the lo- cal quadrupole should not be neglected. We calculate such local quadrupole under the assumption that there is a huge density fluctuation field in the direction (284°, 74°), where the density fluctuation is 10-3, and its center is - 112 h-1 Mpc away from us. After removing such mock signals from WMAP data, the power in the quadrupole, C2, increases from the range (200 - 260 μK2) to - 1000 μK2. The quantity S, which is used to estimate the alignment between the quadrupole and the octopole, decreases from (0.7 - 0.74) to (0.31 - 0.37), while the model predicts that C2 = 1071.5 μK2, and S = 0.412. So our local density inhomogeneity model can, in part, explain the WMAP low-l anomalies.
Language英语
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/47866
Collection中国科学院国家天文台
Affiliation中国科学院国家天文台
First Author AffilicationNational Astronomical Observatories, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
He Liping,Guo Quan. modelingthewmaplargeangleanomaliesasaneffectofalocaldensityinhomogeneity[J]. researchinastronomyandastrophysics,2010,000(002):116.
APA He Liping,&Guo Quan.(2010).modelingthewmaplargeangleanomaliesasaneffectofalocaldensityinhomogeneity.researchinastronomyandastrophysics,000(002),116.
MLA He Liping,et al."modelingthewmaplargeangleanomaliesasaneffectofalocaldensityinhomogeneity".researchinastronomyandastrophysics 000.002(2010):116.
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