Cubic anomalies in the Wilkinson Microwave Anisotropy Probe

被引:88
作者
Land, K [1 ]
Magueijo, J [1 ]
机构
[1] Univ London Imperial Coll Sci Technol & Med, Theoret Phys Grp, London SW7 2BZ, England
关键词
cosmic microwave background;
D O I
10.1111/j.1365-2966.2005.08707.x
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We perform a frequentist analysis of the bispectrum of the Wilkinson Microwave Anisotropy Probe first-year data. We find clear signal domination up to 200, with overall consistency with Gaussianity, except for the following features. There is a flat patch (i.e. a low 2 region) in the same-l components of the bispectrum spanning the range l=32-62; this may be interpreted as ruling out Gaussianity at the 99.6 per cent confidence level. There is also an asymmetry between the north and south inter-l bispectrum components at the 99 per cent confidence level. The preferred asymmetry axis correlates well with the (l,b) = (57, 10) direction quoted in the literature for asymmetries in the power spectrum and three-point correlation function. However, our analysis of the quadrupole (its bispectrum and principal axes) fails to make contact with previously claimed anomalies.
引用
收藏
页码:994 / 1002
页数:9
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