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The microwave sky and the local Rees-Sciama effect
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DOI：10.1111/j.1745-3933.2006.00167.x.png)
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Abstract
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The microwave sky shows unexpected features at the largest angular scales, among them the alignments of the dipole, quadrupole and octopole. Motivated by recent X-ray cluster studies, we investigate the possibility that local structures at the 100 h(-1) Mpc scale could be responsible for such correlations. These structures give rise to a local Rees - Sciama contribution to the microwave sky that may amount to Delta T / T similar to 10(-5) at the largest angular scales. We model local structures by a spherical overdensity (Lemaitre - Tolman - Bondi model) and assume that the Local Group is falling toward the centre. We superimpose the local Rees - Sciama effect on a statistically isotropic, Gaussian sky. As expected, we find alignments among low multipoles, but a closer look reveals that they do not agree with the type of correlations revealed by the data.
Keywords:
cosmic microwave background
large-scale structure of Universe
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