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arXiv:1105.5051astro-ph.CO

Application of the Kolmogorov-Smirnov test to CMB data: Is the universe really weakly random?

Sigurd Kirkevold Næss

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Abstract

A recent application of the Kolmogorov-Smirnov test to the WMAP 7 year W-band maps claims evidence that the CMB is "weakly random", and that only 20% of the signal can be explained as a random Gaussian field. I here repeat this analysis, and in contrast to the original result find no evidence for deviation from the standard ΛCDM model. Instead, the results of the original analysis are consistent with not properly taking into account the correlations of the ΛCDM power spectrum.

arXiv comments
4 pages, 5 figures, submitted to A&A
Journal reference
DOI
doi:10.1051/0004-6361/201117344
Subjects
astro-ph.COCosmology and Nongalactic Astrophysics

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Discussed in comments1 thread

    • This is mainly Gurzadyan's work, and it shows such a complete lack of understanding for basic statistical analysis it's not even funny. They basically assume that if you have an i.i.d. random vector x, then a linearly transformed vector z = Q x, with Q some linear map, should…

      dagssView on HNParent context

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