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Genus topology of the cosmic microwave background from the WMAP 3-year data

2006/10/25 by J. R. Gott, J. Richard Gott III, W. N. Colley +7 · 2 citations
Physics and Astronomy · #Anisotropy #CMB cold spot #Cosmic background radiation #Cosmic microwave background #Cosmology and Gravitation Theories #Electrical and Electromagnetic Research #Galaxies: Formation, Evolution, Phenomena #Gaussian #Genus #Microwave #Topology (electrical circuits) #astro-ph

paper · pdf · doi:10.1111/j.1365-2966.2007.11730.x

MNRAS LaTeX style (mn2e.cls), EPS and JPEG figures

arxiv created 2006/10/25 · openalex publication_date 2007/05/10 · arxiv updated 2009/12/01 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05

Abstract

We have independently measured the genus topology of the temperature fluctuations in the cosmic microwave background seen in the Wilkinson Microwave Anisotropy Probe (WMAP) 3-yr data. A genus analysis of the WMAP data indicates consistency with Gaussian random-phase initial conditions, as predicted by standard inflation. We set 95 per cent confidence limits on non-linearities of −101 < fnl < 107. We also find that the observed low-ℓ(ℓ≤ 8) modes show a slight anticorrelation with the Galactic foreground, but not exceeding 95 per cent confidence, and that the topology defined by these modes is consistent with that of a Gaussian random-phase distribution (within 95 per cent confidence).

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