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Large‐Angle Anomalies in the CMB

2010/01/01 by Craig J. Copi, Dragan Huterer, Dominik J. Schwarz +1 · 3 citations
Earth and Planetary Sciences · Physics and Astronomy · #Cosmology and Gravitation Theories #Galaxies: Formation, Evolution, Phenomena #Geophysics and Gravity Measurements #astro-ph.CO #gr-qc #hep-th

paper · pdf · doi:10.1155/2010/847541

published as Advances in Astronomy vol. 2010, Article ID 847541 (2010) · Review in the Advances in Astronomy special issue "Testing the Gaussianity and Statistical Isotropy of the Universe" (eds. D. Huterer, E. Komatsu and S. Shandera); 16 pages, 7 figures. v2 matches the published version

openalex publication_date 2010/01/01 · arxiv created 2010/11/10 · arxiv updated 2012/12/10 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/01

Abstract

We review the recently found large‐scale anomalies in the maps of temperature anisotropies in the cosmic microwave background. These include alignments of the largest modes of CMB anisotropy with each other and with geometry and direction of motion of the solar ssystem, and the unusually low power at these largest scales. We discuss these findings in relation to expectation from standard inflationary cosmology, their statistical significance, the tools to study them, and the various attempts to explain them.

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