Lack of large-angle TT correlations persists in WMAP and Planck

2013/10/31 by Craig J. Copi, Dragan Huterer, Dominik J. Schwarz +1 · 96 citations
Physics and Astronomy · #Astronomy #Astrophysics #CMB cold spot #Cold dark matter #Cosmic background radiation #Cosmic microwave background #Cosmology #Cosmology and Gravitation Theories #Dark Matter and Cosmic Phenomena #Physics #Planck #Quantum mechanics #Radio Astronomy Observations and Technology #astro-ph.CO

paper · pdf · doi:10.1093/mnras/stv1143

published in Monthly Notices of the Royal Astronomical Society 451(3), 2978-2985 (Oxford University Press) · 8 pages, 4 figures, submitted to MNRAS, v2: Minor corrections, updated references, v3: Minor corrections to agree with published version

arxiv created 2015/06/03 · openalex publication_date 2015/06/18 · arxiv updated 2015/10/14 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05

Abstract

The lack of large-angle correlations in the observed microwave background temperature fluctuations persists in the final-year maps from Wilkinson Microwave Anisotropy Probe (WMAP) and the first cosmological data release from Planck. We find a statistically robust and significant result: p-values for the missing correlations lying below 0.24 per cent (i.e. evidence at more than 3σ) for foreground cleaned maps, in complete agreement with previous analyses based upon earlier WMAP data. A cut-sky analysis of the PlanckHFI 100 GHz frequency band, the ‘cleanest CMB channel’ of this instrument, returns a p-value as small as 0.03 per cent, based on the conservative mask defined by WMAP. These findings are in stark contrast to expectations from the inflationary Lambda cold dark matter model and still lack a convincing explanation. If this lack of large-angle correlations is a true feature of our Universe, and not just a statistical fluke, then the cosmological dipole must be considerably smaller than that predicted in the best-fitting model.

Citations

• An estimate of the local integrated Sachs-Wolfe signal and its impact on cosmic microwave background anomalies
• Large-angle cosmic microwave background suppression and polarization predictions
• Large-scale alignments from WMAP and Planck
• No large-angle correlations on the non-Galactic microwave sky

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