The small scale power asymmetry in the cosmic microwave background

Abstract

We investigate the hemispherical power asymmetry in the cosmic microwave background on small angular scales. We find an anomalously high asymmetry in the multipole range l=601-2048, with a naive statistical significance of 6.5 sigma. However, we show that this extreme anomaly is simply a coincidence of three other effects, relativistic power modulation, edge effects from the mask applied, and inter-scale correlations. After correcting for all of these effects, the significance level drops to ~1 sigma, i.e., there is no anomalous intrinsic asymmetry in the small angular scales. Using this null result, we derive a constraint on a potential dipolar modulation amplitude, A(k)<0.0045 on the ~10 Mpc-scale, at 95% C.L. This new constraint must be satisfied by any theoretical model attempting to explain the hemispherical asymmetry at large angular scales.

16 pages, 6 figures. v2: journal version (minor changes compared to v1)

References in corpus (6)

• A Hemispherical Power Asymmetry from Inflation
• Superhorizon Perturbations and the Cosmic Microwave Background
• Constraints on cosmic hemispherical power anomalies from quasars
• Broken Isotropy from a Linear Modulation of the Primordial Perturbations
• Observing the evolution of the CMB
• Consistency tests for Planck and WMAP in the low multipole domain

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