Closing in on the large-scale CMB power asymmetry

Abstract

Measurements of the cosmic microwave background (CMB) temperature anisotropies have revealed a dipolar asymmetry in power at the largest scales, in apparent contradiction with the statistical isotropy of standard cosmological models. The significance of the effect is not very high, and is dependent on a posteriori choices. Nevertheless, a number of models have been proposed that produce a scale-dependent asymmetry. We confront several such models for a physical, position-space modulation with CMB temperature observations. We find that, while some models that maintain the standard isotropic power spectrum are allowed, others, such as those with modulated tensor or uncorrelated isocurvature modes, can be ruled out on the basis of the overproduction of isotropic power. This remains the case even when an extra isocurvature mode fully anti-correlated with the adiabatic perturbations is added to suppress power on large scales.

6 pages, 3 figures. Comments welcome

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• Towards testing CMB anomalies using the kinetic and polarized Sunyaev Zel'dovich effects
• An Anisotropic Model for the Universe
• Constraints on ${\tau }_{\mathrm{NL}}$ from Planck temperature and polarization
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