Impact of reionization on CMB polarization tests of slow-roll inflation

Abstract

Estimates of inflationary parameters from the CMB B-mode polarization spectrum on the largest scales depend on knowledge of the reionization history, especially at low tensor-to-scalar ratio. Assuming an incorrect reionization history in the analysis of such polarization data can strongly bias the inflationary parameters. One consequence is that the single-field slow-roll consistency relation between the tensor-to-scalar ratio and tensor tilt might be excluded with high significance even if this relation holds in reality. We explain the origin of the bias and present case studies with various tensor amplitudes and noise characteristics. A more model-independent approach can account for uncertainties about reionization, and we show that parametrizing the reionization history by a set of its principal components with respect to E-mode polarization removes the bias in inflationary parameter measurement with little degradation in precision.

9 pages, 6 figures; submitted to Phys. Rev. D

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• Planck and reionization history: a model selection view
• Model independent approaches to reionization in the analysis of upcoming CMB data
• CMBPol Mission Concept Study: Reionization Science with the Cosmic Microwave Background
• Effect of the Early Reionization on the Cosmic Microwave Background and Cosmological Parameter Estimates
• Impact of reionization history on constraining primordial gravitational waves in future all-sky cosmic microwave background experiments