Published February 15, 2008 | Version v1
Journal article

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

  • 1. Department of Physics, University of Chicago, Chicago, Illinois 60637 (United States)
  • 2. Kavli Institute for Cosmological Physics, Enrico Fermi Institute, University of Chicago, Chicago, Illinois 60637 (United States)
  • 3. Department of Astronomy and Astrophysics, University of Chicago, Chicago, Illinois 60637 (United States)

Description

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

Additional details

Publishing Information

Journal Title
Physical Review. D, Particles Fields
Journal Volume
77
Journal Issue
4
Journal Page Range
p. 043506-043506.9
ISSN
0556-2821
CODEN
PRVDAQ

INIS

Country of Publication
United States
Country of Input or Organization
International Atomic Energy Agency (IAEA)
INIS RN
39059094
Subject category
S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS; S71: CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS;
Descriptors DEI
ACCURACY; AMPLITUDES; COSMOLOGY; ENERGY SPECTRA; INFLATIONARY UNIVERSE; POLARIZATION; SCALARS; TENSORS
Descriptors DEC
COSMOLOGICAL MODELS; MATHEMATICAL MODELS; SPECTRA

Optional Information

Notes
(c) 2008 The American Physical Society