arXiv · astro-ph/0312416
Constraining the reionization history with large angle CMB polarization
Abstract
The first-year WMAP data release showed that the reionization optical depth to CMB photons is greater than previously thought. This follows from unexpectedly high values of the C^TE_l spectrum, for l up to ~30, presumably allowing a measurement of the E-mode polarization spectrum C^E_l sooner than expected. This note aims to test the capability of large-angle polarization experiments to explore the history of the cosmological reionization, considering also the impact of cosmic variance. In particular, here we discuss how well the ionized fraction x_e and the reionization redshift z_r can be separately measured, at various levels of instrumental noise.
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Loris PL Colombo. 2004-02-11. Constraining the reionization history with large angle CMB polarization. https://doi.org/10.1088/1475-7516%2F2004%2F03%2F003
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