On the large-scale cosmic microwave background polarization

Details On the large-scale cosmic microwave background polarization On the large-scale cosmic microwave background polarization

Jul 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010mnras.406..586c&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Volume 406, Issue 1, pp. 586-589.

Astronomy and Astrophysics

Astronomy

5

Cosmic Background Radiation, Cosmology: Theory

Scientific paper

We discuss the large-scale polarization of the cosmic microwave background induced by the anisotropy of the spatial geometry of our Universe. Assuming an eccentricity at decoupling of about 0.64 × 10-2, we find an average large-scale polarization Δ Tpol/T0 = (0.5-1.0) × 10-6. We suggest that the forthcoming polarization data at large scales from Planck will be able to discriminate between our proposal and the generally accepted re-ionization scenario.

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