Anna Mangilli: Constraining the reionization era and inflation with the CMB polarization at large angular scales: new preliminary Planck results and future prospects
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Europe/Paris
1222-RC-08 (LPNHE)
1222-RC-08
LPNHE
Description
The accurate measurement of the CMB polarization at large
angular scales is one of the key challenges left for the current and
future CMB experiments. The large scale enhancement of the CMB
polarization power spectra due to the reionization of the Universe in
fact encodes unique informations about the reionization history and the
inflationary epoch. In this talk I will go through a brief introduction
about the CMB polarization, highlighting the scientific goals related to
the analysis of the CMB data at large angular scales. I will show how
the Planck 2015 release represented a first step towards the accurate
characterization of the CMB polarization on the full sky. I will then
present the new and improved -yet preliminary- results of the Planck
data analysis at large angular scales. I will show that these
preliminary Planck results confirm the trend towards a significantly
smaller value of the reionization optical depth parameter τ with respect
to previous estimations from CMB polarization data. This result reduces
the tension between CMB based analyses and constraints from other
astrophysical sources. Finally I will discuss the improvement on the
estimation of the tensor-to-scalar ratio parameter r when the B-modes
data at large scales are included and I will present the theoretical
implications of the results and the future prospects for forthcoming
proposed CMB space missions like CoRE++/LiteBird.