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K. M. Smith, W. Hu, and M. Kaplinghat, Phys. Rev. D74
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N. Aghanim et al. (Planck), Submitted to: Astron. Astrophys. (2015), arXiv:1507.02704 [astro-ph.CO]
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2016

Complete Reionization Constraints from Planck 2015 Polarization

Heinrich, Chen He, Miranda, V, Hu, Wayne

Understand

We conduct an analysis of the Planck 2015 data that is complete in reionization observables from the large angle polarization $E$-mode spectrum in the redshift range $6 < z < 30$.

Based on 5 principal components, all of which are constrained by the data, this single analysis can be used to infer constraints on any model for reionization in the same range; we develop an effective likelihood approach for applying these constraints to models.
By allowing for an arbitrary ionization history, this technique tests the robustness of inferences on the total optical depth from the usual step-like transition assumption, which is important for the interpretation of many other cosmological parameters such as the dark energy and neutrino mass.
The Planck 2015 data not only allow a high redshift $z>15$ component to the optical depth but prefer it at the $2\sigma$ level.

Built on

A. Lewis, A. Challinor, and A. Lasenby, Astrophys. J. 538
2000
Earlier work this paper cites.
A. Lewis and S. Bridle, Phys. Rev. D66
2002
Earlier work this paper cites.
W. Hu, Phys. Rev. D65
2002
Earlier work this paper cites.
A. Kogut et al. (WMAP), Astrophys. J. Suppl. 148
2003
Earlier work this paper cites.
W. Hu and G. P. Holder, Phys. Rev. D68
2003
Earlier work this paper cites.
W. Hu and B. Jain, Phys. Rev. D70
2004
Earlier work this paper cites.
K. M. Smith, W. Hu, and M. Kaplinghat, Phys. Rev. D74
2006
Earlier work this paper cites.
A. Lewis, J. Weller, and R. Battye, Mon. Not. Roy. Astron. Soc. 373
2006
Earlier work this paper cites.
M. J. Mortonson and W. Hu, Phys. Rev. D80
Original
2009
Earlier work this paper cites.