%0 Journal Article
%T Was there an early reionization component in our universe?
%A Villanueva-Domingo, P.
%A Gariazzo, S.
%A Gnedin, N. Y.
%A Mena, O.
%J Journal of Cosmology and Astroparticle Physics
%D 2018
%V 04
%N 4
%I Iop Publishing Ltd
%@ 1475-7516
%G English
%F Villanueva-Domingo_etal2018
%O WOS:000429339200001
%O exported from refbase (https://references.ific.uv.es/refbase/show.php?record=3555), last updated on Mon, 23 Apr 2018 10:32:17 +0000
%X A deep understanding of the epoch of reionization is still missing in our knowledge of the universe. While future probes will allow us to test the precise evolution of the free electron fraction from redshifts between z similar or equal to 6 and z similar or equal to 20, at present one could ask what kind of reionization processes are allowed by present cosmic microwave background temperature and polarization measurements. An early contribution to reionization could imply a departure from the standard picture where star formation determines the reionization onset. By considering a broad class of possible reionization parameterizations, we find that current data do not require an early reionization component in our universe and that only one marginal class of models, based on a particular realization of reionization, may point to that. In addition, the frequentist Akaike information criterion (AIC) provides strong evidence against alternative reionization histories, favoring the most simple reionization scenario, which describes reionization by means of only one (constant) reionization optical depth tau.
%K cosmological parameters from CMBR
%K reionization
%R 10.1088/1475-7516/2018/04/024
%U http://arxiv.org/abs/1712.02807
%U https://doi.org/10.1088/1475-7516/2018/04/024
%P 024-17pp