The Reionization Parameter Space Consistent with the Thomson Optical Depth from Planck
Cosmology and Nongalactic Astrophysics
2018-08-10 v2
Abstract
We study the reionization parameter space consistent with the current measurement of the Thomson optical depth using a new parametrization of the reionization history. The mass-weighted ionization fraction is specified in terms of the redshift midpoint, duration, and asymmetry shape parameters. We perform an MCMC analysis using conservative flat priors and physical constraints. Our analysis yields a redshift midpoint of z_{50}=7.66\substack{+0.57-0.61}\text{(68%)}\substack{+1.26-1.02}\text{(95%)}, and upper limits on the duration and asymmetry for . The reconstructed mass-weighted ionization fraction is asymmetric, but early contributions to reionization are minor.
Keywords
Cite
@article{arxiv.1808.00553,
title = {The Reionization Parameter Space Consistent with the Thomson Optical Depth from Planck},
author = {Daniel Glazer and Markus Michael Rau and Hy Trac},
journal= {arXiv preprint arXiv:1808.00553},
year = {2018}
}
Comments
AAS Research Note