English

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 Δz<7.5\Delta_\text{z} < 7.5 and asymmetry Az<5.3A_\text{z}<5.3 for τ=0.054±0.007\tau = 0.054 \pm 0.007. The reconstructed mass-weighted ionization fraction xi(z)x_\text{i}(z) 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

R2 v1 2026-06-23T03:22:10.301Z