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      The Reionization Parameter Space Consistent with the Thomson Optical Depth from Planck

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          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 \(\Delta_\text{z} < 7.5\) and asymmetry \(A_\text{z}<5.3\) for \(\tau = 0.054 \pm 0.007\). The reconstructed mass-weighted ionization fraction \(x_\text{i}(z)\) is asymmetric, but early contributions to reionization are minor.

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          Author and article information

          Journal
          01 August 2018
          Article
          10.3847/2515-5172/aad68a
          1808.00553
          31957e15-5abd-4df9-86eb-c089eb387734

          http://arxiv.org/licenses/nonexclusive-distrib/1.0/

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          Research Note
          astro-ph.CO

          Cosmology & Extragalactic astrophysics
          Cosmology & Extragalactic astrophysics

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