Concordance models of reionization: Implications for faint galaxies and escape fraction evolution

Michael Kuhlen*, Claude André Faucher-Giguère

*Corresponding author for this work

Research output: Contribution to journalArticle

246 Scopus citations

Abstract

Recent observations have constrained the galaxy ultraviolet (UV) luminosity function up to z∼ 10. However, these observations alone allow for a wide range of reionization scenarios due to uncertainties in the abundance of faint galaxies and the escape fraction of ionizing photons. We show that requiring continuity with post-reionization (z < 6) measurements, where the Lyα forest provides a complete probe of the cosmological emissivity of ionizing photons, significantly reduces the permitted parameter space. Models that are simultaneously consistent with the measured UV luminosity function, the Thomson optical depth to the microwave background and the Lyα forest data require either (1) extrapolation of the galaxy luminosity function down to very faint UV magnitudes M lim∼-10, corresponding roughly to the UV background suppression scale; (2) an increase of the escape fraction by a factor ≳10 from z= 4 (where the best fit is 4per cent) to 9; or (3) more likely, a hybrid solution in which undetected galaxies contribute significantly and the escape fraction increases more modestly. Models in which star formation is strongly suppressed in low-mass, reionization-epoch haloes of mass up to M h∼ 10 10 M (e.g. owing to a metallicity dependence) are only allowed for extreme assumptions for the redshift evolution of the escape fraction. However, variants of such models in which the suppression mass is reduced (e.g. assuming an earlier or higher metallicity floor) are in better agreement with the data. Interestingly, concordance scenarios satisfying the available data predict a consistent redshift of 50per cent ionized fraction z reion(50percent) ∼ 10. On the other hand, the duration of reionization is sensitive to the relative contribution of bright versus faint galaxies, with scenarios dominated by faint galaxies predicting a more extended reionization event. Scenarios relying too heavily on high-redshift dwarfs are disfavoured by kinetic Sunyaev-Zeldovich measurements, which prefer a short reionization history.

Original languageEnglish (US)
Pages (from-to)862-876
Number of pages15
JournalMonthly Notices of the Royal Astronomical Society
Volume423
Issue number1
DOIs
StatePublished - Jun 2012

Keywords

  • Cosmology: theory
  • Dark ages, reionization, first stars
  • Galaxies: dwarf
  • Galaxies: formation
  • Galaxies: high-redshift
  • Intergalactic medium

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

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