Journal Article

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

Michael Kuhlen and Claude-André Faucher-Giguère

in Monthly Notices of the Royal Astronomical Society

Published on behalf of The Royal Astronomical Society

Volume 423, issue 1, pages 862-876
Published in print June 2012 | ISSN: 0035-8711
Published online May 2012 | e-ISSN: 1365-2966 | DOI:
Concordance models of reionization: implications for faint galaxies and escape fraction evolution

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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 Mlim∼−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 4 per 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 Mh∼ 1010 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 50 per cent ionized fraction zreion(50 per cent) ∼ 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.

Keywords: galaxies: dwarf; galaxies: formation; galaxies: high-redshift; intergalactic medium; cosmology: theory; dark ages, reionization, first stars

Journal Article.  11428 words.  Illustrated.

Subjects: Astronomy and Astrophysics

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