A.J. Benson
Non-uniform reionization by galaxies and its effect on the cosmic microwave background
Benson, A.J.; Nusser, A.; Sugiyama, N.; Lacey, C.G.
Abstract
We present predictions for the reionization of the intergalactic medium (IGM) by stars in high-redshift galaxies, based on a semi-analytic model of galaxy formation. We calculate ionizing luminosities of galaxies, including the effects of absorption by interstellar gas and dust on the escape fraction ƒesc, and follow the propagation of the ionization fronts around each galaxy in order to calculate the filling factor of ionized hydrogen in the IGM. For a ΛCDM cosmology, with parameters of the galaxy formation model chosen to match observations of present-day galaxies, and a physical calculation of the escape fraction, we find that the hydrogen in the IGM will be reionized at redshift z=6.1 if the IGM has uniform density, but only by z=4.5 if the IGM is clumped. If instead we assume a constant escape fraction of 20 per cent for all galaxies, then we find reionization at z=4.5 and 7.8 for the same two assumptions about IGM clumping. We combine our semi-analytic model with an N-body simulation of the distribution of dark matter in the Universe in order to calculate the evolution of the spatial and velocity distribution of the ionized gas in the IGM, and use this to calculate the secondary temperature anisotropies induced in the cosmic microwave background (CMB) by scattering off free electrons. The models predict a spectrum of secondary anisotropies covering a broad range of angular scales, with fractional temperature fluctuations ∼10−7-10−6 on arcminute scales. The amplitude depends strongly on the total baryon density, and less sensitively on ƒesc. The amplitude also depends somewhat on the geometry of reionization, with models in which the regions of highest gas density are reionized first giving larger CMB fluctuations than the case where galaxies ionize surrounding spherical regions, and models where low-density regions reionize first giving the smallest fluctuations. Measurement of these anisotropies can therefore put important constraints on the reionization process, in particular, the redshift evolution of the filling factor, and should be a primary objective of a next generation submillimetre telescope such as the Atacama Large Millimeter Array.
Citation
Benson, A., Nusser, A., Sugiyama, N., & Lacey, C. (2001). Non-uniform reionization by galaxies and its effect on the cosmic microwave background. Monthly Notices of the Royal Astronomical Society, 320(1), 153-176. https://doi.org/10.1046/j.1365-8711.2001.03957.x
Journal Article Type | Article |
---|---|
Publication Date | Jan 1, 2001 |
Deposit Date | Feb 20, 2015 |
Publicly Available Date | Feb 24, 2015 |
Journal | Monthly Notices of the Royal Astronomical Society |
Print ISSN | 0035-8711 |
Electronic ISSN | 1365-2966 |
Publisher | Royal Astronomical Society |
Peer Reviewed | Peer Reviewed |
Volume | 320 |
Issue | 1 |
Pages | 153-176 |
DOI | https://doi.org/10.1046/j.1365-8711.2001.03957.x |
Keywords | Intergalactic medium, Cosmology: theory, Dark matter, Large-scale structure of Universe. |
Files
Published Journal Article
(984 Kb)
PDF
Copyright Statement
This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society © 2001 RAS. Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.
You might also like
The complex interplay of AGN jet-inflated bubbles and the intracluster medium
(2023)
Journal Article
Active galactic nuclei jets simulated with smoothed particle hydrodynamics
(2023)
Journal Article
QWIND3: UV line-driven accretion disc wind models for AGN feedback
(2022)
Journal Article
Spin-driven jet feedback in idealized simulations of galaxy groups and clusters
(2022)
Journal Article