Effect of halo bias and Lyman Limit Systems on the history of cosmic reionization

A.A. Kaurov1, N.Y. Gnedin1,2,3

1Department of Astronomy and Astrophysics, The University of Chicago, Chicago, IL 60637, USA
2Particle Astrophysics Center, Fermi National Accelerator Laboratory, Batavia, IL 60510, USA
3Kavli Institute for Cosmological Physics and Enrico Fermi Institute, The University of Chicago, Chicago, IL 60637, USA

We extend the existing analytical model of reionization by Furlanetto et al. (2004) to include the biasing of reionization sources and additional absorption by Lyman Limit systems. Our model is, by construction, consistent with the observed evolution of the galaxy luminosity function at z<8 and with the observed evolution of Ly-α forest at z<6. We also find that, for a wide range of values for the relative escape fraction that we consider reasonable, and which are consistent with the observational constraints on the relative escape fraction from lower redshifts, our reionization model is consistent with the WMAP constraint on the Thompson optical depth and with the SPT and EDGES constraints on the duration of reionization. We, therefore, conclude that it is possible to develop physically realistic models of reionization that are consistent with all existing observational constraints.

E-print: arXiv:1212.1458

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