Studying the sources of cosmic reionization with 21-cm fluctuations |
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| Authors: | Rennan Barkana |
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| Institution: | Institute for Cosmic Ray Research, University of Tokyo, Kashiwa 277-8582, Japan;Division of Physics, Mathematics and Astronomy, California Institute of Technology, Mail Code 130-33, Pasadena, CA 91125, USA;Guggenheim Fellow;on sabbatical leave from the School of Physics and Astronomy, Tel Aviv University, Israel |
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| Abstract: | We explore the ability of measurements of the 21-cm power spectrum during reionization to enable the simultaneous reconstruction of the reionization history and the properties of the ionizing sources. For various sets of simulated 21-cm observations, we perform maximum likelihood fits in order to constrain the reionization and galaxy formation histories. We employ a flexible six-parameter model that parametrizes the uncertainties in the properties of high-redshift galaxies. The computational speed needed is attained through the use of an analytical model that is in reasonable agreement with numerical simulations of reionization. We find that one-year observations, with the Murchison Widefield Array, should measure the cosmic ionized fraction to ∼1 per cent accuracy at the very end of reionization, and a few per cent accuracy around the mid-point of reionization. The mean halo mass of the ionizing sources should be measurable to 10 per cent accuracy when reionization is 2/3 of the way through, and to 20 per cent accuracy throughout the central stage of reionization, if this mass is anywhere in the range 1/3 to 100 billion solar masses. |
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| Keywords: | galaxies: formation galaxies: high-redshift cosmology: theory |
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