Results from EDGES High-Band. III. New Constraints on Parameters of the Early Universe

We present new constraints on parameters of cosmic dawn and the epoch of reionization derived from the EDGES High-Band spectrum (90-190 MHz). The parameters are probed by evaluating global 21 cm signals generated with the recently developed Global21cm tool. This tool uses neural networks trained and...

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Published inThe Astrophysical journal Vol. 875; no. 1; pp. 67 - 83
Main Authors Monsalve, Raul A., Fialkov, Anastasia, Bowman, Judd D., Rogers, Alan E. E., Mozdzen, Thomas J., Cohen, Aviad, Barkana, Rennan, Mahesh, Nivedita
Format Journal Article
LanguageEnglish
Published Philadelphia The American Astronomical Society 10.04.2019
IOP Publishing
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Summary:We present new constraints on parameters of cosmic dawn and the epoch of reionization derived from the EDGES High-Band spectrum (90-190 MHz). The parameters are probed by evaluating global 21 cm signals generated with the recently developed Global21cm tool. This tool uses neural networks trained and tested on ∼30,000 spectra produced with semi-numerical simulations that assume the standard thermal evolution of the cosmic microwave background and the intergalactic medium. From our analysis, we constrain at 68% (1) the minimum virial circular velocity of star-forming halos to Vc < 19.3 km s−1, (2) the X-ray heating efficiency of early sources to fX > 0.0042, and (3) the low-energy cutoff of the X-ray spectral energy distribution to min < 2.3 keV. We also constrain the star formation efficiency (f*), the electron scattering optical depth (τe), and the mean-free path of ionizing photons (Rmfp). We recompute the constraints after incorporating into the analysis four estimates for the neutral hydrogen fraction from high-z quasars and galaxies, and a prior on τe from Planck 2018. The largest impact of the external observations is on the parameters that most directly characterize reionization. Specifically, we derive the combined 68% constraints τe < 0.063 and Rmfp > 27.5 Mpc. The external observations also have a significant effect on Vc due to its degeneracy with τe, while the constraints on f*, fX, and min, remain primarily determined by EDGES.
Bibliography:Galaxies and Cosmology
AAS13912
ISSN:0004-637X
1538-4357
DOI:10.3847/1538-4357/ab07be