TY - JOUR
T1 - Results from EDGES High-Band. III. New Constraints on Parameters of the Early Universe
AU - Monsalve, Raul A.
AU - Fialkov, Anastasia
AU - Bowman, Judd D.
AU - Rogers, Alan E.E.
AU - Mozdzen, Thomas J.
AU - Cohen, Aviad
AU - Barkana, Rennan
AU - Mahesh, Nivedita
N1 - Publisher Copyright:
© 2019. The American Astronomical Society. All rights reserved.
PY - 2019/4/10
Y1 - 2019/4/10
N2 - 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 V c <19.3 km s-1, (2) the X-ray heating efficiency of early sources to f X > 0.0042, and (3) the low-energy cutoff of the X-ray spectral energy distribution to ν min <2.3 keV. We also constrain the star formation efficiency (f ∗), the electron scattering optical depth (τ e), and the mean-free path of ionizing photons (R mfp). 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 τ e 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 τ e <0.063 and R mfp > 27.5 Mpc. The external observations also have a significant effect on V c due to its degeneracy with τ e, while the constraints on f ∗, f X, and ν min, remain primarily determined by EDGES.
AB - 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 V c <19.3 km s-1, (2) the X-ray heating efficiency of early sources to f X > 0.0042, and (3) the low-energy cutoff of the X-ray spectral energy distribution to ν min <2.3 keV. We also constrain the star formation efficiency (f ∗), the electron scattering optical depth (τ e), and the mean-free path of ionizing photons (R mfp). 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 τ e 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 τ e <0.063 and R mfp > 27.5 Mpc. The external observations also have a significant effect on V c due to its degeneracy with τ e, while the constraints on f ∗, f X, and ν min, remain primarily determined by EDGES.
KW - cosmology: observations
KW - early universe
KW - galaxies: high-redshift
KW - methods: data analysis
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U2 - 10.3847/1538-4357/ab07be
DO - 10.3847/1538-4357/ab07be
M3 - Article
AN - SCOPUS:85067192452
SN - 0004-637X
VL - 875
JO - Astrophysical Journal
JF - Astrophysical Journal
IS - 1
M1 - 67
ER -