SCORCH. II. Radiation-Hydrodynamic simulations of reionization with varying radiation escape fractions

Abstract

In the Simulations and Constructions of the Reionization of Cosmic Hydrogen (SCORCH) project, we present new radiation-hydrodynamic simulations with updated high-redshift galaxy populations and varying radiation escape fractions. The simulations are designed to have fixed Thomson optical depth $\tau \approx 0.06$, consistent with recent Planck observations, and similar midpoints of reionization $7.5\lesssim z\lesssim 8.0$, but with different ionization histories. The galaxy luminosity functions and ionizing photon production rates in our model are in good agreement with recent HST observations. Adopting a power-law form for the radiation escape fraction $f_{\text{esc}}(z)=f_8[(1+z)/9{]}^{a_8}$, we simulate the cases for $a_8=0$, 1, and 2 and find $a_8\lesssim 2$ in order to end reionization in the range $5.5\lesssim z\lesssim 6.5$ to be consistent with Lyman alpha forest observations. At fixed $\tau$ and as the power-law slope $a_8$ increases, the reionization process starts earlier but ends later with a longer duration $\Delta z$ and the decreased redshift asymmetry $Az$. We find a range of durations $3.9\lesssim \Delta z\lesssim 4.6$ that is currently in tension with the upper limit $\Delta z<2.8$ inferred from a recent joint analysis of Planck and South Pole Telescope observations.

12 pages, 11 figures, 3 tables, published in ApJ

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• A halo model approach for the 21-cm power spectrum at cosmic dawn
• A systematic study of the escape of LyC and Ly$\alpha$ photons from star-forming, magnetized turbulent clouds
• AMBER: A Semi-numerical Abundance Matching Box for the Epoch of Reionization
• Minimum size of 21-cm simulations
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• The Escape Fraction of Ionizing Photons During the Epoch of Reionization: observability with the Square Kilometre Array
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• Patchy Kinetic Sunyaev-Zel'dovich Effect with Controlled Reionization History and Morphology
• Constraining Reionization in Progress at z=5.7 with Lyman-$\alpha$ Emitters: Voids, Peaks, and Cosmic Variance
• Optical depth to reionization from perturbative 21cm clustering
• The impact and response of minihalos and the inter-halo medium on cosmic reionization
• SCORCH. III. Analytical Models of Reionization with Varying Clumping Factors