The First Billion Years Project: The escape fraction of ionizing photons in the epoch of reionization

TL;DR

This study uses high-resolution cosmological simulations to analyze how the escape fraction of ionizing photons from proto-galaxies depends on halo properties during the epoch of reionization, revealing complex dependencies and anisotropies.

Contribution

It provides a detailed analysis of the physical factors influencing escape fractions in high-redshift galaxies using a large simulation dataset, highlighting the mass dependence and variability.

Findings

Escape fraction strongly depends on gas column density within 10 pc.

Halos below 10^8 solar masses have higher escape fractions due to lower potential wells.

Significant variability and anisotropy in escape fractions among similar halos.

Abstract

Proto-galaxies forming in low-mass dark matter haloes are thought to provide the majority of ionizing photons needed to reionize the Universe, due to their high escape fractions of ionizing photons. We study how the escape fraction in high-redshift galaxies relates to the physical properties of the halo in which the galaxies form, by computing escape fractions in more than 75000 haloes between redshifts 27 and 6 that were extracted from the First Billion Years project, high-resolution cosmological hydrodynamics simulations of galaxy formation. We find that the main constraint on the escape fraction is the gas column density in a radius of 10 pc around the stellar populations, causing a strong mass dependence of the escape fraction. The lower potential well in haloes with virial mass below 1e8 solar mass results in low column densities that can be penetrated by radiation from young stars (age < 5 Myr). In haloes with virial mass above 1e8 solar mass supernova feedback is important, but only 30% of the haloes in this mass range have an escape fraction higher than 1%. We find a large range of escape fractions in haloes with similar properties, caused by different distributions of the dense gas in the halo. This makes it very hard to predict the escape fraction on the basis of halo properties and results in a highly anisotropic escape fraction. The strong mass dependence, the large spread and the large anisotropy of the escape fraction may strongly affect the topology of reionization and is something current models of cosmic reionization should strive to take into account.