Imprint of Inhomogeneous Hydrogen Reionization on the Temperature Distribution of the Intergalactic Medium

Abstract

We study the impact of inhomogeneous hydrogen reionization on the thermal evolution of the intergalactic medium (IGM) using hydrodynamic + radiative transfer simulations where reionization is completed either early (z ~ 9) or late (z ~ 6). In general, we find that low-density gas near large-scale overdensities is ionized and heated earlier than gas in the large-scale, underdense voids. Furthermore, at a later time the IGM temperature is inversely related to the reionization redshift because gas that is heated earlier has more time to cool through adiabatic expansion and Compton scattering. Thus, at the end of reionization the median temperature-density relation is an inverted power-law with slope gamma-1 ~ -0.2, in both models. However, at fixed density, there is up to order unity scatter in the temperature due to the distribution of reionization redshifts. Because of the complex equation-of-state, the evolved IGM temperature-density relations for the redshift range 4 < z < 6 can still have significant curvature and scatter. These features must be taken into account when interpreting the Lyman alpha absorption in high redshift quasar spectra.

4 pages, 5 figures, accepted by ApJ Letters

References in corpus (10)

• Observational constraints on Cosmic Reionization
• The halo mass function from the dark ages through the present day
• Radiative transfer simulations of cosmic reionization I: methodology and initial results
• The Halo Mass Function: High-Redshift Evolution and Universality
• The Cosmic Code Comparison Project
• Glimpsing through the high redshift neutral hydrogen fog
• The History and Morphology of Helium Reionization
• Dark matter halo abundances, clustering and assembly histories at high redshift
• The Topology of Cosmological Reionization
• Out-of-Core Hydrodynamic Simulations for Cosmological Applications

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