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Title: Self-consistent Modeling of Reionization in Cosmological Hydrodynamical Simulations

Journal Article · · The Astrophysical Journal (Online)
ORCiD logo [1];  [1];  [2]
  1. Max Planck Inst. for Astronomy, Heidelberg (Germany)
  2. Lawrence Berkeley National Lab. (LBNL), Berkeley, CA (United States)

The ultraviolet background (UVB) emitted by quasars and galaxies governs the ionization and thermal state of the intergalactic medium (IGM), regulates the formation of high-redshift galaxies, and is thus a key quantity for modeling cosmic reionization. The vast majority of cosmological hydrodynamical simulations implement the UVB via a set of spatially uniform photoionization and photoheating rates derived from UVB synthesis models. In this paper, we show that simulations using canonical UVB rates reionize and, perhaps more importantly, spuriously heat the IGM, much earlier ($$z\sim 15$$) than they should. This problem arises because at $$z\gt 6$$, where observational constraints are nonexistent, the UVB amplitude is far too high. We introduce a new methodology to remedy this issue, and we generate self-consistent photoionization and photoheating rates to model any chosen reionization history. Following this approach, we run a suite of hydrodynamical simulations of different reionization scenarios and explore the impact of the timing of reionization and its concomitant heat injection on the thermal state of the IGM. We present a comprehensive study of the pressure smoothing scale of IGM gas, illustrating its dependence on the details of both hydrogen and helium reionization, and argue that it plays a fundamental role in interpreting Lyα forest statistics and the thermal evolution of the IGM. The premature IGM heating we have uncovered implies that previous work has likely dramatically overestimated the impact of photoionization feedback on galaxy formation, which sets the minimum halo mass able to form stars at high redshifts. Finally, we make our new UVB photoionization and photoheating rates publicly available for use in future simulations.

Research Organization:
Lawrence Berkeley National Laboratory (LBNL), Berkeley, CA (United States)
Sponsoring Organization:
USDOE Office of Science (SC), Advanced Scientific Computing Research (ASCR); USDOE Office of Science (SC), High Energy Physics (HEP); Alexander von Humboldt Foundation (Germany); German Federal Ministry of Education and Research (BMBF)
Grant/Contract Number:
AC02-05CH11231
OSTI ID:
1379770
Journal Information:
The Astrophysical Journal (Online), Vol. 837, Issue 2; ISSN 1538-4357
Publisher:
Institute of Physics (IOP)Copyright Statement
Country of Publication:
United States
Language:
English
Citation Metrics:
Cited by: 59 works
Citation information provided by
Web of Science

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New synthesis models of consistent extragalactic background light over cosmic time journal January 2019
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Dark-ages reionization and galaxy formation simulation – XVI. The thermal memory of reionization journal August 2019
Consistent modelling of the meta-galactic UV background and the thermal/ionization history of the intergalactic medium text January 2019
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New Constraints on the free-streaming of warm dark matter from intermediate and small scale Lyman-$α$ forest data text January 2017
Spatial fluctuations of the intergalactic temperature-density relation after hydrogen reionization text January 2018
A New Measurement of the Temperature Density Relation of the IGM From Voigt Profile Fitting text January 2017
New synthesis models of consistent extragalactic background light over cosmic time text January 2018
The Local Group on FIRE: Dwarf galaxy populations across a suite of hydrodynamic simulations text January 2018
Inhomogeneous Reionization Models in Cosmological Hydrodynamical Simulations text January 2018