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Self-consistent Modeling of Reionization in Cosmological Hydrodynamical Simulations

Journal Article · · The Astrophysical Journal (Online)
 [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) (SC-21); USDOE Office of Science (SC), High Energy Physics (HEP) (SC-25); Alexander von Humboldt Foundation (Germany); Federal Ministry of Education and Research (BMBF) (Germany)
Grant/Contract Number:
AC02-05CH11231
OSTI ID:
1379770
Alternate ID(s):
OSTI ID: 22869243
Journal Information:
The Astrophysical Journal (Online), Journal Name: The Astrophysical Journal (Online) Journal Issue: 2 Vol. 837; ISSN 1538-4357
Publisher:
Institute of Physics (IOP)Copyright Statement
Country of Publication:
United States
Language:
English

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Chemical enrichment in cosmological, smoothed particle hydrodynamics simulations text January 2009
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A consistent determination of the temperature of the intergalactic medium at redshift z=2.4 text January 2013
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Planck intermediate results. XLVI. Reduction of large-scale systematic effects in HFI polarization maps and estimation of the reionization optical depth text January 2016
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A Measurement of the Temperature-Density Relation in the Intergalactic Medium Using a New Lyman-alpha Absorption Line Fitting Method text January 2000
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Radiative Transfer Effects during Photoheating of the Intergalactic Medium text January 1999
Faint dwarfs as a test of DM models: WDM versus CDM text January 2015
Cosmic Dawn (CoDa): the first radiation-hydrodynamics simulation of reionization and galaxy formation in the Local Universe text January 2016
Dependence of the local reionization history on halo mass and environment: did Virgo reionize the Local Group? text January 2007
The photoheating of the intergalactic medium in synthesis models of the UV background text January 2015
Fossil remnants of reionization in the halo of the milky way text January 2008
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Spatial fluctuations of the intergalactic temperature–density relation after hydrogen reionization journal April 2018
The Local Group on FIRE: dwarf galaxy populations across a suite of hydrodynamic simulations journal May 2019
Evolution of the AGN UV luminosity function from redshift 7.5 journal June 2019
Simulating the effect of photoheating feedback during reionization journal June 2019
New synthesis models of consistent extragalactic background light over cosmic time journal January 2019
How low does it go? Too few Galactic satellites with standard reionization quenching journal July 2019
Consistent modelling of the meta-galactic UV background and the thermal/ionization history of the intergalactic medium journal January 2019
Dark-ages reionization and galaxy formation simulation – XVI. The thermal memory of reionization journal August 2019
Local photoionization feedback effects on galaxies journal September 2019
Effect of non-equilibrium ionization on derived physical conditions of the high-z intergalactic medium journal October 2019
Imprints of temperature fluctuations on the z ∼ 5 Lyman-α forest: a view from radiation-hydrodynamic simulations of reionization journal October 2019
The power spectrum of the Lyman-α Forest at z < 0.5 journal February 2019
Inhomogeneous reionization models in cosmological hydrodynamical simulations journal May 2019
Large Ly α opacity fluctuations and low CMB τ in models of late reionization with large islands of neutral hydrogen extending to z < 5.5 journal February 2019
Supermassive black holes in the early Universe journal December 2015
Measurement of the small-scale structure of the intergalactic medium using close quasar pairs journal April 2017
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
New constraints on the free-streaming of warm dark matter from intermediate and small scale Lyman-α forest data text January 2017
Consistent modelling of the meta-galactic UV background and the thermal/ionization history of the intergalactic medium text January 2019
A New Precision Measurement of the Small-scale Line-of-sight Power Spectrum of the Ly α Forest journal December 2017
A Fundamental Test for Galaxy Formation Models: Matching the Lyman- α Absorption Profiles of Galactic Halos Over Three Decades in Distance journal May 2018
Modeling the He ii Transverse Proximity Effect: Constraints on Quasar Lifetime and Obscuration journal July 2018
A New Measurement of the Temperature–density Relation of the IGM from Voigt Profile Fitting journal September 2018
New Constraints on IGM Thermal Evolution from the Ly α Forest Power Spectrum journal February 2019
Dancing in the Dark: Uncertainty in Ultrafaint Dwarf Galaxy Predictions from Cosmological Simulations journal March 2019
The Evolution of the He ii-ionizing Background at Redshifts 2.3 < z < 3.8 Inferred from a Statistical Sample of 24 HST /COS He ii Ly α Absorption Spectra journal April 2019
A Novel Statistical Method for Measuring the Temperature–Density Relation in the IGM Using the b N H i Distribution of Absorbers in the Ly α Forest journal May 2019
Anomaly in the Opacity of the Post-reionization Intergalactic Medium in the Ly α and Ly β Forest journal August 2019
Mapping Quasar Light Echoes in 3D with Ly α Forest Tomography journal September 2019
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


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