SCORCH. II. Radiation-Hydrodynamic simulations of reionization with varying radiation escape fractions
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 $τ\ap...
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ftdatacite:10.48550/arxiv.1712.04464 2023-05-15T18:22:49+02:00 SCORCH. II. Radiation-Hydrodynamic simulations of reionization with varying radiation escape fractions Doussot, Aristide Trac, Hy Cen, Renyue 2017 https://dx.doi.org/10.48550/arxiv.1712.04464 https://arxiv.org/abs/1712.04464 unknown arXiv https://dx.doi.org/10.3847/1538-4357/aaef75 arXiv.org perpetual, non-exclusive license http://arxiv.org/licenses/nonexclusive-distrib/1.0/ Cosmology and Nongalactic Astrophysics astro-ph.CO FOS Physical sciences article-journal Article ScholarlyArticle Text 2017 ftdatacite https://doi.org/10.48550/arxiv.1712.04464 https://doi.org/10.3847/1538-4357/aaef75 2022-04-01T10:09:43Z 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 $τ\approx 0.06$, 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 $τ$ and as the power-law slope $a_8$ increases, the reionization process starts earlier but ends later with a longer duration $Δz$ and the decreased redshift asymmetry $Az$. We find a range of durations $3.9 \lesssim Δz \lesssim 4.6$ that is currently in tension with the upper limit $Δz < 2.8$ inferred from a recent joint analysis of Planck and South Pole Telescope observations. : 12 pages, 11 figures, 3 tables, published in ApJ Text South pole DataCite Metadata Store (German National Library of Science and Technology) South Pole |
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Cosmology and Nongalactic Astrophysics astro-ph.CO FOS Physical sciences |
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Cosmology and Nongalactic Astrophysics astro-ph.CO FOS Physical sciences Doussot, Aristide Trac, Hy Cen, Renyue SCORCH. II. Radiation-Hydrodynamic simulations of reionization with varying radiation escape fractions |
topic_facet |
Cosmology and Nongalactic Astrophysics astro-ph.CO FOS Physical sciences |
description |
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 $τ\approx 0.06$, 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 $τ$ and as the power-law slope $a_8$ increases, the reionization process starts earlier but ends later with a longer duration $Δz$ and the decreased redshift asymmetry $Az$. We find a range of durations $3.9 \lesssim Δz \lesssim 4.6$ that is currently in tension with the upper limit $Δz < 2.8$ inferred from a recent joint analysis of Planck and South Pole Telescope observations. : 12 pages, 11 figures, 3 tables, published in ApJ |
format |
Text |
author |
Doussot, Aristide Trac, Hy Cen, Renyue |
author_facet |
Doussot, Aristide Trac, Hy Cen, Renyue |
author_sort |
Doussot, Aristide |
title |
SCORCH. II. Radiation-Hydrodynamic simulations of reionization with varying radiation escape fractions |
title_short |
SCORCH. II. Radiation-Hydrodynamic simulations of reionization with varying radiation escape fractions |
title_full |
SCORCH. II. Radiation-Hydrodynamic simulations of reionization with varying radiation escape fractions |
title_fullStr |
SCORCH. II. Radiation-Hydrodynamic simulations of reionization with varying radiation escape fractions |
title_full_unstemmed |
SCORCH. II. Radiation-Hydrodynamic simulations of reionization with varying radiation escape fractions |
title_sort |
scorch. ii. radiation-hydrodynamic simulations of reionization with varying radiation escape fractions |
publisher |
arXiv |
publishDate |
2017 |
url |
https://dx.doi.org/10.48550/arxiv.1712.04464 https://arxiv.org/abs/1712.04464 |
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South Pole |
geographic_facet |
South Pole |
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South pole |
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South pole |
op_relation |
https://dx.doi.org/10.3847/1538-4357/aaef75 |
op_rights |
arXiv.org perpetual, non-exclusive license http://arxiv.org/licenses/nonexclusive-distrib/1.0/ |
op_doi |
https://doi.org/10.48550/arxiv.1712.04464 https://doi.org/10.3847/1538-4357/aaef75 |
_version_ |
1766202228255752192 |