The Global 21 cm Absorption from Cosmic Dawn with Inhomogeneous Gas Distribution

We make an analytical estimate of the maximum 21 cm absorption signal from the cosmic dawn, taking into account the inhomogeneity of gas distribution in the intergalactic medium (IGM) due to nonlinear structure formation. The gas located near halos is overdense but adiabatically heated, while the ga...

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Bibliographic Details
Published in:The Astrophysical journal 2018-12, Vol.869 (1), p.42
Main Authors: Xu, Yidong, Yue, Bin, Chen, Xuelei
Format: Article
Language:English
Subjects:
Absorption
Adiabatic flow
Astrophysics
Cooling effects
cosmology: theory
dark ages, reionization, first stars
Halos
Heating and cooling
Hydrogen
Inhomogeneity
Intergalactic media
intergalactic medium
Spin temperature
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Summary:We make an analytical estimate of the maximum 21 cm absorption signal from the cosmic dawn, taking into account the inhomogeneity of gas distribution in the intergalactic medium (IGM) due to nonlinear structure formation. The gas located near halos is overdense but adiabatically heated, while the gas far from halos is underdense and hence cooler. The cumulative effect of adiabatic heating and cooling from this gas inhomogeneity results in a reduction in the maximum global 21 cm absorption depth by about 40% as compared with the homogeneous IGM model, assuming saturated coupling between the spin temperature of neutral hydrogen (H i) and the adiabatic gas kinetic temperature.
ISSN:0004-637X
1538-4357
DOI:10.3847/1538-4357/aae97b