Distinguishing models of reionization using future radio observations of 21-cm 1-point statistics
Dec 4, 201317 pages
Published in:
- Mon.Not.Roy.Astron.Soc. 443 (2014) 4, 3090-3106
- Published: Oct 1, 2014
e-Print:
- 1312.1342 [astro-ph.CO]
View in:
Citations per year
Abstract: (Oxford University Press)
We explore the impact of reionization topology on 21-cm statistics. Four reionization models are presented which emulate large ionized bubbles around overdense regions (21cmfast/global-inside-out), small ionized bubbles in overdense regions (local-inside-out), large ionized bubbles around underdense regions (global-outside-in) and small ionized bubbles around underdense regions (local-outside-in). We show that first generation instruments might struggle to distinguish global models using the shape of the power spectrum alone. All instruments considered are capable of breaking this degeneracy with the variance, which is higher in outside-in models. Global models can also be distinguished at small scales from a boost in the power spectrum from a positive correlation between the density and neutral-fraction fields in outside-in models. Negative skewness is found to be unique to inside-out models and we find that pre-Square Kilometre Array (SKA) instruments could detect this feature in maps smoothed to reduce noise errors. The early, mid- and late phases of reionization imprint signatures in the brightness-temperature moments, we examine their model dependence and find pre-SKA instruments capable of exploiting these timing constraints in smoothed maps. The dimensional skewness is introduced and is shown to have stronger signatures of the early and mid-phase timing if the inside-out scenario is correct.Note:
- 18 pages, 13 figures, updated to agree with published version
- methods: statistical
- intergalactic medium
- cosmology: theory
- dark ages, reionization, first stars
References(78)
Figures(15)