An improved model of H II bubbles during the epoch of reionization


METADATA ONLY
Loading...

Date

2014

Publication Type

Journal Article

ETH Bibliography

yes

Citations

Altmetric
METADATA ONLY

Data

Rights / License

Abstract

The size distribution of ionized regions during the epoch of reionization - a key ingredient in understanding the H I power spectrum observable by 21 cm experiments - can be modelled analytically using the excursion set formalism of random walks in the smoothed initial density field. To date, such calculations have been based on simplifying assumptions carried forward from the earliest excursion set models of two decades ago. In particular, these models assume that the random walks have uncorrelated steps and that haloes can form at arbitrary locations in the initial density field. We extend these calculations by incorporating recent technical developments that allow us to (a) include the effect of correlations in the steps of the walks induced by a realistic smoothing filter and (b) more importantly, account for the fact that dark matter haloes preferentially form near peaks in the initial density. A comparison with previous calculations shows that including these features, particularly the peaks constraint on halo locations, has large effects on the size distribution of the HII bubbles surrounding these haloes. For example, when comparing models at the same value of the globally averaged ionized volume fraction, the typical bubble sizes predicted by our model are more than a factor of 2 larger than earlier calculations. Our results can potentially have a significant impact on estimates of the observable HI power spectrum. © 2014 The Authors. Published by Oxford University Press on behalf of the Royal Astronomical Society.

Publication status

published

Editor

Book title

Volume

442 (2)

Pages / Article No.

1470 - 1482

Publisher

Oxford University Press

Event

Edition / version

Methods

Geographic location

Date collected

Date created

Subject

Intergalactic medium; Cosmology: theory; Dark ages, reionization, first stars; Large-scale structure of Universe

Organisational unit

03928 - Refregier, Alexandre / Refregier, Alexandre check_circle

Notes

Accepted 5 May 2014, Received 7 April 2014, In original form 30 January 2014, First published online 16 June 2014.

Funding Info about funding

Related publications and datasets