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The cross-correlation between 21 cm intensity mapping maps and the Lyα forest in the post-reionization era

Carucci, Isabella Paola
•
Viel, Matteo
•
Villaescusa Navarro, F.
2017
  • journal article

Periodico
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS
Abstract
We investigate the cross-correlation signal between 21cm intensity mapping maps and the Lyα forest in the fully non-linear regime using state-of-the-art hydrodynamic simulations. The cross-correlation signal between the Lyα forest and 21cm maps can provide a coherent and comprehensive picture of the neutral hydrogen (HI) content of our Universe in the post-reionization era, probing both its mass content and volume distribution. We compute the auto-power spectra of both fields together with their cross-power spectrum at z=2.4 and find that on large scales the fields are completely anti-correlated. This anti-correlation arises because regions with high (low) 21cm emission, such as those with a large (low) concentration of damped Lyα systems, will show up as regions with low (high) transmitted flux. We find that on scales smaller than k'0.2h Mpc−1 the cross-correlation coefficient departs from−1, at a scale where non-linearities show up. We use the anisotropy of the power spectra in redshift-space to determine the values of the bias and of the redshift-space distortion parameters of both fields. We find that the errors on the value of the cosmological and astrophysical parameters could decrease by 30% when adding data from the cross-power spectrum, in a conservative analysis. Our results point out that linear theory is capable of reproducing the shape and amplitude of the cross-power up to rather non-linear scales. Finally, we find that the 21cm-Lyα cross-power spectrum can be detected by combining data from a BOSS-like survey together with 21cm intensity mapping observations by SKA1-MID with a S/N ratio higher than 3 in k∈[0.06,1]h Mpc−1. We emphasize that while the shape and amplitude of the 21cm auto-power spectrum can be severely affected by residual foreground contamination, cross-power spectra will be less sensitive to that and therefore can be used to identify systematics in the 21cm maps. © Copyright 2017 IOP Publishing
DOI
10.1088/1475-7516/2017/04/001
WOS
WOS:000401806200001
Archivio
http://hdl.handle.net/20.500.11767/48338
info:eu-repo/semantics/altIdentifier/scopus/2-s2.0-85019415403
https://arxiv.org/abs/1611.07527
Diritti
closed access
Soggetti
  • cosmological paramete...

  • power spectrum

  • cosmic web

  • cosmological simulati...

  • Settore FIS/05 - Astr...

Scopus© citazioni
14
Data di acquisizione
Jun 7, 2022
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Web of Science© citazioni
22
Data di acquisizione
Mar 23, 2024
Visualizzazioni
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Data di acquisizione
Apr 19, 2024
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