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  5. Improved CMB anisotropy constraints on primordial magnetic fields from the post-recombination ionization history
 

Improved CMB anisotropy constraints on primordial magnetic fields from the post-recombination ionization history

Journal
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY  
Date Issued
2019
Author(s)
PAOLETTI, DANIELA  
•
Chluba, J.
•
FINELLI, FABIO  
•
Rubiño-Martín, J. A.
DOI
10.1093/mnras/sty3521
Description
DP and FF acknowledge support by the ASI/INAF Agreement 2014-024-R.0 for the Planck LFI Activity of Phase E2 and the financial support by ASI grant 2016-24-H.0. JC is supported by the Royal Society as a Royal Society University Research Fellow at the University of Manchester, UK. JARM acknowledges financial support from the Spanish Ministry of Economy and Competitiveness (MINECO) under the projects AYA2014-60438-P and AYA2017-84185-P.
Abstract
We investigate the impact of a stochastic background of primordial magnetic fields (PMF) generated before recombination on the ionization history of the Universe and on the cosmic microwave background (CMB) radiation. Pre-recombination PMFs are dissipated during recombination and reionization via decaying MHD turbulence and ambipolar diffusion. This modifies the local matter and electron temperatures and thus affects the ionization history and Thomson visibility function. We use this effect to constrain PMFs described by a spectrum of power-law type extending our previous study (based on a scale-invariant spectrum) to arbitrary spectral index, assuming that the fields are already present at the onset of recombination. We improve previous analyses by solving several numerical issues which appeared for positively tilted PMFs indices. We derive upper bounds on the integrated amplitude of PMFs due to the separate effect of ambipolar diffusion and MHD decaying turbulence and their combination. We show that ambipolar diffusion is relevant for nB > 0 whereas for nB < 0 MHD turbulence is more important. The bound marginalized over the spectral index on the integrated amplitude of PMFs with a sharp cut-off is \sqrt{< B^2 \rangle }< 0.83 nG. We discuss the quantitative relevance of the assumptions on the damping mechanism and the comparison with previous bounds.
Volume
484
Issue
1
Start page
185
Uri
http://hdl.handle.net/20.500.12386/29559
Url
https://academic.oup.com/mnras/article-abstract/484/1/185/5270738
Issn Identifier
0035-8711
Ads BibCode
2019MNRAS.484..185P
Rights
open.access
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P015_PaolettietAl_CMBConstraintsPMFPostREc_MNRAS2019sty3521.pdf

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2.02 MB

Format

Adobe PDF

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