Please use this identifier to cite or link to this item:
http://hdl.handle.net/20.500.12386/29559
DC Field | Value | Language |
---|---|---|
dc.contributor.author | PAOLETTI, DANIELA | en_US |
dc.contributor.author | Chluba, J. | en_US |
dc.contributor.author | FINELLI, FABIO | en_US |
dc.contributor.author | Rubiño-Martín, J. A. | en_US |
dc.date.accessioned | 2021-01-07T14:57:25Z | - |
dc.date.available | 2021-01-07T14:57:25Z | - |
dc.date.issued | 2019 | en_US |
dc.identifier.issn | 0035-8711 | en_US |
dc.identifier.uri | http://hdl.handle.net/20.500.12386/29559 | - |
dc.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. | en_US |
dc.description.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 n<SUB>B</SUB> > 0 whereas for n<SUB>B</SUB> < 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. | en_US |
dc.language.iso | eng | en_US |
dc.title | Improved CMB anisotropy constraints on primordial magnetic fields from the post-recombination ionization history | en_US |
dc.type | Article | - |
dc.identifier.doi | 10.1093/mnras/sty3521 | en_US |
dc.identifier.scopus | 2-s2.0-85063942476 | en_US |
dc.identifier.isi | 000462293100014 | en_US |
dc.identifier.url | https://academic.oup.com/mnras/article-abstract/484/1/185/5270738 | en_US |
dc.relation.medium | STAMPA | en_US |
dc.relation.volume | 484 | en_US |
dc.relation.issue | 1 | en_US |
dc.relation.firstpage | 185 | en_US |
dc.type.referee | REF_1 | en_US |
dc.description.numberofauthors | 4 | en_US |
dc.description.international | sì | en_US |
dc.contributor.country | ITA | en_US |
dc.contributor.country | GBR | en_US |
dc.contributor.country | ESP | en_US |
dc.relation.scientificsector | FIS/05 - ASTRONOMIA E ASTROFISICA | en_US |
dc.relation.journal | MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | en_US |
dc.type.miur | 262 Articolo in rivista | - |
dc.identifier.adsbibcode | 2019MNRAS.484..185P | en_US |
dc.relation.ercsector | ERC sectors::Physical Sciences and Engineering::PE9 Universe sciences: astro-physics/chemistry/biology; solar systems; stellar, galactic and extragalactic astronomy, planetary systems, cosmology, space science, instrumentation::PE9_14 Cosmology | en_US |
dc.description.apc | no | en_US |
dc.description.oa | 1 – prodotto con file in versione Open Access (allegare il file al passo 5-Carica) | en_US |
item.openairecristype | http://purl.org/coar/resource_type/c_18cf | - |
item.openairetype | Article | - |
item.languageiso639-1 | en | - |
item.cerifentitytype | Publications | - |
item.grantfulltext | open | - |
item.fulltext | With Fulltext | - |
crisitem.author.dept | OAS Bologna | - |
crisitem.author.dept | OAS Bologna | - |
crisitem.author.orcid | 0000-0003-4761-6147 | - |
crisitem.author.orcid | 0000-0002-6694-3269 | - |
crisitem.journal.journalissn | 0035-8711 | - |
crisitem.journal.ance | E112946 | - |
Appears in Collections: | 1.01 Articoli in rivista |
Files in This Item:
File | Description | Size | Format | |
---|---|---|---|---|
P015_PaolettietAl_CMBConstraintsPMFPostREc_MNRAS2019sty3521.pdf | PDF editoriale | 2.07 MB | Adobe PDF | View/Open |
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