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Statistical anisotropy from inflationary magnetogenesis

Provided the quantum fluctuations are amplified in the presence of a classical gauge field configuration the resulting curvature perturbations exhibit a mild statistical anisotropy which should be sufficiently weak not to conflict with current observational data. The curvature power spectra induced...

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Autor principal: Giovannini, Massimo
Lenguaje:eng
Publicado: 2016
Materias:
Acceso en línea:https://dx.doi.org/10.1103/PhysRevD.93.043543
http://cds.cern.ch/record/2124315
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author Giovannini, Massimo
author_facet Giovannini, Massimo
author_sort Giovannini, Massimo
collection CERN
description Provided the quantum fluctuations are amplified in the presence of a classical gauge field configuration the resulting curvature perturbations exhibit a mild statistical anisotropy which should be sufficiently weak not to conflict with current observational data. The curvature power spectra induced by weakly anisotropic initial states are computed here for the first time when the electric and the magnetic gauge couplings evolve at different rates as it happens, for instance, in the relativistic theory of van der Waals interactions. After recovering the results valid for coincident gauge couplings, the constraints imposed by the isotropy and the homogeneity of the initial states are discussed. The obtained bounds turn out to be more stringent than naively expected and cannot be ignored when discussing the underlying magnetogenesis scenarios.
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institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2016
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spelling cern-21243152022-08-10T12:39:47Zdoi:10.1103/PhysRevD.93.043543http://cds.cern.ch/record/2124315engGiovannini, MassimoStatistical anisotropy from inflationary magnetogenesisAstrophysics and AstronomyProvided the quantum fluctuations are amplified in the presence of a classical gauge field configuration the resulting curvature perturbations exhibit a mild statistical anisotropy which should be sufficiently weak not to conflict with current observational data. The curvature power spectra induced by weakly anisotropic initial states are computed here for the first time when the electric and the magnetic gauge couplings evolve at different rates as it happens, for instance, in the relativistic theory of van der Waals interactions. After recovering the results valid for coincident gauge couplings, the constraints imposed by the isotropy and the homogeneity of the initial states are discussed. The obtained bounds turn out to be more stringent than naively expected and cannot be ignored when discussing the underlying magnetogenesis scenarios.Provided the quantum fluctuations are amplified in the presence of a classical gauge field configuration the resulting curvature perturbations exhibit a mild statistical anisotropy which should be sufficiently weak not to conflict with current observational data. The curvature power spectra induced by weakly anisotropic initial states are computed here for the first time when the electric and the magnetic gauge couplings evolve at different rates as it happens, for instance, in the relativistic theory of van der Waals interactions. After recovering the results valid for coincident gauge couplings, the constraints imposed by the isotropy and the homogeneity of the initial states are discussed. The obtained bounds turn out to be more stringent than naively expected and cannot be ignored when discussing the underlying magnetogenesis scenarios.CERN-PH-TH-2015-196arXiv:1601.03556CERN-PH-TH-2015-196oai:cds.cern.ch:21243152016-01-14
spellingShingle Astrophysics and Astronomy
Giovannini, Massimo
Statistical anisotropy from inflationary magnetogenesis
title Statistical anisotropy from inflationary magnetogenesis
title_full Statistical anisotropy from inflationary magnetogenesis
title_fullStr Statistical anisotropy from inflationary magnetogenesis
title_full_unstemmed Statistical anisotropy from inflationary magnetogenesis
title_short Statistical anisotropy from inflationary magnetogenesis
title_sort statistical anisotropy from inflationary magnetogenesis
topic Astrophysics and Astronomy
url https://dx.doi.org/10.1103/PhysRevD.93.043543
http://cds.cern.ch/record/2124315
work_keys_str_mv AT giovanninimassimo statisticalanisotropyfrominflationarymagnetogenesis