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Magnetized CMB anisotropies

Possible effects of large-scale magnetic fields on the Cosmic Microwave Background (CMB) are reviewed. Depending on the specific branch of the spectrum of plasma excitations, magnetic fields are treated either within a two-fluid plasma description or within an effective (one-fluid) approach. The uni...

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Autor principal: Giovannini, Massimo
Lenguaje:eng
Publicado: 2005
Materias:
Acceso en línea:https://dx.doi.org/10.1088/0264-9381/23/2/R01
http://cds.cern.ch/record/879481
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author Giovannini, Massimo
author_facet Giovannini, Massimo
author_sort Giovannini, Massimo
collection CERN
description Possible effects of large-scale magnetic fields on the Cosmic Microwave Background (CMB) are reviewed. Depending on the specific branch of the spectrum of plasma excitations, magnetic fields are treated either within a two-fluid plasma description or within an effective (one-fluid) approach. The uniform field approximation is contrasted with the fully inhomogeneous field approximation. It is argued that the interplay between CMB physics and large-scale magnetic fields will represent a rather interesting cross-disciplinary arena along the next few years.
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institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2005
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spelling cern-8794812023-10-04T06:50:29Zdoi:10.1088/0264-9381/23/2/R01http://cds.cern.ch/record/879481engGiovannini, MassimoMagnetized CMB anisotropiesAstrophysics and AstronomyPossible effects of large-scale magnetic fields on the Cosmic Microwave Background (CMB) are reviewed. Depending on the specific branch of the spectrum of plasma excitations, magnetic fields are treated either within a two-fluid plasma description or within an effective (one-fluid) approach. The uniform field approximation is contrasted with the fully inhomogeneous field approximation. It is argued that the interplay between CMB physics and large-scale magnetic fields will represent a rather interesting cross-disciplinary arena along the next few years.Possible effects of large-scale magnetic fields on the Cosmic Microwave Background (CMB) are reviewed. Depending on the specific branch of the spectrum of plasma excitations, magnetic fields are treated either within a two-fluid plasma description or within an effective (one-fluid) approach. The uniform field approximation is contrasted with the fully inhomogeneous field approximation. It is argued that the interplay between CMB physics and large-scale magnetic fields will represent a rather interesting cross-disciplinary arena along the next few years.astro-ph/0508544CERN-PH-TH-2005-152CERN-PH-TH-2005-152oai:cds.cern.ch:8794812005-08-25
spellingShingle Astrophysics and Astronomy
Giovannini, Massimo
Magnetized CMB anisotropies
title Magnetized CMB anisotropies
title_full Magnetized CMB anisotropies
title_fullStr Magnetized CMB anisotropies
title_full_unstemmed Magnetized CMB anisotropies
title_short Magnetized CMB anisotropies
title_sort magnetized cmb anisotropies
topic Astrophysics and Astronomy
url https://dx.doi.org/10.1088/0264-9381/23/2/R01
http://cds.cern.ch/record/879481
work_keys_str_mv AT giovanninimassimo magnetizedcmbanisotropies