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Birefringence, CMB polarization and magnetized B-mode

Even in the absence of a sizable tensor contribution, a B-mode polarization can be generated because of the competition between a pseudo-scalar background and pre-decoupling magnetic fields. By investigating the dispersion relations of a magnetoactive plasma supplemented by a pseudo-scalar interacti...

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Detalles Bibliográficos
Autores principales: Giovannini, Massimo, Kunze, Kerstin E.
Lenguaje:eng
Publicado: 2008
Materias:
Acceso en línea:https://dx.doi.org/10.1103/PhysRevD.79.087301
http://cds.cern.ch/record/1151655
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author Giovannini, Massimo
Kunze, Kerstin E.
author_facet Giovannini, Massimo
Kunze, Kerstin E.
author_sort Giovannini, Massimo
collection CERN
description Even in the absence of a sizable tensor contribution, a B-mode polarization can be generated because of the competition between a pseudo-scalar background and pre-decoupling magnetic fields. By investigating the dispersion relations of a magnetoactive plasma supplemented by a pseudo-scalar interaction, the total B-mode polarization is shown to depend not only upon the plasma and Larmor frequencies but also on the pseudo-scalar rotation rate. If the (angular) frequency channels of a given experiment are larger than the pseudo-scalar rotation rate, the only possible source of (frequency dependent) B-mode autocorrelations must be attributed to Faraday rotation. In the opposite case the pseudo-scalar contribution dominates and the total rate becomes, in practice, frequency-independent. The B-mode cross-correlations can be used, under certain conditions, to break the degeneracy by disentangling the two birefringent contributions.
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spelling cern-11516552023-03-14T16:44:04Zdoi:10.1103/PhysRevD.79.087301http://cds.cern.ch/record/1151655engGiovannini, MassimoKunze, Kerstin E.Birefringence, CMB polarization and magnetized B-modeAstrophysics and AstronomyEven in the absence of a sizable tensor contribution, a B-mode polarization can be generated because of the competition between a pseudo-scalar background and pre-decoupling magnetic fields. By investigating the dispersion relations of a magnetoactive plasma supplemented by a pseudo-scalar interaction, the total B-mode polarization is shown to depend not only upon the plasma and Larmor frequencies but also on the pseudo-scalar rotation rate. If the (angular) frequency channels of a given experiment are larger than the pseudo-scalar rotation rate, the only possible source of (frequency dependent) B-mode autocorrelations must be attributed to Faraday rotation. In the opposite case the pseudo-scalar contribution dominates and the total rate becomes, in practice, frequency-independent. The B-mode cross-correlations can be used, under certain conditions, to break the degeneracy by disentangling the two birefringent contributions.Even in the absence of a sizable tensor contribution, a B-mode polarization can be generated because of the competition between a pseudo-scalar background and pre-decoupling magnetic fields. By investigating the dispersion relations of a magnetoactive plasma supplemented by a pseudo-scalar interaction, the total B-mode polarization is shown to depend not only upon the plasma and Larmor frequencies but also on the pseudo-scalar rotation rate. If the (angular) frequency channels of a given experiment are larger than the pseudo-scalar rotation rate, the only possible source of (frequency dependent) B-mode autocorrelations must be attributed to Faraday rotation. In the opposite case the pseudo-scalar contribution dominates and the total rate becomes, in practice, frequency-independent. The B-mode cross-correlations can be used, under certain conditions, to break the degeneracy by disentangling the two birefringent contributions.arXiv:0812.2804CERN-TH-PH-2008-233CERN-PH-TH-2008-233CERN-PH-TH-2008-233oai:cds.cern.ch:11516552008-12-16
spellingShingle Astrophysics and Astronomy
Giovannini, Massimo
Kunze, Kerstin E.
Birefringence, CMB polarization and magnetized B-mode
title Birefringence, CMB polarization and magnetized B-mode
title_full Birefringence, CMB polarization and magnetized B-mode
title_fullStr Birefringence, CMB polarization and magnetized B-mode
title_full_unstemmed Birefringence, CMB polarization and magnetized B-mode
title_short Birefringence, CMB polarization and magnetized B-mode
title_sort birefringence, cmb polarization and magnetized b-mode
topic Astrophysics and Astronomy
url https://dx.doi.org/10.1103/PhysRevD.79.087301
http://cds.cern.ch/record/1151655
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