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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...
Autores principales: | , |
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Lenguaje: | eng |
Publicado: |
2008
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Acceso en línea: | https://dx.doi.org/10.1103/PhysRevD.79.087301 http://cds.cern.ch/record/1151655 |
_version_ | 1780915673645449216 |
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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. |
id | cern-1151655 |
institution | Organización Europea para la Investigación Nuclear |
language | eng |
publishDate | 2008 |
record_format | invenio |
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 |
work_keys_str_mv | AT giovanninimassimo birefringencecmbpolarizationandmagnetizedbmode AT kunzekerstine birefringencecmbpolarizationandmagnetizedbmode |