English

Birefringence, CMB polarization and magnetized B-mode

Astrophysics 2010-04-29 v1 General Relativity and Quantum Cosmology High Energy Physics - Phenomenology High Energy Physics - Theory

Abstract

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.

Keywords

Cite

@article{arxiv.0812.2804,
  title  = {Birefringence, CMB polarization and magnetized B-mode},
  author = {Massimo Giovannini and Kerstin E. Kunze},
  journal= {arXiv preprint arXiv:0812.2804},
  year   = {2010}
}

Comments

8 pages, 2 figures

R2 v1 2026-06-21T11:52:10.609Z