Propagation of Polarized Cosmic Microwave Background Radiation in an Anisotropic Magnetized Plasma

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Plasma Magnetohydrodynamics, Electromagnetic Fields, Cosmic Background Radiation, Electron Gas, General Theory And Basic Studies Of Plasma Lifetime, Particle And Heat Loss, Energy Balance, Field Structure, Etc., Classical Electromagnetism, Maxwell Equations, Neutrino, Muon, Pion, And Other Elementary Particles, Cosmic Rays, Electron Gas, Fermi Gas

Scientific paper

The polarization plane of the cosmic microwave background radiation (CMBR) can be rotated either in a space-time with metric of anisotropic type and in a magnetized plasma or in the presence of a quintessential background with pseudoscalar coupling to electromagnetism. A unified treatment of these three phenomena is presented for cold anisotropic plasma at the pre-recombination epoch. It is argued that the generalized expressions derived in the present study may be relevant for direct searches of a possible rotation of the cosmic microwave background polarization.

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