Polarization effects in cosmological models with anisotropic curvature

Details Polarization effects in cosmological models with anisotropic curvature Polarization effects in cosmological models with anisotropic curvature

Jul 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980ncimb..58..113f&link_type=abstract

Nuovo Cimento B, Serie 11, vol. 58B, July 11, 1980, p. 113-122. Research supported by the Consiglio Nazionale delle Ricerche.

Mathematics

Logic

1

Anisotropy, Astronomical Models, Cosmology, Polarization Characteristics, Relic Radiation, Curvature, Perturbation Theory, Polarized Electromagnetic Radiation, Universe

Scientific paper

The evolution of the polarization states for an electromagnetic radiation propagating in diagonal-metric cosmological models with anisotropic curvature tensor of 3-space is analyzed. It is found that the rotation of the polarization vector is small, provided the experimental constraints on the expansion anisotropy are satisfied. It is concluded that any primordial polarization of the cosmic-background radiation can survive up to the present epoch if the universe is suitably described by one of these models.

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