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• W2079437097 abstract "We show that the difference between the theoretically expected and measured by WMAP amplitude of the quadrupole fluctuations of the cosmic microwave background (CMB) can be related to the impact of the anisotropic curvature of the homogeneous universe dominated by dark energy. In such a universe the matter expansion becomes practically isotropic just after the period of inflation, and only at small redshifts is the anisotropic expansion generated again by the small curvature ${ensuremath{Omega}}_{K}=1ensuremath{-}{ensuremath{Omega}}_{m}ensuremath{-}{ensuremath{Omega}}_{ensuremath{Lambda}}ensuremath{le}{10}^{ensuremath{-}4}$. For such models the possible deviations from the parameters derived for the standard cosmological model are evidently negligible but the correlations of large scale perturbations and distortions of their Gaussianity are possible. Such models are also compatible with the existence of a homogeneous magnetic field and matter rotation which contribute to the low $ensuremath{ell}$ anisotropy and can be considered as ``hidden parameters'' of the model. Their influence can be observed as, for example, special correlations of small scale fluctuations and the Faraday rotation of the CMB and radiation of the farthest quasars. However, both the magnetic field and matter rotation also require modifications of the simple models of isotropic inflation, and they change the evolutionary history of the early Universe." @default.
• W2079437097 created "2016-06-24" @default.
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• W2079437097 date "2007-06-26" @default.
• W2079437097 modified "2023-09-26" @default.
• W2079437097 title "Extensions of the standard cosmological model: Anisotropy, rotation, and the magnetic field" @default.
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• W2079437097 doi "https://doi.org/10.1103/physrevd.75.123517" @default.
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