Extensions of the standard cosmological model: Anisotropy, rotation, and the magnetic field
Extensions of the standard cosmological model: Anisotropy, rotation, and the magnetic field
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 …