Anisotropic dark energy and ellipsoidal universe

Abstract

A cosmological model with anisotropic dark energy is analyzed. The amount of deviation from isotropy of the equation of state of dark energy, the skewness δ, generates an anisotropization of the large-scale geometry of the Universe, quantifiable by means of the actual shear Σ_0. Requiring that the level of cosmic anisotropization at the time of decoupling is such to solve the "quadrupole problem" of cosmic microwave background radiation, we find that |δ| \sim 10^{-4} and |Σ_0| \sim 10^{-5}, compatible with existing limits derived from the magnitude-redshift data on type Ia supernovae.

10 pages, 3 figures. Revised version to match published version. References added

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• Unified dark fluid in Brans-Dicke theory
• Testing the isotropy of the Universe with type Ia supernovae in a model-independent way
• Testing Isotropy in the Local Universe
• Screening anisotropy via energy-momentum squared gravity: $\Lambda$CDM model with hidden anisotropy
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