Can Relic Superhorizon Inhomogeneities be Responsible for Large-Scale CMB Anomalies?

Details Can Relic Superhorizon Inhomogeneities be Responsible for Large-Scale CMB Anomalies? Can Relic Superhorizon Inhomogeneities be Responsible for Large-Scale CMB Anomalies?

2009-03-09

arxiv.org/abs/0903.1412v3

Phys.Lett.B702:12-15,2011

Astronomy and Astrophysics

Astrophysics

Cosmology and Extragalactic Astrophysics

5 pages, 4 figures, v2 references added in; v3 to match the published version

Scientific paper

10.1016/j.physletb.2011.06.066

We investigate the effects of the presence of relic classical superhorizon inhomogeneities during inflation. This superhorizon inhomogeneity appears as a gradient locally and picks out a preferred direction. Quantum fluctuations on this slightly inhomogeneous background are generally statistical anisotropic. We find a quadrupole modification to the ordinary isotropic spectrum. Moreover, this deviation from statistical isotropy is scale-dependent, with a $\sim -1/k^2$ factor. This result implies that the statistical anisotropy mainly appears on large scales, while the spectrum on small scales remains highly isotropic. Moreover, due to this $-1/k^2$ factor, the power on large scales is suppressed. Thus, our model can simultaneously explain the observed anisotropic alignments of the low-$\ell$ multipoles and their low power.

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