arXiv:1711.11539·v1·Cosmology and Nongalactic Astrophysics
Does Anisotropic "Inflation" Produce a Small Statistical Anisotropy?
Tomohiro Fujita🇯🇵 · Ippei Obata🇯🇵
Abstract
Anisotropic inflation is an interesting model with an U(1) gauge field and it predicts the statistical anisotropy of the curvature perturbation characterized by a parameter . However, we find that the background gauge field does not follow the classical attractor solution due to the stochastic effect. We develop the stochastic formalism of a vector field and solve Langevin and Fokker-Planck equations. It is shown that this model is excluded by the CMB constraint with a high probability about .