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 g∗. 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 g∗≤ 10-2 with a high probability about 99.999%.
Original language | English |
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Article number | 049 |
Journal | Journal of Cosmology and Astroparticle Physics |
Volume | 2018 |
Issue number | 1 |
DOIs | |
Publication status | Published - 2018 Jan |
Externally published | Yes |
Keywords
- Ination
- physics of the early universe
- quantum cosmology
ASJC Scopus subject areas
- Astronomy and Astrophysics