Published November 1, 2020 | Version v1
Journal article

Inflation with multiple vector fields and non-Gaussianities

  • 1. Center for Gravitational Physics, Yukawa Institute for Theoretical Physics, Kyoto University, Kyoto 606-8502 (Japan)
  • 2. Faculty of Physics, Shahrood University of Technology, P.O. Box 3619995161 Shahrood (Iran, Islamic Republic of)
  • 3. School of Astronomy, Institute for Research in Fundamental Sciences (IPM), P.O. Box 19395-5531, Tehran (Iran, Islamic Republic of)

Description

We consider a model of inflation consisting a triplet of U(1) vector fields with the parity violating interaction which is non-minimally coupled to inflaton. The vector field sector enjoys global O ( 3 ) symmetry which admits isotropic configuration and provides not only vector modes but also scalar and tensor modes. We decompose the scalar perturbations into the adiabatic, entropy and isocurvature perturbations and compute all power spectra and cross correlations of the scalar and the tensor sectors. The tensor modes associated with the vector fields contribute to the power spectrum of gravitational waves while the parity violating term generates chirality in gravitational power spectra and bispectra. We study nonlinear scalar and tensor perturbations and compute all bispectra and three-point cross-correlations. In particular, it is shown that the non-Gaussianity of curvature perturbations and gravitational waves are enhanced by the vector field perturbations. We show that non-Gaussianities put strong constraints on the model parameters such as the parity violating coupling and the fractional energy of the vector fields.

Availability note (English)

Available from http://dx.doi.org/10.1088/1475-7516/2020/11/041

Additional details

Publishing Information

Journal Title
Journal of Cosmology and Astroparticle Physics
Journal Volume
2020
Journal Issue
11
Journal Page Range
p. 041
ISSN
1475-7516