Abstract
We consider a simple inflation model with a complex scalar field coupled to gravity non-minimally. Both the modulus and the angular directions of the complex scalar are slowly rolling, leading to two-field inflation. The modulus direction becomes flat due to the non-minimal coupling, and the angular direction becomes a pseudo-Goldstone boson from a small breaking of the global U(1) symmetry. We show that large non-Gaussianity can be produced during slow-roll inflation under a reasonable assumption on the initial condition of the angular direction. This scenario may be realized in particle physics models such as the Standard Model with two Higgs doublets.
Original language | English |
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Article number | 040 |
Journal | Journal of Cosmology and Astroparticle Physics |
Volume | 2011 |
Issue number | 11 |
DOIs | |
State | Published - Nov 2011 |
Keywords
- cosmological perturbation theory
- cosmology of theories beyond the SM
- inflation
- non-gaussianity