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Автор Aaron C. Vincent
Автор James M. Cline
Дата выпуска 2008-10-01
dc.description Using the gradient expansion method of Rigopoulos, Shellard and van Tent which treats cosmological perturbations as gradients on top of a homogeneous and isotropic FRW background, we study the production of nongaussianities in the roulette model of inflation. Investigating a number of trajectories within this two-field model of inflation, we find that while the superhorizon influence of the isocurvature modes on the curvature bispectrum produces nonzero contribution to f<sub>NL</sub>, the effect is negligible next to the standard inflationary prediction |f<sub>NL</sub>| ∼ n<sub>s</sub>−1. This is the case in both the squeezed and equilateral configurations of the bispectrum, although the former is slightly larger in the trajectories under consideration.
Формат application.pdf
Издатель Institute of Physics Publishing
Название Curvature spectra and nongaussianities in the roulette inflation model
Тип paper
DOI 10.1088/1126-6708/2008/10/093
Electronic ISSN 1029- 8479
Print ISSN 1126-6708
Журнал Journal of High Energy Physics
Том 2008
Первая страница 93
Последняя страница 093
Аффилиация Aaron C. Vincent; Department of Physics, Rutherford Physics Building, McGill University, 3600 Rue University, Montreal, QC, H3A 2T8, Canada
Аффилиация James M. Cline; Department of Physics, Rutherford Physics Building, McGill University, 3600 Rue University, Montreal, QC, H3A 2T8, Canada
Выпуск 10

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