Large non-Gaussianities with intermediate shapes from quasi-single-field inflation

被引:249
作者
Chen, Xingang [1 ,2 ]
Wang, Yi [3 ,4 ]
机构
[1] MIT, Ctr Theoret Phys, Cambridge, MA 02139 USA
[2] Univ Cambridge, Ctr Theoret Cosmol, DAMTP, Cambridge CB3 0WA, England
[3] McGill Univ, Dept Phys, Montreal, PQ H3A 2T8, Canada
[4] Chinese Acad Sci, Inst Theoret Phys, KITPC, Beijing 100190, Peoples R China
基金
加拿大自然科学与工程研究理事会;
关键词
PERTURBATIONS; FLATNESS; UNIVERSE; HORIZON;
D O I
10.1103/PhysRevD.81.063511
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We study the slow-roll inflation models, where the inflaton slow-rolls along a trajectory whose orthogonal directions are lifted by potentials with masses of order the Hubble parameter. In these models large non-Gaussianities can be generated through the transformation from the isocurvature modes to the curvature mode, once the inflaton trajectory turns. We find large bispectra with a one-parameter family of novel shapes, interpolating between the equilateral and local shape. According to the in-in formalism, the shapes of these non-Gaussianities are different from a simple projection from the isocurvature non-Gaussian correlation functions.
引用
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页数:5
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