作者: Xingang Chen , Yi Wang
DOI: 10.1088/1475-7516/2010/04/027
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摘要: In quasi-single field inflation models, massive isocurvature modes, that are coupled to the inflaton and have mass of order Hubble parameter, can nontrivial impacts on density perturbations, especially non-Gaussianities. We study a simple example in terms turning trajectory. Large bispectra with one-parameter family novel shapes arise, lying between well-known local equilateral shape. The trispectra also be very large its magnitude tNL much larger than fNL2.