Covariant second-order perturbations in generalized two-field inflation

被引:4
|
作者
Tzavara, Eleftheria [1 ,2 ]
Mizuno, Shuntaro [1 ,2 ,3 ]
van Tent, Bartjan [1 ,2 ]
机构
[1] Univ Paris 11, Phys Theor Lab, Batiment 210, F-91405 Orsay, France
[2] CNRS, F-91405 Orsay, France
[3] Univ Paris 07, CNRS, UMR 7164, APC, F-75205 Paris, France
关键词
inflation; cosmological perturbation theory; cosmological applications of theories with extra dimensions; non-gaussianity; CURVATURE PERTURBATION; DENSITY PERTURBATIONS; NON-GAUSSIANITY; GENERATION; DYNAMICS;
D O I
10.1088/1475-7516/2014/07/027
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We examine the covariant properties of generalized models of two-field inflation, with non-canonical kinetic terms and a possibly non-trivial field metric. We demonstrate that kinetic-term derivatives and covariant field derivatives do commute in a proper covariant framework, which was not realized before in the literature. We also define a set of generalized slow-roll parameters, using a unified notation. Within this framework, we study the most general class of models that allows for well-defined adiabatic and entropic sound speeds, which we identify as the models with parallel momentum and field velocity vectors. For these models we write the exact cubic action in terms of the adiabatic and isocurvature perturbations. We thus provide the tool to calculate the exact non-Gaussianity beyond slow-roll and at any scale for these generalized models. We illustrate our general results by considering their long-wavelength limit, as well as with the example of two-field DBI inflation.
引用
收藏
页数:39
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