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2011

Inflation and primordial non-Gaussianities of "generalized Galileons"

Gao, Xian, Steer, Daniele A.

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We set up cosmological perturbation theory and study the cosmological implications of the so-called ``generalized Galileon'' developed in \cite{Deffayet:2011gz,horndeski}.

This is the most general scalar field theory whose Lagrangian contains derivatives up to second order while keeping second order equations of motion, and contains as sub-cases $k$-inflation, $G$-inflation and many other models.
We calculate the power spectrum of the primordial curvature perturbation, finding a modification of the usual consistency relation of the tensor-to-scalar ratio in $k$-inflation or perfect fluid models.
Finally we also calculate the bispectrum, which contains no new shapes beyond those of $k$-inflation.

Inflation and primordial non-Gaussianities of "generalized Galileons" · Around

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