Galileon inflation

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Published 14 January 2011 Published under licence by IOP Publishing Ltd
, , Citation Clare Burrage et al JCAP01(2011)014 DOI 10.1088/1475-7516/2011/01/014

1475-7516/2011/01/014

Abstract

Galileon inflation is a radiatively stable higher derivative model of inflation. The model is determined by a finite number of relevant operators which are protected by a covariant generalization of the Galileon shift symmetry.We show that the nongaussianity of the primordial density perturbation generated during an epoch of Galileon inflation is a particularly powerful observational probe of these models and that, when the speed of sound is small, fNL can be larger than the usual result fNLcs−2.

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10.1088/1475-7516/2011/01/014